Author: "R. Saldanha" / Topic: 0103 physical sciences - Searchworks@Jio Institute Digital Library Search Results

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1. A New Strategy for Optimizing HSIL Transmission Lines

Author: Sandro T. M. Goncalves, André Luiz Paganotti, Marcio Matias Afonso, Isabella Abrão Marques Duane, Marco Aurélio O. Schroeder, and Rodney R. Saldanha
Subjects: 010302 applied physics, Computer science, 020209 energy, Energy Engineering and Power Technology, 02 engineering and technology, 01 natural sciences, Ellipsoid, Characteristic impedance, Line (electrical engineering), Computer Science Applications, Conductor, Electric power transmission, Transmission (telecommunications), Control and Systems Engineering, Electric field, 0103 physical sciences, 0202 electrical engineering, electronic engineering, information engineering, Electronic engineering, Electrical and Electronic Engineering, Electrical conductor
Abstract: This paper presents an efficient procedure for optimizing the electric field at ground level of high surge impedance loading transmission lines. Such lines have the capacity to achieve higher power transmission rates than the conventional ones. The ellipsoidal method is applied in order to maximize the transmitted power and minimize the electric field at ground level through the variation of the conductor’s positions in the tower, given its physical and electrical constraints. By means of an efficient new approach to handle the conductors, the optimization gives birth to compact line designs combined with conventional bundles of conductors. Furthermore, it is shown that the proposed strategy can increase the transmitted power, reduce the electric field at ground level, and shorten the running time of the optimization algorithm.
Published: 2020

2. Imaging individual barium atoms in solid xenon for barium tagging in nEXO

Author: X. S. Jiang, A. Der Mesrobian-Kabakian, T. Tolba, S. Rescia, D. Fairbank, A. Piepke, Y. Y. Ding, O. Zeldovich, D. Kodroff, T. Daniels, J. Echevers, R. DeVoe, M. Hughes, Simon Johnston, R. Saldanha, O. Nusair, R. Krücken, Alexis G. Schubert, R. MacLellan, G. St-Hilaire, C. Chambers, I. J. Arnquist, Lorenzo Fabris, J.-L. Vuilleumier, N. Roy, Yuehe Lin, U. Wichoski, L. Cao, David Moore, B. T. Cleveland, John L. Orrell, S. Kravitz, F. Nolet, Veljko Radeka, Jens Dilling, B. Mong, M. Wagenpfeil, J. Dalmasson, T. Ziegler, J. P. Brodsky, T. Bhatta, P. C. Rowson, A.C. Odian, I. Badhrees, M. Heffner, Z. Li, Gerrit Wrede, D. Fudenberg, S. X. Wu, M. Tarka, F. Vachon, G. Li, Douglas H Beck, L. J. Wen, S. Parent, Samuele Sangiorgio, A. House, David Leonard, W. Cree, L. Darroch, J. Todd, G. Gallina, Y-R Yen, Thomas Koffas, W. M. Fairbank, I. Ostrovskiy, K. S. Kumar, D. A. Harris, X.L. Sun, J. B. Zhao, S. Delaquis, T. Stiegler, A. Kuchenkov, M. J. Dolinski, X. F. Wu, A. Larson, Yunyan Zhou, O. Njoya, E. V. Hansen, Giorgio Gratta, K. Skarpaas, Ethan Brown, A. Iverson, Triveni Rao, M. Weber, Shu Li, A. Karelin, P. Hufschmidt, David A. Sinclair, Wei Wu, R.J. Newby, T. Rossignol, M. J. Jewell, Qun-Yao Wang, Zhijun Ning, Y. Ito, L. J. Kaufman, Wei Wei, Rejean Fontaine, S. J. Daugherty, F. Bourque, Y. Lan, Liang Yang, R. Tsang, A. Jamil, S. Feyzbakhsh, C. Licciardi, W. R. Cen, R. Gornea, Guofu Cao, E. Raguzin, J. Farine, Eric W. Hoppe, Gerard Visser, A. Burenkov, T. Brunner, Arun Kumar Soma, Justin Albert, J. Watkins, V.N. Stekhanov, M. Coon, A. Pocar, Cory T. Overman, T. Tsang, A. Craycraft, Venkatesh Veeraraghavan, F. Retiere, Angelo Dragone, Jochen M. Schneider, Qing Xia, X. Zhang, M. Chiu, J. Hößl, P. S. Barbeau, G. S. Ortega, Jean-Francois Pratte, V. A. Belov, M. Oriunno, Serge A. Charlebois, T. I. Totev, K. Murray, Gisela Anton, T. Walton, J. Daughhetee, A. E. Robinson, K. Odgers, M. Côté, Thilo Michel, and Gabriele Giacomini
Subjects: Physics, Sapphire window, Multidisciplinary, 010308 nuclear & particles physics, Analytical chemistry, chemistry.chemical_element, Barium, 01 natural sciences, Particle identification, Background level, Xenon, chemistry, Double beta decay, 0103 physical sciences, Atom, Neutrino, 010306 general physics
Abstract: Author(s): Chambers, C; Walton, T; Fairbank, D; Craycraft, A; Yahne, DR; Todd, J; Iverson, A; Fairbank, W; Alamare, A; Albert, JB; Anton, G; Arnquist, IJ; Badhrees, I; Barbeau, PS; Beck, D; Belov, V; Bhatta, T; Bourque, F; Brodsky, JP; Brown, E; Brunner, T; Burenkov, A; Cao, GF; Cao, L; Cen, WR; Charlebois, SA; Chiu, M; Cleveland, B; Coon, M; Cree, W; Cote, M; Dalmasson, J; Daniels, T; Darroch, L; Daugherty, SJ; Daughhetee, J; Delaquis, S; Mesrobian-Kabakian, A Der; DeVoe, R; Dilling, J; Ding, YY; Dolinski, MJ; Dragone, A; Echevers, J; Fabris, L; Farine, J; Feyzbakhsh, S; Fontaine, R; Fudenberg, D; Giacomini, G; Gornea, R; Gratta, G; Hansen, EV; Heffner, M; Hoppe, EW; Hosl, J; House, A; Hufschmidt, P; Hughes, M; Ito, Y; Jamil, A; Jessiman, C; Jewell, MJ; Jiang, XS; Karelin, A; Kaufman, LJ; Kodroff, D; Koffas, T; Kravitz, S; Krucken, R; Kuchenkov, A; Kumar, KS; Lan, Y; Larson, A; Leonard, DS; Li, G; Li, S; Li, Z; Licciardi, C; Lin, YH; Lv, P; MacLellan, R; Michel, T; Mong, B; Moore, DC | Abstract: The search for neutrinoless double beta decay probes the fundamental properties of neutrinos, including whether or not the neutrino and antineutrino are distinct. Double beta detectors are large and expensive, so background reduction is essential for extracting the highest sensitivity. The identification, or 'tagging', of the $^{136}$Ba daughter atom from double beta decay of $^{136}$Xe provides a technique for eliminating backgrounds in the nEXO neutrinoless double beta decay experiment. The tagging scheme studied in this work utilizes a cryogenic probe to trap the barium atom in solid xenon, where the barium atom is tagged via fluorescence imaging in the solid xenon matrix. Here we demonstrate imaging and counting of individual atoms of barium in solid xenon by scanning a focused laser across a solid xenon matrix deposited on a sapphire window. When the laser sits on an individual atom, the fluorescence persists for $\sim$30~s before dropping abruptly to the background level, a clear confirmation of one-atom imaging. No barium fluorescence persists following evaporation of a barium deposit to a limit of $\leq$0.16\%. This is the first time that single atoms have been imaged in solid noble element. It establishes the basic principle of a barium tagging technique for nEXO.
Published: 2019

3. Reflectivity of VUV-sensitive Silicon Photomultipliers in Liquid Xenon

Author: M. Heffner, Thilo Michel, M. Hughes, F. Vachon, Jean-Francois Pratte, Aleksey E. Bolotnikov, A. Craycraft, R. DeVoe, C. Gingras, C.R. Natzke, A. De St. Croix, T. I. Totev, K. Murray, Gisela Anton, J. C. Nzobadila Ondze, S. Al Kharusi, R. Saldanha, O. Nusair, J. Ringuette, R. Krücken, W. M. Fairbank, M. Worcester, A. Der Mesrobian-Kabakian, N. Massacret, Lorenzo Fabris, David Moore, Wen-Qi Yan, K. Harouaka, R. Gornea, E. Hansen, C. T. Overman, Samuele Sangiorgio, I. Ostrovskiy, H. Rasiwala, M. Tarka, K. S. Kumar, M. Elbeltagi, R. Tsang, A. Larson, John L. Orrell, T. Daniels, E. Caden, F. Retière, Z. Li, Mike Richman, N. Roy, S. Feyzbakhsh, G. Giacomini, M. Murra, G. Li, E. Raguzin, A. Pocar, A. Iverson, Ethan Brown, B. Mong, C. Licciardi, F. Nolet, J. P. Brodsky, A. Tidball, T. McElroy, Shu Li, T. Rossignol, V. A. Belov, R. MacLellan, O. Zeldovich, M. Medina Peregrina, A. Karelin, B. T. Cleveland, K. Odgers, I. Badhrees, Venkatesh Veeraraghavan, D. Fairbank, A. Kuchenkov, M. Wagenpfeil, M. Walent, Giorgio Gratta, Qing Xia, Sergio Ferrara, C. Vivo-Vilches, D. Schulte, Govinda Adhikari, G. S. Ortega, J. Todd, Arun Kumar Soma, C. Weinheimer, T. Brunner, D. S. Leonard, Serge A. Charlebois, A. Odian, L. Darroch, S. Rescia, C. Huhmann, M. J. Dolinski, M. J. Jewell, R. Lindsay, D. Chernyak, L. Althueser, V.N. Stekhanov, M. L. Di Vacri, T. Ziegler, Y. Lan, S. Parent, L. J. Kaufman, A. Gorham, S. X. Wu, P. A. Breur, J. Bane, A. E. Robinson, Eric W. Hoppe, J. Echevers, D. Goeldi, G.J. Ramonnye, Liang Yang, A. Jamil, S. Thibado, C. Richard, M. Chiu, J. Farine, P. Martel-Dion, Guofu Cao, T. Bhatta, J. Nattress, E. Angelico, B. Chana, Douglas H Beck, T. Stiegler, J. Schneider, K. Deslandes, P. C. Rowson, A. House, A. Fieguth, C.A. Hardy, U. Wichoski, S. Viel, G. Gallina, A. Piepke, I. J. Arnquist, P. Gautam, K. G. Leach, R.J. Newby, S. Triambak, F. Spadoni, and C. Chambers
Subjects: Materials science, Physics - Instrumentation and Detectors, APDS, chemistry.chemical_element, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, 030218 nuclear medicine & medical imaging, law.invention, 03 medical and health sciences, 0302 clinical medicine, Optics, Silicon photomultiplier, Xenon, law, 0103 physical sciences, Wafer, Angular resolution, Instrumentation, Mathematical Physics, 010308 nuclear & particles physics, business.industry, Detector, Instrumentation and Detectors (physics.ins-det), Avalanche photodiode, chemistry, Angle of incidence (optics), business
Abstract: Silicon photomultipliers are regarded as a very promising technology for next-generation, cutting-edge detectors for low-background experiments in particle physics. This work presents systematic reflectivity studies of Silicon Photomultipliers (SiPM) and other samples in liquid xenon at vacuum ultraviolet (VUV) wavelengths. A dedicated setup at the University of M\"unster has been used that allows to acquire angle-resolved reflection measurements of various samples immersed in liquid xenon with 0.45{\deg} angular resolution. Four samples are investigated in this work: one Hamamatsu VUV4 SiPM, one FBK VUV-HD SiPM, one FBK wafer sample and one Large-Area Avalanche Photodiode (LA-APD) from EXO-200. The reflectivity is determined to be 25-36% at an angle of incidence of 20{\deg} for the four samples and increases to up to 65% at 70{\deg} for the LA-APD and the FBK samples. The Hamamatsu VUV4 SiPM shows a decline with increasing angle of incidence. The reflectivity results will be incorporated in upcoming light response simulations of the nEXO detector., Comment: 18 pages, 11 figures
Published: 2021

4. NEXO: Neutrinoless double beta decay search beyond $10^{28}$ year half-life sensitivity

Author: G Adhikari, S Al Kharusi, E Angelico, G Anton, I J Arnquist, I Badhrees, J Bane, V Belov, E P Bernard, T Bhatta, A Bolotnikov, P A Breur, J P Brodsky, E Brown, T Brunner, E Caden, G F Cao, L Cao, C Chambers, B Chana, S A Charlebois, D Chernyak, M Chiu, B Cleveland, R Collister, S A Czyz, J Dalmasson, T Daniels, L Darroch, R DeVoe, M L Di Vacri, J Dilling, Y Y Ding, A Dolgolenko, M J Dolinski, A Dragone, J Echevers, M Elbeltagi, L Fabris, D Fairbank, W Fairbank, J Farine, S Ferrara, S Feyzbakhsh, Y S Fu, G Gallina, P Gautam, G Giacomini, W Gillis, C Gingras, D Goeldi, R Gornea, G Gratta, C A Hardy, K Harouaka, M Heffner, E W Hoppe, A House, A Iverson, A Jamil, M Jewell, X S Jiang, A Karelin, L J Kaufman, I Kotov, R Krücken, A Kuchenkov, K S Kumar, Y Lan, A Larson, K G Leach, B G Lenardo, D S Leonard, G Li, S Li, Z Li, C Licciardi, R Lindsay, R MacLellan, M Mahtab, P Martel-Dion, J Masbou, N Massacret, T McElroy, K McMichael, M Medina Peregrina, T Michel, B Mong, D C Moore, K Murray, J Nattress, C R Natzke, R J Newby, K Ni, F Nolet, O Nusair, J C Nzobadila Ondze, K Odgers, A Odian, J L Orrell, G S Ortega, C T Overman, S Parent, A Perna, A Piepke, A Pocar, J-F Pratte, N Priel, V Radeka, E Raguzin, G J Ramonnye, T Rao, H Rasiwala, S Rescia, F Retière, J Ringuette, V Riot, T Rossignol, P C Rowson, N Roy, R Saldanha, S Sangiorgio, X Shang, A K Soma, F Spadoni, V Stekhanov, X L Sun, M Tarka, S Thibado, A Tidball, J Todd, T Totev, S Triambak, R H M Tsang, T Tsang, F Vachon, V Veeraraghavan, S Viel, C Vivo-Vilches, P Vogel, J-L Vuilleumier, M Wagenpfeil, T Wager, M Walent, K Wamba, Q Wang, W Wei, L J Wen, U Wichoski, S Wilde, M Worcester, S X Wu, W H Wu, X Wu, Q Xia, W Yan, H Yang, L Yang, O Zeldovich, J Zhao, T Ziegler, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), and nEXO
Subjects: Nuclear and High Energy Physics, background: effect, Physics - Instrumentation and Detectors, FOS: Physical sciences, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], time-projection chambers, 01 natural sciences, neutrinoless double beta decay, Monte Carlo simulations, double-beta decay: (0neutrino), 0103 physical sciences, neutrino: mass, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, detector: design, xenon: liquid, 010308 nuclear & particles physics, neutrinos, Instrumentation and Detectors (physics.ins-det), sensitivity, time projection chamber, 3. Good health, photon: scintillation counter, copper, radioactivity, Xe-136, experimental results
Abstract: The nEXO neutrinoless double beta decay experiment is designed to use a time projection chamber and 5000 kg of isotopically enriched liquid xenon to search for the decay in $^{136}$Xe. Progress in the detector design, paired with higher fidelity in its simulation and an advanced data analysis, based on the one used for the final results of EXO-200, produce a sensitivity prediction that exceeds the half-life of $10^{28}$ years. Specifically, improvements have been made in the understanding of production of scintillation photons and charge as well as of their transport and reconstruction in the detector. The more detailed knowledge of the detector construction has been paired with more assays for trace radioactivity in different materials. In particular, the use of custom electroformed copper is now incorporated in the design, leading to a substantial reduction in backgrounds from the intrinsic radioactivity of detector materials. Furthermore, a number of assumptions from previous sensitivity projections have gained further support from interim work validating the nEXO experiment concept. Together these improvements and updates suggest that the nEXO experiment will reach a half-life sensitivity of $1.35\times 10^{28}$ yr at 90% confidence level in 10 years of data taking, covering the parameter space associated with the inverted neutrino mass ordering, along with a significant portion of the parameter space for the normal ordering scenario, for almost all nuclear matrix elements. The effects of backgrounds deviating from the nominal values used for the projections are also illustrated, concluding that the nEXO design is robust against a number of imperfections of the model., Comment: 26 pages, 19 figures, version accepted by Journal of Phys. G
Published: 2021
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5. Cosmogenic activation of silicon

Author: S. R. Elliott, R. C. Thomas, K. Ramanathan, A. Matalon, J. L. Burnett, R. Saldanha, Radomir Smida, A. Piers, R. H. M. Tsang, R. Bunker, A. E. Chavarria, Paolo Privitera, and P. Mitra
Subjects: Physics, Physics - Instrumentation and Detectors, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Silicon, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, chemistry.chemical_element, Computer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing), Instrumentation and Detectors (physics.ins-det), 7. Clean energy, 01 natural sciences, chemistry, 13. Climate action, 0103 physical sciences, Production (computer science), Sensitivity (control systems), Nuclear Experiment (nucl-ex), Atomic physics, 010306 general physics, Nuclear Experiment, Astrophysics - Cosmology and Nongalactic Astrophysics, Production rate
Abstract: The production of $^{3}$H, $^{7}$Be, and $^{22}$Na by interactions of cosmic-ray particles with silicon can produce radioactive backgrounds in detectors used to search for rare events. Through controlled irradiation of silicon CCDs and wafers with a neutron beam that mimics the cosmic-ray neutron spectrum, followed by direct counting, we determined that the production rate from cosmic-ray neutrons at sea level is ($112 \pm 24$) atoms/(kg day) for $^{3}$H, ($8.1 \pm 1.9 $) atoms/(kg day) for $^{7}$Be, and ($43.0 \pm 7.1 $) atoms/(kg day) for $^{22}$Na. Complementing these results with the current best estimates of activation cross sections for cosmic-ray particles other than neutrons, we obtain a total sea-level cosmic-ray production rate of ($124 \pm 24$) atoms/(kg day) for $^{3}$H, ($9.4 \pm 2.0 $) atoms/(kg day) for $^{7}$Be, and ($49.6 \pm 7.3 $) atoms/(kg day) for $^{22}$Na. These measurements will help constrain background estimates and determine the maximum time that silicon-based detectors can remain unshielded during detector fabrication before cosmogenic backgrounds impact the sensitivity of next-generation rare-event searches., Comment: 21 pages, 16 figures, 10 tables. Accepted version of the article published in Physical Review D
Published: 2020

6. Event Reconstruction in a Liquid Xenon Time Projection Chamber with an Optically-Open Field Cage

Author: B. Chana, N. Roy, L. Cao, O. Nusair, G. St-Hilaire, Douglas H Beck, R. Krücken, F. Nolet, E. Raguzin, P. A. Breur, T. McElroy, T. Bhatta, L. J. Kaufman, Gerard Visser, D. Goeldi, M. Coon, Eric W. Hoppe, F. Vachon, Z. Li, C. Chambers, Veljko Radeka, Cory T. Overman, L. J. Wen, J. L. Vuilleumier, Samuele Sangiorgio, L. Darroch, P. Gautam, P. Nakarmi, Kaixuan Ni, K. S. Kumar, A. De St. Croix, R. Tsang, Haijun Yang, E. V. Hansen, P. Lv, E. Caden, S. X. Wu, J. Hößl, P. S. Barbeau, Lorenzo Fabris, I. J. Arnquist, R. Gornea, P. C. Rowson, V.N. Stekhanov, X. S. Jiang, C. Licciardi, A. Jamil, A. House, A. Piepke, J. Todd, G. Gallina, S. Thibado, Y. Y. Ding, A. Der Mesrobian-Kabakian, N. Massacret, M. Heffner, R. MacLellan, S. Viel, M. Worcester, Thilo Michel, V. Veeraraghavan, Qing Xia, M. Hughes, G. Li, Sergio Ferrara, S. Al Kharusi, R. DeVoe, A. Pocar, M. Walent, B. G. Lenardo, Arun Kumar Soma, S. Feyzbakhsh, Y. Lan, G. S. Ortega, B. T. Cleveland, K. Deslandes, T. Brunner, A. Kuchenkov, M. Medina-Peregrina, Serge A. Charlebois, F. Retiere, David Moore, M. Chiu, J. P. Brodsky, M. Tarka, F. Edaltafar, T. Wager, K. G. Leach, Wei Wu, R.J. Newby, Qun-Yao Wang, Zhijun Ning, M. Oriunno, Aleksey E. Bolotnikov, K. Murray, Gisela Anton, K. Odgers, B. Mong, M. J. Dolinski, David Leonard, Thomas Koffas, W. M. Fairbank, T. Tsang, T. Stiegler, Jean-Francois Pratte, Angelo Dragone, M. Elbeltagi, John L. Orrell, T. Daniels, Wei Wei, H. Rasiwala, I. Ostrovskiy, Yu-Guang Zhou, S. Rescia, D. Fairbank, Guofu Cao, Mike Richman, O. Njoya, T. I. Totev, A. Iverson, K. Skarpaas Viii, Shu Li, Giorgio Gratta, U. Wichoski, L. Yang, T. Rossignol, M. J. Jewell, A. Craycraft, T. Ziegler, Gabriele Giacomini, J. Echevers, Jens Dilling, C.R. Natzke, I. Badhrees, A. Tidball, M. L. di Vacri, C. Vivo-Vilches, S. Parent, A. Odian, O. Zeldovich, R. Saldanha, M. Wagenpfeil, J. Dalmasson, X.L. Sun, J. B. Zhao, X. F. Wu, A. Larson, Ethan Brown, A. Karelin, J. Farine, V. Belov, and A. Robinson
Subjects: Physics, Nuclear and High Energy Physics, Scintillation, Photon, Time projection chamber, Physics - Instrumentation and Detectors, Field (physics), 010308 nuclear & particles physics, chemistry.chemical_element, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, Xenon, chemistry, Double beta decay, Ionization, 0103 physical sciences, Atomic physics, 010306 general physics, Instrumentation, Event reconstruction
Abstract: nEXO is a proposed tonne-scale neutrinoless double beta decay ($0\nu\beta\beta$) experiment using liquid ${}^{136}Xe$ (LXe) in a Time Projection Chamber (TPC) to read out ionization and scintillation signals. Between the field cage and the LXe vessel, a layer of LXe ("skin" LXe) is present, where no ionization signal is collected. Only scintillation photons are detected, owing to the lack of optical barrier around the field cage. In this work, we show that the light originating in the skin LXe region can be used to improve background discrimination by 5% over previous published estimates. This improvement comes from two elements. First, a fraction of the $\gamma$-ray background is removed by identifying light from interactions with an energy deposition in the skin LXe. Second, background from ${}^{222}Rn$ dissolved in the skin LXe can be efficiently rejected by tagging the $\alpha$ decay in the ${}^{214}Bi-{}^{214}Po$ chain in the skin LXe., Comment: 11 pages, 12 figures
Published: 2020
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7. CFS-PML-DEC formulation in two-dimensional convex and non-convex domains

Author: Werley G. Facco, Elson J. Silva, Alex S. Moura, and Rodney R. Saldanha
Subjects: 010302 applied physics, Attenuation function, Mathematical analysis, Boundary curve, Regular polygon, 020206 networking & telecommunications, 02 engineering and technology, 01 natural sciences, Mathematics::Numerical Analysis, k-nearest neighbors algorithm, Computational Mathematics, Formalism (philosophy of mathematics), Perfectly matched layer, Discrete exterior calculus, Computational Theory and Mathematics, Modeling and Simulation, 0103 physical sciences, 0202 electrical engineering, electronic engineering, information engineering, Time domain, Mathematics
Abstract: In this paper, the time domain Maxwell’s equations are solved using the discrete exterior calculus (DEC) formalism in the two-dimensional space. To truncate the computational domain, the complex frequency-shifted perfectly matched layer (CFS-PML) concept is applied to create a reflectionless artificial layer. The paper presents a new numerical procedure to easily implement the CFS-PML with curved inner boundary. In order to numerically realize the PML, in a simplicial mesh, this paper proposes to utilize the nearest neighbor algorithm to associate point sets to boundary points. The distance from points to the boundary curve defines the attenuation function inside the PML. The performance of the approach is assessed by measuring the reflection error for three numerical experiments.
Published: 2018

8. Measurements of electron transport in liquid and gas Xenon using a laser-driven photocathode

Author: R. Saldanha, I. Ostrovskiy, D. Kodroff, M. J. Dolinski, S. Rescia, John L. Orrell, T. Daniels, P. Gautam, D. Fairbank, Z. Li, E. Caden, E. V. Hansen, Gerard Visser, J. Watkins, Mike Richman, O. Njoya, R. MacLellan, He-Run Yang, A. Iverson, Triveni Rao, K. Skarpaas Viii, Liang Yang, R. Tsang, Gabriele Giacomini, A. Jamil, Pengpeng Lv, O. Nusair, R. Krücken, Shu Li, J. Echevers, Yu-Guang Zhou, Sergio Ferrara, B. Chana, Y. Lan, M. L. di Vacri, U. Wichoski, T. Wager, J. P. Brodsky, C. Vivo-Vilches, I. J. Arnquist, D. Beck, Thilo Michel, Y-R Yen, T. Tsang, T. Tolba, J. Runge, Yuehe Lin, T. Ziegler, Qun-Yao Wang, P. Nakarmi, Guofu Cao, M. Hughes, Jens Dilling, R. Fontaine, David Leonard, M. Heffner, Angelo Dragone, J. L. Vuilleumier, M. Walent, S. Al Kharusi, I. Badhrees, M. Tarka, Thomas Koffas, W. M. Fairbank, B. G. Lenardo, S. Viel, Arun Kumar Soma, T. Brunner, D. Goeldi, L. J. Kaufman, T. Stiegler, Samuele Sangiorgio, Xuan Wu, K. S. Kumar, S. Parent, M. Elbeltagi, M. Coon, K. G. Leach, David Moore, Wei Wei, Qing Xia, J. Farine, G. S. Ortega, Cory T. Overman, Wei Wu, R.J. Newby, P. C. Rowson, S. X. Wu, S. J. Daugherty, Serge A. Charlebois, A. House, G. St-Hilaire, S. Feyzbakhsh, P. S. Barbeau, A. Robinson, T. Bhatta, V. A. Belov, A.C. Odian, O. Zeldovich, Eric W. Hoppe, A. Piepke, J. Todd, L. Darroch, Y. Y. Ding, M. Oriunno, C. Chambers, A. Pocar, V.N. Stekhanov, B. T. Cleveland, T. Rossignol, A. Kuchenkov, M. J. Jewell, Veljko Radeka, X. S. Jiang, C. Licciardi, G. Gallina, A. Der Mesrobian-Kabakian, V. Veeraraghavan, A. Fucarino, Giorgio Gratta, M. Chiu, K. Murray, Gisela Anton, K. Odgers, E. Raguzin, J. Hossl, R. DeVoe, W. R. Cen, M. Medina-Peregrina, R. Gornea, F. Retiere, B. Mong, M. Wagenpfeil, J. Dalmasson, M. Ward, G. S. Li, X.L. Sun, J. B. Zhao, A. Larson, A. Craycraft, Ethan Brown, C.R. Natzke, A. Karelin, Jean-Francois Pratte, Z. Ning, T. I. Totev, A. De St. Croix, Lorenzo Fabris, N. Roy, L. Cao, F. Nolet, T. McElroy, F. Vachon, L. J. Wen, and Marc Weber
Subjects: Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, chemistry.chemical_element, Electron, medicine.disease_cause, 7. Clean energy, 01 natural sciences, Photocathode, Xenon, Electric field, 0103 physical sciences, medicine, Nuclear Experiment (nucl-ex), 010306 general physics, Instrumentation, Nuclear Experiment, Physics, Argon, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), Photoelectric effect, chemistry, Quantum efficiency, High Energy Physics::Experiment, Atomic physics, Ultraviolet
Abstract: Measurements of electron drift properties in liquid and gaseous xenon are reported. The electrons are generated by the photoelectric effect in a semi-transparent gold photocathode driven in transmission mode with a pulsed ultraviolet laser. The charges drift and diffuse in a small chamber at various electric fields and a fixed drift distance of 2.0 cm. At an electric field of 0.5 kV/cm, the measured drift velocities and corresponding temperature coefficients respectively are 1 . 97 ± 0 . 04 m m ∕ μ s and ( − 0 . 69 ± 0 . 05 ) %/K for liquid xenon, and 1 . 42 ± 0 . 03 m m ∕ μ s and ( + 0 . 11 ± 0 . 01 ) %/K for gaseous xenon at 1.5 bar. In addition, we measure longitudinal diffusion coefficients of 25 . 7 ± 4 . 6 cm 2 /s and 149 ± 23 cm 2 /s, for liquid and gas, respectively. The quantum efficiency of the gold photocathode is studied at the photon energy of 4.73 eV in liquid and gaseous xenon, and vacuum. These charge transport properties and the behavior of photocathodes in a xenon environment are important in designing and calibrating future large scale noble liquid detectors.
Published: 2019

9. Cosmogenic production of Ar39 and Ar37 in argon

Author: R. Tsang, H. O. Back, Thomas Alexander, M. Zalavadia, Cory T. Overman, S. R. Elliott, Emily K. Mace, R. Saldanha, and S. Ferrara
Subjects: Physics, Argon, 010308 nuclear & particles physics, chemistry.chemical_element, 01 natural sciences, chemistry, Physics::Space Physics, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Production (computer science), Neutron, Atomic physics, 010306 general physics, Production rate
Abstract: We have experimentally determined the production rate of $^{39}\mathrm{Ar}$ and $^{37}\mathrm{Ar}$ from cosmic ray neutron interactions in argon at sea level. Understanding these production rates is important for argon-based dark matter experiments that plan to utilize argon extracted from deep underground because it is imperative to know what the ingrowth of $^{39}\mathrm{Ar}$ will be during the production, transport, and storage of the underground argon. These measurements also allow for the prediction of $^{39}\mathrm{Ar}$ and $^{37}\mathrm{Ar}$ concentrations in the atmosphere which can be used to determine the presence of other sources of these isotopes. Through controlled irradiation with a neutron beam that mimics the cosmic ray neutron spectrum, followed by direct counting of $^{39}\mathrm{Ar}$ and $^{37}\mathrm{Ar}$ decays with sensitive ultralow background proportional counters, we determined that the production rate from cosmic ray neutrons at sea level is expected to be $(759\ifmmode\pm\else\textpm\fi{}128)\phantom{\rule{0.16em}{0ex}}\mathrm{atoms}/({\mathrm{kg}}_{\mathrm{Ar}}\mathrm{day})$ for $^{39}\mathrm{Ar}$, and $(51.0\ifmmode\pm\else\textpm\fi{}7.4)\phantom{\rule{0.16em}{0ex}}\mathrm{atoms}/({\mathrm{kg}}_{\mathrm{Ar}}\mathrm{day})$ for $^{37}\mathrm{Ar}$. We also performed a survey of the alternate production mechanisms based on the state of knowledge of the associated cross sections to obtain a total sea-level cosmic ray production rate of $(1048\ifmmode\pm\else\textpm\fi{}133)\phantom{\rule{0.16em}{0ex}}\mathrm{atoms}/({\mathrm{kg}}_{\mathrm{Ar}}\mathrm{day})$ for $^{39}\mathrm{Ar}, (56.7\ifmmode\pm\else\textpm\fi{}7.5)\phantom{\rule{0.16em}{0ex}}\mathrm{atoms}/({\mathrm{kg}}_{\mathrm{Ar}}\mathrm{day})$ for $^{37}\mathrm{Ar}$ in underground argon, and $(92\ifmmode\pm\else\textpm\fi{}13)\phantom{\rule{0.16em}{0ex}}\mathrm{atoms}/({\mathrm{kg}}_{\mathrm{Ar}}\mathrm{day})$ for $^{37}\mathrm{Ar}$ in atmospheric argon.
Published: 2019

10. Characterization of the Hamamatsu VUV4 MPPCs for nEXO

Author: P. Giampa, G. Li, D. Kodroff, M. Wagenpfeil, J. Dalmasson, Eric W. Hoppe, N. Roy, David Leonard, J. Blatchford, Thomas Koffas, E. V. Hansen, W. M. Fairbank, P. Gautam, B. T. Cleveland, K. Odgers, L. Cao, Liang Yang, A. Jamil, S. Rescia, T. Stiegler, E. Raguzin, M. Elbeltagi, R. MacLellan, A. Kuchenkov, Arun Kumar Soma, F. Nolet, X.L. Sun, T. Bhatta, D. Fairbank, J. B. Zhao, T. McElroy, A. Larson, Jean-Francois Pratte, B. Mong, F. Vachon, Marc Weber, G. St-Hilaire, P. Margetak, P. Nakarmi, M. Chiu, J. Farine, J. Echevers, C. Chambers, G. Zhang, M. Oriunno, P. C. Rowson, A. Robinson, I. J. Arnquist, S. X. Wu, Douglas H Beck, Qing Xia, U. Wichoski, Ethan Brown, A. House, K. Murray, Y-R Yen, L. Darroch, G. S. Ortega, R. DeVoe, Gisela Anton, T. Ziegler, O. Zeldovich, J. P. Brodsky, T. I. Totev, M. Heffner, Qun-Yao Wang, T. Tolba, W. R. Cen, S. J. Daugherty, A. De St. Croix, G. Gallina, R. Gornea, Serge A. Charlebois, T. Rossignol, Zhijun Ning, M. Tarka, M. J. Jewell, Lorenzo Fabris, J. L. Vuilleumier, M. Walent, John L. Orrell, T. Daniels, R. Tsang, B. G. Lenardo, T. Brunner, K. Skarpaas, P. Lv, V. Veeraraghavan, A. Karelin, J. Todd, Y. Y. Ding, O. Nusair, R. Krücken, Veljko Radeka, Wei Wu, R.J. Newby, M. Hughes, R. Saldanha, S. Al Kharusi, Giorgio Gratta, Martin Ward, He-Run Yang, David Moore, M. Alfaris, S. Feyzbakhsh, A. Craycraft, Y. Ito, L. J. Kaufman, Y. Lan, Yuehe Lin, Z. Li, Samuele Sangiorgio, Wei Wei, F. Retière, K. S. Kumar, J. Hößl, P. S. Barbeau, V. A. Belov, Thilo Michel, J. Kroeger, Xuan Wu, A. Pocar, A. Piepke, V.N. Stekhanov, D. Qiu, M. Coon, Cory T. Overman, T. Tsang, Angelo Dragone, Gabriele Giacomini, Jens Dilling, I. Badhrees, S. Parent, A. Odian, I. Ostrovskiy, Gerard Visser, Mike Richman, O. Njoya, A. Iverson, Shu Li, J. Watkins, M. Medina-Peregrina, X. S. Jiang, C. Licciardi, A. Der Mesrobian-Kabakian, Yu-Guang Zhou, Liangjian Wen, Luca Doria, Guofu Cao, Rejean Fontaine, and M. J. Dolinski
Subjects: 010302 applied physics, Physics, Nuclear and High Energy Physics, Scintillation, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Analytical chemistry, FOS: Physical sciences, chemistry.chemical_element, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, Xenon, chemistry, 0103 physical sciences, Saturation (graph theory), Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Instrumentation, Photon detection, Dark current
Abstract: In this paper we report on the characterization of the Hamamatsu VUV4 (S/N: S13370-6152) Vacuum Ultra-Violet (VUV) sensitive Multi-Pixel Photon Counters (MPPC)s as part of the development of a solution for the detection of liquid xenon scintillation light for the nEXO experiment. Various MPPC features, such as: dark noise, gain, correlated avalanches, direct crosstalk and Photon Detection Efficiency (PDE) were measured in a dedicated setup at TRIUMF. MPPCs were characterized in the range 163 K ≤ T ≤ 233 K . At an over voltage of 3 . 1 ± 0 . 2 V and at T = 163 K we report a number of Correlated Avalanches (CAs) per pulse in the 1 μ s interval following the trigger pulse of 0 . 161 ± 0 . 005 . At the same settings the Dark-Noise (DN) rate is 0 . 137 ± 0 . 002 Hz/mm 2 . Both the number of CAs and the DN rate are within nEXO specifications. The PDE of the Hamamatsu VUV4 was measured for two different devices at T = 233 K for a mean wavelength of 189 ± 7 nm . At 3 . 6 ± 0 . 2 V and 3 . 5 ± 0 . 2 V of over voltage we report a PDE of 13 . 4 ± 2 . 6 % and 11 ± 2 % , corresponding to a saturation PDE of 14 . 8 ± 2 . 8 % and 12 . 2 ± 2 . 3 % , respectively. Both values are well below the 24 % saturation PDE advertised by Hamamatsu. More generally, the second device tested at 3 . 5 ± 0 . 2 V of over voltage is below the nEXO PDE requirement. The first one instead yields a PDE that is marginally close to meeting the nEXO specifications. This suggests that with modest improvements the Hamamatsu VUV4 MPPCs could be considered as an alternative to the FBK-LF Silicon Photo-Multipliers for the final design of the nEXO detector.
Published: 2019

11. Reflectance of Silicon Photomultipliers at Vacuum Ultraviolet Wavelengths

Author: E. Caden, S. Rescia, D. Fairbank, G. St-Hilaire, Thilo Michel, A. Craycraft, Jens Dilling, I. Badhrees, A. De St. Croix, X. S. Jiang, C. Licciardi, J. Farine, M. Walent, S. Feyzbakhsh, V. Belov, C.R. Natzke, B. G. Lenardo, A. Robinson, P. Nakarmi, A. Der Mesrobian-Kabakian, T. Brunner, L. Darroch, J. Echevers, Xuan Wu, S. Parent, A. Odian, A. Fucarino, Jean-Francois Pratte, Yu-Guang Zhou, E. Raguzin, T. Rossignol, Z. Li, O. Nusair, J. L. Vuilleumier, R. Krücken, M. Hughes, V. Veeraraghavan, M. J. Jewell, R. Saldanha, T. I. Totev, P. A. Breur, K. Skarpaas, Gerard Visser, S. Al Kharusi, I. Ostrovskiy, B. T. Cleveland, A. Kuchenkov, Liangjian Wen, Luca Doria, Guofu Cao, Samuele Sangiorgio, Wei Wei, K. S. Kumar, Mike Richman, David Moore, O. Njoya, A. Iverson, T. Bhatta, M. Chiu, G. S. Li, Thomas Tsang, Shu Li, Y. Lan, B. Chana, Douglas H Beck, L. Yang, M. Oriunno, J. P. Brodsky, P. S. Barbeau, He-Run Yang, R. DeVoe, K. Murray, J. Watkins, M. Tarka, Gisela Anton, R. Tsang, M. L. di Vacri, K. Odgers, M. J. Dolinski, M. Medina-Peregrina, C. Vivo-Vilches, F. Retiere, U. Wichoski, Sergio Ferrara, O. Zeldovich, K. G. Leach, T. Ziegler, R. Gornea, K. Deslandes, David Leonard, Giorgio Gratta, Thomas Koffas, W. M. Fairbank, Wei Wu, R.J. Newby, P. C. Rowson, T. Stiegler, M. Elbeltagi, Lorenzo Fabris, J. Hobl, A. House, N. Roy, L. Cao, F. Nolet, N. Massacret, T. McElroy, S. X. Wu, F. Vachon, C. Chambers, R. MacLellan, A. Pocar, V.N. Stekhanov, P. Gautam, F. Edaltafar, D. Goeldi, M. Coon, I. J. Arnquist, J. Runge, Cory T. Overman, M. Heffner, S. Viel, G. Gallina, Angelo Dragone, Gabriele Giacomini, P. Lv, A. Piepke, J. Todd, Y. Y. Ding, Veljko Radeka, T. Wager, Qun-Yao Wang, Zhijun Ning, E. V. Hansen, A. Jamil, Arun Kumar Soma, Qing Xia, S. Byrne Mamahit, Ethan Brown, A. Karelin, G. S. Ortega, M. Wagenpfeil, J. Dalmasson, X.L. Sun, J. B. Zhao, A. Larson, Serge A. Charlebois, John L. Orrell, T. Daniels, B. Mong, L. J. Kaufman, and Eric W. Hoppe
Subjects: Nuclear and High Energy Physics, Materials science, Physics - Instrumentation and Detectors, Silicon, chemistry.chemical_element, Photodetector, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Xenon, Silicon photomultiplier, 0103 physical sciences, Wafer, Electrical and Electronic Engineering, 010308 nuclear & particles physics, business.industry, Instrumentation and Detectors (physics.ins-det), Nuclear Energy and Engineering, chemistry, Optoelectronics, Diffuse reflection, Photonics, business, Refractive index
Abstract: Characterization of the vacuum ultraviolet (VUV) reflectance of silicon photomultipliers (SiPMs) is important for large-scale SiPM-based photodetector systems. We report the angular dependence of the specular reflectance in a vacuum of SiPMs manufactured by Fondazionc Bruno Kessler (FBK) and Hamamatsu Photonics K.K. (HPK) over wavelengths ranging from 120 nm to 280 nm. Refractive index and extinction coefficient of the thin silicon-dioxide film deposited on the surface of the FBK SiPMs are derived from reflectance data of a FBK silicon wafer with the same deposited oxide film as SiPMs. The diffuse reflectance of SiPMs is also measured at 193 nm. We use the VUV spectral dependence of the optical constants to predict the reflectance of the FBK silicon wafer and FBK SiPMs in liquid xenon.
Published: 2019
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12. Simulation of charge readout with segmented tiles in nEXO

Author: F. Retière, M. Medina-Peregrina, Venkatesh Veeraraghavan, J. Hößl, Gerard Visser, J. L. Vuilleumier, L. Darroch, M. Chiu, J. Watkins, V. A. Belov, Yang Haibo, A. De St. Croix, V. Radeka, D. Fairbank, T. McElroy, T. Bhatta, A. Pocar, D. S. Leonard, J. Echevers, E. Caden, A. Craycraft, R. DeVoe, Lorenzo Fabris, C. T. Overman, E. Raguzin, C. Vivo-Vilches, Qing Xia, M. J. Jewell, Xiaoyang Sun, R. Gornea, J. Dalmasson, S. Feyzbakhsh, P. Gautam, G. S. Ortega, A. Piepke, I. Ostrovskiy, P. Lv, M. Hughes, Thilo Michel, T. Ziegler, C.R. Natzke, Z. Ning, Xuan Wu, F. Vachon, Sergio Ferrara, Serge A. Charlebois, S. X. Wu, V.N. Stekhanov, M. Walent, S. Al Kharusi, J. B. Zhao, A. Larson, A. Der Mesrobian-Kabakian, A. E. Robinson, Mike Richman, B. G. Lenardo, T. Brunner, A. Fucarino, David Moore, N. Roy, L. Cao, F. Nolet, J. Todd, M. Heffner, D. Kodroff, T. Tolba, Jean-Francois Pratte, M. Oriunno, John L. Orrell, T. Daniels, B. Mong, Rejean Fontaine, Ethan Brown, Qian Wang, Y. Lan, K. Murray, G. Giacomini, T. Stiegler, O. Njoya, A. Iverson, K. Skarpaas Viii, Thomas Tsang, R. Saldanha, Shu Li, Y. Y. Ding, Z. Li, Gisela Anton, O. Zeldovich, Marc Weber, E. Hansen, A. Karelin, O. Nusair, R. Krücken, Jens Dilling, R. MacLellan, B. Chana, Giorgio Gratta, P. S. Barbeau, Yumei Zhou, I. Badhrees, R. Tsang, Martin Ward, T. I. Totev, D. Goeldi, M. Coon, Liangjian Wen, Douglas H Beck, Guofu Cao, Angelo Dragone, W. R. Cen, S. J. Daugherty, Thomas Koffas, Xiaoshan Jiang, W. M. Fairbank, M. Elbeltagi, Y-R Yen, S. Rescia, M. J. Dolinski, A. Odian, S. Parent, J. Runge, J. P. Brodsky, P. Nakarmi, U. Wichoski, S. Viel, C. Licciardi, G. Gallina, T. Rossignol, M. L. Di Vacri, L. J. Kaufman, Eric W. Hoppe, Liang Yang, A. Jamil, Arun Kumar Soma, Yuehe Lin, Samuele Sangiorgio, Wei Wei, K. S. Kumar, J. Farine, I. J. Arnquist, K. G. Leach, G. St-Hilaire, Wei Wu, R.J. Newby, P. C. Rowson, A. House, M. Tarka, G. Li, B. T. Cleveland, K. Odgers, A. Kuchenkov, M. Wagenpfeil, and C. Chambers
Subjects: Physics, Physics - Instrumentation and Detectors, Time projection chamber, 010308 nuclear & particles physics, Detector, chemistry.chemical_element, FOS: Physical sciences, Charge (physics), Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 030218 nuclear medicine & medical imaging, Anode, Nuclear physics, 03 medical and health sciences, 0302 clinical medicine, Xenon, chemistry, Double beta decay, 0103 physical sciences, Beta (velocity), Sensitivity (control systems), Nuclear Experiment (nucl-ex), Nuclear Experiment, Instrumentation, Mathematical Physics
Abstract: nEXO is a proposed experiment to search for the neutrino-less double beta decay ($0\nu\beta\beta$) of $^{136}$Xe in a tonne-scale liquid xenon time projection chamber (TPC). The nEXO TPC will be equipped with charge collection tiles to form the anode. In this work, the charge reconstruction performance of this anode design is studied with a dedicated simulation package. A multi-variate method and a deep neural network are developed to distinguish simulated $0\nu\beta\beta$ signals from backgrounds arising from trace levels of natural radioactivity in the detector materials. These simulations indicate that the nEXO TPC with charge-collection tiles shows promising capability to discriminate the $0\nu\beta\beta$ signal from backgrounds. The estimated half-life sensitivity for $0\nu\beta\beta$ decay is improved by $\sim$20$~(32)\%$ with the multi-variate~(deep neural network) methods considered here, relative to the sensitivity estimated in the nEXO pre-conceptual design report.
Published: 2019
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13. Reflectivity and PDE of VUV4 Hamamatsu SiPMs in Liquid Xenon

Author: Gerard Visser, M. Walent, B. G. Lenardo, T. Brunner, V. Veeraraghavan, T. Bhatta, Giorgio Gratta, F. Edaltafar, T. Rossignol, M. J. Jewell, J. Watkins, P. Nakarmi, Arun Kumar Soma, Ethan Brown, L. Darroch, O. Nusair, R. Krücken, S. X. Wu, David Leonard, J. Blatchford, E. Caden, Thomas Koffas, W. M. Fairbank, T. Stiegler, M. Elbeltagi, L. J. Kaufman, M. Hughes, X. S. Jiang, C. Licciardi, A. Craycraft, Eric W. Hoppe, S. Al Kharusi, A. Karelin, G. Gallina, P. Gautam, R. Saldanha, M. Chiu, J. L. Vuilleumier, T. Wager, A. Der Mesrobian-Kabakian, David Moore, C. Chambers, M. Oriunno, E. V. Hansen, M. Alfaris, M. Wagenpfeil, J. Dalmasson, Sergio Ferrara, R. MacLellan, Qun-Yao Wang, K. Murray, Gabriele Giacomini, I. J. Arnquist, Liang Yang, Y. Lan, U. Wichoski, C.R. Natzke, S. Feyzbakhsh, A. Jamil, Gisela Anton, J. Runge, Zhijun Ning, T. Ziegler, K. G. Leach, R. Tsang, X.L. Sun, J. B. Zhao, M. Heffner, K. Odgers, S. Viel, Wei Wu, R.J. Newby, A. Fucarino, A. Larson, Z. Li, B. Chana, Douglas H Beck, Samuele Sangiorgio, K. S. Kumar, Veljko Radeka, P. C. Rowson, A. House, N. Massacret, Jean-Francois Pratte, P. Lv, J. Todd, Angelo Dragone, B. Mong, Y. Y. Ding, M. Ward, T. I. Totev, G. S. Li, M. L. di Vacri, R. DeVoe, C. Vivo-Vilches, Qing Xia, S. Byrne Mamahit, G. S. Ortega, R. Fontaine, J. Farine, Serge A. Charlebois, John L. Orrell, T. Daniels, V. Belov, A. Robinson, N. Roy, L. Cao, F. Nolet, T. McElroy, F. Vachon, Marc Weber, A. De St. Croix, Lorenzo Fabris, B. T. Cleveland, D. Goeldi, M. Coon, A. Kuchenkov, Cory T. Overman, S. Rescia, D. Fairbank, G. St-Hilaire, J. P. Brodsky, He-Run Yang, A. Piepke, M. Tarka, V.N. Stekhanov, J. Echevers, A. Pocar, O. Zeldovich, Yu-Guang Zhou, Liangjian Wen, Luca Doria, Guofu Cao, Thilo Michel, Wei Wei, I. Ostrovskiy, M. J. Dolinski, E. Raguzin, P. A. Breur, Xuan Wu, Mike Richman, F. Retière, O. Njoya, A. Iverson, M. Medina-Peregrina, J. Hößl, K. Skarpaas Viii, P. S. Barbeau, Thomas Tsang, Shu Li, R. Gornea, Jens Dilling, I. Badhrees, S. Parent, and A. Odian
Subjects: Materials science, Physics - Instrumentation and Detectors, APDS, Physics::Instrumentation and Detectors, Photodetector, chemistry.chemical_element, FOS: Physical sciences, Photodetection, 01 natural sciences, 030218 nuclear medicine & medical imaging, law.invention, High Energy Physics - Experiment, 03 medical and health sciences, High Energy Physics - Experiment (hep-ex), 0302 clinical medicine, Silicon photomultiplier, Optics, Xenon, law, 0103 physical sciences, Specular reflection, Instrumentation, Mathematical Physics, Scintillation, 010308 nuclear & particles physics, business.industry, Instrumentation and Detectors (physics.ins-det), Wavelength, chemistry, business
Abstract: Understanding reflective properties of materials and photodetection efficiency (PDE) of photodetectors is important for optimizing energy resolution and sensitivity of the next generation neutrinoless double beta decay, direct detection dark matter, and neutrino oscillation experiments that will use noble liquid gases, such as nEXO, DARWIN, DarkSide-20k, and DUNE. Little information is currently available about reflectivity and PDE in liquid noble gases, because such measurements are difficult to conduct in a cryogenic environment and at short enough wavelengths. Here we report a measurement of specular reflectivity and relative PDE of Hamamatsu VUV4 silicon photomultipliers (SiPMs) with 50 micrometer micro-cells conducted with xenon scintillation light (~175 nm) in liquid xenon. The specular reflectivity at 15 deg. incidence of three samples of VUV4 SiPMs is found to be 30.4+/-1.4%, 28.6+/-1.3%, and 28.0+/-1.3%, respectively. The PDE at normal incidence differs by +/-8% (standard deviation) among the three devices. The angular dependence of the reflectivity and PDE was also measured for one of the SiPMs. Both the reflectivity and PDE decrease as the angle of incidence increases. This is the first measurement of an angular dependence of PDE and reflectivity of a SiPM in liquid xenon., Comment: 21 pages, 15 figures, 6 tables. As accepted by JINST
Published: 2019
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14. The surge impedance loading optimization by an adaptive Deep Cut Ellipsoidal algorithm

Author: Marcio Matias Afonso, Marco Aurélio O. Schroeder, Rodney R. Saldanha, André Luiz Paganotti, Eduardo Nunes Gonçalves, Rafael Alipio, and Tarcísio Antônio Santos de Oliveira
Subjects: 010302 applied physics, Engineering, business.industry, 020209 energy, Mechanical Engineering, Acoustics, Phase (waves), 02 engineering and technology, Condensed Matter Physics, 01 natural sciences, Characteristic impedance, Electronic, Optical and Magnetic Materials, Electric power transmission, Transmission (telecommunications), Mechanics of Materials, Transmission line, Electric field, 0103 physical sciences, 0202 electrical engineering, electronic engineering, information engineering, Electronic engineering, Electrical and Electronic Engineering, business, Electrical conductor, Energy (signal processing)
Abstract: This paper presents a computational tool intended to achieves optimal configurations of conductors with capacity of transmission of energy improved. This arrangement is obtained by calculate and minimize of electric fields at ground level of High Surge Impedance Loading transmission lines. This type of transmission line has higher power transmission rates by utilizing optimized configuration for the conductors. In the present work, an enhanced Deep Cut Ellipsoidal Method is applied to find a new optimized configuration for the phase conductors. The Surge Impedance Loading of the suggested configuration is analyzed. The new proposed configuration results in reduced profiles of electric fields and higher power transmission capacity.
Published: 2016

15. Recent results from Borexino and the first real time measure of solar pp neutrinos

Author: D. Bravo, N. Rossi, G. Bellini, D. Vignaud, R. Saldanha, E. V. Hungerford, Lino Miramonti, Matthias Laubenstein, M. Göger-Neff, F. von Feilitzsch, R. B. Vogelaar, Marco Giammarchi, Marcin Wójcik, Andrea Ianni, D. Bick, Sandra Zavatarelli, Kai Zuber, M. D. Skorokhvatov, Michael Wurm, P. J. Mosteiro, Laura Cadonati, L. Papp, Michele Montuschi, A. Sotnikov, E. Meroni, C. Salvo, M. Gromov, T. Lewke, A. Caminata, Fausto Ortica, D. Kryn, F. Gabriele, Manuel Meyer, O. Smirnov, G. Lukyanchenko, I. N. Machulin, Aldo Ianni, Aldo Romani, Paolo Lombardi, K. Otis, Marco Pallavicini, K. Fomenko, E. Litvinovich, M. Obolensky, Q. Meindl, A. E. Chavarria, L. Perasso, D. D'Angelo, J. Winter, S. Marcocci, C. Galbiati, D. Franco, F. Lombardi, S. Manecki, A. Razeto, Lothar Oberauer, S. Gazzana, S. Davini, B. Lehnert, R. Tartaglia, A. Pocar, A. V. Derbin, Anton Empl, G. Bonfini, G. Zuzel, Frank Calaprice, Jay Burton Benziger, W. Maneschg, Alessandra Re, Hardy Simgen, Hongwei Wang, S. V. Sukhotin, A. Wright, O. Zaimidoroga, V. V. Kobychev, S. Schönert, G. Korga, Gioacchino Ranucci, B. Caccianiga, G. Testera, Denis Korablev, V. N. Muratova, Y. Suvorov, Livia Ludhova, A. M. Goretti, A. S. Chepurnov, C. Ghiano, Caren Hagner, P. Cavalcante, M. Misiaszek, A.V. Etenko, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Zavatarelli, S., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Cadonati, L., Calaprice, F., Caminata, A., Cavalcante, P., Chavarria, A., Chepurnov, A., D'Angelo, D., Davini, S., Derbin, A., Empl, A., Etenko, A., Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Hungerford, E., Ianni, Aldo, Ianni, Andrea, Kobychev, V., Korablev, D., Korga, G., Kryn, D., Laubenstein, M., Lehnert, B., Lewke, T., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Meindl, Q., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Saldanha, R., Salvo, C., Schoenert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wright, A., Wurm, M., Zaimidoroga, O., Zuber, K., Zuzel, G., Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: geo-neutrinos, Nuclear and High Energy Physics, Particle physics, Neutrino oscillation, neutrino: solar, Physics::Instrumentation and Detectors, Geo-neutrinos, Neutrino oscillations, Solar neutrinos, Solar neutrino, talk: Valencia 2014/07/02, 01 natural sciences, 7. Clean energy, Physics::Geophysics, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], ddc:530, 010306 general physics, Borexino, Physics, neutrino oscillations, 010308 nuclear & particles physics, Solar neutrino problem, Gran Sasso, Neutrino detector, Geo-neutrino, solar neutrinos, Measurements of neutrino speed, High Energy Physics::Experiment, neutrino: oscillation, neutrino: geophysics, Neutrino astronomy, Neutrino, experimental results
Abstract: International audience; The Borexino detector was built starting from 1996 in the underground hall C of Gran Sasso National Laboratory (LNGS) in Italy under about 1400 m of rock (3800 m.w.e) and it is mostly aimed to the study in real-time of the low-energy solar neutrinos.Since the beginning of data taking, in May 2007, the unprecedented detector radio-purity made the performances of the detector unique: a milestone has been very recently achieved with the measurement of solar pp neutrino flux, providing the first direct observation in real time of the key fusion reaction powering the Sun.In this contribution the most important Borexino achievements to the fields of solar, geo-neutrino and particle physics are reviewed and the future perspectives discussed, emphasizing in particular the unique possibility of Borexino to cover at the end of its program the entire solar neutrino spectrum and to exploit the possible existence of a fourth sterile neutrino (SOX project).
Published: 2016

16. Analysis of the Out-of-Plane Coordinate Transformation to Obtain Anisotropic Layered Cloaks

Author: Fabio J. F. Goncalves, Rodney R. Saldanha, Elson J. Silva, and Renato C. Mesquita
Subjects: 010302 applied physics, Physics, Electromagnetics, Magnetoresistance, Scattering, Coordinate system, Cloak, Physics::Optics, 01 natural sciences, Finite element method, Electronic, Optical and Magnetic Materials, Transformation (function), Classical mechanics, 0103 physical sciences, Electrical and Electronic Engineering, 010306 general physics, Anisotropy
Abstract: A possible strategy for avoiding singular material parameters in a transformation-based invisibility cloak involves an out-of-plane stretching, calculated to compensate the in-plane singular transformation. In this paper, we used numerical simulations to analyze the relation among the out-of-plane transformation, the resulting material anisotropy, and the total scattering cross width. Moreover, we show how this information can be used to optimize a cloak with homogeneous anisotropic layers.
Published: 2016

17. VUV-sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO

Author: A. Jamil, T. Ziegler, P. Hufschmidt, G. Li, L. Lupin-Jimenez, T. Michel, I. Ostrovskiy, F. Retiere, J. Schneider, M. Wagenpfeil, A. Alamre, J. B. Albert, G. Anton, I. J. Arnquist, I. Badhrees, P. S. Barbeau, D. Beck, V. Belov, T. Bhatta, F. Bourque, J. P. Brodsky, E. Brown, T. Brunner, A. Burenkov, G. F. Cao, L. Cao, W. R. Cen, C. Chambers, S. A. Charlebois, M. Chiu, B. Cleveland, M. Coon, M. Cote, A. Craycraft, W. Cree, J. Dalmasson, T. Daniels, L. Darroch, S. J. Daugherty, J. Daughhetee, S. Delaquis, A. Der Mesrobian-Kabakian, R. DeVoe, J. Dilling, Y. Y. Ding, M. J. Dolinski, A. Dragone, J. Echevers, L. Fabris, D. Fairbank, W. Fairbank, J. Farine, S. Feyzbakhsh, R. Fontaine, D. Fudenberg, G. Gallina, G. Giacomini, R. Gornea, G. Gratta, E. V. Hansen, D. Harris, M. Hasan, M. Heffner, J. HoBl, E. W. Hoppe, A. House, M. Hughes, Y. Ito, A. Iverson, C. Jessiman, M. J. Jewell, X. S. Jiang, A. Karelin, L. J. Kaufman, T. Koffas, S. Kravitz, R. Krucken, A. Kuchenkov, K. S. Kumar, Y. Lan, A. Larson, D. S. Leonard, S. Li, Z. Li, C. Licciardi, Y. H. Lin, P. Lv, R. MacLellan, B. Mong, D. C. Moore, K. Murray, R. J. Newby, Z. Ning, O. Njoya, F. Nolet, O. Nusair, K. Odgers, A. Odian, M. Oriunno, J. L. Orrell, G. S. Ortega, C. T. Overman, S. Parent, A. Piepke, A. Pocar, J.-F. Pratte, D. Qiu, V. Radeka, E. Raguzin, T. Rao, S. Rescia, A. Robinson, T. Rossignol, P. C. Rowson, N. Roy, R. Saldanha, S. Sangiorgio, S. Schmidt, A. Schubert, D. Sinclair, K. Skarpaas, A. K. Soma, G. St-Hilaire, V. Stekhanov, T. Stiegler, X. L. Sun, M. Tarka, J. Todd, T. Tolba, T. I. Totev, R. Tsang, T. Tsang, F. Vachon, B. Veenstra, V. Veeraraghavan, G. Visser, J.-L. Vuilleumier, Q. Wang, J. Watkins, M. Weber, W. Wei, L. J. Wen, U. Wichoski, G. Wrede, S. X. Wu, W. H. Wu, Q. Xia, L. Yang, Y.-R. Yen, O. Zeldovich, X. Zhang, J. Zhao, and Y. Zhou
Subjects: Physics, Nuclear and High Energy Physics, Photomultiplier, Scintillation, Time projection chamber, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, Noble gas, chemistry.chemical_element, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Avalanche photodiode, 01 natural sciences, Optics, Silicon photomultiplier, Xenon, Nuclear Energy and Engineering, chemistry, Double beta decay, 0103 physical sciences, Electrical and Electronic Engineering, 010306 general physics, business
Abstract: Future tonne-scale liquefied noble gas detectors depend on efficient light detection in the VUV range. In the past years Silicon Photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large area avalanche photodiodes. The next generation double beta decay experiment, nEXO, with a 5 tonne liquid xenon time projection chamber, will use SiPMs for detecting the $178\,\text{nm}$ xenon scintillation light, in order to achieve an energy resolution of $\sigma / Q_{\beta\beta} = 1\, \%$. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler in two complementary setups. It includes measurements of the photon detection efficiency with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved photon detection efficiency at $175\,\text{nm}$ compared to previous generation devices, that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs., Comment: 11 pages, 13 figures, 2 tables
Published: 2018
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18. The XENON1T Dark Matter Experiment

Author: E. Aprile, J. Aalbers, F. Agostini, M. Alfonsi, F. D. Amaro, M. Anthony, B. Antunes, F. Arneodo, M. Balata, P. Barrow, L. Baudis, B. Bauermeister, M. L. Benabderrahmane, T. Berger, A. Breskin, P. A. Breur, A. Brown, E. Brown, S. Bruenner, G. Bruno, R. Budnik, L. Bütikofer, J. Calvén, J. M. R. Cardoso, M. Cervantes, A. Chiarini, D. Cichon, D. Coderre, A. P. Colijn, J. Conrad, R. Corrieri, J. P. Cussonneau, M. P. Decowski, P. de Perio, P. Di Gangi, A. Di Giovanni, S. Diglio, J.-M. Disdier, M. Doets, E. Duchovni, G. Eurin, J. Fei, A. D. Ferella, A. Fieguth, D. Franco, D. Front, W. Fulgione, A. Gallo Rosso, M. Galloway, F. Gao, M. Garbini, C. Geis, K.-L. Giboni, L. W. Goetzke, L. Grandi, Z. Greene, C. Grignon, C. Hasterok, E. Hogenbirk, C. Huhmann, R. Itay, A. James, B. Kaminsky, S. Kazama, G. Kessler, A. Kish, H. Landsman, R. F. Lang, D. Lellouch, L. Levinson, Q. Lin, S. Lindemann, M. Lindner, F. Lombardi, J. A. M. Lopes, R. Maier, A. Manfredini, I. Maris, T. Marrodán Undagoitia, J. Masbou, F. V. Massoli, D. Masson, D. Mayani, M. Messina, K. Micheneau, A. Molinario, K. Morå, M. Murra, J. Naganoma, K. Ni, U. Oberlack, D. Orlandi, R. Othegraven, P. Pakarha, S. Parlati, B. Pelssers, R. Persiani, F. Piastra, J. Pienaar, V. Pizzella, M.-C. Piro, G. Plante, N. Priel, D. Ramírez García, L. Rauch, S. Reichard, C. Reuter, A. Rizzo, S. Rosendahl, N. Rupp, J. M. F. dos Santos, R. Saldanha, G. Sartorelli, M. Scheibelhut, S. Schindler, J. Schreiner, M. Schumann, L. Scotto Lavina, M. Selvi, P. Shagin, E. Shockley, M. Silva, H. Simgen, M. v. Sivers, M. Stern, A. Stein, D. Tatananni, L. Tatananni, D. Thers, A. Tiseni, G. Trinchero, C. Tunnell, N. Upole, M. Vargas, O. Wack, R. Walet, H. Wang, Z. Wang, Y. Wei, C. Weinheimer, C. Wittweg, J. Wulf, J. Ye, Y. Zhang, XENON Collaboration, XENON (IHEF, IoP, FNWI), Laboratoire de physique subatomique et des technologies associées ( SUBATECH ), IMT Atlantique Bretagne-Pays de la Loire ( IMT Atlantique ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ) -Université de Nantes ( UN ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), XENON, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Aprile, E., Aalbers, J., Agostini, F., Alfonsi, M., Amaro, F.D., Anthony, M., Antunes, B., Arneodo, F., Balata, M., Barrow, P., Baudis, L., Bauermeister, B., Benabderrahmane, M.L., Berger, T., Breskin, A., Breur, P.A., Brown, A., Brown, E., Bruenner, S., Bruno, G., Budnik, R., Bütikofer, L., Calvén, J., Cardoso, J.M.R., Cervantes, M., Chiarini, A., Cichon, D., Coderre, D., Colijn, A.P., Conrad, J., Corrieri, R., Cussonneau, J.P., Decowski, M.P., de Perio, P., Gangi, P. Di, Giovanni, A. Di, Diglio, S., Disdier, J.-M., Doets, M., Duchovni, E., Eurin, G., Fei, J., Ferella, A.D., Fieguth, A., Franco, D., Front, D., Fulgione, W., Rosso, A. Gallo, Galloway, M., Gao, F., Garbini, M., Geis, C., Giboni, K.-L., Goetzke, L.W., Grandi, L., Greene, Z., Grignon, C., Hasterok, C., Hogenbirk, E., Huhmann, C., Itay, R., James, A., Kaminsky, B., Kazama, S., Kessler, G., Kish, A., Landsman, H., Lang, R.F., Lellouch, D., Levinson, L., Lin, Q., Lindemann, S., Lindner, M., Lombardi, F., Lopes, J.A.M., Maier, R., Manfredini, A., Maris, I., Undagoitia, T. Marrodán, Masbou, J., Massoli, F.V., Masson, D., Mayani, D., Messina, M., Micheneau, K., Molinario, A., Morå, K., Murra, M., Naganoma, J., Ni, K., Oberlack, U., Orlandi, D., Othegraven, R., Pakarha, P., Parlati, S., Pelssers, B., Persiani, R., Piastra, F., Pienaar, J., Pizzella, V., Piro, M.-C., Plante, G., Priel, N., García, D. Ramírez, Rauch, L., Reichard, S., Reuter, C., Rizzo, A., Rosendahl, S., Rupp, N., Santos, J.M.Fdos., Saldanha, R., Sartorelli, G., Scheibelhut, M., Schindler, S., Schreiner, J., Schumann, M., Lavina, L. Scotto, Selvi, M., Shagin, P., Shockley, E., Silva, M., Simgen, H., Sivers, Mv., Stern, M., Stein, A., Tatananni, D., Tatananni, L., Thers, D., Tiseni, A., Trinchero, G., Tunnell, C., Upole, N., Vargas, M., Wack, O., Walet, R., Wang, H., Wang, Z., Wei, Y., Weinheimer, C., Wittweg, C., Wulf, J., Ye, J., and Zhang, Y.
Subjects: xenon: target, Photomultiplier, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), WIMP, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Dark matter, chemistry.chemical_element, FOS: Physical sciences, lcsh:Astrophysics, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), XENON, Xenon, background: low, [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], Ionization, 0103 physical sciences, lcsh:QB460-466, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Dark Matter, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Engineering (miscellaneous), Instrumentation and Methods for Astrophysics (astro-ph.IM), [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Astrophysique, Physics, Scintillation, xenon: liquid, Time projection chamber, photomultiplier, 010308 nuclear & particles physics, Detector, Instrumentation and Detectors (physics.ins-det), dark matter: detector, time projection chamber, chemistry, lcsh:QC770-798, TPC, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], performance, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2 t liquid xenon inventory, 2.0 t constitute the active target of the dual-phase time projection chamber. The scintillation and ionization signals from particle interactions are detected with low-background photomultipliers. This article describes the XENON1T instrument and its subsystems as well as strategies to achieve an unprecedented low background level. First results on the detector response and the performance of the subsystems are also presented. © 2017, The Author(s)., info:eu-repo/semantics/published
Published: 2017

19. First results from the DarkSide-50 dark matter experiment at Laboratori Nazionali del Gran Sasso

Author: S. Kidner, R. Tartaglia, A. L. Renshaw, E. V. Hungerford, Yanchu Wang, P. Cavalcante, A. Candela, C. Zhu, M. Cariello, S. Westerdale, A. Sotnikov, Samuele Sangiorgio, E. Shields, N. Rossi, F. Gabriele, E. Pantic, L. Crippa, D. Sablone, An. Ianni, V. N. Muratova, G. Testera, M. D. Skorokhvatov, L. Grandi, G. Forster, A. Devoto, A. E. Chavarria, K. Pelczar, K. Fomenko, Cristiano Galbiati, M. Wada, C. Love, G. Di Pietro, Min-Xin Guan, R. B. Vogelaar, Laura Cadonati, L. Papp, Y. Guardincerri, Gioacchino Ranucci, E. Edkins, P. Musico, K. Herner, M. E. Monzani, S. D. Rountree, P. J. Mosteiro, B. Baldin, Hui Wang, R. Parsells, G. Bonfini, A. Pocar, Thomas Alexander, Y. Q. Ma, Fausto Ortica, B. Rossi, K. Randle, P. Saggese, L. Marini, M. Bossa, N. Canci, Paolo Lombardi, B. R. Hackett, A. Empl, R. Saldanha, K. Arisaka, Henning O. Back, Stuart Derek Walker, M. Montuschi, M. Orsini, E. Meroni, Jilei Xu, A. Zec, O. Smirnov, D. Franco, G. Fiorillo, A. Monte, M. Okounkova, G. Zuzel, Alan Watson, J. Yoo, C. L. Kendziora, F. Di Eusanio, A. Razeto, L. Pagani, M. D'Incecco, J. Tatarowicz, D. Korablev, M. De Deo, A. V. Derbin, Nicomede Pelliccia, I. N. Machulin, B. Reinhold, Anselmo Meregaglia, H. Qian, S. Davini, E. Segreto, A. Wright, C. J. Martoff, A. Mandarano, Marcin Wójcik, S. Luitz, Marco Pallavicini, D. D'Angelo, K. J. Keeter, Frank Calaprice, F. Budano, X. Xiang, Sandra Zavatarelli, P. X. Li, V. V. Kobychev, W. Sands, Aldo Romani, B. Loer, M. Gromov, A. Tonazzo, S. Pordes, P. Agnes, Al. Ianni, G. Koh, J. Maricic, A. Nelson, G. Korga, Stefano Maria Mari, R. Milincic, Cécile Jollet, D. A. Semenov, A. Kurlej, S. Parmeggiano, K. Biery, A. Fan, D. A. Pugachev, S. Perasso, A. G. Cocco, A. K. Alton, B. J. Mount, Chung-Yao Yang, Augusto Brigatti, D. Montanari, E. V. Unzhakov, J. Brodsky, H. Cao, S. Odrowski, Peter Daniel Meyers, Y. Suvorov, Livia Ludhova, A. M. Goretti, A. S. Chepurnov, C. Stanford, Agnes, P, Alexander, T., Alton, A., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Cadonati, L., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Cavalcante, P., Chavarria, A., Chepurnov, A., Cocco, A. G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., De Deo, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Gromov, M., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., Jollet, C., Keeter, K., Kendziora, C., Kidner, S., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Loer, B., Lombardi, P., Love, C., Ludhova, L., Luitz, S., Ma, Y. Q., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meroni, E., Meyers, P. D., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B., Muratova, V., Musico, P., Nelson, A., Odrowski, S., Okounkova, M., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Papp, L., Parmeggiano, S., Parsells, R., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Segreto, E., Semenov, D., Shields, E., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, Susan Elizabeth, Wang, H., Wang, Y., Watson, A., Westerdale, S., Wojcik, M., Wright, A., Xiang, X., Xu, J., Yang, C. G., Yoo, J., Zavatarelli, S., Zec, A., Zhu, C., Zuzel, G., P. Agnes, Mari, Stefano Maria, and The Darkside, Collaboration
Subjects: Nuclear and High Energy Physics, Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Liquid scintillator, Physics - Instrumentation and Detectors, WIMP, Physics::Instrumentation and Detectors, low-background detectors, Dark matter, Noble liquid detectors, FOS: Physical sciences, liquid scintillators, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, WIMP Argon Programme, 01 natural sciences, dark matter, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Low-background detectors, 0103 physical sciences, Nuclear Experiment, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, ICARUS, Time projection chamber, 010308 nuclear & particles physics, Liquid scintillators, Dark matter WIMP Noble liquid detectors Low-background detectors Liquid scintillators, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Low-background detector, noble liquid detectors, lcsh:QC1-999, DAMA/NaI, Weakly interacting massive particles, High Energy Physics::Experiment, Noble liquid detector, Astrophysics - Instrumentation and Methods for Astrophysics, lcsh:Physics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We report the first results of DarkSide-50, a direct search for dark matter operating in the underground Laboratori Nazionali del Gran Sasso (LNGS) and searching for the rare nuclear recoils possibly induced by weakly interacting massive particles (WIMPs). The dark matter detector is a Liquid Argon Time Projection Chamber with a (46.4+-0.7) kg active mass, operated inside a 30 t organic liquid scintillator neutron veto, which is in turn installed at the center of a 1 kt water Cherenkov veto for the residual flux of cosmic rays. We report here the null results of a dark matter search for a (1422+-67) kg d exposure with an atmospheric argon fill. This is the most sensitive dark matter search performed with an argon target, corresponding to a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 6.1x10^-44 cm^2 for a WIMP mass of 100 GeV/c^2., 26 pages, 7 figures; updated figures and references, notably Fig. 7 has updated CDMSII curve; fixed typos; clarified some language and figures; updated references
Published: 2015

20. Sensitivity and discovery potential of the proposed nEXO experiment to neutrinoless double beta decay

Author: J. L. Vuilleumier, B. Mong, M. Wagenpfeil, J. Dalmasson, A. Piepke, J. Todd, Y. Y. Ding, M. Heffner, Yuehe Lin, John L. Orrell, E. Raguzin, X.L. Sun, J. B. Zhao, C. T. Overman, R. Krücken, D. Qiu, Z. Li, Giorgio Gratta, A. Burenkov, M. Hasan, Arun Kumar Soma, L. J. Kaufman, R. DeVoe, S. J. Daugherty, Samuele Sangiorgio, M. Hughes, K. S. Kumar, V. Veeraraghavan, Y. Lan, Wei Wei, Petr Vogel, Rejean Fontaine, J. Daughhetee, A. Craycraft, U. Wichoski, Ethan Brown, F. Bourque, M. J. Jewell, M. Coon, D. Harris, Yu-Guang Zhou, T. Ziegler, T. Tolba, G. St-Hilaire, T. Tsang, Qun-Yao Wang, T. Stiegler, M. Chiu, J. P. Brodsky, David Moore, F. Retiere, Y. Ito, J. Zettlemoyer, Douglas H Beck, M. Oriunno, Zhijun Ning, S. Johnston, O. Zeldovich, G. Visser, A. Karelin, J. Hößl, A. Pocar, R. Tsang, T. Didberidze, S. Kravitz, Guofu Cao, T. N. Johnson, J. Schneider, P. Hufschmidt, E. V. Hansen, Y-R Yen, David A. Sinclair, F. Vachon, Ryan Killick, David Leonard, K. Murray, Liang Yang, R. J. Newby, Thomas Koffas, A. Jamil, D. Fudenberg, W. M. Fairbank, Gisela Anton, M. Côté, P. C. Rowson, T. Daniels, K. Graham, G. S. Ortega, B. T. Cleveland, M. J. Dolinski, V.N. Stekhanov, K. Odgers, Angelo Dragone, A. House, S. Rescia, A. Kuchenkov, W. Cree, Jean-Francois Pratte, Veljko Radeka, T. Rossignol, S. Feyzbakhsh, R. Saldanha, S. Delaquis, T. Brunner, W. R. Cen, Serge A. Charlebois, C. Licciardi, G. S. Li, R. Gornea, K. Skarpaas, G. Wrede, I. J. Arnquist, M. Tarka, Wei Wu, X. S. Jiang, A. Der Mesrobian-Kabakian, C. Chambers, A.C. Odian, G. Giacomini, A. Schubert, S. Parent, J. Farine, V. Belov, A. Robinson, L. Cao, F. Nolet, L. J. Wen, Marc Weber, S. X. Wu, Lorenzo Fabris, J. B. Albert, R. MacLellan, Thilo Michel, P. S. Barbeau, Jens Dilling, Xuan Zhang, I. Badhrees, I. Ostrovskiy, O. Njoya, A. Iverson, Shu Li, S. Schmidt, T. Rao, N. Roy, and E. W. Hoppe
Subjects: Physics, Time projection chamber, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Active medium, Detector, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 7. Clean energy, 3. Good health, Nuclear physics, Homogeneous, 0103 physical sciences, Sensitivity (control systems), Nuclear Experiment (nucl-ex), 010306 general physics, Enriched Xenon Observatory, Nuclear Experiment, Order of magnitude
Abstract: The next-generation Enriched Xenon Observatory (nEXO) is a proposed experiment to search for neutrinoless double beta ($0\nu\beta\beta$) decay in $^{136}$Xe with a target half-life sensitivity of approximately $10^{28}$ years using $5\times10^3$ kg of isotopically enriched liquid-xenon in a time projection chamber. This improvement of two orders of magnitude in sensitivity over current limits is obtained by a significant increase of the $^{136}$Xe mass, the monolithic and homogeneous configuration of the active medium, and the multi-parameter measurements of the interactions enabled by the time projection chamber. The detector concept and anticipated performance are presented based upon demonstrated realizable background rates., Comment: v2 as published
Published: 2017

21. The Electronics, Trigger and Data Acquisition System for the Liquid Argon Time Projection Chamber of the DarkSide-50 Search for Dark Matter

Author: A. Nelson, M. Carlini, K. Arisaka, E. V. Hungerford, G. Fiorillo, W. Bonivento, P. N. Singh, C. Dionisi, L. Pagani, M. D'Incecco, S. Luitz, Chung-Yao Yang, A. Sotnikov, A. V. Derbin, D. A. Semenov, Augusto Brigatti, H. Qian, K. Fomenko, F. Budano, I. N. Machulin, T. Miletic, N. Canci, Marco Pallavicini, P. Trinchese, C. Giganti, E. Edkins, D. D'Angelo, R. Saldanha, R. Tartaglia, An. Ianni, B. R. Hackett, Hui Wang, A. Zec, S. Pordes, F. Di Eusanio, B. Bottino, P. J. Mosteiro, Fausto Ortica, Thomas Alexander, A. Monte, M. Rescigno, B. Baldin, Anton Empl, A. K. Alton, S. Parmeggiano, Michele Montuschi, Aldo Romani, G. De Rosa, A. Razeto, S. De Cecco, M. M. Wojcik, G. K. Giovanetti, A. de Candia, E. Pantic, P. Agnes, B. J. Mount, F. Gabriele, Q. Riffard, A. Oleinik, B. Schlitzer, D. Franco, M. Orsini, T. N. Johnson, M. Ave, C. Savarese, R. B. Vogelaar, Monica Verducci, C. Zhu, W. Zhong, P. Cavalcante, Nicomede Pelliccia, J. Maricic, Giuseppe Longo, D. Montanari, D. Sablone, C. J. Martoff, G. Bonfini, B. Reinhold, Sandra Zavatarelli, G. Zuzel, Ivone F. M. Albuquerque, E. Shields, V. N. Muratova, K. Biery, Yanchu Wang, K. J. Keeter, Frank Calaprice, S. Davini, D. M. Asner, X. Xiang, Vittorio Cataudella, Samuele Sangiorgio, A. Tonazzo, Stefano Giagu, A. L. Renshaw, A. Navrer Agasson, A. M. Goretti, G. Korga, Paolo Musico, A. Fan, D. A. Pugachev, F. Granato, M. Cariello, Stefano Maria Mari, M. D. Skorokhvatov, L. Grandi, K. Herner, G. Di Pietro, Yanhui Ma, A. Candela, S. Catalanotti, Stuart Derek Walker, A. G. Cocco, Jingke Xu, A. A. Machado, Min-Xin Guan, K. Pelczar, Cristiano Galbiati, D. Hughes, M. De Deo, J. Tatarowicz, A. S. Kubankin, M. De Vincenzi, Gioacchino Ranucci, C. L. Kendziora, Irina James, M. Caravati, Mariano Cadoni, N. Rossi, G. Forster, L. Crippa, O. Smirnov, M. Gromov, P. D. Meyers, M. Wada, E. V. Unzhakov, Y. Guardincerri, M. E. Monzani, A. Pocar, P. Saggese, V. Bocci, M. Cadeddu, C. Cicalo, Giovanni Covone, Severino Angelo Maria Bussino, K. Randle, A. Vishneva, X. Li, M. Razeti, J. Yoo, B. Loer, H. Cao, S. Odrowski, G. Testera, Y. Suvorov, S. Westerdale, A. S. Chepurnov, C. Stanford, Denis Korablev, J. Brodsky, P. Humble, A. Devoto, S. D. Rountree, Paolo Lombardi, E. Segreto, A. Mandarano, V. V. Kobychev, W. Sands, L. Marini, M. Bossa, B. Rossi, Alan Watson, M. Lissia, G. De Filippis, Xiang Xiao, R. Milincic, G. Koh, Henning O. Back, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), DarkSide, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Agnes, P., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Asner, D. M., Ave, M., Back, H. O., Baldin, B., Biery, K., Bocci, V., Bonfini, G., Bonivento, W., Bossa, Maria, Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Caravati, M., Cariello, M., Carlini, M., Catalanotti, S., Cataudella, V., Cavalcante, P., Chepurnov, A., Cicaló, C., Cocco, A. G., Covone, G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., de Candia, A., Cecco, S. De, Deo, M. De, Filippis, G. De, Rosa, G. De, Vincenzi, M. De, Derbin, A., Devoto, A., Eusanio, F. Di, Dionisi, C., Pietro, G. Di, Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Giagu, S., Giganti, C., Giovanetti, G. K., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K. R., Hughes, D., Humble, P., Hungerford, E. V., Ianni, A., James, I., Johnson, T. N., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Loer, B., Lombardi, P., Longo, G., Luitz, S., Ma, Y., Machado, A., Machulin, I. N., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Agasson, A. Navrer, Nelson, A., Odrowski, S., Oleinik, A., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeti, M., Razeto, A., Reinhold, B., Renshaw, A. L., Rescigno, M., Riffard, Q., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Schlitzer, B., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Verducci, M., Vishneva, A., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wojcik, M. M., Xiang, X., Xiao, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Bossa, M., De Candia, A., De Cecco, S., De Deo, M., De Filippis, G., De Rosa, Gianfranca, De Vincenzi, M., Di Eusanio, F., Di Pietro, G., Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Universidade de São Paulo = University of São Paulo (USP), University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS), Fermi National Accelerator Laboratory (Fermilab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ANR-10-LABX-0023,UnivEarthS,Earth - Planets - Universe: observation, modeling, transfer(2010), and ANR-11-IDEX-0005,USPC,Université Sorbonne Paris Cité(2011)
Subjects: axions, Physics - Instrumentation and Detectors, data acquisition, Noble liquid detectors (scintillation, ionization, double-phase), 01 natural sciences, Dark Matter, DarkSide Detector, TPC, High Energy Physics - Experiment, Dark Matter detectors (WIMPs, axions, etc.), High Energy Physics - Experiment (hep-ex), Data acquisition, Noble liquid detectors (scintillation, etc.), [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation, Mathematical Physics, Physics, Resistive touchscreen, Time projection chamber, photomultiplier, Instrumentation and Detectors (physics.ins-det), double-phase), amplifier, Cryostat, Photomultiplier, FOS: Physical sciences, chemistry.chemical_element, Optics, [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], 0103 physical sciences, ionization, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, background: radioactivity, noble liquid detectors, scintillation, double-phase, Dark Matter detectors (WIMPs, MESH: LArTPC, Argon, 010308 nuclear & particles physics, business.industry, Amplifier, Voltage divider, dark matter: detector, trigger, time projection chamber: liquid argon, Gran Sasso, chemistry, electronics: readout, business, electronics: design
Abstract: The DarkSide-50 experiment at the Laboratori Nazionali del Gran Sasso is a search for dark matter using a dual phase time projection chamber with 50 kg of low radioactivity argon as target. Light signals from interactions in the argon are detected by a system of 38 photo-multiplier tubes (PMTs), 19 above and 19 below the TPC volume inside the argon cryostat. We describe the electronics which processes the signals from the photo-multipliers, the trigger system which identifies events of interest, and the data-acquisition system which records the data for further analysis. The electronics include resistive voltage dividers on the PMTs, custom pre-amplifiers mounted directly on the PMT voltage dividers in the liquid argon, and custom amplifier/discriminators (at room temperature). After amplification, the PMT signals are digitized in CAEN waveform digitizers, and CAEN logic modules are used to construct the trigger, the data acquisition system for the TPC is based on the Fermilab "artdaq" software. The system has been in operation since early 2014., 24 pages
Published: 2017

22. Online $$^{222}$$ 222 Rn removal by cryogenic distillation in the XENON100 experiment

Author: April S. Brown, P. Shagin, R. Itay, A. Kish, D. Mayani, Jochen Schreiner, M. P. Decowski, T. Berger, M. Anthony, D. Thers, R. F. Lang, S. Rosendahl, Manfred Lindner, M. Cervantes, M. v. Sivers, Julien Masbou, Michelle Galloway, M. Le Calloch, D. Lellouch, Laura Baudis, A. Tiseni, Yuehuan Wei, V. Pizzella, D. Cichon, S. E. A. Orrigo, C. Hasterok, Z. Greene, R. Saldanha, G. Eurin, M. L. Benabderrahmane, Ethan Brown, M. Messina, Hulin Wang, G. C. Trinchero, J. Pienaar, K. Micheneau, J. Naganoma, T. Marrodán Undagoitia, Ehud Duchovni, João Cardoso, G. Kessler, J.M.F. dos Santos, F. Gao, Elena Aprile, Jelle Aalbers, F. Arneodo, Ran Budnik, L. Levinson, Ioana Codrina Maris, F. Agostini, F. V. Massoli, Qing Lin, F. Piastra, Marc Schumann, F. D. Amaro, P. Pakarha, Sebastian Lindemann, Guillaume Plante, Giacomo Bruno, E. Hogenbirk, E. Shockley, A. Di Giovanni, Boris Bauermeister, W. Fulgione, S. Reichard, C. Reuter, M. Alfonsi, Y. Meng, M. Selvi, M. Murra, L. Rauch, J. Ye, A. Fieguth, D. Coderre, Manuel Gameiro da Silva, A. Stein, R. Persiani, B. Kaminsky, C. Tunnell, A. Molinario, Sara Diglio, M. Scheibelhut, A. Gallo Rosso, Jan Conrad, P. Barrow, Yanxi Zhang, C. Geis, J. Fei, N. Upole, A. Rizzo, N. Priel, Jean-Pierre Cussonneau, L. Bütikofer, Auke-Pieter Colijn, Bart Pelssers, Uwe Oberlack, P. Di Gangi, M. Garbini, J. A. M. Lopes A. Manfredini, C. Grignon, Kaixuan Ni, S. Schindler, D. Franco, H. Landsman, I. Cristescu, P. de Perio, D. Masson, B. Miguez, N. Rupp, L. Scotto Lavina, Hardy Simgen, A. D. Ferella, Ch. Weinheimer, P. A. Breur, G. Sartorelli, S. Bruenner, J. Wulf, M.-C. Piro, L. Grandi, Luke Goetzke, and J. Calvén
Subjects: Air separation, Materials science, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, Detector, Analytical chemistry, chemistry.chemical_element, Noble gas, Radon, 01 natural sciences, Xenon, chemistry, Fractionating column, 0103 physical sciences, Activity concentration, 010306 general physics, Engineering (miscellaneous), Reduction factor
Abstract: We describe the purification of xenon from traces of the radioactive noble gas radon using a cryogenic distillation column. The distillation column is integrated into the gas purification loop of the XENON100 detector for online radon removal. This enabled us to significantly reduce the constant $^{222}$Rn background originating from radon emanation. After inserting an auxiliary $^{222}$Rn emanation source in the gas loop, we determined a radon reduction factor of R > 27 (95% C.L.) for the distillation column by monitoring the $^{222}$Rn activity concentration inside the XENON100 detector.
Published: 2017

23. The DarkSide Experiment: Present Status and Future

Author: S. Odrowski, M. Gromov, E. Segreto, D. Sablone, Peter Daniel Meyers, D. Rountree, Y. Suvorov, S. Westerdale, E. V. Unzhakov, C. Stanford, J. Brodsky, S. M. Mari, P. Saggese, A. M. Goretti, A. S. Chepurnov, S. Walker, Andrea Ianni, T. N. Johnson, E. V. Hungerford, Mariano Cadoni, Hui Wang, M. Guan, L. Pagani, Q. Riffard, Thomas Alexander, Maria Rescigno, A. Devoto, A. Sotnikov, M. D. Skorokhvatov, N. Rossi, A. Navrer Agasson, L. Grandi, F. Di Eusanio, A. K. Alton, Jim Napolitano, A. Tonazzo, M. Carlini, H. O. Back, M. Orsini, I. N. Machulin, Marcello Lissia, K. Biery, Yanchu Wang, P. N. Singh, Paolo Lombardi, J. Tatarowicz, G. Fiorillo, N. Canci, Aldo Romani, G. Di Pietro, Giovanni Covone, R. Saldanha, K. Fomenko, N. Pelliccia, B. J. Mount, J. Maricic, B. Reinhold, P. Agnes, S. Pordes, Marco Pallavicini, D. Korablev, A. Zec, M. Cariello, A. V. Derbin, F. Budano, D. M. Asner, B. Baldin, D. D'Angelo, M. De Vincenzi, A. L. Renshaw, A. Brigatti, G. Testera, D. Franco, K. Randle, K. Pelczar, Cristiano Galbiati, Irina James, D. Semenov, R. Milincic, M. D'Incecco, W. Zhong, S. De Cecco, G. Forster, C. J. Martoff, D. Hughes, M. Caravati, Anselmo Meregaglia, H. Qian, C. Dionisi, C. L. Kendziora, J. Wilhelmi, Chung-Yao Yang, Monica Verducci, G. Bonfini, A. Vishneva, Ivone F. M. Albuquerque, G. K. Giovanetti, B. R. Hackett, P. Cavalcante, A. Empl, M. Wada, W. Bonivento, M. De Deo, S. Davini, Frank Calaprice, X. Xiang, Y. Guardincerri, B. Vogelaar, M. Razeti, S. Catalanotti, S. Bussino, J. D. Miller, Paul H. Humble, E. Pantic, C. Savarese, K. Keeter, C. Giganti, Laura Cadonati, A. S. Kubankin, G. Zuzel, A. G. Cocco, Stefano Giagu, Giuseppe Longo, A. Razeto, R. Tartaglia, Al. Ianni, Xiaoyuan Li, E. Edkins, D. Montanari, V. Bocci, Fausto Ortica, Cécile Jollet, A. Candela, B. Loer, B. Schlitzer, C. Zhu, F. Gabriele, G. Korga, Gioacchino Ranucci, P. Trinchese, F. Granato, E. Shields, K. Herner, M. Cadeddu, C. Cicalo, Paolo Musico, A. Fan, D. A. Pugachev, V. N. Muratova, B. Bottino, A. Monte, A. Pocar, Jilei Xu, O. Smirnov, S. Parmeggiano, Marcin Wójcik, W. Sands, Y. Q. Ma, L. Marini, M. Bossa, B. Rossi, G. Koh, Alan Watson, A. Mandarano, Xiang Xiao, Zuzel, G., Agnes, P., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Asner, D. M., Back, H. O., Baldin, B., Biery, K., Bocci, V., Bonfini, G., Bonivento, W., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Caravati, M., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cicalo, C., Cocco, A. G., Covone, G., D'Angelo, D., D'Incecco, M., Davini, S., De Cecco, S., De Deo, M., De Vincenzi, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Dionisi, C., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Giagu, S., Giganti, C., Giovanetti, G. K., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K., Hughes, D., Humble, P., Hungerford, E. V., Ianni, A. L., Ianni, A. N., James, I., Johnson, T. N., Jollet, C., Keeter, K., Kendziora, C. L., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Loer, B., Lombardi, P., Longo, G., Ma, Y., Machulin, I. N., Mandarano, Marina, Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Milincic, R., Miller, J. D., Montanari, D., Monte, A., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Agasson, A. Navrer, Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeti, M., Razeto, A., Reinhold, B., Renshaw, A. L., Rescigno, M., Riffard, Q., Romani, A., Rossi, B., Rossi, N., Rountree, D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Savarese, C., Schlitzer, B., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Verducci, M., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X. I., Xiao, X., Xu, J., Yang, C., Zec, A., Zhong, W., Zhu, C., Budano, Federico, Bussino, Severino Angelo Maria, DE VINCENZI, Mario, Eusanio, F. Di, Pietro, G. Di, Ianni, A. l., Ianni, A. n., James, Irina, Mandarano, A., Mari, Stefano Maria, Xiang, X. i., AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)
Subjects: WIMP nucleon: scattering, History, Physics::Instrumentation and Detectors, Dark matter, WIMP: mass, chemistry.chemical_element, talk: Moscow 2016/10/10, DarkSide, 4/3, spin: dependence, WIMP: dark matter, channel cross section: upper limit, 01 natural sciences, argon: target, dark matter, Education, Nuclear physics, Physics and Astronomy (all), WIMP, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Physics, Argon, Time projection chamber, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, WIMP nucleon: cross section, time projection chamber: liquid argon, Gran Sasso, Computer Science Applications, Elementary particle physics, Double phase, chemistry, Liquid argon, High Energy Physics::Experiment, MATTER, experimental results
Abstract: International audience; DarkSide is a multi-stage program devoted to direct searches of Dark Matter particles with detectors based on double phase liquid Argon Time Projection Chamber. The DarkSide-50 setup is running underground at the Laboratori Nazionali del Gran Sasso. First it was operated with Atmospheric Argon and during that run (1422 ± 67) kg×d of truly background-free exposure has been accumulated. Obtained data made it possible to set a 90% C.L. upper limit on the WIMP-nucleon cross section of 6.1 × 10(−)(44) cm(2) (for a WIMP mass of 100 GeV/c(2)). Presently the detector is filled with Underground Argon, which is depleted in (39)Ar by a factor of (1.4 ± 0.2)×10(3) with respect to Atmospheric Argon. Acquired so far (2616 ± 43) kg×d (71 live days) in combination with the data from the Atmospheric Argon run give us the 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section of 2.0×10(−)(44) cm(2) for a WIMP mass of 100 GeV/c(2). Up to date this is the best limit obtained with an argon target.
Published: 2017

24. Characterization of an Ionization Readout Tile for nEXO

Author: T. Stiegler, Douglas H Beck, R. Tsang, K. Murray, Gisela Anton, D. Fudenberg, R. Saldanha, Angelo Dragone, J. Todd, Y. Y. Ding, R. Krücken, Jochen M. Schneider, Y-R Yen, Jean-Francois Pratte, P. C. Rowson, K. Skarpaas, S. Kravitz, E. V. Hansen, Liang Yang, S. Feyzbakhsh, A. House, V. Veeraraghavan, R. J. Newby, A. Jamil, Ethan Brown, M. Chiu, W. Cree, A. Burenkov, S. Delaquis, M. Hughes, M. Côté, T. Daniels, Gabriele Giacomini, A. Pocar, Maulik R. Patel, M. Hasan, J. Farine, A. Karelin, R. DeVoe, Jens Dilling, Arun Kumar Soma, Zhijun Ning, T. Tolba, M. J. Jewell, I. Badhrees, David Moore, A. Robinson, T. Didberidze, B. Mong, M. Wagenpfeil, J. Dalmasson, I. J. Arnquist, Xiaoshan Jiang, Yuehe Lin, Veljko Radeka, A. Piepke, Gerrit Wrede, V.N. Stekhanov, J. B. Zhao, S. Parent, U. Wichoski, M. Oriunno, W. R. Cen, C. Chambers, R. Gornea, M. Heffner, A. Odian, D. Qiu, M. Tarka, S. Johnston, T. Ziegler, I. Ostrovskiy, John L. Orrell, E. Raguzin, Z. Li, T. Brunner, S. Rescia, S. X. Wu, Eric W. Hoppe, M. Coon, S. J. Daugherty, A. Schubert, O. Zeldovich, Cory T. Overman, G. Visser, Wei Wu, O. Njoya, A. Iverson, Triveni Rao, Y. Lan, Thomas Tsang, Shu Li, S. Schmidt, J. Daughhetee, Qian Wang, David Leonard, G. S. Ortega, Thomas Koffas, W. M. Fairbank, Samuele Sangiorgio, Giorgio Gratta, J. L. Vuilleumier, B. T. Cleveland, K. Odgers, Serge A. Charlebois, R. MacLellan, Yumei Zhou, Wei Wei, K. S. Kumar, Rejean Fontaine, A. Kuchenkov, P. Hufschmidt, David A. Sinclair, F. Bourque, J. P. Brodsky, G. St-Hilaire, D. Harris, Y. Ito, L. J. Kaufman, M. J. Dolinski, A. Craycraft, Liangjian Wen, Guofu Cao, G. S. Li, Thilo Michel, T. Rossignol, Xiaoyang Sun, C. Licciardi, A. Der Mesrobian-Kabakian, N. Roy, L. Cao, F. Nolet, F. Vachon, Marc Weber, F. Retière, J. B. Albert, X. Zhang, J. Hößl, P. S. Barbeau, V. A. Belov, and Lorenzo Fabris
Subjects: Physics - Instrumentation and Detectors, Materials science, Physics::Instrumentation and Detectors, chemistry.chemical_element, FOS: Physical sciences, STRIPS, 01 natural sciences, law.invention, Optics, Xenon, law, Ionization, 0103 physical sciences, Wafer, 010306 general physics, Instrumentation, Mathematical Physics, Time projection chamber, 010308 nuclear & particles physics, business.industry, Detector, Instrumentation and Detectors (physics.ins-det), Anode, chemistry, visual_art, visual_art.visual_art_medium, Tile, business
Abstract: A new design for the anode of a time projection chamber, consisting of a charge-detecting "tile", is investigated for use in large scale liquid xenon detectors. The tile is produced by depositing 60 orthogonal metal charge-collecting strips, 3~mm wide, on a 10~\si{\cm} $\times$ 10~\si{\cm} fused-silica wafer. These charge tiles may be employed by large detectors, such as the proposed tonne-scale nEXO experiment to search for neutrinoless double-beta decay. Modular by design, an array of tiles can cover a sizable area. The width of each strip is small compared to the size of the tile, so a Frisch grid is not required. A grid-less, tiled anode design is beneficial for an experiment such as nEXO, where a wire tensioning support structure and Frisch grid might contribute radioactive backgrounds and would have to be designed to accommodate cycling to cryogenic temperatures. The segmented anode also reduces some degeneracies in signal reconstruction that arise in large-area crossed-wire time projection chambers. A prototype tile was tested in a cell containing liquid xenon. Very good agreement is achieved between the measured ionization spectrum of a $^{207}$Bi source and simulations that include the microphysics of recombination in xenon and a detailed modeling of the electrostatic field of the detector. An energy resolution $\sigma/E$=5.5\% is observed at 570~\si{keV}, comparable to the best intrinsic ionization-only resolution reported in literature for liquid xenon at 936~V/\si{cm}., Comment: 18 pages, 13 figures, as published
Published: 2017
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25. The electronics and data acquisition system for the DarkSide-50 veto detectors

Author: V. N. Muratova, B. Bottino, E. V. Unzhakov, C. Stanford, G. Koh, B. Baldin, J. Brodsky, J. Wilhelmi, S. De Cecco, P. Saggese, Chung-Yao Yang, C. Savarese, A. Tonazzo, S. D. Rountree, M. Montuschi, Paolo Lombardi, S. Davini, C. J. Martoff, M. Carlini, Peter Daniel Meyers, Yufeng Wang, M. D. Skorokhvatov, L. Grandi, P. N. Singh, M. Gromov, A. Mandarano, A. Kubankin, M. Guan, Y. Suvorov, G. Zuzel, S. Luitz, E. Segreto, A. Candela, S. Westerdale, G. Testera, A. M. Goretti, A. S. Chepurnov, F. Budano, V. V. Kobychev, Mariano Cadoni, E. Pantic, P. J. Mosteiro, A. K. Alton, A. Sotnikov, Aldo Ianni, B. Reinhold, B. R. Hackett, A. Empl, F. Gabriele, E. Edkins, B. J. Mount, A. Zec, L. Agostino, H. Cao, D. Semenov, M. Orsini, J. Maricic, Hui Wang, R. B. Vogelaar, M. De Vincenzi, N. Canci, Caoxiang Zhu, M. De Deo, R. Tartaglia, D. Montanari, Ivone F. M. Albuquerque, A. L. Renshaw, A. Devoto, Griffin Foster, P. Cavalcante, Samuele Sangiorgio, M. Cadeddu, Stefano Maria Mari, J. Tatarowicz, T. Alexander, S. Odrowski, T. Miletic, D. Franco, Sandra Zavatarelli, W. Zhong, C. Giganti, K. Arisaka, K. Herner, R. Saldanha, Fausto Ortica, G. Fiorillo, L. Crippa, K. Fomenko, M. Wada, F. Calaprice, M. D'Incecco, Stuart Derek Walker, A. Vishneva, K. Randle, Anselmo Meregaglia, X. Li, H. Qian, Irina James, Y. Guardincerri, M. E. Monzani, A. Pocar, K. Keeter, A. Monte, Jilei Xu, Q. Riffard, S. Parmeggiano, D. Korablev, A. Brigatti, Jim Napolitano, D. Sablone, N. Pelliccia, X. Xiang, E. Shields, Gioacchino Ranucci, Y. Q. Ma, L. Marini, M. Bossa, B. Rossi, Alan Watson, K. Biery, A. Fan, D. A. Pugachev, Oleg Smirnov, S. Catalanotti, A. G. Cocco, F. Di Eusanio, Aldo Romani, P. Agnes, A. Razeto, P. Musico, W. Sands, M. Cariello, Andrea Ianni, A. V. Derbin, K. Pelczar, Cristiano Galbiati, C. L. Kendziora, M. M. Wojcik, G. Korga, F. Granato, Ann E. Nelson, I. N. Machulin, N. Rossi, Marco Pallavicini, D. D'Angelo, E. Hungerford, R. Milincic, S. Pordes, Henning O. Back, G. Bonfini, Cécile Jollet, J. Yoo, G. Di Pietro, Giovanni Covone, Severino Angelo Maria Bussino, L. Pagani, Marcello Lissia, P. Trinchese, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre Hospitalier Universitaire de Nice (CHU de Nice), Biomécanique et Bioingénierie (BMBI), Université de Technologie de Compiègne (UTC)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), Stanford University [Stanford], Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS Paris)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Departamento de Engenharia Elétrica [Minas Gerais] (DEE - UFMG), Universidade Federal de Minas Gerais, Rhodes University, inconnu, Inconnu, Key Lab of Computer System and Architecture, Institute of Computing Technology [Beijing] (ICT), Chinese Academy of Sciences [Beijing] (CAS), Institut Européen des membranes (IEM), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Centre National de la Recherche Scientifique (CNRS), Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., Dececco, S., De Deo, M., De Vincenzi, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Foster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K. R., Hungerford, E. V., Ianni, Aldo, Ianni, Andrea, James, I., Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Nelson, A., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Riffard, Q., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Budano, Federico, Bussino, Severino Angelo Maria, DE VINCENZI, Mario, James, Irina, and Mari, Stefano Maria
Subjects: Physics - Instrumentation and Detectors, gas and liquid scintillators), architecture, Physics::Instrumentation and Detectors, Dark matter, FOS: Physical sciences, Scintillator, algorithms, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Data acquisition, Front-end electronics for detector readout, 0103 physical sciences, hardware, Neutron, Detector control systems (detector and experiment monitoring and slow control systems, 010306 general physics, Instrumentation, Cherenkov radiation, ComputingMilieux_MISCELLANEOUS, Mathematical Physics, Physics, [PHYS]Physics [physics], Time projection chamber, Data acquisition concepts, Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators), Detector control systems (detector and experiment monitoring and slow control systems, architecture, hardware, algorithms, databases), 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), scintillation and light emission processes (solid, Weakly interacting massive particles, Scintillators, High Energy Physics::Experiment, databases), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: International audience; DarkSide-50 is a detector for dark matter candidates in the form of weakly interacting massive particles. It utilizes a liquid argon time projection chamber for the inner main detector, surrounded by a liquid scintillator veto (LSV) and a water Cherenkov veto detector (WCV). The LSV and WCV act as the neutron and cosmogenic muon veto detectors for DarkSide-50. This paper describes the electronics and data acquisition system used for these two detectors. The system is made of a custom built front end electronics and commercial National Instruments high speed digitizers. The front end electronics, the DAQ, and the trigger system have been used to acquire data in the form of zero-suppressed waveform samples from the 110 PMTs of the LSV and the 80 PMTs of the WCV. The veto DAQ system has proven its performance and reliability. This electronics and DAQ system can be scaled and used as it is for the veto of the next generation DarkSide-20k detector
Published: 2016

26. Discovery of underground argon with low level of radioactive 39Ar and possible applications to WIMP dark matter detectors

Author: D. Marks, M. Roncadelli, K. McCarty, L. Basgall, C. Vignoli, Alfredo G. Cocco, L. Grandi, A. P. Burgers, D. Cheng, F. Di Pompeo, G. Meng, Alexey Yushkov, M. Antonello, N. Canci, F. Fitch, F. Resnati, T. Hohman, Brendan Lyons, F. Carbonara, Matthias Laubenstein, Richard Vondrasek, R. Saldanha, R. Acciarri, C. J. Ballentine, Daniel Robertson, Tiberiu Tesileanu, A. Shirley, J. Ruderman, S. Gazzana, A. Rappoldi, Frank Calaprice, R Highfill, R. Bansal, M. Cambiaghi, C. Rubbia, A. LaCava, A. Pocar, F. Pietropaolo, E. Calligarich, D. Acosta-Kane, Sandro Ventura, A. O. Bazarko, Michael K.H. Leung, G. Fiorillo, A. M. Szelc, P. Benetti, T. Pivonka, F. Cavanna, Luciano Pandola, C. Schmitt, Jay Burton Benziger, R. Tartaglia, Roland Purtschert, O Amaize, M. Gaull, S. Centro, Al. Ianni, F. Dalnoki-Veress, M. Baldo Ceolin, E. de Haas, B. Loer, An. Ianni, Philippe Collon, H.H. Loosli, Robert G. Scott, A. E. Chavarria, Massimo Rossella, A. M. Goretti, V. Gallo, C. Montanari, Cristiano Galbiati, M. Cassidy, B. Baibussinov, T Highfill, O. Palamara, Hye Young Lee, E. Segreto, C. Visnjic, G.L. Raselli, Sujoy Mukhopadhyay, A. Nelson, C., Galbiati, D., Acosta Kane, R., Acciarri, O., Amaize, M., Antonello, B., Baibussinov, M. B., Ceolin, C. J., Ballentine, R., Bansal, L., Basgall, A., Bazarko, P., Benetti, J., Benziger, A., Burger, F., Calaprice, E., Calligarich, M., Cambiaghi, N., Canci, F., Carbonara, M., Cassidy, F., Cavanna, S., Centro, A., Chavarria, D., Cheng, A. G., Cocco, P., Collon, F., Dalnoki Vere, E. d., Haasi, F. D., Pompeo, Fiorillo, Giuliana, F., Fitch, V., Gallo, M., Gaull, S., Gazzana, L., Grandi, A., Gorettil, R., Highfill, T., Highfill, T., Hohman, A., Ianni, A., Lacava, M., Laubenstein, H. Y., Lee, M., Leung, B., Loer, H. H., Loosli, B., Lyon, D., Mark, K., Mccarty, G., Meng, C., Montanari, S., Mukhopadhyay, A., Nelson, O., Palamara, L., Pandola, F., Pietropaolo, T., Pivonka, A., Pocar, R., Purtschert, A., Rappoldi, G., Raselli, F., Resnati, D., Robertson, M., Roncadelli, M., Rossella, C., Rubbia, J., Ruderman, R., Saldanha, C., Schmitt, R., Scott, E., Segreto, A., Shirley, A. M., Szelc, R., Tartaglia, T., Tesileanu, S., Ventura, C., Vignoli, C., Visnjic, R., Vondrasek, A., Yushkov, E. d., Haa, and A., Goretti
Subjects: History, Nuclear and High Energy Physics, ADSORPTION, Physics::Instrumentation and Detectors, Dark matter, FOS: Physical sciences, chemistry.chemical_element, Astrophysics, WIMP Argon Programme, 01 natural sciences, Education, Nuclear physics, WIMP, Natural gas, LIQUID ARGON, 0103 physical sciences, Physics::Atomic and Molecular Clusters, Physics::Chemical Physics, 010306 general physics, Instrumentation, Helium, Physics, Argon, 010308 nuclear & particles physics, business.industry, Astrophysics (astro-ph), Detector, Isotopes of argon, Computer Science Applications, NITROGEN, chemistry, 13. Climate action, business
Abstract: We report on the first measurement of 39Ar in argon from underground natural gas reservoirs. The gas stored in the US National Helium Reserve was found to contain a low level of 39Ar. The ratio of 39Ar to stable argon was found to be, 6 pages, 2 figures, 2 tables
Published: 2008

27. Journal of Instrumentation

Author: P. Agnes, I.F.M. Albuquerque, T. Alexander, A.K. Alton, D.M. Asner, H.O. Back, B. Baldin, K. Biery, V. Bocci, G. Bonfini, W. Bonivento, M. Bossa, B. Bottino, A. Brigatti, J. Brodsky, F. Budano, S. Bussino, M. Cadeddu, L. Cadonati, M. Cadoni, F. Calaprice, N. Canci, A. Candela, M. Caravati, M. Cariello, M. Carlini, S. Catalanotti, P. Cavalcante, A. Chepurnov, C. Cicalò, A.G. Cocco, G. Covone, D. D'Angelo, M. D'Incecco, S. Davini, S. De Cecco, M. De Deo, M. De Vincenzi, A. Derbin, A. Devoto, F. Di Eusanio, G. Di Pietro, C. Dionisi, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, G. Forster, D. Franco, F. Gabriele, C. Galbiati, S. Giagu, C. Giganti, G.K. Giovanetti, A.M. Goretti, F. Granato, L. Grandi, M. Gromov, M. Guan, Y. Guardincerri, B.R. Hackett, K. Herner, D. Hughes, P. Humble, E.V. Hungerford, Al. Ianni, An. Ianni, I. James, T.N. Johnson, C. Jollet, K. Keeter, C.L. Kendziora, G. Koh, D. Korablev, G. Korga, A. Kubankin, X. Li, M. Lissia, B. Loer, P. Lombardi, G. Longo, Y. Ma, A.A. Machado, I.N. Machulin, A. Mandarano, S.M. Mari, J. Maricic, L. Marini, C.J. Martoff, A. Meregaglia, P.D. Meyers, R. Milincic, J.D. Miller, D. Montanari, A. Monte, B.J. Mount, V.N. Muratova, P. Musico, J. Napolitano, A. Navrer Agasson, S. Odrowski, M. Orsini, F. Ortica, L. Pagani, M. Pallavicini, E. Pantic, S. Parmeggiano, K. Pelczar, N. Pelliccia, A. Pocar, S. Pordes, D.A. Pugachev, H. Qian, K. Randle, G. Ranucci, M. Razeti, A. Razeto, B. Reinhold, A.L. Renshaw, M. Rescigno, Q. Riffard, A. Romani, B. Rossi, N. Rossi, D. Rountree, D. Sablone, P. Saggese, R. Saldanha, W. Sands, C. Savarese, B. Schlitzer, E. Segreto, D.A. Semenov, E. Shields, P.N. Singh, M.D. Skorokhvatov, O. Smirnov, A. Sotnikov, C. Stanford, Y. Suvorov, R. Tartaglia, J. Tatarowicz, G. Testera, A. Tonazzo, P. Trinchese, E.V. Unzhakov, M. Verducci, A. Vishneva, B. Vogelaar, M. Wada, S. Walker, H. Wang, Y. Wang, A.W. Watson, S. Westerdale, J. Wilhelmi, M.M. Wojcik, Xi. Xiang, X. Xiao, J. Xu, C. Yang, A. Zec, W. Zhong, C. Zhu, G. Zuzel, AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Pluridisciplinaire Hubert Curien ( IPHC ), Université de Strasbourg ( UNISTRA ) -Centre National de la Recherche Scientifique ( CNRS ), DarkSide, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Physics, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), Agnes, P., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Asner, D. M., Back, H. O., Baldin, B., Biery, K., Bocci, V., Bonfini, G., Bonivento, W., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Caravati, M., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cicalo, C., Cocco, A. G., D'Angelo, D., D'Incecco, M., Davini, S., De Cecco, S., De Deo, M., De Vincenzi, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Dionisi, C., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Giagu, S., Giganti, C., Giovanetti, G. K., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K., Hughes, D., Humble, P., Hungerford, E. V., Ianni, Al., Ianni, An., James, I., Johnson, T. N., Jollet, C., Keeter, K., Kendziora, C. L., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Loer, B., Lombardi, P., Longo, G., Ma, Y., Machado, A. A., Machulin, I. N., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Milincic, R., Miller, J. D., Montanari, D., Monte, A., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Agasson, A. Navrer, Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeti, M., Razeto, A., Reinhold, B., Renshaw, A. L., Rescigno, M., Riffard, Q., Romani, A., Rossi, B., Rossi, N., Rountree, D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Savarese, C., Schlitzer, B., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Verducci, M., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, Xi., Xiao, X., Xu, J., Yang, C., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Covone, G., Navrer Agasson, A., and Semenova, D. A.
Subjects: axions, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Detector alignment and calibration methods (lasers, sources, particle-beams), scintillation counter: liquid, remote operation, 01 natural sciences, Dark Matter detectors (WIMPs, axions, etc.), Instrumentation, Mathematical Physics, Low-background detectors, etc.), hardware, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Physics, Radioactive source calibration, Time projection chamber, Detector, Instrumentation and Detectors (physics.ins-det), particle-beams), Physics - Instrumentation and Detector, organic compounds, sources, Fabrication, WIMP, Dark matter, Noble liquid detectors, FOS: Physical sciences, fabrication, Scintillator, Optics, 0103 physical sciences, Calibration, Neutron, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Dark Matter detectors (WIMPs, detector: design, 010308 nuclear & particles physics, business.industry, dark matter: detector, calibration, time projection chamber: liquid argon, Liquid scintillators, calibration device, insertion device, Detector alignment and calibration methods (lasers, efficiency, Neutron source, business
Abstract: This paper describes the design, fabrication, commissioning and use of a CALibration source Insertion System (CALIS) in the DarkSide-50 direct dark matter search experiment. CALIS deploys radioactive sources into the liquid scintillator veto to characterize the detector response and detection efficiency of the DarkSide-50 Liquid Argon Time Projection Chamber, and the surrounding 30 t organic liquid scintillator neutron veto. It was commissioned in September 2014 and has been used successfully in several gamma and neutron source campaigns since then. A description of the hardware and an excerpt of calibration analysis results are given below., 21 pages, 11 figures
Published: 2016

28. The DarkSide awakens

Author: B. Bottino, R. Tartaglia, A. K. Alton, K. Randle, A. Vishneva, Mariano Cadoni, Denis Korablev, P. Cavalcante, P. J. Mosteiro, J. Brodsky, Michele Montuschi, L. Marini, M. Bossa, P. Saggese, I. N. Machulin, Samuele Sangiorgio, B. J. Mount, N. Rossi, L. Agostino, E. Pantic, A. M. Goretti, N. Canci, C. L. Kendziora, Irina James, B. Rossi, M. Orsini, D. Montanari, S. Catalanotti, Marco Pallavicini, D. D'Angelo, M. Cariello, E. Shields, A. G. Cocco, Jingke Xu, Alan Watson, A. Mandarano, P Trinchese, V. N. Muratova, K. Biery, Yanchu Wang, L. Pagani, K. Pelczar, Cristiano Galbiati, S. Perasso, M. D. Skorokhvatov, S. De Cecco, P. D. Meyers, S. Bussino, Nicomede Pelliccia, L. Grandi, K. Arisaka, G. Korga, C. Stanford, B. Vogelaar, G. Fiorillo, Anton Empl, B. Reinhold, M. M. Wojcik, Chung-Yao Yang, E. Edkins, Paolo Musico, A. V. Derbin, A. Razeto, J. Wilhelmi, A. Fan, M. Wada, Y. Guardincerri, D. A. Pugachev, M. D'Incecco, Anselmo Meregaglia, J. Yoo, M. Lissia, H. Qian, F. Gabriele, G. Zuzel, E. V. Hungerford, G. Testera, D. Sablone, A. Candela, O. Smirnov, M. Gromov, G. Di Pietro, Giovanni Covone, A. Sotnikov, Jim Napolitano, A. S. Kubankin, F. Di Eusanio, A. Tonazzo, S. Parmeggiano, J. Maricic, Aldo Romani, E. V. Unzhakov, P. Agnes, S. Walker, Yanhui Ma, C. Savarese, M. De Deo, W. Sands, Thomas Alexander, M. E. Monzani, Andrea Ianni, Sandra Zavatarelli, A. Pocar, M. Cadeddu, Xiujiang Li, D. Franco, Gioacchino Ranucci, K. Herner, T. Miletic, W. Zhong, Griffin Foster, R. Saldanha, J. Tatarowicz, D. A. Semenov, Caoxiang Zhu, H. Cao, S. Luitz, F. Granato, Cécile Jollet, Han Wang, A. Devoto, Y. Suvorov, S. Westerdale, B. Baldin, S. M. Mari, A. S. Chepurnov, S. Davini, Henning O. Back, S. D. Rountree, Paolo Lombardi, E. Segreto, A. Monte, V. V. Kobychev, B. R. Hackett, A. Brigatti, C. J. Martoff, G. Bonfini, K. J. Keeter, Frank Calaprice, X. Xiang, A. Zec, S. Pordes, R. Milincic, G. Koh, A. L. Renshaw, Aldo Ianni, M. Carlini, P. N. Singh, K. Fomenko, F. Budano, C. Giganti, Laura Cadonati, Fausto Ortica, Min-Xin Guan, M. De Vincenzi, Ivone F. M. Albuquerque, Davini, S., Agnes, P., Agostino, L., M. Albuquerque, I. F., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, Federico, Bussino, Severino Angelo Maria, Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., D'Angelo, D., D'Incecco, M., De Cecco, S., De Deo, M., DE VINCENZI, Mario, Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, G., Fomenko, K., Foster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K. R., Hungerford, E. V., Ianni, Aldo, Ianni, Andrea, James, Irina, Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, Stefano Maria, Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Gran Sasso Science Institute (GSSI), Istituto Nazionale di Fisica Nucleare (INFN), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), DarkSide, Albuquerque, I. F. M., Back, H., Budano, F., Bussino, S., Catalanotti, Sergio, Cocco, ALFREDO GIUSEPPE, Covone, Giovanni, De Vincenzi, M., Di Pietra, G., Fiorillo, Giuliana, James, I., Mari, S. M., Muratova, N., and Walker, Susan Elizabeth
Subjects: History, chemistry.chemical_element, DarkSide, WIMP Argon Programme, WIMP: detector, 01 natural sciences, Education, Atmosphere, Nuclear physics, Physics and Astronomy (all), 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, Physics, Argon, 010308 nuclear & particles physics, Astronomy, suppression, time projection chamber: liquid argon, Computer Science Applications, Gran Sasso, chemistry, radioactivity, argon, atmosphere, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: International audience; The DarkSide program at LNGS aims to perform background-free WIMP searches using two phase liquid argon time projection chambers, with the ultimate goal of covering all parameters down to the so-called neutrino floor. One of the distinct features of the program is the use of underground argon with has a reduced content of the radioactive $^{39}$Ar compared to atmospheric argon. The DarkSide Collaboration is currently operating the DarkSide-50 experiment, the first such WIMP detector using underground argon. Operations with underground argon indicate a suppression of $^{39}$Ar by a factor (1.4 ± 0.2) × 10$^3$ relative to atmospheric argon. The new results obtained with DarkSide-50 and the plans for the next steps of the DarkSide program, the 20t fiducial mass DarkSide-20k detector and the 200 t fiducial Argo, are reviewed in this proceedings.
Published: 2016

29. The veto system of the DarkSide-50 experiment

Author: E. Shields, J. Yoo, Nicomede Pelliccia, A. G. Cocco, B. Reinhold, E. Pantic, C. Giganti, Laura Cadonati, Cécile Jollet, Fausto Ortica, Mariano Cadoni, Andrea Ianni, Sandra Zavatarelli, M. Carlini, E. Edkins, P. N. Singh, K. Fomenko, F. Budano, O. Smirnov, K. Biery, Yanchu Wang, M. D. Skorokhvatov, N. Rossi, L. Agostino, Henning O. Back, L. Grandi, Griffin Foster, H. Cao, S. Parmeggiano, B. R. Hackett, B. Baldin, S. Perasso, A. Zec, Paolo Musico, T. Miletic, A. Fan, D. A. Pugachev, E. V. Unzhakov, E. Segreto, J. Tatarowicz, Ivone F. M. Albuquerque, C. Savarese, A. K. Alton, S. Pordes, S. Walker, Hui Wang, L. Pagani, K. Arisaka, P. Trinchese, P. J. Mosteiro, E. V. Hungerford, S. Davini, A. Brigatti, M. Orsini, L. Crippa, G. Fiorillo, D. Sablone, C. J. Martoff, G. Bonfini, R. Saldanha, Michele Montuschi, A. Candela, S. Odrowski, P. D. Meyers, Thomas Alexander, Jingke Xu, S. Westerdale, G. Testera, D. A. Semenov, K. Pelczar, Cristiano Galbiati, Yanhui Ma, G. Di Pietro, Giovanni Covone, J. Wilhelmi, R. Milincic, M. De Deo, A. Nelson, M. Wada, M. D'Incecco, Stefano Maria Mari, A. S. Kubankin, R. Tartaglia, K. J. Keeter, Frank Calaprice, X. Xiang, Severino Angelo Maria Bussino, G. Koh, Anselmo Meregaglia, H. Qian, Y. Guardincerri, A. Sotnikov, A. Mandarano, S. Catalanotti, D. Franco, W. Zhong, B. J. Mount, Y. Suvorov, M. Gromov, S. Luitz, V. N. Muratova, V. V. Kobychev, A. S. Chepurnov, W. Sands, C. Zhu, P. Cavalcante, B. Bottino, M. E. Monzani, A. Devoto, F. Di Eusanio, C. Stanford, A. Pocar, Denis Korablev, Samuele Sangiorgio, Aldo Romani, J. Brodsky, P. Saggese, P. Agnes, S. D. Rountree, D. Montanari, M. Cadeddu, Paolo Lombardi, M. Lissia, A. Monte, A. V. Derbin, S. De Cecco, Chung-Yao Yang, L. Marini, M. Bossa, B. Rossi, Alan Watson, G. Zuzel, Gioacchino Ranucci, K. Herner, F. Gabriele, Jim Napolitano, K. Randle, A. Tonazzo, A. Vishneva, X. Li, C. L. Kendziora, Irina James, J. Maricic, G. Korga, F. Granato, I. N. Machulin, N. Canci, Marco Pallavicini, D. D'Angelo, Anton Empl, M. M. Wojcik, A. L. Renshaw, Aldo Ianni, A. M. Goretti, M. Cariello, A. Razeto, T. N. Johnson, R. B. Vogelaar, Min-Xin Guan, M. De Vincenzi, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), DarkSide, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., De Cecco, S., De Deo, M., De Vincenzi, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Foster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K. R., Hungerford, E. V., Ianni, Aldo, Ianni, Andrea, James, I., Johnson, T., Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Nelson, A., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Pluridisciplinaire Hubert Curien ( IPHC ), Centre National de la Recherche Scientifique ( CNRS ) -Université de Strasbourg ( UNISTRA ), Bussino, Severino Angelo Maria, DE VINCENZI, Mario, Fiorillo, G., James, Irina, Mari, Stefano Maria, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), ANR-10-LABX-0023,UnivEarthS,Earth - Planets - Universe: observation, modeling, transfer(2010), and ANR-11-IDEX-0005,USPC,Université Sorbonne Paris Cité(2011)
Subjects: fast neutrons), Physics - Instrumentation and Detectors, axions, gas and liquid scintillators), Cherenkov detector, Cherenkov and transition radiation, Physics::Instrumentation and Detectors, Cherenkov counter: water, Nuclear Theory, scintillation counter: liquid, FOS: Physical sciences, Scintillator, 01 natural sciences, Particle detector, High Energy Physics - Experiment, law.invention, thermal, Dark Matter detectors (WIMPs, axions, etc.), Nuclear physics, High Energy Physics - Experiment (hep-ex), WIMP, [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], law, etc.), 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Neutron detection, Neutron, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Nuclear Experiment, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation, Dark Matter detectors (WIMPs, Mathematical Physics, Event reconstruction, nucleus: recoil, Physics, 010308 nuclear & particles physics, Detector, Instrumentation and Detectors (physics.ins-det), Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators), Neutron detectors (cold, thermal, fast neutrons), Neutron detectors (cold, scintillation and light emission processes (solid, Scintillators, High Energy Physics::Experiment, performance
Abstract: International audience; Nuclear recoil events produced by neutron scatters form one of the most important classes of background in WIMP direct detection experiments, as they may produce nuclear recoils that look exactly like WIMP interactions. In DarkSide-50, we both actively suppress and measure the rate of neutron-induced background events using our neutron veto, composed of a boron-loaded liquid scintillator detector within a water Cherenkov detector. This paper is devoted to the description of the neutron veto system of DarkSide-50, including the detector structure, the fundamentals of event reconstruction and data analysis, and basic performance parameters.
Published: 2016

30. SOX : short distance neutrino oscillations with Borexino

Author: Lino Miramonti, A. Caminata, A.V. Etenko, F. Gabriele, M. Vivier, F. Lombardi, V. Fischer, G. Zuzel, D. Korablev, M. Cribier, P. J. Mosteiro, S. Gazzana, Hui Wang, B. Lehnert, G. Bellini, M. Montuschi, Aldo Romani, Laura Cadonati, R. Tartaglia, G. Bonfini, J. Winter, N. Berton, S. Marcocci, L. Di Noto, Michael Meyer, J. Gaffiot, L. Papp, Matteo Agostini, D. Franco, S. Farinon, Frank Calaprice, Kai Zuber, Lothar Oberauer, L. Scola, M. Göger-Neff, A. Razeto, Hardy Simgen, D. Bravo-Berguño, E. V. Hungerford, Fausto Ortica, Matthias Laubenstein, W. Maneschg, V. N. Muratova, S. Schönert, A. Sotnikov, Aldo Ianni, A. E. Chavarria, L. Perasso, Gioacchino Ranucci, M. D. Skorokhvatov, Michael Wurm, L. Grandi, R. B. Vogelaar, Alessandra Re, Andrea Ianni, C. Salvo, Livia Ludhova, E. Meroni, R. Saldanha, D. Bick, Sandra Zavatarelli, A. M. Goretti, A. S. Chepurnov, K. Fomenko, Q. Meindl, F. von Feilitzsch, A. V. Derbin, Thierry Lasserre, C. Veyssiere, M. Durero, G. Testera, Cristiano Galbiati, Marco Giammarchi, S. Davini, N. Rossi, R. Musenich, N. Jonquères, J. Maricic, M. Gromov, T. Houdy, E. Litvinovich, G. Mention, I. N. Machulin, Marco Pallavicini, D. D'Angelo, Y. Suvorov, T. Lewke, D. Kryn, Jonathan M. Link, O. Smirnov, G. Korga, S. Manecki, K. Otis, B. Caccianiga, C. Ghiano, Anton Empl, Caren Hagner, P. Cavalcante, M. Misiaszek, K. Althenmüller, A. Pocar, M. Obolensky, Marcin Wójcik, S. V. Sukhotin, A. Wright, O. Zaimidoroga, G. Lukyanchenko, V. V. Kobychev, Paolo Lombardi, Jay Burton Benziger, Département de Physique Nucléaire (ex SPhN) (DPHN), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), SOX, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Bravo-Berguño, D., Suvorov, Y., Et, Al., Bureau de Conception Calculs et Réalisations (BCCR), Service d'Etudes Mécaniques et Thermiques (SEMT), Département de Modélisation des Systèmes et Structures (DM2S), CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département de Modélisation des Systèmes et Structures (DM2S), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Subjects: Sterile neutrino, Physics::Instrumentation and Detectors, scintillation counter: liquid, talk: Valencia 2014/07/02, 7. Clean energy, 01 natural sciences, [SPI]Engineering Sciences [physics], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Borexino, gallium, Physics, Oscillation, neutrino: sterile, solar, cerium, chromium, chromium-51, neutrino: geophysics, Neutrino, performance, Nuclear and High Energy Physics, Particle physics, Anomalous oscillations, Cerium-144, Chromium-51, SOX, Sterile neutrinos, anomaly, neutrino/e: beam, Scintillator, cerium-144, MiniBooNE, sterile neutrinos, 0103 physical sciences, 010306 general physics, Neutrino oscillation, 010308 nuclear & particles physics, chromium-51cerium-144, calibration, Gran Sasso, LSND, Anomalous oscillation, neutrino: family, High Energy Physics::Experiment, nuclear reactor, neutrino: oscillation, Anomaly (physics), anomalous oscillations, experimental results, neutrino/e: oscillation
Abstract: The Borexino detector has convincingly shown its outstanding performance in the in the sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection, which make it the ideal tool to unambiguously test the long-standing issue of the existence of a sterile neutrino, as suggested by several anomalies: the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar ν experiments, and the recently hinted reactor anomaly. The SOX project will exploit two sources, based on chromium and cerium, which deployed under the experiment will emit two intense beams of ν e (Cr) and ν e ‾ (Ce). Interacting in the active volume of the liquid scintillator, each beam would create a spatial wave pattern in case of oscillation of the ν e (or ν e ‾ ) into the sterile state, which would be the smoking gun proving the existence of the new sterile member of the neutrino family. Otherwise, its absence will allow setting very stringent limit on its existence.
Published: 2016

31. Study of silicon photomultiplier performance in external electric fields

Author: A. Alamre, T. Stiegler, John L. Orrell, T. Daniels, M. Côté, J. Schneider, Z. Li, N. Roy, L. Cao, F. Nolet, M. Oriunno, M. Hughes, Ethan Brown, J. Farine, D. Fairbank, D. Qiu, Y. Ito, M. Coon, Thilo Michel, Qing Xia, V.N. Stekhanov, C. T. Overman, M. Chiu, G. S. Ortega, A. Karelin, A. Pocar, D. S. Leonard, T. Tolba, Venkatesh Veeraraghavan, J. Hößl, Marc Weber, S. Kravitz, Yuehe Lin, David Moore, Y. Lan, R. DeVoe, Serge A. Charlebois, K. Murray, A. Craycraft, J. Echevers, Gisela Anton, M. Wagenpfeil, J. Dalmasson, T. Brunner, E. Raguzin, O. Nusair, Jens Dilling, R. Krücken, Z. Ning, Samuele Sangiorgio, Wei Wei, K. S. Kumar, S. X. Wu, Gerard Visser, P. S. Barbeau, D. A. Harris, A. Der Mesrobian-Kabakian, J. B. Zhao, A. Larson, D. Fudenberg, O. Zeldovich, A. Piepke, I. Badhrees, Angelo Dragone, M. J. Jewell, F. Vachon, Rejean Fontaine, Jean-Francois Pratte, R. Saldanha, L. Darroch, D. Kodroff, B. Veenstra, F. Bourque, S. Parent, S. Rescia, Lorenzo Fabris, T. Bhatta, A. Odian, S. J. Daugherty, J. Watkins, I. Ostrovskiy, R. MacLellan, G. Giacomini, J. P. Brodsky, T. I. Totev, Stefan Schmidt, R. Tsang, O. Njoya, A. Iverson, Triveni Rao, K. Skarpaas Viii, T. Rossignol, G. Wrede, B. Mong, Thomas Tsang, Shu Li, P. Fierlinger, W. R. Cen, Liangjian Wen, Guofu Cao, L. J. Kaufman, A. E. Robinson, M. Tarka, J. B. Albert, Qian Wang, G. Li, S. Feyzbakhsh, Giorgio Gratta, Yumei Zhou, M. J. Dolinski, P. Hufschmidt, David A. Sinclair, B. T. Cleveland, K. Odgers, A. Kuchenkov, U. Wichoski, G. St-Hilaire, C. Licciardi, V. Radeka, T. Ziegler, Thomas Koffas, W. M. Fairbank, Xilei Sun, I. J. Arnquist, Wei Wu, R.J. Newby, P. C. Rowson, A. House, W. Cree, S. Delaquis, Xiaoshan Jiang, C. Chambers, G. Gallina, P. Lv, J. Todd, Y. Y. Ding, E. V. Hansen, Liang Yang, A. Jamil, Douglas H Beck, A. Burenkov, Y-R Yen, J. L. Vuilleumier, Arun Kumar Soma, C. Jessiman, M. K. Moe, Eric W. Hoppe, M. Heffner, J. Daughhetee, R. Gornea, F. Retière, and V. A. Belov
Subjects: 010302 applied physics, Physics - Instrumentation and Detectors, Materials science, 010308 nuclear & particles physics, business.industry, FOS: Physical sciences, Observable, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 7. Clean energy, Silicon photomultiplier, Electric field, 0103 physical sciences, Optoelectronics, business, Instrumentation, Photon detection, Mathematical Physics
Abstract: We report on the performance of silicon photomultiplier (SiPM) light sensors operating in electric field strength up to 30 kV/cm and at a temperature of 149K, relative to their performance in the absence of an external electric field. The SiPM devices used in this study show stable gain, photon detection efficiency, and rates of correlated pulses, when exposed to external fields, within the estimated uncertainties. No observable physical damage to the bulk or surface of the devices was caused by the exposure., Comment: 16 pages, 12 figures, 2 tables and two conferences (INPC2016 and TIPP2017)
Published: 2018

32. Characterization of photomultiplier tubes with a realistic model through GPU-boosted simulation

Author: L. Grandi, M. Anthony, Qing Lin, Elena Aprile, and R. Saldanha
Subjects: Physics, Photomultiplier, 010308 nuclear & particles physics, FOS: Physical sciences, 01 natural sciences, Characterization (materials science), symbols.namesake, Cascade, 0103 physical sciences, symbols, Electronic engineering, Current (fluid), Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Instrumentation, Gaussian network model, Mathematical Physics, Voltage
Abstract: The accurate characterization of a photomultiplier tube (PMT) is crucial in a wide-variety of applications. However, current methods do not give fully accurate representations of the response of a PMT, especially at very low light levels. In this work, we present a new and more realistic model of the response of a PMT, called the cascade model, and use it to characterize two different PMTs at various voltages and light levels. The cascade model is shown to outperform the more common Gaussian model in almost all circumstances and to agree well with a newly introduced model independent approach. The technical and computational challenges of this model are also presented along with the employed solution of developing a robust GPU-based analysis framework for this and other non-analytical models.
Published: 2018

33. Observation of the dependence on drift field of scintillation from nuclear recoils in liquid argon

Author: B. Rossi, F. DeJongh, D. Olvitt, L. Grandi, A. G. Cocco, S. Westerdale, Alan Watson, G. Fiorillo, T. Alexander, H. O. Back, H. Qian, Cristiano Galbiati, P. J. Mosteiro, R. Saldanha, J. Yoo, Ben Loer, D. Montanari, C. J. Martoff, W. H. Lippincott, Hui Wang, Y. Meng, Stuart Derek Walker, C. L. Kendziora, J. Tatarowicz, Laura Manenti, C. Love, S. Pordes, H. Cao, Wanpeng Tan, T., Alexander, H. O., Back, H., Cao, A. G., Cocco, F., Dejongh, Fiorillo, Giuliana, C., Galbiati, L., Grandi, C., Kendziora, W. H., Lippincott, B., Loer, C., Love, L., Manenti, C. J., Martoff, Y., Meng, D., Montanari, P., Mosteiro, D., Olvitt, S., Porde, H., Qian, B., Rossi, R., Saldanha, W., Tan, J., Tatarowicz, S., Walker, H., Wang, A. W., Watson, S., Westerdale, and J., Yoo
Subjects: Physics, Nuclear and High Energy Physics, Scintillation, EFFICIENCY, Time projection chamber, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Liquid scintillation counting, Dark matter, Neutron radiation, 01 natural sciences, 7. Clean energy, ENERGY, Nuclear physics, XENON, YIELD, Electric field, LUMINESCENCE, 0103 physical sciences, Nuclear astrophysics, Neutron, Atomic physics, Nuclear Experiment, 010306 general physics
Abstract: We have exposed a dual-phase liquid argon time projection chamber (LAr-TPC) to a low energy pulsed narrow-band neutron beam, produced at the Notre Dame Institute for Structure and Nuclear Astrophysics, to study the scintillation light yield of recoiling nuclei. Liquid scintillation counters were arranged to detect and identify neutrons scattered in the LAr-TPC and to select the energy of the recoiling nuclei. We report the observation of a significant dependence (up to 32%) on the drift field of liquid argon scintillation from nuclear recoils of energies between 10.8 and 49.9 keV. The field dependence is stronger at lower energies. Since it is the first measurement of such an effect in liquid argon, this observation is important because, to date, estimates of the sensitivity of LAr-TPC dark matter searches are based on the assumption that the electric field has only a small effect on the light yield from nuclear recoils.
Published: 2013

34. The DarkSide Project

Author: Mariano Cadoni, L. Marini, M. Bossa, E. Shields, N. Rossi, B. Rossi, F. Gabriele, S. Bussino, D. A. Semenov, Jim Napolitano, Giovanni Covone, F. Di Eusanio, Alan Watson, V. N. Muratova, S. Perasso, Aldo Romani, K. Biery, Yanchu Wang, A. Tonazzo, P. Agnes, A. K. Alton, B. R. Hackett, A. M. Goretti, R. Tartaglia, M. Cariello, M. E. Monzani, A. Nelson, Al. Ianni, P. J. Mosteiro, T. Miletic, A. Pocar, Min-Xin Guan, A. Zec, S. Pordes, G. Forster, Sandra Zavatarelli, R. Milincic, Jingke Xu, Stefano Maria Mari, Hui Wang, B. J. Mount, C. Zhu, P. Cavalcante, Thomas Alexander, P. Trinchese, R. Saldanha, G. Koh, K. Pelczar, M. Montuschi, Paolo Musico, A. Fan, D. A. Pugachev, Cristiano Galbiati, B. Baldin, Ivone F. M. Albuquerque, J. Tatarowicz, M. Lissia, D. Montanari, S. Walker, E. Pantic, Samuele Sangiorgio, An. Ianni, Gioacchino Ranucci, C. Savarese, E. Segreto, H. Cao, M. Orsini, B. Bottino, M. De Vincenzi, A. Vishneva, D. Franco, S. Davini, W. Zhong, A. Mandarano, L. Crippa, C. L. Kendziora, M. D. Skorokhvatov, A. Monte, L. Grandi, Irina James, M. Carlini, A. L. Renshaw, Nicomede Pelliccia, V. V. Kobychev, Cécile Jollet, J. Wilhelmi, P. N. Singh, Chung-Yao Yang, A. V. Derbin, B. Reinhold, M. Wada, O. Smirnov, S. Parmeggiano, Y. Guardincerri, K. Fomenko, F. Budano, B. Vogelaar, Yanhui Ma, C. Giganti, Laura Cadonati, S. Odrowski, G. Di Pietro, E. V. Unzhakov, M. De Deo, E. Edkins, A. Brigatti, Fausto Ortica, D. Sablone, C. J. Martoff, G. Bonfini, A. Devoto, G. Testera, L. Agostino, D. Rountree, K. J. Keeter, J. Yoo, Paolo Lombardi, Henning O. Back, M. Gromov, J. Maricic, W. Sands, Frank Calaprice, X. Xiang, Peter Daniel Meyers, A. Kubankin, Y. Suvorov, S. Westerdale, A. Candela, A. S. Chepurnov, C. Stanford, Denis Korablev, J. Brodsky, P. Saggese, K. Randle, X. Li, G. Korga, F. Granato, I. N. Machulin, N. Canci, Marco Pallavicini, D. D'Angelo, Anton Empl, M. M. Wojcik, K. Arisaka, G. Fiorillo, L. Pagani, M. D'Incecco, Anselmo Meregaglia, H. Qian, M. Cadeddu, S. Luitz, A. Razeto, E. V. Hungerford, A. Sotnikov, K. Herner, S. De Cecco, G. Zuzel, S. Catalanotti, A. G. Cocco, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), DarkSide project, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Agnes, P., Agostino, L., Albuquerque, I. F. M., Alexander, T., Alton, A. K., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Bottino, B., Brigatti, A., Brodsky, J., Budano, F., Bussino, S., Cadeddu, M., Cadonati, L., Cadoni, M., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Carlini, M., Catalanotti, S., Cavalcante, P., Chepurnov, A., Cocco, A. G., Covone, G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., De Cecco, S., De Deo, M., De Vincenzi, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Giganti, C., Goretti, A. M., Granato, F., Grandi, L., Gromov, M., Guan, M., Guardincerri, Y., Hackett, B. R., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., James, I., Jollet, C., Keeter, K., Kendziora, C. L., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kubankin, A., Li, X., Lissia, M., Lombardi, P., Luitz, S., Ma, Y., Machulin, I. N., Mandarano, A., Mari, S. M., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meyers, P. D., Miletic, T., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M., Mosteiro, P., Mount, B. J., Muratova, V. N., Musico, P., Napolitano, J., Nelson, A., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Parmeggiano, S., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D. A., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A. L., Romani, A., Rossi, B., Rossi, N., Rountree, D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Savarese, C., Segreto, E., Semenov, D. A., Shields, E., Singh, P. N., Skorokhvatov, M. D., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Trinchese, P., Unzhakov, E. V., Vishneva, A., Vogelaar, B., Wada, M., Walker, S., Wang, H., Wang, Y., Watson, A. W., Westerdale, S., Wilhelmi, J., Wojcik, M. M., Xiang, X., Xu, J., Yang, C., Yoo, J., Zavatarelli, S., Zec, A., Zhong, W., Zhu, C., Zuzel, G., Bussino, Severino Angelo Maria, DE VINCENZI, Mario, Fiorillo, G., James, Irina, Mari, Stefano Maria, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: axions, Dark matter, chemistry.chemical_element, DarkSide, Noble liquid detectors (scintillation, ionization, double-phase), WIMP Argon Programme, Scintillator, dark matter: direct detection, 01 natural sciences, argon: nuclide, Dark Matter detectors (WIMPs, axions, etc.), Nuclear physics, Noble liquid detectors (scintillation, etc.), 0103 physical sciences, ionization, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, Dark Matter detectors (WIMPs, Mathematical Physics, Physics, Argon, 010308 nuclear & particles physics, Large detector systems for particle and astroparticle physics, Time projection Chambers (TPC), double-phase), time projection chamber: liquid argon, deep underground detector, Gran Sasso, chemistry, Project based, Large detector systems for particle and astroparticle physic, National laboratory, performance, ArDM
Abstract: International audience; DarkSide is a graded experimental project based on radiopure argon, and is now, and will be, used in direct dark matter searches. The present DarkSide-50 detector, operating at the Gran Sasso National Laboratory, is a dual-phase, 50 kg, liquid argon time-projection-chamber surrounded by an active liquid scintillator veto. It is designed to be background free in 3 years of operation. DS-50 performances, when filled with atmospheric argon, are reported. However DS-50 filled with underground argon, shows impressive reduction of the (39)Ar isotope. The application of this powerful technology in a future generation of the DarkSide program is discussed.
Published: 2015

35. DarkSide search for dark matter

Author: I. N. Machulin, R. Klemmer, Marco Pallavicini, N. Rossi, G. Forster, K. Fomenko, W. Sands, G. Di Pietro, H. Cao, D. D'Angelo, M. Komor, A. Razeto, N. N. Nurakhov, R. Saldanha, S. Parmeggiano, A. Nemtzow, E. Shields, F. Perfetto, Min-Xin Guan, M. Gromov, K. Randle, E. V. Unzhakov, S. Bussino, M. Orsini, M. Montuschi, E. Meroni, G. Korga, Austin P. Lund, Marc S. Seigar, A. Tonazzo, E. de Haas, G. Testera, L. Lukyanchenko, S. Gazzana, M. D. Skorokhvatov, B. Rossi, M. De Vincenzi, J. Maricic, L. Grandi, G. Zuzel, Laura Cadonati, M. E. Monzani, Yanhui Ma, D. Durben, M. Zehfus, B. J. Mount, Chung-Yao Yang, Augusto Brigatti, Lawrence Pinsky, A. Kayunov, R. B. Vogelaar, A. Meregaglia, S. Chidzik, C. Joliet, C. Condon, C. Ghiano, A. Pocar, N. Pelliccia, C. L. Kendziora, P. Saggese, A. Nelson, Sandra Zavatarelli, P. X. Li, O. Smirnov, S. Westerdale, Livia Ludhova, A. M. Goretti, A. S. Chepurnov, Thomas Alexander, S. Pordes, E. V. Hungerford, G. Koh, G. Guray, A. Sotnikov, Fausto Ortica, C. Guo, D. A. Semenov, R. Tartaglia, E. Pantic, K. Arisaka, G. Fiorillo, D. Korablev, I. Dratchnev, C. J. Martoff, Frank Calaprice, J. Brodsky, J. Tatarowicz, K. Keeter, Gioacchino Ranucci, Marcin Wójcik, D. Franco, W. Zhong, P. Cavalcante, Henning O. Back, G. Bonfini, P. Beltrame, P. D. Meyers, J. Thompson, An. Ianni, V. N. Muratova, L. Perasso, D. Alton, C. Salvo, S. Perasso, A.V. Etenko, R. Parsells, S. Davini, A. G. Cocco, Al. Ianni, Stefano Maria Mari, S. Luitz, Han Wang, P. J. Mosteiro, F. Gabriele, Jingke Xu, Cristiano Galbiati, D. Montanari, A. Fan, A. Empl, S. Kidner, S. V. Sukhotin, A. Wright, V. V. Kobychev, K. Lung, C. Love, T. Mohayai, A. Candela, S. D. Rountree, Paolo Lombardi, Aldo Romani, B Loer, A. V. Derbin, Y Suvarov, Jay Burton Benziger, T., Alexander, D., Alton, K., Arisaka, H. O., Back, P., Beltrame, J., Benziger, G., Bonfini, A., Brigatti, J., Brodsky, S., Bussino, L., Cadonati, F., Calaprice, A., Candela, H., Cao, P., Cavalcante, A., Chepurnov, S., Chidzik, A. G., Cocco, C., Condon, D., D'Angelo, S., Davini, M. D., Vincenzi, E. D., Haa, A., Derbin, G. D., Pietro, I., Dratchnev, D., Durben, A., Empl, A., Etenko, A., Fan, Fiorillo, Giuliana, D., Franco, K., Fomenko, G., Forster, F., Gabriele, C., Galbiati, S., Gazzana, C., Ghiano, A., Goretti, L., Grandi, M., Gromov, M., Guan, C., Guo, G., Guray, E. V., Hungerford, A., Ianni, C., Joliet, A., Kayunov, K., Keeter, C., Kendziora, S., Kidner, R., Klemmer, V., Kobychev, G., Koh, M., Komor, D., Korablev, G., Korga, P., Li, B., Loer, P., Lombardi, C., Love, L., Ludhova, S., Luitz, L., Lukyanchenko, A., Lund, K., Lung, Y., Ma, I., Machulin, S., Mari, J., Maricic, C. J., Martoff, A., Meregaglia, E., Meroni, P., Meyer, T., Mohayai, D., Montanari, M., Montuschi, M. E., Monzani, P., Mosteiro, B., Mount, V., Muratova, A., Nelson, A., Nemtzow, N., Nurakhov, M., Orsini, F., Ortica, M., Pallavicini, E., Pantic, S., Parmeggiano, R., Parsell, N., Pelliccia, L., Perasso, S., Perasso, Perfetto, Francesco, L., Pinsky, A., Pocar, S., Porde, K., Randle, G., Ranucci, A., Razeto, A., Romani, B., Rossi, N., Rossi, S. D., Rountree, P., Saggese, R., Saldanha, C., Salvo, W., Sand, M., Seigar, D., Semenov, E., Shield, M., Skorokhvatov, O., Smirnov, A., Sotnikov, S., Sukhotin, Y., Suvarov, R., Tartaglia, J., Tatarowicz, G., Testera, J., Thompson, A., Tonazzo, E., Unzhakov, R. B., Vogelaar, H., Wang, S., Westerdale, M., Wojcik, A., Wright, J., Xu, C., Yang, S., Zavatarelli, M., Zehfu, W., Zhong, G., Zuzel, Physics Department, Amherst U., University of Massachusetts System (UMASS), Biomécanique et Bioingénierie (BMBI), Université de Technologie de Compiègne (UTC)-Centre National de la Recherche Scientifique (CNRS), Régulation de l'expression génétique chez les microorganismes (REGCM), Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire Kastler Brossel (LKB (Jussieu)), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), departement de physique, Albert-Ludwigs-Universität Freiburg, SLAC National Accelerator Laboratory (SLAC), Stanford University, Anhui University [Hefei], Physics Department, Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Department of Geological Sciences, University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), Università degli studi di Genova = University of Genoa (UniGe), Departamento de Engenharia Elétrica [Minas Gerais] (DEE - UFMG), Universidade Federal de Minas Gerais, Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Rhodes University, Grahamstown, EAST CHINA UNIVERSITY, KEY LAB, Institute of Physics, Polish Academy of Sciences, Polska Akademia Nauk = Polish Academy of Sciences (PAN), International Iberian Nanotechnology Laboratory (INL), Centre de Recherche en Information Biomédicale sino-français (CRIBS), Université de Rennes (UR)-Southeast University [Jiangsu]-Institut National de la Santé et de la Recherche Médicale (INSERM), Institut Européen des membranes (IEM), Université Montpellier 2 - Sciences et Techniques (UM2)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Alexander, T, Alton, D, Arisaka, K, Back, Ho, Beltrame, P, Benziger, J, Bonfini, G, Brigatti, A, Brodsky, J, Bussino, Severino Angelo Maria, Cadonati, L, Calaprice, F, Candela, A, Cao, H, Cavalcante, P, Chepurnov, A, Chidzik, S, Cocco, Ag, Condon, C, D'Angelo, D, Davini, S, DE VINCENZI, Mario, De Haas, E, Derbin, A, Di Pietro, G, Dratchnev, I, Durben, D, Empl, A, Etenko, A, Fan, A, Fiorillo, G, Franco, D, Fomenko, K, Forster, G, Gabriele, F, Galbiati, C, Gazzana, S, Ghiano, C, Goretti, A, Grandi, L, Gromov, M, Guan, M, Guo, C, Guray, G, Hungerford, Ev, Ianni, Al, Ianni, An, Joliet, C, Kayunov, A, Keeter, K, Kendziora, C, Kidner, S, Klemmer, R, Kobychev, V, Koh, G, Komor, M, Korablev, D, Korga, G, Li, P, Loer, B, Lombardi, P, Love, C, Ludhova, L, Luitz, S, Lukyanchenko, L, Lund, A, Lung, K, Ma, Y, Machulin, I, Mari, Stefano Maria, Maricic, J, Martoff, Cj, Meregaglia, A, Meroni, E, Meyers, P, Mohayai, T, Montanari, D, Montuschi, M, Monzani, Me, Mosteiro, P, Mount, B, Muratova, V, Nelson, A, Nemtzow, A, Nurakhov, N, Orsini, M, Ortica, F, Pallavicini, M, Pantic, E, Parmeggiano, S, Parsells, R, Pelliccia, N, Perasso, L, Perasso, S, Perfetto, F, Pinsky, L, Pocar, A, Pordes, S, Randle, K, Ranucci, G, Razeto, A, Romani, A, Rossi, B, Rossi, N, Rountree, Sd, Saggese, P, Saldanha, R, Salvo, C, Sands, W, Seigar, M, Semenov, D, Shields, E, Skorokhvatov, M, Smirnov, O, Sotnikov, A, Sukhotin, S, Suvarov, Y, Tartaglia, R, Tatarowicz, J, Testera, G, Thompson, J, Tonazzo, A, Unzhakov, E, Vogelaar, Rb, Wang, H, Westerdale, S, Wojcik, M, Wright, A, Xu, J, Yang, C, Zavatarelli, S, Zehfus, M, Zhong, W, Zuzel, G., Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Dip. di Fisica dell'Università di Genova - Italy, Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Southeast University [Jiangsu]-Institut National de la Santé et de la Recherche Médicale (INSERM), and Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut de Chimie du CNRS (INC)-Université de Montpellier (UM)
Subjects: Physics::Instrumentation and Detectors, Dark matter, chemistry.chemical_element, 7. Clean energy, 01 natural sciences, Nuclear physics, 0103 physical sciences, Neutron, Dark Matter detector, 010306 general physics, Instrumentation, Mathematical Physics, ComputingMilieux_MISCELLANEOUS, Event reconstruction, Physics, [PHYS]Physics [physics], Scintillation, Argon, Time projection chamber, 010308 nuclear & particles physics, Detector, chemistry, Scintillation counter, High Energy Physics::Experiment, Noble liquid detector, DarkSide detector, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: "The DarkSide staged program utilizes a two-phase time projection chamber (TPC) with liquid argon as the target material for the scattering of dark matter particles. Efficient background reduction is achieved using low radioactivity underground argon as well as several experimental handles such as pulse shape, ratio of ionization over scintillation signal, 3D event reconstruction, and active neutron and muon vetos. The DarkSide-10 prototype detector has proven high scintillation light yield, which is a particularly important parameter as it sets the energy threshold for the pulse shape discrimination technique. The DarkSide-50 detector system, currently in commissioning phase at the Gran Sasso Underground Laboratory, will reach a sensitivity to dark matter spin-independent scattering cross section of 10(-45) cm(2) within 3 years of operation."
Published: 2013

36. Measurement of scintillation and ionization yield and scintillation pulse shape from nuclear recoils in liquid argon

Author: Laura Manenti, Hui Wang, L. Grandi, S. Westerdale, F. DeJongh, H. Qian, C. J. Martoff, R. Saldanha, Cristiano Galbiati, P. J. Mosteiro, Ani Aprahamian, S. Pordes, G. Fiorillo, S. Strauss, Stephanie Lyons, D. Montanari, H. O. Back, Y. Guardincerri, H. Cao, C. Love, Y. Meng, J. Yoo, Roza Avetisyan, J. Tatarowicz, D. Olvitt, Wanpeng Tan, K. Siegl, Samuele Sangiorgio, A. G. Cocco, Stuart Derek Walker, C. L. Kendziora, B. Rossi, Alan Watson, T. Alexander, W. H. Lippincott, Cao, H., Alexander, T., Aprahamian, A., Avetisyan, R., Back, H. O., Cocco, A. G., Dejongh, F., Fiorillo, Giuliana, Galbiati, C., Grandi, L., Guardincerri, Y., Kendziora, C., Lippincott, W. H., Love, C., Lyons, S., Manenti, L., Martoff, C. J., Meng, Y., Montanari, D., Mosteiro, P., Olvitt, D., Pordes, S., Qian, H., Rossi, B., Saldanha, R., Sangiorgio, S., Siegl, K., Strauss, S. Y., Tan, W., Tatarowicz, J., Walker, Susan Elizabeth, Wang, H., Watson, A. W., Westerdale, S., and Yoo, J.
Subjects: Physics, Nuclear and High Energy Physics, Scintillation, Time projection chamber, Physics - Instrumentation and Detectors, Nuclear and High Energy Physics liquid argon nuclear recoils, 010308 nuclear & particles physics, Physics::Instrumentation and Detectors, FOS: Physical sciences, Alpha particle, Electron, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Internal conversion, Ionization, 0103 physical sciences, Neutron, Atomic physics, 010306 general physics, Nuclear Experiment, Energy (signal processing)
Abstract: We have measured the scintillation and ionization yield of recoiling nuclei in liquid argon as a function of applied electric field by exposing a dual-phase liquid argon time projection chamber (LAr-TPC) to a low energy pulsed narrow band neutron beam produced at the Notre Dame Institute for Structure and Nuclear Astrophysics. Liquid scintillation counters were arranged to detect and identify neutrons scattered in the TPC and to select the energy of the recoiling nuclei. We report measurements of the scintillation yields for nuclear recoils with energies from 10.3 to 57.3 keV and for median applied electric fields from 0 to 970 V/cm. For the ionization yields, we report measurements from 16.9 to 57.3 keV and for electric fields from 96.4 to 486 V/cm. We also report the observation of an anticorrelation between scintillation and ionization from nuclear recoils, which is similar to the anticorrelation between scintillation and ionization from electron recoils. Assuming that the energy loss partitions into excitons and ion pairs from $^{83m}$Kr internal conversion electrons is comparable to that from $^{207}$Bi conversion electrons, we obtained the numbers of excitons ($N_{ex}$) and ion pairs ($N_i$) and their ratio ($N_{ex}/N_i$) produced by nuclear recoils from 16.9 to 57.3 keV. Motivated by arguments suggesting direction sensitivity in LAr-TPC signals due to columnar recombination, a comparison of the light and charge yield of recoils parallel and perpendicular to the applied electric field is presented for the first time., v2 to reflect published version
Published: 2015

37. First real–time detection of solar pp neutrinos by Borexino

Author: R. Tartaglia, J. Winter, Alessandra Re, W. Maneschg, A. Caminata, An. Ianni, L. Papp, M. D. Skorokhvatov, Michael Wurm, A. E. Chavarria, Denis Korablev, Kai Zuber, Marcin Wójcik, V. N. Muratova, L. Perasso, E. V. Hungerford, Fausto Ortica, R. B. Vogelaar, M. Obolensky, A. V. Derbin, O. Smirnov, A. Sotnikov, B. Lehnert, Matthias Laubenstein, K. Otis, T. Lewke, D. Kryn, P. J. Mosteiro, Michele Montuschi, S. Schönert, C. Ghiano, C. Salvo, S. Davini, Hui Wang, G. Testera, F. Lombardi, Cristiano Galbiati, Anton Empl, A.V. Etenko, Y. Suvorov, A. Razeto, D. Bick, Sandra Zavatarelli, S. Marcocci, E. Litvinovich, Gioacchino Ranucci, Livia Ludhova, D. Bravo, A. M. Goretti, A. S. Chepurnov, N. Rossi, D. Franco, E. Meroni, A. Pocar, R. Saldanha, Al. Ianni, D. Vignaud, S. V. Sukhotin, Marco Giammarchi, F. Gabriele, O. Zaimidoroga, M. Gromov, Lothar Oberauer, G. Zuzel, V. V. Kobychev, S. Manecki, M. Göger-Neff, Jay Burton Benziger, Manuel Meyer, Paolo Lombardi, S. Gazzana, G. Korga, K. Fomenko, G. Lukyanchenko, B. Caccianiga, I. N. Machulin, Aldo Romani, Marco Pallavicini, D. D'Angelo, Q. Meindl, M. Kayser, F. von Feilitzsch, G. Bellini, G. Bonfini, Frank Calaprice, Lino Miramonti, Caren Hagner, P. Cavalcante, M. Misiaszek, Hardy Simgen, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Pallavicini, M., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Calaprice, F., Caminata, A., Cavalcante, P., Chavarria, A., Chepurnov, A., D'Angelo, D., Davini, S., Derbin, A., Empl, A., Etenko, A., Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Hungerford, E., Ianni, Al., Ianni, An., Kayser, M., Kobychev, V., Korablev, D., Korga, G., Kryn, D., Laubenstein, M., Lehnert, B., Lewke, T., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Meindl, Q., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Mosteiro, P., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Saldanha, R., Salvo, C., Schoenert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., Zuzel, G., and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: deuteron, Particle physics, neutrino: solar, Physics::Instrumentation and Detectors, QC1-999, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, scintillation counter: liquid, gap, 7. Clean energy, 01 natural sciences, Nuclear physics, Physics and Astronomy (all), 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], ddc:530, flavor: oscillation, 010306 general physics, Nuclear Experiment, Borexino, Physics, ICARUS, p p: fusion, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, talk: Noto 2014/09/30, Solar neutrino problem, Gran Sasso, Neutrino detector, neutrino: flavor, Measurements of neutrino speed, COUNTING TEST FACILITY, High Energy Physics::Experiment, direct detection, neutrino: oscillation, Neutrino astronomy, Neutrino, experimental results, neutrino: luminosity
Abstract: International audience; Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the keystone pp reaction, in which two protons fuse to make a deuteron, have so far eluded direct detection. The Borexino experiment, an ultra-pure liquid scintillator detector running at the Laboratori Nazionali del Gran Sasso in Italy, has now filled the gap, providing the first direct real time measurement of pp neutrinos and of the solar neutrino luminosity.
Published: 2014

38. The DarkSide Program

Author: Giovanni Covone, Min-Xin Guan, A. V. Derbin, G. Korga, L. Grandi, S. Luitz, B. Reinhold, K. Fomenko, M. Orsini, N. Rossi, Jingke Xu, A. L. Renshaw, G. Testera, Cristiano Galbiati, J. Yoo, Michele Montuschi, S. Catalanotti, I. N. Machulin, D. Korablev, A. G. Cocco, Marco Pallavicini, M. E. Monzani, L. Marini, M. Bossa, D. D'Angelo, G. Bonfini, K. Randle, S. Perasso, M. Cariello, L. Pagani, P. Cavalcante, A. Zec, Nicomede Pelliccia, A. Pocar, Anton Empl, S. Pordes, A. Kurlej, C. J. Martoff, B. Rossi, S. Parmeggiano, O. Smirnov, Paolo Musico, A. Fan, Hui Wang, A. Candela, Stuart Derek Walker, D. Montanari, Alan Watson, Frank Calaprice, X. Xiang, K. Arisaka, R. B. Vogelaar, J. Tatarowicz, G. Fiorillo, F. Di Eusanio, A. Razeto, J. Maricic, E. Segreto, C. L. Kendziora, A. Mandarano, Aldo Romani, Gioacchino Ranucci, Henning O. Back, P. D. Meyers, P. Agnes, F. Budano, R. Tartaglia, M. Wada, M. D'Incecco, M. De Deo, D. Franco, H. Qian, Y. Guardincerri, Marcin Wójcik, A. Devoto, L. Papp, C. Zhu, R. Saldanha, K. Biery, S. D. Rountree, Sandra Zavatarelli, P. X. Li, Paolo Lombardi, W. Sands, A. Tonazzo, Fausto Ortica, B. R. Hackett, G. Koh, F. Gabriele, D. Sablone, An. Ianni, A. K. Alton, A. E. Chavarria, B. Baldin, Chung-Yao Yang, Augusto Brigatti, E. Pantic, Al. Ianni, E. Edkins, Stefano Maria Mari, E. V. Unzhakov, C. Stanford, J. Brodsky, K. Herner, E. Shields, N. Canci, T. Alexander, S. Odrowski, Y. Suvorov, S. Westerdale, G. Zuzel, A. M. Goretti, A. S. Chepurnov, E. V. Hungerford, A. Sotnikov, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Piattelli, P., Rossi, B., Agnes, P., Alexander, T., Alton, A., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Calaprice, F., Canci, N., Candela, A., Cariello, M., Cavalcante, P., Catalanotti, S., Chavarria, A., Chepurnov, A., Cocco, A. G., Covone, G., D'Angelo, D., D'Incecco, M., Deo, M. De, Derbin, A., Devoto, A., Eusanio, F. Di, Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., Kendziora, C., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Lombardi, P., Luitz, S., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Marini, L., Martoff, C. J., Meyers, P. D., Montanari, D., Montuschi, M., Monzani, M. E., Musico, P., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Papp, L., Parmeggiano, S., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A., Romani, A., Rossi, N., Rountree, S. D., Sablone, D., Saldanha, R., Sands, W., Segreto, E., Shields, E., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Watson, A., Westerdale, S., Wojcik, M., Xiang, X., Xu, J., Yang, C. G., Yoo, J., Zavatarelli, S., Zec, A., Zhu, C., and Zuzel, G.
Subjects: Particle physics, Physics::Instrumentation and Detectors, QC1-999, Dark matter, chemistry.chemical_element, Cryogenics, DarkSide, dark matter: direct detection, 01 natural sciences, Nuclear physics, Physics and Astronomy (all), 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment, 010303 astronomy & astrophysics, Physics, Time projection chamber, Argon, 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, time projection chamber: liquid argon, Gran Sasso, chemistry, Liquid argon, Underground laboratory, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], performance, experimental results
Abstract: International audience; DarkSide-50 at Gran Sasso underground laboratory (LNGS), Italy, is a direct dark matter search experiment based on a liquid argon TPC. DS-50 has completed its first dark matter run using atmospheric argon as target. The detector performances and the results of the first physics run are presented in this proceeding.
Published: 2014

39. Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

Author: A. V. Derbin, Al. Ianni, A. Empl, M. Obolensky, Matthias Laubenstein, M. Göger-Neff, Hui Wang, M. D. Skorokhvatov, G. Bonfini, An. Ianni, Michael Wurm, Frank Calaprice, J. Winter, S. Manecki, Hardy Simgen, P. J. Mosteiro, D. Franco, Marcin Wójcik, Michele Montuschi, Gioacchino Ranucci, I. N. Machulin, T. Lewke, D. Kryn, A. E. Chavarria, E. Meroni, D. Bick, Sandra Zavatarelli, Jay Burton Benziger, L. Perasso, G. Bellini, Cristiano Galbiati, C. Ghiano, R. Saldanha, Marco Pallavicini, D. D'Angelo, Aldo Romani, Caren Hagner, O. Smirnov, Q. Meindl, Manuel Meyer, P. Cavalcante, E. Litvinovich, A.V. Etenko, N. Rossi, M. Misiaszek, Marco Giammarchi, K. Otis, Paolo Lombardi, D. Bravo, M. Gromov, S. Gazzana, G. Zuzel, G. Lukyanchenko, S. V. Sukhotin, K. Fomenko, G. Testera, R. Tartaglia, E. V. Hungerford, A. Wright, O. Zaimidoroga, V. N. Muratova, Lino Miramonti, S. Marcocci, Lothar Oberauer, V. V. Kobychev, A. Sotnikov, Denis Korablev, B. Lehnert, G. Korga, A. Pocar, F. Gabriele, D. Vignaud, B. Caccianiga, W. Maneschg, C. Salvo, F. von Feilitzsch, S. Schönert, S. Davini, Laura Cadonati, L. Papp, Y. Suvorov, Livia Ludhova, Kai Zuber, A. M. Goretti, A. S. Chepurnov, Fausto Ortica, F. Lombardi, A. Razeto, A. Caminata, Alessandra Re, R. B. Vogelaar, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Mosteiro, P., Bellini, G., Benziger, J., Bick, D., Bonfini, G., Bravo, D., Caccianiga, B., Cadonati, L., Calaprice, F., Caminata, A., Cavalcante, P., Chavarria, A., Chepurnov, A., D'Angelo, D., Davini, S., Derbin, A., Empl, A., Etenko, A., Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Gazzana, S., Ghiano, C., Giammarchi, M., Goeger-Neff, M., Goretti, A., Gromov, M., Hagner, C., Hungerford, E., Ianni, Al., Ianni, An., Kobychev, V., Korablev, D., Korga, G., Kryn, D., Laubenstein, M., Lehnert, B., Lewke, T., Litvinovich, E., Lombardi, F., Lombardi, P., Ludhova, L., Lukyanchenko, G., Machulin, I., Manecki, S., Maneschg, W., Marcocci, S., Meindl, Q., Meroni, E., Meyer, M., Miramonti, L., Misiaszek, M., Montuschi, M., Muratova, V., Oberauer, L., Obolensky, M., Ortica, F., Otis, K., Pallavicini, M., Papp, L., Perasso, L., Pocar, A., Ranucci, G., Razeto, A., Re, A., Romani, A., Rossi, N., Saldanha, R., Salvo, C., Schoenert, S., Simgen, H., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Sukhotin, S., Suvorov, Y., Tartaglia, R., Testera, G., Vignaud, D., Vogelaar, R. B., von Feilitzsch, F., Wang, H., Winter, J., Wojcik, M., Wright, A., Wurm, M., Zaimidoroga, O., Zavatarelli, S., Zuber, K., and Zuzel, G.
Subjects: Nuclear reaction, Physics - Instrumentation and Detectors, Proton, neutrino: solar, Physics::Instrumentation and Detectors, 01 natural sciences, 7. Clean energy, nuclear reaction, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Positron, star, Primary (astronomy), [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Nuclear Experiment (nucl-ex), [ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear Experiment, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Borexino, Physics, SPECTROSCOPY, Instrumentation and Detectors (physics.ins-det), SOLAR NEUTRINOS, Astrophysics - Solar and Stellar Astrophysics, Neutrino, model: solar, deuteron, GRAN SASSO, Particle physics, Nuclear and High Energy Physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], talk: Conca Specchiulla 2014/09/07, [ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex], 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Neutrino oscillation, DETECTOR, Solar and Stellar Astrophysics (astro-ph.SR), neutrino: model, p p: fusion, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Deuterium, 13. Climate action, spectral, High Energy Physics::Experiment, neutrino: oscillation, experimental results
Abstract: The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as well as further validation of the LMA-MSW model of neutrino oscillations., Comment: Proceedings from NOW (Neutrino Oscillation Workshop) 2014
Published: 2014

40. A first walk on the DarkSide

Author: K. Arisaka, Hui Wang, G. Fiorillo, Thomas Alexander, C. J. Martoff, G. Bonfini, Frank Calaprice, M. D'Incecco, X. Xiang, H. Qian, M. Orsini, W. Sands, D. Franco, E. Shields, Y. Suvorov, S. Westerdale, L. Marini, M. Bossa, A. M. Goretti, A. S. Chepurnov, E. Pantic, B. Rossi, P. D. Meyers, G. Korga, N. Rossi, E. Segreto, Nicomede Pelliccia, Al. Ianni, E. Edkins, E. V. Hungerford, A. Candela, A. Mandarano, M. Wada, Alan Watson, Jingke Xu, Cristiano Galbiati, R. B. Vogelaar, L. Papp, S. Odrowski, Stefano Maria Mari, Anton Empl, Y. Guardincerri, S. Parmeggiano, G. Testera, Fausto Ortica, M. Cariello, B. R. Hackett, M. M. Wojcik, S. Luitz, A. L. Renshaw, G. Koh, A. Sotnikov, J. Yoo, A. Zec, K. Randle, D. Sablone, S. Pordes, C. Stanford, Denis Korablev, Henning O. Back, J. Brodsky, An. Ianni, I. N. Machulin, M. E. Monzani, K. Fomenko, F. Budano, A. Pocar, B. Baldin, A. Devoto, R. Saldanha, Min-Xin Guan, O. Smirnov, D. D'Angelo, Sandra Zavatarelli, P. X. Li, S. Davini, S. D. Rountree, Michele Montuschi, B. Reinhold, E. V. Unzhakov, Paolo Lombardi, J. Tatarowicz, A. E. Chavarria, J. Maricic, M. De Deo, K. Herner, N. Canci, A. Kurlej, G. Zuzel, Gioacchino Ranucci, F. Gabriele, K. Biery, A. Tonazzo, Stuart Derek Walker, C. L. Kendziora, D. Montanari, F. Di Eusanio, Aldo Romani, P. Agnes, Paolo Musico, A. Fan, A. Razeto, A. G. Cocco, A. K. Alton, Chung-Yao Yang, A. V. Derbin, Augusto Brigatti, C. Zhu, L. Grandi, L. Pagani, P. Cavalcante, S. Perasso, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Davini, S, Agnes, P., Alexander, T., Alton, A., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Calaprice, F., Canci, N., Candela, A., Cariello, M., Cavalcante, P., Chavarria, A., Chepurnov, A., Cocco, A. G., D'Angelo, D., D'Incecco, M., De Deo, M., Derbin, A., Devoto, A., Di Eusanio, F., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., Kendziora, C., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Lombardi, P., Luitz, S., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Marini, L., Martoff, C. J., Meyers, P. D., Montanari, D., Montuschi, M., Monzani, M. E., Musico, P., Odrowski, S., Orsini, M., Ortica, F., Pagani, L., Pantic, E., Papp, L., Parmeggiano, S., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saldanha, R., Sands, W., Segreto, E., Shields, E., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, S., Wang, H., Watson, A., Westerdale, S., Wojcik, M., Xiang, X., Xu, J., Yang, C. G., Yoo, J., Zavatarelli, S., Zec, A., Zhu, C., Zuzel, G., and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: Particle physics, Nuclear and High Energy Physics, Large Underground Xenon experiment, detector: performance, scintillation detectors, Dark matter, talk: Valencia 2014/07/02, chemistry.chemical_element, DarkSide, Scintillation detectors, 01 natural sciences, dark matter, argon: target, Nuclear physics, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Physics, Argon, Time projection chamber, 010308 nuclear & particles physics, Detector, liquid argon, time projection chamber, Gran Sasso, Scintillation detector, chemistry, atmosphere, Cryogenic Dark Matter Search, Dark Matter Time Projection Chamber, experimental results
Abstract: International audience; DarkSide-50 (DS-50) at Gran Sasso underground laboratory (LNGS), Italy, is a direct dark matter search experiment based on a TPC with liquid argon. DS-50 has completed its first dark matter run using atmospheric argon as target. The DS-50 detector performances and the results of the first physics run are reviewed in this proceeding.
Published: 2014

41. New limits on heavy sterile neutrino mixing inB8decay obtained with the Borexino detector

Author: A. M. Goretti, Aldo Ianni, Anton Empl, R. Tartaglia, S. V. Sukhotin, A. Wright, O. Zaimidoroga, A.V. Etenko, Jingke Xu, S. Schönert, Cristiano Galbiati, D. Bravo, V. V. Kobychev, E. V. Hungerford, C. Ghiano, Caren Hagner, P. Cavalcante, I. S. Drachnev, M. Misiaszek, W. Maneschg, P. J. Mosteiro, A. Sotnikov, Gioacchino Ranucci, Laura Cadonati, L. Papp, G. Bellini, D. Franco, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Lothar Oberauer, Paolo Lombardi, Fausto Ortica, Matthias Laubenstein, B. Caccianiga, Andrea Ianni, D. Bick, Sandra Zavatarelli, Y. Suvorov, T. Lewke, D. Kryn, A. V. Derbin, F. Lombardi, Ben Loer, M. Obolensky, Q. Meindl, A. Razeto, G. Lukyanchenko, A. E. Chavarria, L. Perasso, S. Manecki, E. Meroni, M. Buizza Avanzini, V. N. Muratova, S. Gazzana, Lino Miramonti, S. Davini, G. Zuzel, E. Litvinovich, C. Salvo, G. Korga, K. Fomenko, D. Vignaud, N. Rossi, G. Manuzio, G. Bonfini, F. von Feilitzsch, Frank Calaprice, Hardy Simgen, R. Saldanha, J. Winter, M. Göger-Neff, Marco Giammarchi, A. Pocar, O. Smirnov, K. Otis, S. Perasso, M. M. Wojcik, Aldo Romani, Jay Burton Benziger, I. N. Machulin, Livia Ludhova, A. S. Chepurnov, Marco Pallavicini, D. D'Angelo, Denis Korablev, G. Testera, Alessandra Re, and R. B. Vogelaar
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Sterile neutrino, 010308 nuclear & particles physics, 7. Clean energy, 01 natural sciences, Side branch, 0103 physical sciences, High Energy Physics::Experiment, Heavy neutrino, Neutrino, 010306 general physics, Mixing (physics), Borexino
Abstract: If heavy neutrinos with mass ${m}_{{\ensuremath{\nu}}_{H}}\ensuremath{\ge}2{m}_{e}$ are produced in the Sun via the decay $^{8}\mathrm{B}\ensuremath{\rightarrow}^{8}\mathrm{Be}+{e}^{+}+{\ensuremath{\nu}}_{H}$ in a side branch of the $pp$ chain, they would undergo the observable decay into an electron, a positron and a light neutrino ${\ensuremath{\nu}}_{H}\ensuremath{\rightarrow}{\ensuremath{\nu}}_{L}+{e}^{+}+{e}^{\ensuremath{-}}$. In the present work Borexino data are used to set a bound on the existence of such decays. We constrain the mixing of a heavy neutrino with mass $1.5\text{ }\text{ }\mathrm{MeV}\ensuremath{\le}{m}_{{\ensuremath{\nu}}_{H}}\ensuremath{\le}14\text{ }\text{ }\mathrm{MeV}$ to be $|{U}_{eH}{|}^{2}\ensuremath{\le}({10}^{\ensuremath{-}3}\ensuremath{-}4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}6})$, respectively. These are tighter limits on the mixing parameters than obtained in previous experiments at nuclear reactors and accelerators.
Published: 2013

42. Cosmogenic Backgrounds in Borexino at 3800 m water-equivalent depth

Author: L. Oberauer, V. N. Muratova, A. E. Chavarria, L. Perasso, A.V. Etenko, D. Bravo, C. Salvo, O. Zaimidoroga, Michael Wurm, L. Grandi, M. Göger-Neff, R. Möllenberg, S. Perasso, R. Tartaglia, S. V. Sukhotin, Laura Cadonati, G. Korga, Andrea Ianni, A. Wright, Jilei Xu, Y. Suvorov, D. Franco, G. Zuzel, Livia Ludhova, G. Testera, Fausto Ortica, A. M. Goretti, V. V. Kobychev, A. S. Chepurnov, A. V. Derbin, K. Otis, I. Machulin, A. Sotnikov, Aldo Ianni, Gioacchino Ranucci, A. Empl, Stefan Schönert, G. Bonfini, P. Cavalcante, S. Davini, Q. Meindl, C. Ghiano, M. Obolensky, W. Maneschg, G. Lukyanchenko, R. Saldanha, P. J. Mosteiro, E. Litvinovich, S. Manecki, G. Bellini, K. Fomenko, F. von Feilitzsch, B. Caccianiga, D. Bick, Sandra Zavatarelli, Marco Giammarchi, J. Winter, Aldo Romani, L. Papp, F. Calaprice, Lino Miramonti, S. Gazzana, Cristiano Galbiati, Oleg Smirnov, N. Rossi, A. Pocar, Caren Hagner, D. Vignaud, Marco Pallavicini, D. D'Angelo, D. Korablev, T. Lewke, E. Hungerford, M. Misiaszek, M. Skorokhvatov, Marcin Wójcik, M. Buizza Avanzini, R. B. Vogelaar, Hardy Simgen, Paolo Lombardi, Alessandra Re, Matthias Laubenstein, A. Razeto, G. Manuzio, D. Kryn, B. Loer, J. Benziger, F. Lombardi, E. Meroni, Physics Department, Amherst U., University of Massachusetts System (UMASS), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratori Nazionali del Gran Sasso (LNGS), Istituto Nazionale di Fisica Nucleare (INFN), Laboratoire Kastler Brossel (LKB (Jussieu)), Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Dept. Microelectronics and Nanoscience, Chalmers University of Technology [Göteborg], departement de physique, Albert-Ludwigs-Universität Freiburg, Dip. di Fisica dell'Università di Genova - Italy, Università degli studi di Torino (UNITO), Departamento de Engenharia Elétrica [Minas Gerais] (DEE - UFMG), Universidade Federal de Minas Gerais, Rhodes University, Grahamstown, Laboratoire de Spectroscopie Hertzienne de l'ENS (LSH-ENS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Institute of Physics, Polish Academy of Sciences, Polska Akademia Nauk = Polish Academy of Sciences (PAN), International Iberian Nanotechnology Laboratory (INL), Bellini, G., Suvorov, Y., Et, Al., Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Genova = University of Genoa (UniGe), and Università degli studi di Torino = University of Turin (UNITO)
Subjects: Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Solar neutrino, Monte Carlo method, dark matter experiment, cosmic ray experiment, FOS: Physical sciences, Scintillator, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), neutrino experiments, 0103 physical sciences, Neutron, 010306 general physics, Borexino, ComputingMilieux_MISCELLANEOUS, Physics, [PHYS]Physics [physics], Muon, 010308 nuclear & particles physics, dark matter experiments, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Neutron capture, Neutrino detector, neutrino experiment, High Energy Physics::Experiment, cosmic ray experiments, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The solar neutrino experiment Borexino, which is located in the Gran Sasso underground laboratories, is in a unique position to study muon-induced backgrounds in an organic liquid scintillator. In this study, a large sample of cosmic muons is identified and tracked by a muon veto detector external to the liquid scintillator, and by the specific light patterns observed when muons cross the scintillator volume. The yield of muon-induced neutrons is found to be Yn =(3.10+-0.11)10-4 n/({\mu} (g/cm2)). The distance profile between the parent muon track and the neutron capture point has the average value {\lambda} = (81.5 +- 2.7)cm. Additionally the yields of a number of cosmogenic radioisotopes are measured for 12N, 12B, 8He, 9C, 9Li, 8B, 6He, 8Li, 11Be, 10C and 11C. All results are compared with Monte Carlo simulation predictions using the Fluka and Geant4 packages. General agreement between data and simulation is observed for the cosmogenic production yields with a few exceptions, the most prominent case being 11C yield for which both codes return about 50% lower values. The predicted {\mu}-n distance profile and the neutron multiplicity distribution are found to be overall consistent with data., Comment: 26 pages, 13 figures (in 14 files), 4 tables. 3 extra data files. accepted by JCAP
Published: 2013

43. Lifetime measurements of 214Po and 212Po with the CTF liquid scintillator detector at LNGS

Author: R. B. Vogelaar, Alessandra Re, Matthias Laubenstein, C. Carraro, P. Cavalcante, W. Maneschg, A. Razeto, G. Manuzio, J. Benziger, Michael Wurm, L. Grandi, A. Pocar, V. Chubakov, M. Skorokhvatov, F. Lombardi, D. Korablev, D. Bick, Sandra Zavatarelli, F. von Feilitzsch, Fabio Mantovani, S. Perasso, S. Davini, S. Nisi, G. Zuzel, L. Oberauer, R. Saldanha, S. Manecki, M. Buizza Avanzini, V. N. Muratova, A. E. Chavarria, G. Testera, Hardy Simgen, L. Perasso, A. Sotnikov, Aldo Ianni, Marco Giammarchi, Y. Suvorov, Q. Meindl, A.V. Etenko, Gioacchino Ranucci, D. Kryn, D. Franco, D. Bravo, Aldo Romani, L. Papp, Laura Cadonati, E. Meroni, N. Rossi, Fausto Ortica, I. Machulin, Marco Pallavicini, D. D'Angelo, C. Salvo, O. Zaimidoroga, B. Loer, Yusuke Koshio, Andrea Ianni, M. Obolensky, A. V. Derbin, M. M. Wojcik, Cristiano Galbiati, Oleg Smirnov, G. Bellini, Paolo Lombardi, M. Göger-Neff, E. Guardincerri, S. V. Sukhotin, A. Wright, D. Montanari, V. V. Kobychev, Stefan Schönert, Livia Ludhova, A. A. Sabelnikov, A. M. Goretti, A. S. Chepurnov, S. Hardy, Marcello Lissia, C. Ghiano, Jilei Xu, K. Otis, P. J. Mosteiro, G. Bonfini, Lino Miramonti, T. Lewke, R. Tartaglia, G. Korga, E. Litvinovich, K. Fomenko, S. Gazzana, B. Caccianiga, F. Calaprice, J. Winter, Gerti Xhixha, M. Misiaszek, Borexino Collaboration, Physics Department, University of Massachusetts System (UMASS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratori Nazionali del Gran Sasso (LNGS), Istituto Nazionale di Fisica Nucleare (INFN), Dept. Microelectronics and Nanoscience, Chalmers University of Technology [Göteborg], Paul Scherrer Institute (PSI), Rhodes University, Grahamstown, Laboratoire de Spectroscopie Hertzienne de l'ENS (LSH-ENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), International Iberian Nanotechnology Laboratory (INL), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Bellini, G., Suvorov, Y., and Et, Al.
Subjects: Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Nuclear Theory, Hadron, FOS: Physical sciences, Scintillator, 01 natural sciences, Coincidence, Nuclear Theory (nucl-th), Nuclear physics, High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, Nuclear fusion, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Nuclear theory, ComputingMilieux_MISCELLANEOUS, Physics, [PHYS]Physics [physics], Test facility, 010308 nuclear & particles physics, Detector, Instrumentation and Detectors (physics.ins-det), High Energy Physics - Phenomenology, National laboratory, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: We have studied the alpha decays of 214Po into 210Pb and of 212Po into 208Pb tagged by the coincidence with the preceding beta decays from 214Bi and 212Bi, respectively. The employed 222Rn, 232Th, and 220Rn sources were sealed inside quartz vials and inserted in the Counting Test Facility at the underground Gran Sasso National Laboratory in Italy. We find that the mean lifetime of 214Po is (236.00 +- 0.42(stat) +- 0.15(syst)) \mu s and that of 212Po is (425.1 +- 0.9(stat) +- 1.2(syst)) ns. Our results, obtained from data with signal-to-background ratio larger than 1000, reduce the overall uncertainties and are compatible with previous measurements., Comment: RevTex, 11 pages, 5 figures, 3 tables. This second version matches the one accepted for publication in EPJA: minor stylistic changes plus a discussion of calibration of TDC time scale
Published: 2013

44. SOX : short distance neutrino Oscillations with BoreXino

Author: E. Litvinovich, M. D. Skorokhvatov, Michael Wurm, N. Rossi, G. Lukyanchenko, R. Saldanha, Gioacchino Ranucci, M. Göger-Neff, D. A. Semenov, Lino Miramonti, A. Pocar, D. Korablev, Livia Ludhova, R. Tartaglia, Y. Suvorov, A. M. Goretti, A. S. Chepurnov, G. Bonfini, O. Smirnov, E. Pantic, K. Otis, C. Ghiano, P. J. Mosteiro, Frank Calaprice, Caren Hagner, D. Kryn, Jonathan M. Link, D. Krasnicky, E. V. Unzhakov, F. Lombardi, K. Fomenko, W. Maneschg, Hardy Simgen, L. Papp, P. Cavalcante, Andrea Ianni, D. Bick, Sandra Zavatarelli, Lothar Oberauer, Matthias Laubenstein, I. N. Machulin, M. Misiaszek, Fausto Ortica, S. Manecki, Marco Pallavicini, D. D'Angelo, E. Meroni, E. V. Hungerford, Marcin Wójcik, G. Fernandes, A. Sotnikov, G. Bellini, G. Korga, B. Caccianiga, S. Schönert, A. Razeto, G. Zuzel, R. B. Vogelaar, Alessandra Re, A. Caminata, Aldo Ianni, D. Franco, V. N. Muratova, A. E. Chavarria, C. Salvo, A.V. Etenko, D. Bravo, Aldo Romani, Michael Meyer, S. Davini, S. Perasso, G. Testera, Cristiano Galbiati, A. V. Derbin, Paolo Lombardi, M. Obolensky, S. V. Sukhotin, O. Zaimidoroga, H. Wang, V. V. Kobychev, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratori Nazionali del Gran Sasso (LNGS), Istituto Nazionale di Fisica Nucleare (INFN), Dept. Microelectronics and Nanoscience, Chalmers University of Technology [Göteborg], Paul Scherrer Institute (PSI), Physik-Department E15, Technische Universität Munchen - Université Technique de Munich [Munich, Allemagne] (TUM), Dip. di Fisica dell'Università di Genova - Italy, Università degli studi di Torino (UNITO), Departamento de Engenharia Elétrica [Minas Gerais] (DEE - UFMG), Universidade Federal de Minas Gerais, Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Department of Physics-Electronics, Rhodes University, Grahamstown, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), EAST CHINA UNIVERSITY, KEY LAB, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Genova = University of Genoa (UniGe), and Università degli studi di Torino = University of Turin (UNITO)
Subjects: Nuclear and High Energy Physics, Sterile neutrino, Particle physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, ddc:530, 010306 general physics, Neutrino oscillation, ComputingMilieux_MISCELLANEOUS, Borexino, [PHYS]Physics [physics], Physics, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, exotics, neutrino detectors and telescopes, Instrumentation and Detectors (physics.ins-det), Solar neutrino problem, oscillation, Neutrino detector, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The very low radioactive background of the Borexino detector, its large size, and the well proved capability to detect both low energy neutrino and anti-neutrino make an ideal case for the study of short distance neutrino oscillations with artificial sources at Gran Sasso. This paper describes the possible layouts of 51Cr neutrino and 144Ce-144Pr anti-neutrino source experiments in Borexino and shows the expected sensitivity for three possible different phases of the experiment., Comment: 11 pages, 5 figures
Published: 2013

45. Measurement of CNGS muon neutrino speed with Borexino

Author: Y. Suvorov, R. Saldanha, S. V. Sukhotin, T. Lewke, S. Hardy, D. Kryn, Matthias Laubenstein, A. Wright, D. Missiaen, O. Zaimidoroga, G. Korga, M. M. Wojcik, Aldo Romani, Marco Giammarchi, V. V. Kobychev, S. Schoenert, Matthew Jones, B. Caccianiga, G. Cerretto, E. Meroni, C. Ghiano, S. Gazzana, E. Litvinovich, N. Rossi, I. N. Machulin, P. Spinnato, C. I. De Gaetani, Marco Pallavicini, D. D'Angelo, P. Cavalcante, V. Pettiti, Alessandra Re, B. Loer, M. Goeger-Neff, M. Misiaszek, P. J. Mosteiro, Paolo Lombardi, Aldo Ianni, M. Obolensky, Yusuke Koshio, S. Manecki, Lothar Oberauer, G. Zuzel, D. Franco, R. S. Raghavan, G. Manuzio, R. B. Vogelaar, M. G. Visconti, B. Betti, Jay Burton Benziger, M. Buizza Avanzini, A. Sotnikov, F. Lombardi, Riccardo Barzaghi, A. Razeto, O. Smirnov, D. Passoni, K. Otis, C. Plantard, K. Fomenko, F. von Feilitzsch, Laura Cadonati, L. Papp, Fausto Ortica, A. Pocar, S. Perasso, S. Davini, C. Carraro, Andrea Ianni, D. Bick, Sandra Zavatarelli, G. Testera, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Q. Meindl, Denis Korablev, G. Bonfini, Hardy Simgen, P. Alvarez Sanchez, R. Tartaglia, Lino Miramonti, W. Maneschg, J. Serrano, A. Kayunov, E. Guardincerri, A. V. Derbin, Ludovico Biagi, Livia Ludhova, D. Vignaud, H. Esteban, A. M. Goretti, Jingke Xu, Cristiano Galbiati, A. A. Sabelnikov, D. Montanari, G. Bellini, A.V. Etenko, J. Winter, D. Bravo, Gioacchino Ranucci, Livio Pinto, V. N. Muratova, A. E. Chavarria, L. Perasso, C. Salvo, AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Borexino, Alvarez Sanchez, P., Suvorov, Y., Et, Al., Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Particle physics, Special relativity, Nuclear and High Energy Physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Neutrino beam, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Muon neutrino, Nuclear Experiment, 010306 general physics, Neutrino oscillation, neutrino speed, Borexino, Physics, Muon, GPS time-link, special relativity, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Neutrino detector, neutrino beams, Measurements of neutrino speed, Physics::Accelerator Physics, Neutrino speed, High Energy Physics::Experiment, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Particle Physics - Experiment
Abstract: We have measured the speed of muon neutrinos with the Borexino detector using short-bunch CNGS beams. The final result for the difference in time-of-flight between a =17 GeV muon neutrino and a particle moving at the speed of light in vacuum is {\delta}t = 0.8 \pm 0.7stat \pm 2.9sys ns, well consistent with zero., Comment: 6 pages, 5 figures
Published: 2012

46. Search for solar axions produced in thep(d,He3)Areaction with Borexino detector

Author: D. Vignaud, M. D. Skorokhvatov, Michael Wurm, L. Grandi, Y. Suvorov, Livia Ludhova, A. M. Goretti, R. B. Vogelaar, Q. Meindl, Matthias Laubenstein, O. Smirnov, A. Kobychev, Denis Korablev, I. N. Machulin, Aldo Ianni, Alessandra Re, K. Otis, L. Lewke, G. Bonfini, G. Korga, K. Fomenko, M. Buizza Avanzini, Marco Pallavicini, D. D'Angelo, Frank Calaprice, R. Tartaglia, G. Bellini, Jingke Xu, Hardy Simgen, P. A. Romani, S. Hardy, E. Meroni, Cristiano Galbiati, S. Manecki, C. Carraro, W. Maneschg, M. Obolensky, J. Winter, S. Davini, G. Testera, D. Kryn, Lino Miramonti, S. Gazzana, A. Pocar, F. von Feilitzsch, R. S. Raghavan, G. Manuzio, Lothar Oberauer, B. Caccianiga, M. Goeger-Neff, M. M. Wojcik, C. Ghiano, E. Litvinovich, A. A. Sabelnikov, Laura Cadonati, L. Papp, Jay Burton Benziger, A. V. Derbin, P. Cavalcante, D. Franco, Fausto Ortica, M. Misiaszek, A. Kayunov, E. Guardincerri, S. Perasso, B. Loer, Paolo Lombardi, S. V. Sukhotin, G. Zuzel, Yusuke Koshio, A. Wright, O. Zaimidoroga, Gioacchino Ranucci, A. Sotnikov, F. Lombardi, A. Razeto, V. N. Muratova, C. Salvo, D. Montanari, A.V. Etenko, D. Bravo, P. J. Mosteiro, A. E. Chavarria, L. Perasso, R. Saldanha, S. Schönert, Marco Giammarchi, Andrea Ianni, D. Bick, and Sandra Zavatarelli
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Isovector, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Inverse, 7. Clean energy, 01 natural sciences, 0103 physical sciences, Nuclear Experiment, 010306 general physics, Axion, Borexino
Abstract: A search for 5.5 MeV solar axions produced in the $p+d\ensuremath{\rightarrow}^{3}\mathrm{He}+\mathrm{A}$ (5.5 MeV) reaction was performed using the Borexino detector. The Compton conversion of axions to photons, $\mathrm{A}+e\ensuremath{\rightarrow}e+\ensuremath{\gamma}$; the axioelectric effect, $\mathrm{A}+e+Z\ensuremath{\rightarrow}e+Z$; the decay of axions into two photons, $\mathrm{A}\ensuremath{\rightarrow}2\ensuremath{\gamma}$; and inverse Primakoff conversion on nuclei, $\mathrm{A}+Z\ensuremath{\rightarrow}\ensuremath{\gamma}+Z$, are considered. Model-independent limits on axion-electron (${g}_{Ae}$), axion-photon (${g}_{A\ensuremath{\gamma}}$), and isovector axion-nucleon (${g}_{3AN}$) couplings are obtained: $|{g}_{Ae}\ifmmode\times\else\texttimes\fi{}{g}_{3AN}|\ensuremath{\le}5.5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}13}$ and $|{g}_{A\ensuremath{\gamma}}\ifmmode\times\else\texttimes\fi{}{g}_{3AN}|\ensuremath{\le}4.6\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}11}\text{ }\text{ }{\mathrm{GeV}}^{\ensuremath{-}1}$ at ${m}_{A}l1\text{ }\text{ }\mathrm{MeV}$ (90% confidence level). These limits are 2--4 orders of magnitude stronger than those obtained in previous laboratory-based experiments using nuclear reactors and accelerators.
Published: 2012

47. Cosmic-muon flux and annual modulation in Borexino at 3800 m water-equivalent depth

Author: Jilei Xu, R. Tartaglia, K. Otis, D. Vignaud, G. Testera, C. Carraro, A. Sotnikov, Aldo Ianni, Caren Hagner, G. Zuzel, P. J. Mosteiro, T. Lewke, L. Oberauer, J. Benziger, V. N. Muratova, P. Cavalcante, A. Razeto, A. E. Chavarria, G. Manuzio, S. Manecki, W. Maneschg, L. Perasso, Gioacchino Ranucci, C. Ghiano, F. Lombardi, S. Davini, M. Misiaszek, Cristiano Galbiati, Y. Suvorov, A. Pocar, Michael Wurm, L. Grandi, B. Loer, M. Skorokhvatov, Yusuke Koshio, H. Simgen, Oleg Smirnov, D. Korablev, D. Kryn, C. Salvo, Matthias Laubenstein, G. Bonfini, M. Buizza Avanzini, E. Litvinovich, K. Fomenko, E. Guardincerri, F. von Feilitzsch, J. Winter, R. Saldanha, D. Montanari, R. S. Raghavan, Paolo Lombardi, B. Caccianiga, S. Gazzana, O. Zaimidoroga, A.V. Etenko, S. Hardy, S. V. Sukhotin, F. Calaprice, Laura Cadonati, Marco Giammarchi, D. Bravo, R. B. Vogelaar, Lino Miramonti, A. Wright, M. Goeger-Neff, E. Meroni, Alessandra Re, Fausto Ortica, I. Machulin, Stefan Schönert, D. Franco, G. Bellini, M. Obolensky, Livia Ludhova, A. A. Sabelnikov, A. M. Goretti, A. S. Chepurnov, Andrea Ianni, D. Bick, A. V. Derbin, Sandra Zavatarelli, M. M. Wojcik, S. Perasso, Q. Meindl, Aldo Romani, L. Papp, Marco Pallavicini, D. D'Angelo, G. Korga, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Borexino, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Bellini, G., Suvorov, Y., and Et, Al.
Subjects: Particle physics, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], FOS: Physical sciences, Water equivalent, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Relative amplitude, Borexino, Physics, [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph], COSMIC cancer database, Muon, 010308 nuclear & particles physics, Astronomy and Astrophysics, Atmospheric temperature, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Physics - Atmospheric and Oceanic Physics, neutrino detector, 13. Climate action, Modulation, Atmospheric and Oceanic Physics (physics.ao-ph), Muon flux, neutrino experiment, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We have measured the muon flux at the underground Gran Sasso National Laboratory (3800 m w.e.) to be (3.41 \pm 0.01) \times 10-4m-2s-1 using four years of Borexino data. A modulation of this signal is observed with a period of (366\pm3) days and a relative amplitude of (1.29 \pm 0.07)%. The measured phase is (179 \pm 6) days, corresponding to a maximum on the 28th of June. Using the most complete atmospheric data models available, muon rate fluctuations are shown to be positively correlated with atmospheric temperature, with an effective coefficient {\alpha}T = 0.93 \pm 0.04. This result represents the most precise study of the muon flux modulation for this site and is in good agreement with expectations., Comment: 14 pages, 8 figures, published on JCAP as JCAP05(2012)015 on May 15th 2012
Published: 2012

48. Absence of a day-night asymmetry in the7Be solar neutrino rate in Borexino

Author: A. Etenkog, W. Maneschg, Cristiano Galbiati, Lothar Oberauer, R. Saldanha, G. Testera, Marco Giammarchi, Laura Cadonati, Andrea Ianni, D. Bick, Sandra Zavatarelli, L. Papp, Matthias Laubenstein, A. Sotnikov, D. Vignaud, M. D. Skorokhvatov, A. Pocar, Michael Wurm, L. Grandi, J. Winter, S. Hardy, D. Franco, M. Göger-Neff, T. Lewke, D. Kryn, B. Caccianiga, Livia Ludhova, R. B. Vogelaar, A. M. Goretti, Fausto Ortica, S. Davinic, Q. Meindl, Y. Suvorov, C. Carraro, A. Derbinm, E. Meroni, Stefano Bonetti, Denis Korablev, Marcin Wójcik, E. Litvinovich, S. Gazzana, F. Lombardi, S. Schoenert, C. Salvo, Jilei Xu, O. Smirnov, Alessandra Re, A. Razeto, F. von Feilitzsch, G. Bellini, I. N. Machulin, Marco Pallavicini, S. Manecki, Jay Burton Benziger, Aldo Ianni, D. D'Angelo, Aldo Romani, A. E. Chavarria, L. Perasso, G. Zuzel, Carlos Pena-Garay, R. S. Raghavan, Lino Miramonti, S. Perasso, G. Manuzio, B. Loer, Yusuke Koshio, G. Korga, K. Fomenko, G. Bonfini, M. Buizza Avanzini, Frank Calaprice, Hardy Simgen, P. J. Mosteiro, C. Ghiano, P. Cavalcante, M. Misiaszek, V. N. Muratova, D. Montanari, Gioacchino Ranucci, E. Guardincerri, A. A. Sabelnikov, M. Obolensky, Paolo Lombardi, S. V. Sukhotin, A. Wright, O. Zaimidoroga, V. V. Kobychev, R. Tartaglia, Bellini, G., Suvorov, Y., and Et, Al.
Subjects: Particle physics, Nuclear and High Energy Physics, Neutrino oscillation, Physics::Instrumentation and Detectors, media_common.quotation_subject, Solar neutrino, 01 natural sciences, Asymmetry, Nuclear physics, Day-night effect, 0103 physical sciences, 010306 general physics, Nuclear Experiment, day–night effect, Borexino, media_common, Physics, neutrino oscillations, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Física, Solar neutrino problem, Neutrino detector, solar neutrinos, Measurements of neutrino speed, High Energy Physics::Experiment, Neutrino, CPT violation
Abstract: We report on a search for the day-night asymmetry of the Be-7 solar neutrino rate measured by Borexino at the Laboratori Nazionali del Gran Sasso (LNGS), Italy. The measured value, Adn=0.001 +- 0.012 (stat) +- 0.007 (syst), shows the absence of a significant asymmetry. This result alone rejects the so-called LOW solution at more than 8.5 sigma. Combined with the other solar neutrino data, it isolates the Large Mixing Angle (LMA) -- MSW solution at DeltaChi2 > 190 without relying on the assumption of CPT symmetry in the neutrino sector. We also show that including the day-night asymmetry, data from Borexino alone restricts the MSW neutrino oscillations to the LMA solution at 90% confidence level.
Published: 2012

49. First evidence of pep solar neutrinos by direct detection in Borexino

Author: A.V. Etenko, A. Pocar, D. Bravo, R. Tartaglia, Livia Ludhova, Denis Korablev, A. S. Chepurnov, A. Razeto, S. Davini, S. Schönert, Marcin Wójcik, G. Manuzio, B. Loer, R. S. Raghavan, C. Ghiano, G. Zuzel, R. B. Vogelaar, M. Obolensky, R. Saldanha, Yusuke Koshio, M. Goeger-Neff, K. Otis, Y. Suvorov, D. Montanari, Alessandra Re, L. Oberauer, A. A. Sabelnikov, P. Cavalcante, A. Derbin, M. Misiaszek, A. E. Chavarria, L. Perasso, Aldo Ianni, Marco Giammarchi, A. Sotnikov, E. Litvinovich, E. Meroni, F. Lombardi, V. Muratova, B. Caccianiga, P. J. Mosteiro, J. Benziger, Andrea Ianni, F. Calaprice, D. Bick, Sandra Zavatarelli, C. Salvo, O. Zaimidoroga, A. Goretti, E. Guardincerri, O. Smirnov, G. Testera, S. Manecki, Aldo Romani, L. Papp, Paolo Lombardi, J. Winter, S. Perasso, S. V. Sukhotin, Gioacchino Ranucci, A. Wright, Jingke Xu, Cristiano Galbiati, G. Bellini, S. Hardy, M. Skorokhvatov, Matthias Laubenstein, J. Quirk, T. Lewke, D. Kryn, Marco Pallavicini, D. D'Angelo, Stefano Bonetti, K. Fomenko, S. Gazzana, Michael Wurm, L. Grandi, Q. Meindl, F. von Feilitzsch, W. Maneschg, Laura Cadonati, Fausto Ortica, I. Machulin, Lino Miramonti, D. Vignaud, G. Korga, D. Franco, G. Bonfini, M. Buizza Avanzini, Hardy Simgen, C. Carraro, Bellini, G., Suvorov, Y., Et, Al., APC - Neutrinos, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), AstroParticule et Cosmologie (APC (UMR_7164)), Borexino, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: History, Metallicity, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, Solar neutrinos, General Physics and Astronomy, FOS: Physical sciences, Astrophysics, 01 natural sciences, Main-sequence: late-type stars, Education, High Energy Physics - Experiment, 26.65.+t, 14.60.Lm, 95.55.Vj, 97.20.Jg, Nuclear physics, Physics and Astronomy (all), High Energy Physics - Experiment (hep-ex), Ordinary neutrinos (nuW bosons, muon, 0103 physical sciences, Neutrino, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Astrophysics::Solar and Stellar Astrophysics, 010306 general physics, Neutrino oscillation, Borexino, Solar and Stellar Astrophysics (astro-ph.SR), Physics, Range (particle radiation), Standard solar model, Muon, 010308 nuclear & particles physics, [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], High Energy Physics::Phenomenology, pion, cosmic ray detectors, [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], and other elementary particle detectors, Computer Science Applications, 3. Good health, Astrophysics - Solar and Stellar Astrophysics, 13. Climate action, Physics::Space Physics, High Energy Physics::Experiment
Abstract: We observed, for the first time, solar neutrinos in the 1.0-1.5 MeV energy range. We measured the rate of pep solar neutrino interactions in Borexino to be [3.1+-0.6(stat)+-0.3(syst)] counts/(day x 100 ton) and provided a constraint on the CNO solar neutrino interaction rate of, Submitted to Physical Review Letters (2011)
Published: 2011
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50. Measurement of the solarB8neutrino rate with a liquid scintillator target and 3 MeV energy threshold in the Borexino detector

Author: Livia Ludhova, A. M. Goretti, A. S. Chepurnov, G. Testera, S. Manecki, R. S. Raghavan, G. Manuzio, Matthias Laubenstein, M. Obolensky, Jay Burton Benziger, E. Meroni, S. Davini, S. Hardy, B. Ricci, T. Lewke, I. N. Machulin, M. D. Skorokhvatov, Michael Wurm, Lothar Oberauer, P. Risso, S. V. Sukhotin, M. Goeger-Neff, Stefano Bonetti, A. Wright, O. Zaimidoroga, Marco Pallavicini, Aldo Ianni, E. Litvinovich, D. D'Angelo, D. Franco, F. Dalnoki-Veress, F. von Feilitzsch, F. Ortica, D. Kryn, Q. Meindl, G. Bellini, D. Rountree, A. Romani, C. Carraro, Paolo Lombardi, R. B. Vogelaar, H. de Kerret, R. Tartaglia, Jingke Xu, Cristiano Galbiati, G. Korga, K. Fomenko, Laura Cadonati, L. Papp, S. Gazzana, R. Saldanha, Lino Miramonti, Marco Giammarchi, W. Maneschg, Michael K.H. Leung, Alessandra Re, M. Buizza Avanzini, B. Caccianiga, Frank Calaprice, Hardy Simgen, D. Vinaud, Andrea Ianni, O. Smirnov, Sandra Zavatarelli, S. Schönert, Marcin Wójcik, A. Sotnikov, V. N. Muratova, A. Pocar, D. Montanari, G. Zuzel, Gioacchino Ranucci, Y. Suvorov, A. E. Chavarria, L. Perasso, C. Salvo, A.V. Etenko, A. Razeto, E. Gurdincerri, B. Loer, A. A. Sabelnikov, Yusuke Koshio, A. V. Derbin, S. Perasso, J. Winter, Malcolm J. Joyce, C. Ghiano, and M. Misiaszek
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Solar neutrino, 01 natural sciences, 7. Clean energy, Nuclear physics, Neutrino detector, 13. Climate action, 0103 physical sciences, High Energy Physics::Experiment, Astrophysics::Earth and Planetary Astrophysics, Neutrino, 010306 general physics, Neutrino oscillation, Isotopes of beryllium, Energy (signal processing), Borexino, Lepton
Abstract: We report the measurement of {nu}-e elastic scattering from {sup 8}B solar neutrinos with 3 MeV energy threshold by the Borexino detector in Gran Sasso (Italy). The rate of solar neutrino-induced electron scattering events above this energy in Borexino is 0.22{+-}0.04(stat){+-}0.01(syst) cpd/100 t, which corresponds to {Phi}{sub {sup 8}B}{sup ES}=2.4{+-}0.4{+-}0.1x10{sup 6} cm{sup -2} s{sup -1}, in good agreement with measurements from SNO and SuperKamiokaNDE. Assuming the {sup 8}B neutrino flux predicted by the high metallicity standard solar model, the average {sup 8}B {nu}{sub e} survival probability above 3 MeV is measured to be 0.29{+-}0.10. The survival probabilities for {sup 7}Be and {sup 8}B neutrinos as measured by Borexino differ by 1.9{sigma}. These results are consistent with the prediction of the MSW-LMA solution of a transition in the solar {nu}{sub e} survival probability P{sub ee} between the low-energy vacuum-driven and the high-energy matter-enhanced solar neutrino oscillation regimes.
Published: 2010

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