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51. Unfolding Neutron Spectrum with Markov Chain Monte Carlo at MIT Research Reactor with He-3 Neutral Current Detectors

Author: Leder, A. F., Anderson, A. J., Billard, J., Figueroa-Feliciano, E., Formaggio, J. A., Hasselkus, C., Newman, E., Palladino, K., Phuthi, M., Winslow, L., and Zhang, L.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment, Nuclear Experiment
Abstract: The Ricochet experiment seeks to measure Coherent (neutral-current) Elastic Neutrino-Nucleus Scattering using dark-matter-style detectors with sub-keV thresholds placed near a neutrino source, such as the MIT (research) Reactor (MITR), which operates at 5.5 MW generating approximately 2.2e18 neutrinos/second in its core. Currently, Ricochet is characterizing the backgrounds at MITR, the main component of which comes in the form of neutrons emitted from the core simultaneous with the neutrino signal. To characterize this background, we wrapped Bonner cylinders around a He-3 thermal neutron detector, whose data was then unfolded via a Markov Chain Monte Carlo (MCMC) to produce a neutron energy spectrum across several orders of magnitude. We discuss the resulting spectrum and its implications for deploying Ricochet at the MITR site as well as the feasibility of reducing this background level via the addition of polyethylene shielding around the detector setup., Comment: 14 pages, 9 figures, 1 table, published in JINST
Published: 2017
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52. Ultra-Low Energy Calibration of LUX Detector using $^{127}$Xe Electron Capture

Author: LUX Collaboration, Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Druszkiewicz, E., Edwards, B. N., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract: We report an absolute calibration of the ionization yields($\textit{Q$_y$})$ and fluctuations for electronic recoil events in liquid xenon at discrete energies between 186 eV and 33.2 keV. The average electric field applied across the liquid xenon target is 180 V/cm. The data are obtained using low energy $^{127}$Xe electron capture decay events from the 95.0-day first run from LUX (WS2013) in search of Weakly Interacting Massive Particles (WIMPs). The sequence of gamma-ray and X-ray cascades associated with $^{127}$I de-excitations produces clearly identified 2-vertex events in the LUX detector. We observe the K- (binding energy, 33.2 keV), L- (5.2 keV), M- (1.1 keV), and N- (186 eV) shell cascade events and verify that the relative ratio of observed events for each shell agrees with calculations. The N-shell cascade analysis includes single extracted electron (SE) events and represents the lowest-energy electronic recoil $\textit{in situ}$ measurements that have been explored in liquid xenon., Comment: 10 pages, 10 figures, 2 tables
Published: 2017
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53. 3D Modeling of Electric Fields in the LUX Detector

Author: LUX Collaboration, Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Druszkiewicz, E., Edwards, B. N., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment, Physics - Computational Physics
Abstract: This work details the development of a three-dimensional (3D) electric field model for the LUX detector. The detector took data during two periods of searching for weakly interacting massive particle (WIMP) searches. After the first period completed, a time-varying non-uniform negative charge developed in the polytetrafluoroethylene (PTFE) panels that define the radial boundary of the detector's active volume. This caused electric field variations in the detector in time, depth and azimuth, generating an electrostatic radially-inward force on electrons on their way upward to the liquid surface. To map this behavior, 3D electric field maps of the detector's active volume were built on a monthly basis. This was done by fitting a model built in COMSOL Multiphysics to the uniformly distributed calibration data that were collected on a regular basis. The modeled average PTFE charge density increased over the course of the exposure from -3.6 to $-5.5~\mu$C/m$^2$. From our studies, we deduce that the electric field magnitude varied while the mean value of the field of $\sim200$~V/cm remained constant throughout the exposure. As a result of this work the varying electric fields and their impact on event reconstruction and discrimination were successfully modeled.
Published: 2017
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54. $^{83\textrm{m}}$Kr calibration of the 2013 LUX dark matter search

Author: LUX Collaboration, Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Druszkiewicz, E., Edwards, B. N., Fallon, S. R., Fan, A., Fiorucci, S., Gaitskell, R. J., Genovesi, J., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors
Abstract: LUX was the first dark matter experiment to use a $^{83\textrm{m}}$Kr calibration source. In this paper we describe the source preparation and injection. We also present several $^{83\textrm{m}}$Kr calibration applications in the context of the 2013 LUX exposure, including the measurement of temporal and spatial variation in scintillation and charge signal amplitudes, and several methods to understand the electric field within the time projection chamber.
Published: 2017
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55. Input Comparison of Radiogenic Neutron Estimates for Ultra-low Background Experiments

Author: Cooley, J., Palladino, K. J., Qiu, H., Selvi, M., Scorza, S., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Ultra-low-background experiments address some of the most important open questions in particle physics, cosmology and astrophysics: the nature of dark matter, whether the neutrino is its own antiparticle, and does the proton decay. These rare event searches require well-understood and minimized backgrounds. Simulations are used to understand backgrounds caused by naturally occurring radioactivity in the rock and in every piece of shielding and detector material used in these experiments. Most important are processes like spontaneous fission and ({\alpha},n) reactions in material close to the detectors that can produce neutrons. A comparison study between two dedicated software packages is detailed. The cross section libraries, neutron yields, and spectra from the Mei-Zhang-Hime and the SOURCES-4A codes are presented. The resultant yields and spectra are used as inputs to direct dark matter detector toy models in GEANT4, to study the impact of their differences on background estimates and fits. Although differences in neutron yield calculations up to 50% were seen, there was no systematic difference between the Mei-Hime-Zhang and SOURCES-4A results. Neutron propagation simulations smooth differences in spectral shape and yield, and both tools were found to meet the broad requirements of the low-background community.
Published: 2017
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56. Limits on spin-dependent WIMP-nucleon cross section obtained from the complete LUX exposure

Author: LUX Collaboration, Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fallon, S. R., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present experimental constraints on the spin-dependent WIMP-nucleon elastic cross sections from the total 129.5 kg-year exposure acquired by the Large Underground Xenon experiment (LUX), operating at the Sanford Underground Research Facility in Lead, South Dakota (USA). A profile likelihood ratio analysis allows 90% CL upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of $\sigma_n$ = 1.6$\times 10^{-41}$ cm$^{2}$ ($\sigma_p$ = 5$\times 10^{-40}$ cm$^{2}$) at 35 GeV$c^{-2}$, almost a sixfold improvement over the previous LUX spin-dependent results. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date., Comment: 7 pages, 3 figures, version accepted by PRL
Published: 2017
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57. First Searches for Axions and Axion-Like Particles with the LUX Experiment

Author: Akerib, D. S., Alsum, S., Aquino, C., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fallon, S. R., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Velan, V., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology
Abstract: The first searches for axions and axion-like particles with the Large Underground Xenon (LUX) experiment are presented. Under the assumption of an axio-electric interaction in xenon, the coupling constant between axions and electrons, gAe is tested, using data collected in 2013 with an exposure totalling 95 live-days $\times$ 118 kg. A double-sided, profile likelihood ratio statistic test excludes gAe larger than 3.5 $\times$ 10$^{-12}$ (90% C.L.) for solar axions. Assuming the DFSZ theoretical description, the upper limit in coupling corresponds to an upper limit on axion mass of 0.12 eV/c$^{2}$, while for the KSVZ description masses above 36.6 eV/c$^{2}$ are excluded. For galactic axion-like particles, values of gAe larger than 4.2 $\times$ 10$^{-13}$ are excluded for particle masses in the range 1-16 keV/c$^{2}$. These are the most stringent constraints to date for these interactions.
Published: 2017
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58. LUX-ZEPLIN (LZ) Technical Design Report

Author: Mount, B. J., Hans, S., Rosero, R., Yeh, M., Chan, C., Gaitskell, R. J., Huang, D. Q., Makkinje, J., Malling, D. C., Pangilinan, M., Rhyne, C. A., Taylor, W. C., Verbus, J. R., Kim, Y. D., Lee, H. S., Lee, J., Leonard, D. S., Li, J., Belle, J., Cottle, A., Lippincott, W. H., Markley, D. J., Martin, T. J., Sarychev, M., Tope, T. E., Utes, M., Wang, R., Young, I., Araújo, H. M., Bailey, A. J., Bauer, D., Colling, D., Currie, A., Fayer, S., Froborg, F., Greenwood, S., Jones, W. G., Kasey, V., Khaleeq, M., Olcina, I., Paredes, B. López, Richards, A., Sumner, T. J., Tomás, A., Vacheret, A., Brás, P., Lindote, A., Lopes, M. I., Neves, F., Rodrigues, J. P., Silva, C., Solovov, V. N., Barry, M. J., Cole, A., Dobi, A., Edwards, W. R., Faham, C. H., Fiorucci, S., Gantos, N. J., Gehman, V. M., Gilchriese, M. G. D., Hanzel, K., Hoff, M. D., Kamdin, K., Lesko, K. T., McConnell, C. T., O'Sullivan, K., Oliver-Mallory, K. C., Patton, S. J., Saba, J. S., Sorensen, P., Thomas, K. J., Tull, C. E., Waldron, W. L., Witherell, M. S., Bernstein, A., Kazkaz, K., Xu, J., Akimov, D. Yu., Bolozdynya, A. I., Khromov, A. V., Konovalov, A. M., Kumpan, A. V., Sosnovtsev, V. V., Dahl, C. E., Temples, D., Carmona-Benitez, M. C., de Viveiros, L., Akerib, D. S., Auyeung, H., Biesiadzinski, T. P., Breidenbach, M., Bramante, R., Conley, R., Craddock, W. W., Fan, A., Hau, A., Ignarra, C. M., Ji, W., Krebs, H. J., Linehan, R., Lee, C., Luitz, S., Mizrachi, E., Monzani, M. E., O'Neill, F. G., Pierson, S., Racine, M., Ratcliff, B. N., Shutt, G. W., Shutt, T. A., Skarpaas, K., Stifter, K., To, W. H., Va'vra, J., Whitis, T. J., Wisniewski, W. J., Bai, X., Bunker, R., Coughlen, R., Hjemfelt, C., Leonard, R., Miller, E. H., Morrison, E., Reichenbacher, J., Schnee, R. W., Stark, M. R., Sundarnath, K., Tiedt, D. R., Timalsina, M., Bauer, P., Carlson, B., Horn, M., Johnson, M., Keefner, J., Maupin, C., Taylor, D. J., Balashov, S., Ford, P., Francis, V., Holtom, E., Khazov, A., Kaboth, A., Majewski, P., Nikkel, J. A., O'Dell, J., Preece, R. M., van der Grinten, M. G. D., Worm, S. D., Mannino, R. L., Stiegler, T. M., Terman, P. A., Webb, R. C., Levy, C., Mock, J., Szydagis, M., Busenitz, J. K., Elnimr, M., Hor, J. Y-K., Meng, Y., Piepke, A., Stancu, I., Kreczko, L., Krikler, B., Penning, B., Bernard, E. P., Jacobsen, R. G., McKinsey, D. N., Watson, R., Cutter, J. E., El-Jurf, S., Gerhard, R. M., Hemer, D., Hillbrand, S., Holbrook, B., Lenardo, B. G., Manalaysay, A. G., Morad, J. A., Stephenson, S., Thomson, J. A., Tripathi, M., Uvarov, S., Haselschwardt, S. J., Kyre, S., Nehrkorn, C., Nelson, H. N., Solmaz, M., White, D. T., Cascella, M., Dobson, J. E. Y., Ghag, C., Liu, X., Manenti, L., Reichhart, L., Shaw, S., Utku, U., Beltrame, P., Davison, T. J. R., Marzioni, M. F., Murphy, A. St. J., Nilima, A., Boxer, B., Burdin, S., Greenall, A., Powell, S., Rose, H. J., Sutcliffe, P., Balajthy, J., Edberg, T. K., Hall, C. R., Silk, J. S., Hertel, S., Akerlof, C. W., Arthurs, M., Lorenzon, W., Pushkin, K., Schubnell, M., Boast, K. E., Carels, C., Fruth, T., Kraus, H., Liao, F. -T., Lin, J., Scovell, P. R., Druszkiewicz, E., Khaitan, D., Koyuncu, M., Skulski, W., Wolfs, F. L. H., Yin, J., Korolkova, E. V., Kudryavtsev, V. A., Rossiter, P., Woodward, D., Chiller, A. A., Chiller, C., Mei, D. -M., Wang, L., Wei, W. -Z., While, M., Zhang, C., Alsum, S. K., Benson, T., Carlsmith, D. L., Cherwinka, J. J., Dasu, S., Gregerson, G., Gomber, B., Pagac, A., Palladino, K. J., Vuosalo, C. O., Xiao, Q., Buckley, J. H., Bugaev, V. V., Olevitch, M. A., Boulton, E. M., Emmet, W. T., Hurteau, T. W., Larsen, N. A., Pease, E. K., Tennyson, B. P., and Tvrznikova, L.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract: In this Technical Design Report (TDR) we describe the LZ detector to be built at the Sanford Underground Research Facility (SURF). The LZ dark matter experiment is designed to achieve sensitivity to a WIMP-nucleon spin-independent cross section of three times ten to the negative forty-eighth square centimeters., Comment: 392 pages. Submitted to the Department of Energy as part of the documentation for the Critical Decision Numbers Two and Three (CD-2 and CD-3) management processes. Report also available by chapter at this URL
Published: 2017

59. Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches

Author: Akerib, D. S., Akerlof, C. W., Akimov, D. Yu., Alsum, S. K., Araújo, H. M., Arnquist, I. J., Arthurs, M., Bai, X., Bailey, A. J., Balajthy, J., Balashov, S., Barry, M. J., Belle, J., Beltrame, P., Benson, T., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boast, K. E., Bolozdynya, A., Boxer, B., Bramante, R., Brás, P., Buckley, J. H., Bugaev, V. V., Bunker, R., Burdin, S., Busenitz, J. K., Carels, C., Carlsmith, D. L., Carlson, B., Carmona-Benitez, M. C., Chan, C., Cherwinka, J. J., Chiller, A. A., Chiller, C., Cottle, A., Coughlen, R., Craddock, W. W., Currie, A., Dahl, C. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edberg, T. K., Edwards, W. R., Emmet, W. T., Faham, C. H., Fiorucci, S., Fruth, T., Gaitskell, R. J., Gantos, N. J., Gehman, V. M., Gerhard, R. M., Ghag, C., Gilchriese, M. G. D., Gomber, B., Hall, C. R., Hans, S., Hanzel, K., Haselschwardt, S. J., Hertel, S. A., Hillbrand, S., Hjemfelt, C., Hoff, M. D., Holbrook, B., Holtom, E., Hoppe, E. W., Hor, J. Y-K., Horn, M., Huang, D. Q., Hurteau, T. W., Ignarra, C. M., Jacobsen, R. G., Ji, W., Kaboth, A., Kamdin, K., Kazkaz, K., Khaitan, D., Khazov, A., Khromov, A. V., Konovalov, A. M., Korolkova, E. V., Koyuncu, M., Kraus, H., Krebs, H. J., Kudryavtsev, V. A., Kumpan, A. V., Kyre, S., Lee, C., Lee, H. S., Lee, J., Leonard, D. S., Leonard, R., Lesko, K. T., Levy, C., Liao, F. -T., Lin, J., Lindote, A., Linehan, R. E., Lippincott, W. H., Liu, X., Lopes, M. I., Paredes, B. Lopez, Lorenzon, W., Luitz, S., Majewski, P., Manalaysay, A., Manenti, L., Mannino, R. L., Markley, D. J., Martin, T. J., Marzioni, M. F., McConnell, C. T., McKinsey, D. N., Mei, D. -M., Meng, Y., Miller, E. H., Mizrachi, E., Mock, J., Monzani, M. E., Morad, J. A., Mount, B. J., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., Nikkel, J. A., O'Dell, J., O'Sullivan, K., Olcina, I., Olevitch, M. A., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Piepke, A., Powell, S., Preece, R. M., Pushkin, K., Ratcliff, B. N., Reichenbacher, J., Reichhart, L., Rhyne, C. A., Richards, A., Rodrigues, J. P., Rose, H. J., Rosero, R., Rossiter, P., Saba, J. S., Sarychev, M., Schnee, R. W., Schubnell, M., Scovell, P. R., Shaw, S., Shutt, T. A., Silva, C., Skarpaas, K., Skulski, W., Solmaz, M., Solovov, V. N., Sorensen, P., Sosnovtsev, V. V., Stancu, I., Stark, M. R., Stephenson, S., Stiegler, T. M., Stifter, K., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Temples, D., Terman, P. A., Thomas, K. J., Thomson, J. A., Tiedt, D. R., Timalsina, M., To, W. H., Tomás, A., Tope, T. E., Tripathi, M., Tvrznikova, L., Va'vra, J., Vacheret, A., van der Grinten, M. G. D., Verbus, J. R., Vuosalo, C. O., Waldron, W. L., Wang, R., Watson, R., Webb, R. C., Wei, W. -Z., While, M., White, D. T., Whitis, T. J., Wisniewski, W. J., Witherell, M. S., Wolfs, F. L. H., Woodward, D., Worm, S., Xu, J., Yeh, M., Yin, J., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a double-vessel cryostat. The large mass and proximity of the cryostat to the active detector volume demand the use of material with extremely low intrinsic radioactivity. We report on the radioassay campaign conducted to identify suitable metals, the determination of factors limiting radiopure production, and the selection of titanium for construction of the LZ cryostat and other detector components. This titanium has been measured with activities of $^{238}$U$_{e}$~$<$1.6~mBq/kg, $^{238}$U$_{l}$~$<$0.09~mBq/kg, $^{232}$Th$_{e}$~$=0.28\pm 0.03$~mBq/kg, $^{232}$Th$_{l}$~$=0.25\pm 0.02$~mBq/kg, $^{40}$K~$<$0.54~mBq/kg, and $^{60}$Co~$<$0.02~mBq/kg (68\% CL). Such low intrinsic activities, which are some of the lowest ever reported for titanium, enable its use for future dark matter and other rare event searches. Monte Carlo simulations have been performed to assess the expected background contribution from the LZ cryostat with this radioactivity. In 1,000 days of WIMP search exposure of a 5.6-tonne fiducial mass, the cryostat will contribute only a mean background of $0.160\pm0.001$(stat)$\pm0.030$(sys) counts., Comment: 13 pages, 3 figures, accepted for publication in Astroparticle Physics
Published: 2017
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60. Coherent Neutrino Scattering with Low Temperature Bolometers at Chooz Reactor Complex

Author: Billard, J., Carr, R., Dawson, J., Figueroa-Feliciano, E., Formaggio, J. A., Gascon, J., De Jesus, M., Johnston, J., Lasserre, T., Leder, A., Palladino, K. J., Trowbridge, S. H., Vivier, M., and Winslow, L.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment, Nuclear Experiment
Abstract: We present the potential sensitivity of a future recoil detector for a first detection of the process of coherent elastic neutrino nucleus scattering (CE$\nu$NS). We use the Chooz reactor complex in France as our luminous source of reactor neutrinos. Leveraging the ability to cleanly separate the rate correlated with the reactor thermal power against (uncorrelated) backgrounds, we show that a 10 kilogram cryogenic bolometric array with 100 eV threshold should be able to extract a CE$\nu$NS signal within one year of running., Comment: 12 pages, 5 figures
Published: 2016
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61. Signal yields, energy resolution, and recombination fluctuations in liquid xenon

Author: Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bramante, R., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: This work presents an analysis of monoenergetic electronic recoil peaks in the dark-matter-search and calibration data from the first underground science run of the Large Underground Xenon (LUX) detector. Liquid xenon charge and light yields for electronic recoil energies between 5.2 and 661.7 keV are measured, as well as the energy resolution for the LUX detector at those same energies. Additionally, there is an interpretation of existing measurements and descriptions of electron-ion recombination fluctuations in liquid xenon as limiting cases of a more general liquid xenon re- combination fluctuation model. Measurements of the standard deviation of these fluctuations at monoenergetic electronic recoil peaks exhibit a linear dependence on the number of ions for energy deposits up to 661.7 keV, consistent with previous LUX measurements between 2-16 keV with $^3$H. We highlight similarities in liquid xenon recombination for electronic and nuclear recoils with a comparison of recombination fluctuations measured with low-energy calibration data., Comment: 11 pages, 12 figures, 3 tables
Published: 2016
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62. Results from a search for dark matter in the complete LUX exposure

Author: Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bramante, R., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O`Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract: We report constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35e4 kg-day exposure of the Large Underground Xenon (LUX) experiment. A dual-phase xenon time projection chamber with 250 kg of active mass is operated at the Sanford Underground Research Facility under Lead, South Dakota (USA). With roughly fourfold improvement in sensitivity for high WIMP masses relative to our previous results, this search yields no evidence of WIMP nuclear recoils. At a WIMP mass of 50 GeV/c^2, WIMP-nucleon spin-independent cross sections above 2.2e-46 cm^2 are excluded at the 90% confidence level. When combined with the previously reported LUX exposure, this exclusion strengthens to 1.1e-46 cm^2 at 50 GeV/c^2., Comment: This version includes a combined analysis with previously published LUX results, and matches the version published in PRL
Published: 2016
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63. Low-energy (0.7-74 keV) nuclear recoil calibration of the LUX dark matter experiment using D-D neutron scattering kinematics

Author: LUX Collaboration, Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Brás, P., Byram, D., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., de Viveiros, L., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C. A., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract: The Large Underground Xenon (LUX) experiment is a dual-phase liquid xenon time projection chamber (TPC) operating at the Sanford Underground Research Facility in Lead, South Dakota. A calibration of nuclear recoils in liquid xenon was performed $\textit{in situ}$ in the LUX detector using a collimated beam of mono-energetic 2.45 MeV neutrons produced by a deuterium-deuterium (D-D) fusion source. The nuclear recoil energy from the first neutron scatter in the TPC was reconstructed using the measured scattering angle defined by double-scatter neutron events within the active xenon volume. We measured the absolute charge ($Q_{y}$) and light ($L_{y}$) yields at an average electric field of 180 V/cm for nuclear recoil energies spanning 0.7 to 74 keV and 1.1 to 74 keV, respectively. This calibration of the nuclear recoil signal yields will permit the further refinement of liquid xenon nuclear recoil signal models and, importantly for dark matter searches, clearly demonstrates measured ionization and scintillation signals in this medium at recoil energies down to $\mathcal{O}$(1 keV)., Comment: 24 pages, 15 figures, 6 tables
Published: 2016

64. Chromatographic separation of radioactive noble gases from xenon

Author: LUX Collaboration, Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chiller, A. A., Chiller, C., Coffey, T., Currie, A., Cutter, J. E., Davison, T. J. R., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Pech, K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors
Abstract: The Large Underground Xenon (LUX) experiment operates at the Sanford Underground Research Facility to detect nuclear recoils from the hypothetical Weakly Interacting Massive Particles (WIMPs) on a liquid xenon target. Liquid xenon typically contains trace amounts of the noble radioactive isotopes $^{85}$Kr and $^{39}$Ar that are not removed by the in situ gas purification system. The decays of these isotopes at concentrations typical of research-grade xenon would be a dominant background for a WIMP search exmperiment. To remove these impurities from the liquid xenon, a chromatographic separation system based on adsorption on activated charcoal was built. 400 kg of xenon was processed, reducing the average concentration of krypton from 130 ppb to 3.5 ppt as measured by a cold-trap assisted mass spectroscopy system. A 50 kg batch spiked to 0.001 g/g of krypton was processed twice and reduced to an upper limit of 0.2 ppt., Comment: Accepted in Astropart. Phys
Published: 2016
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65. Characteristics of Four Upward-pointing Cosmic-ray-like Events Observed with ANITA

Author: Gorham, P. W., Nam, J., Romero-Wolf, A., Hoover, S., Allison, P., Banerjee, O., Beatty, J. J., Belov, K., Besson, D. Z., Binns, W. R., Bugaev, V., Cao, P., Chen, C., Chen, P., Clem, J. M., Connolly, A., Dailey, B., Deaconu, C., Cremonesi, L., Dowkonnt, P. F., Duvernois, M. A., Field, R. C., Fox, B. D., Goldstein, D., Gordon, J., Hast, C., Hebert, C. L., Hill, B., Hughes, K., Hupe, R., Israel, M. H., Javaid, A., Kowalski, J., Lam, J., Learned, J. G., Liewer, K. M., Liu, T. C., Link, J. T., Lusczek, E., Matsuno, S., Mercurio, B. C., Miki, C., Miocinovic, P., Mottram, M., Mulrey, K., Naudet, C. J., Ng, J., Nichol, R. J., Palladino, K., Rauch, B. F., Reil, K., Roberts, J., Rosen, M., Rotter, B., Russell, J., Ruckman, L., Saltzberg, D., Seckel, D., Schoorlemmer, H., Stafford, S., Stockham, J., Stockham, M., Strutt, B., Tatem, K., Varner, G. S., Vieregg, A. G., Walz, D., Wissel, S. A., and Wu, F.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We report on four radio-detected cosmic-ray (CR) or CR-like events observed with the Antarctic Impulsive Transient Antenna (ANITA), a NASA-sponsored long-duration balloon payload. Two of the four were previously identified as stratospheric CR air showers during the ANITA-I flight. A third stratospheric CR was detected during the ANITA-II flight. Here we report on characteristics these three unusual CR events, which develop nearly horizontally, 20-30~km above the surface of the Earth. In addition, we report on a fourth steeply upward-pointing ANITA-I CR-like radio event which has characteristics consistent with a primary that emerged from the surface of the ice. This suggests a possible $\tau$-lepton decay as the origin of this event, but such an interpretation would require significant suppression of the Standard Model ${\tau}$-neutrino cross section., Comment: 5pp,4 figures, referees' comments addressed, this version accepted to Phys. Rev. Letters. Supplemental PDF material available; see source files
Published: 2016
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66. Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment

Author: LUX Collaboration, Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., de Viveiros, L., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract: We present the first experimental constraints on the spin-dependent WIMP-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of $1.4~\times~10^{4}~\text{kg}\cdot~\text{days}$ of fiducial exposure allows 90% CL upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of $\sigma_n~=~9.4~\times~10^{-41}~\text{cm}^2$ ($\sigma_p~=~2.9~\times~10^{-39}~\text{cm}^2$) at 33 GeV/c$^2$. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date., Comment: 6 pages, 2 figures
Published: 2016
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67. Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX data

Author: LUX Collaboration, Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., de Viveiros, L., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O`Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Yazdani, K., Young, S. K., and Zhang, C.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract: We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including $1.4\times10^{4}\;\mathrm{kg\; day}$ of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium $\beta$ source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 $\mathrm{GeV}\,c^{-2}$, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 $\mathrm{GeV}\,c^{-2}$ WIMP mass., Comment: Accepted by Phys. Rev. Lett
Published: 2015
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68. Tritium calibration of the LUX dark matter experiment

Author: LUX Collaboration, Akerib, D. S., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., de Viveiros, L., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A. G., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O`Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract: We present measurements of the electron-recoil (ER) response of the LUX dark matter detector based upon 170,000 highly pure and spatially-uniform tritium decays. We reconstruct the tritium energy spectrum using the combined energy model and find good agreement with expectations. We report the average charge and light yields of ER events in liquid xenon at 180 V/cm and 105 V/cm and compare the results to the NEST model. We also measure the mean charge recombination fraction and its fluctuations, and we investigate the location and width of the LUX ER band. These results provide input to a re-analysis of the LUX Run3 WIMP search.
Published: 2015
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69. FPGA-based Trigger System for the LUX Dark Matter Experiment

Author: Akerib, D. S., Araujo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Bradley, A., Bramante, R., Cahn, S. B., Carmona-Benitez, M. C., Chan, C., Chapman, J. J., Chiller, A. A., Chiller, C., Currie, A., Cutter, J. E., Davison, T. J. R., de Viveiros, L., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edwards, B. N., Faham, C. H., Fiorucci, S., Gaitskell, R. J., Gehman, V. M., Ghag, C., Gibson, K. R., Gilchriese, M. G. D., Hall, C. R., Hanhardt, M., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Ihm, M., Jacobsen, R. G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Lindote, A., Lopes, M. I., Malling, D. C., Manalaysay, A. G., Mannino, R. L., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., Nehrkorn, C., Nelson, H. N., Neves, F., O'Sullivan, K., Oliver-Mallory, K. C., Ott, R. A., Palladino, K. J., Pangilinan, M., Pease, E. K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T. A., Silva, C., Skulski, W., Solovov, V. N., Sorensen, P., Stephenson, S., Sumner, T. J., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J. R., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Yen, M., Yin, J., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors
Abstract: LUX is a two-phase (liquid/gas) xenon time projection chamber designed to detect nuclear recoils resulting from interactions with dark matter particles. Signals from the detector are processed with an FPGA-based digital trigger system that analyzes the incoming data in real-time, with just a few microsecond latency. The system enables first pass selection of events of interest based on their pulse shape characteristics and 3D localization of the interactions. It has been shown to be >99% efficient in triggering on S2 signals induced by only few extracted liquid electrons. It is continuously and reliably operating since its full underground deployment in early 2013. This document is an overview of the systems capabilities, its inner workings, and its performance., Comment: 11 pages, 26 figures, added some key points to the abstract, and conclusions, no change in results, accepted for publication in Nuclear Instruments and Methods in Physics Research Section A
Published: 2015
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70. LUX-ZEPLIN (LZ) Conceptual Design Report

Author: The LZ Collaboration, Akerib, D. S., Akerlof, C. W., Akimov, D. Yu., Alsum, S. K., Araújo, H. M., Bai, X., Bailey, A. J., Balajthy, J., Balashov, S., Barry, M. J., Bauer, P., Beltrame, P., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boast, K. E., Bolozdynya, A. I., Boulton, E. M., Bramante, R., Buckley, J. H., Bugaev, V. V., Bunker, R., Burdin, S., Busenitz, J. K., Carels, C., Carlsmith, D. L., Carlson, B., Carmona-Benitez, M. C., Cascella, M., Chan, C., Cherwinka, J. J., Chiller, A. A., Chiller, C., Craddock, W. W., Currie, A., Cutter, J. E., da Cunha, J. P., Dahl, C. E., Dasu, S., Davison, T. J. R., de Viveiros, L., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Edberg, T. K., Edwards, B. N., Edwards, W. R., Elnimr, M. M., Emmet, W. T., Faham, C. H., Fiorucci, S., Ford, P., Francis, V. B., Fu, C., Gaitskell, R. J., Gantos, N. J., Gehman, V. M., Gerhard, R. M., Ghag, C., Gilchriese, M. G. D., Gomber, B., Hall, C. R., Harris, A., Haselschwardt, S. J., Hertel, S. A., Hoff, M. D., Holbrook, B., Holtom, E., Huang, D. Q., Hurteau, T. W., Ignarra, C. M., Jacobsen, R. G., Ji, W., Ji, X., Johnson, M., Ju, Y., Kamdin, K., Kazkaz, K., Khaitan, D., Khazov, A., Khromov, A. V., Konovalov, A. M., Korolkova, E. V., Kraus, H., Krebs, H. J., Kudryavtsev, V. A., Kumpan, A. V., Kyre, S., Larsen, N. A., Lee, C., Lenardo, B. G., Lesko, K. T., Liao, F. -T., Lin, J., Lindote, A., Lippincott, W. H., Liu, J., Liu, X., Lopes, M. I., Lorenzon, W., Luitz, S., Majewski, P., Malling, D. C., Manalaysay, A. G., Manenti, L., Mannino, R. L., Markley, D. J., Martin, T. J., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Meng, Y., Miller, E. H., Mock, J., Monzani, M. E., Morad, J. A., Murphy, A. St. J., Nelson, H. N., Neves, F., Nikkel, J. A., O'Neill, F. G., O'Dell, J., O'Sullivan, K., Olevitch, M. A., Oliver-Mallory, K. C., Palladino, K. J., Pangilinan, M., Patton, S. J., Pease, E. K., Piepke, A., Powell, S., Preece, R. M., Pushkin, K., Ratcliff, B. N., Reichenbacher, J., Reichhart, L., Rhyne, C., Rodrigues, J. P., Rose, H. J., Rosero, R., Saba, J. S., Sarychev, M., Schnee, R. W., Schubnell, M. S. G., Scovell, P. R., Shaw, S., Shutt, T. A., Silva, C., Skarpaas, K., Skulski, W., Solovov, V. N., Sorensen, P., Sosnovtsev, V. V., Stancu, I., Stark, M. R., Stephenson, S., Stiegler, T. M., Sumner, T. J., Sundarnath, K., Szydagis, M., Taylor, D. J., Taylor, W., Tennyson, B. P., Terman, P. A., Thomas, K. J., Thomson, J. A., Tiedt, D. R., To, W. H., Tomás, A., Tripathi, M., Tull, C. E., Tvrznikova, L., Uvarov, S., Va'vra, J., van der Grinten, M. G. D., Verbus, J. R., Vuosalo, C. O., Waldron, W. L., Wang, L., Webb, R. C., Wei, W. -Z., While, M., White, D. T., Whitis, T. J., Wisniewski, W. J., Witherell, M. S., Wolfs, F. L. H., Woods, E., Woodward, D., Worm, S. D., Yeh, M., Yin, J., Young, S. K., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract: The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report. LZ is a second-generation dark-matter detector with the potential for unprecedented sensitivity to weakly interacting massive particles (WIMPs) of masses from a few GeV/c2 to hundreds of TeV/c2. With total liquid xenon mass of about 10 tonnes, LZ will be the most sensitive experiment for WIMPs in this mass region by the end of the decade. This report describes in detail the design of the LZ technical systems. Expected backgrounds are quantified and the performance of the experiment is presented. The LZ detector will be located at the Sanford Underground Research Facility in South Dakota. The organization of the LZ Project and a summary of the expected cost and current schedule are given., Comment: 278 pages. Submitted to the Department of Energy as part of the documentation for the Critical Decision Number One (CD-1) management process. Report also available by chapter at http://hep.ucsb.edu/LZ/CDR. This version includes corrections of minor typographic errors
Published: 2015

71. Energy and Flux Measurements of Ultra-High Energy Cosmic Rays Observed During the First ANITA Flight

Author: Schoorlemmer, H., Belov, K., Romero-Wolf, A., García-Fernández, D., Bugaev, V., Wissel, S. A., Allison, P., Alvarez-Muñiz, J., Barwick, S. W., Beatty, J. J., Besson, D. Z., Binns, W. R., Carvalho Jr., W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Dowkontt, P. F., DuVernois, M. A., Field, R. C., Goldstein, D., Gorham, P. W., Hast, C., Heber, C. L., Huege, T., Hoover, S., Israel, M. H., Javaid, A., Kowalski, J., Lam, J., Learned, J. G., Liewer, K. M., Link, J. T., Lusczek, E., Matsuno, S., Mercurio, B. C., Miki, C., Miočinović, P., Mulrey, K., Nam, J., Naudet, C. J., Ng, J., Nichol, R. J., Palladino, K., Rauch, B. F., Roberts, J., Reil, K., Rotter, B., Rosen, M., Ruckman, L., Saltzberg, D., Seckel, D., Urdaneta, D., Varner, G. S., Vieregg, A. G., Walz, D., Wu, F., and Zas, E.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The first flight of the Antarctic Impulsive Transient Antenna (ANITA) experiment recorded 16 radio signals that were emitted by cosmic-ray induced air showers. For 14 of these events, this radiation was reflected from the ice. The dominant contribution to the radiation from the deflection of positrons and electrons in the geomagnetic field, which is beamed in the direction of motion of the air shower. This radiation is reflected from the ice and subsequently detected by the ANITA experiment at a flight altitude of 36km. In this paper, we estimate the energy of the 14 individual events and find that the mean energy of the cosmic-ray sample is 2.9 EeV. By simulating the ANITA flight, we calculate its exposure for ultra-high energy cosmic rays. We estimate for the first time the cosmic-ray flux derived only from radio observations. In addition, we find that the Monte Carlo simulation of the ANITA data set is in agreement with the total number of observed events and with the properties of those events., Comment: Added more explanation of the experimental setup and textual improvements
Published: 2015
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72. Energy and flux measurements of ultra-high energy cosmic rays observed during the first ANITA flight

Author: Schoorlemmer, H, Belov, K, Romero-Wolf, A, García-Fernández, D, Bugaev, V, Wissel, SA, Allison, P, Alvarez-Muñiz, J, Barwick, SW, Beatty, JJ, Besson, DZ, Binns, WR, Carvalho, WR, Chen, C, Chen, P, Clem, JM, Connolly, A, Dowkontt, PF, DuVernois, MA, Field, RC, Goldstein, D, Gorham, PW, Hast, C, Huege, T, Heber, CL, Hoover, S, Israel, MH, Javaid, A, Kowalski, J, Lam, J, Learned, JG, Link, JT, Lusczek, E, Matsuno, S, Mercurio, BC, Miki, C, Miočinović, P, Mulrey, K, Nam, J, Naudet, CJ, Ng, J, Nichol, RJ, Palladino, K, Rauch, BF, Roberts, J, Reil, K, Rotter, B, Rosen, M, Ruckman, L, Saltzberg, D, Seckel, D, Urdaneta, D, Varner, GS, Vieregg, AG, Walz, D, Wu, F, and Zas, E
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Cosmic rays, Air shower, Radio detection, astro-ph.HE, astro-ph.IM, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: The first flight of the Antarctic Impulsive Transient Antenna (ANITA) experiment recorded 16 radio signals that were emitted by cosmic-ray induced air showers. The dominant contribution to the radiation comes from the deflection of positrons and electrons in the geomagnetic field, which is beamed in the direction of motion of the air shower. For 14 of these events, this radiation is reflected from the ice and subsequently detected by the ANITA experiment at a flight altitude of ∼36 km. In this paper, we estimate the energy of the 14 individual events and find that the mean energy of the cosmic-ray sample is 2.9 × 1018 eV, which is significantly lower than the previous estimate. By simulating the ANITA flight, we calculate its exposure for ultra-high energy cosmic rays. We estimate for the first time the cosmic-ray flux derived only from radio observations and find agreement with measurements performed at other observatories. In addition, we find that the ANITA data set is consistent with Monte Carlo simulations for the total number of observed events and with the properties of those events.
Published: 2016

73. DEAP-3600 Dark Matter Search

Author: DEAP Collaboration, Amaudruz, P. -A., Batygov, M., Beltran, B., Bonatt, J., Boulay, M. G., Broerman, B., Bueno, J. F., Butcher, A., Cai, B., Chen, M., Chouinard, R., Cleveland, B. T., Dering, K., DiGioseffo, J., Duncan, F., Flower, T., Ford, R., Giampa, P., Gorel, P., Graham, K., Grant, D. R., Guliyev, E., Hallin, A. L., Hamstra, M., Harvey, P., Jillings, C. J., Kuźniak, M., Lawson, I., Li, O., Liimatainen, P., Majewski, P., McDonald, A. B., McElroy, T., McFarlane, K., Monroe, J., Muir, A., Nantais, C., Ng, C., Noble, A. J., Ouellet, C., Palladino, K., Pasuthip, P., Peeters, S. J. M., Pollmann, T., Rau, W., Retière, F., Seeburn, N., Singhrao, K., Skensved, P., Smith, B., Sonley, T., Tang, J., Vázquez-Jáuregui, E., Veloce, L., Walding, J., and Ward, M.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract: The DEAP-3600 experiment is located 2 km underground at SNOLAB, in Sudbury, Ontario. It is a single-phase detector that searches for dark matter particle interactions within a 1000-kg fiducial mass target of liquid argon. A first generation prototype detector (DEAP-1) with a 7-kg liquid argon target mass demonstrated a high level of pulse-shape discrimination (PSD) for reducing $\beta$/$\gamma$ backgrounds and helped to develop low radioactivity techniques to mitigate surface-related $\alpha$ backgrounds. Construction of the DEAP-3600 detector is nearly complete and commissioning is starting in 2014. The target sensitivity to spin-independent scattering of Weakly Interacting Massive Particles (WIMPs) on nucleons of 10$^{-46}$ cm$^2$ will allow one order of magnitude improvement in sensitivity over current searches at 100 GeV WIMP mass. This paper presents an overview and status of the DEAP-3600 project and discusses plans for a future multi-tonne experiment, DEAP-50T., Comment: International Conference on High Energy Physics (ICHEP 2014), Valencia, 2014
Published: 2014
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74. Improving Photoelectron Counting and Particle Identification in Scintillation Detectors with Bayesian Techniques

Author: Akashi-Ronquest, M., Amaudruz, P. -A., Batygov, M., Beltran, B., Bodmer, M., Boulay, M. G., Broerman, B., Buck, B., Butcher, A., Cai, B., Caldwell, T., Chen, M., Chen, Y., Cleveland, B., Coakley, K., Dering, K., Duncan, F. A., Formaggio, J. A., Gagnon, R., Gastler, D., Giuliani, F., Gold, M., Golovko, V. V., Gorel, P., Graham, K., Grace, E., Guerrero, N., Guiseppe, V., Hallin, A. L., Harvey, P., Hearns, C., Henning, R., Hime, A., Hofgartner, J., Jaditz, S., Jillings, C. J., Kachulis, C., Kearns, E., Kelsey, J., Klein, J. R., Kuzniak, M., LaTorre, A., Lawson, I., Li, O., Lidgard, J. J., Liimatainen, P., Linden, S., McFarlane, K., McKinsey, D. N., MacMullin, S., Mastbaum, A., Mathew, R., McDonald, A. B., Mei, D. -M., Monroe, J., Muir, A., Nantais, C., Nicolics, K., Nikkel, J. A., Noble, T., O'Dwyer, E., Olsen, K., Gann, G. D. Orebi, Ouellet, C., Palladino, K., Pasuthip, P., Perumpilly, G., Pollmann, T., Rau, P., Retiere, F., Rielage, K., Schnee, R., Seibert, S., Skensved, P., Sonley, T., Vazquez-Jauregui, E., Veloce, L., Walding, J., Wang, B., Wang, J., Ward, M., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment, Nuclear Experiment
Abstract: Many current and future dark matter and neutrino detectors are designed to measure scintillation light with a large array of photomultiplier tubes (PMTs). The energy resolution and particle identification capabilities of these detectors depend in part on the ability to accurately identify individual photoelectrons in PMT waveforms despite large variability in pulse amplitudes and pulse pileup. We describe a Bayesian technique that can identify the times of individual photoelectrons in a sampled PMT waveform without deconvolution, even when pileup is present. To demonstrate the technique, we apply it to the general problem of particle identification in single-phase liquid argon dark matter detectors. Using the output of the Bayesian photoelectron counting algorithm described in this paper, we construct several test statistics for rejection of backgrounds for dark matter searches in argon. Compared to simpler methods based on either observed charge or peak finding, the photoelectron counting technique improves both energy resolution and particle identification of low energy events in calibration data from the DEAP-1 detector and simulation of the larger MiniCLEAN dark matter detector., Comment: 16 pages, 16 figures
Published: 2014
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75. Update on the MiniCLEAN Dark Matter Experiment

Author: Rielage, K., Akashi-Ronquest, M., Bodmer, M., Bourque, R., Buck, B., Butcher, A., Caldwell, T., Chen, Y., Coakley, K., Flores, E., Formaggio, J. A., Gastler, D., Giuliani, F., Gold, M., Grace, E., Griego, J., Guerrero, N., Guiseppe, V., Henning, R., Hime, A., Jaditz, S., Kachulis, C., Kearns, E., Kelsey, J., Klein, J. R., Latorre, A., Lawson, I., Linden, S., Lopez, F., McKinsey, D. N., MacMullin, S., Mastbaum, A., Mei, D. -M., Monroe, J., Nikkel, J. A., Oertel, J., Gann, G. D. Orebi, Palladino, K., Perumpilly, G., Rodriguez, L., Schnee, R., Seibert, S., Walding, J., Wang, B., Wang, J., and Zhang, C.
Subjects: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract: The direct search for dark matter is entering a period of increased sensitivity to the hypothetical Weakly Interacting Massive Particle (WIMP). One such technology that is being examined is a scintillation only noble liquid experiment, MiniCLEAN. MiniCLEAN utilizes over 500 kg of liquid cryogen to detect nuclear recoils from WIMP dark matter and serves as a demonstration for a future detector of order 50 to 100 tonnes. The liquid cryogen is interchangeable between argon and neon to study the A$^{2}$ dependence of the potential signal and examine backgrounds. MiniCLEAN utilizes a unique modular design with spherical geometry to maximize the light yield using cold photomultiplier tubes in a single-phase detector. Pulse shape discrimination techniques are used to separate nuclear recoil signals from electron recoil backgrounds. MiniCLEAN will be spiked with additional $^{39}$Ar to demonstrate the effective reach of the pulse shape discrimination capability. Assembly of the experiment is underway at SNOLAB and an update on the project is given., Comment: To appear in the Proceedings of the TAUP 2013 Conference (F. Avignone & W. Haxton, editors, Physics Procedia, Elsevier)
Published: 2014

76. Erratum to: The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs

Author: Akerib, D. S., Akerlof, C. W., Akimov, D. Yu., Alquahtani, A., Alsum, S. K., Anderson, T. J., Angelides, N., Araújo, H. M., Arbuckle, A., Armstrong, J. E., Arthurs, M., Auyeung, H., Aviles, S., Bai, X., Bailey, A. J., Balajthy, J., Balashov, S., Bang, J., Barry, M. J., Bauer, D., Bauer, P., Baxter, A., Belle, J., Beltrame, P., Bensinger, J., Benson, T., Bernard, E. P., Bernstein, A., Bhatti, A., Biekert, A., Biesiadzinski, T. P., Birch, H. J., Birrittella, B., Boast, K. E., Bolozdynya, A. I., Boulton, E. M., Boxer, B., Bramante, R., Branson, S., Brás, P., Breidenbach, M., Brew, C. A. J., Buckley, J. H., Bugaev, V. V., Bunker, R., Burdin, S., Busenitz, J. K., Cabrita, R., Campbell, J. S., Carels, C., Carlsmith, D. L., Carlson, B., Carmona-Benitez, M. C., Cascella, M., Chan, C., Cherwinka, J. J., Chiller, A. A., Chiller, C., Chott, N. I., Cole, A., Coleman, J., Colling, D., Conley, R. A., Cottle, A., Coughlen, R., Cox, G., Craddock, W. W., Curran, D., Currie, A., Cutter, J. E., da Cunha, J. P., Dahl, C. E., Dardin, S., Dasu, S., Davis, J., Davison, T. J. R., de Viveiros, L., Decheine, N., Dobi, A., Dobson, J. E. Y., Druszkiewicz, E., Dushkin, A., Edberg, T. K., Edwards, W. R., Edwards, B. N., Edwards, J., Elnimr, M. M., Emmet, W. T., Eriksen, S. R., Faham, C. H., Fan, A., Fayer, S., Fiorucci, S., Flaecher, H., Florang, I. M. Fogarty, Ford, P., Francis, V. B., Fraser, E. D., Froborg, F., Fruth, T., Gaitskell, R. J., Gantos, N. J., Garcia, D., Gehman, V. M., Gelfand, R., Genovesi, J., Gerhard, R. M., Ghag, C., Gibson, E., Gilchriese, M. G. D., Gokhale, S., Gomber, B., Gonda, T. G., Greenall, A., Greenwood, S., Gregerson, G., van der Grinten, M. G. D., Gwilliam, C. B., Hall, C. R., Hamilton, D., Hans, S., Hanzel, K., Harrington, T., Harrison, A., Harrison, J., Hasselkus, C., Haselschwardt, S. J., Hemer, D., Hertel, S. A., Heise, J., Hillbrand, S., Hitchcock, O., Hjemfelt, C., Hoff, M. D., Holbrook, B., Holtom, E., Hor, J. Y-K., Horn, M., Huang, D. Q., Hurteau, T. W., Ignarra, C. M., Irving, M. N., Jacobsen, R. G., Jahangir, O., Jeffery, S. N., Ji, W., Johnson, M., Johnson, J., Johnson, P., Jones, W. G., Kaboth, A. C., Kamaha, A., Kamdin, K., Kasey, V., Kazkaz, K., Keefner, J., Khaitan, D., Khaleeq, M., Khazov, A., Khromov, A. V., Khurana, I., Kim, Y. D., Kim, W. T., Kocher, C. D., Kodroff, D., Konovalov, A. M., Korley, L., Korolkova, E. V., Koyuncu, M., Kras, J., Kraus, H., Kravitz, S. W., Krebs, H. J., Kreczko, L., Krikler, B., Kudryavtsev, V. A., Kumpan, A. V., Kyre, S., Lambert, A. R., Landerud, B., Larsen, N. A., Laundrie, A., Leason, E. A., Lee, H. S., Lee, J., Lee, C., Lenardo, B. G., Leonard, D. S., Leonard, R., Lesko, K. T., Levy, C., Li, J., Liu, Y., Liao, J., Liao, F.-T., Lin, J., Lindote, A., Linehan, R., Lippincott, W. H., Liu, R., Liu, X., Loniewski, C., Lopes, M. I., Lopez-Asamar, E., Paredes, B. López, Lorenzon, W., Lucero, D., Luitz, S., Lyle, J. M., Lynch, C., Majewski, P. A., Makkinje, J., Malling, D. C., Manalaysay, A., Manenti, L., Mannino, R. L., Marangou, N., Markley, D. J., MarrLaundrie, P., Martin, T. J., Marzioni, M. F., Maupin, C., McConnell, C. T., McKinsey, D. N., McLaughlin, J., Mei, D.-M., Meng, Y., Miller, E. H., Minaker, Z. J., Mizrachi, E., Mock, J., Molash, D., Monte, A., Monzani, M. E., Morad, J. A., Morrison, E., Mount, B. J., Murphy, A. St. J., Naim, D., Naylor, A., Nedlik, C., Nehrkorn, C., Nelson, H. N., Nesbit, J., Neves, F., Nikkel, J. A., Nikoleyczik, J. A., Nilima, A., O’Dell, J., Oh, H., O’Neill, F. G., O’Sullivan, K., Olcina, I., Olevitch, M. A., Oliver-Mallory, K. C., Oxborough, L., Pagac, A., Pagenkopf, D., Pal, S., Palladino, K. J., Palmaccio, V. M., Palmer, J., Pangilinan, M., Parveen, N., Patton, S. J., Pease, E. K., Penning, B. P., Pereira, G., Pereira, C., Peterson, I. B., Piepke, A., Pierson, S., Powell, S., Preece, R. M., Pushkin, K., Qie, Y., Racine, M., Ratcliff, B. N., Reichenbacher, J., Reichhart, L., Rhyne, C. A., Richards, A., Riffard, Q., Rischbieter, G. R. C., Rodrigues, J. P., Rose, H. J., Rosero, R., Rossiter, P., Rucinski, R., Rutherford, G., Saba, J. S., Sabarots, L., Santone, D., Sarychev, M., Sazzad, A. B. M. R., Schnee, R. W., Schubnell, M., Scovell, P. R., Severson, M., Seymour, D., Shaw, S., Shutt, G. W., Shutt, T. A., Silk, J. J., Silva, C., Skarpaas, K., Skulski, W., Smith, A. R., Smith, R. J., Smith, R. E., So, J., Solmaz, M., Solovov, V. N., Sorensen, P., Sosnovtsev, V. V., Stancu, I., Stark, M. R., Stephenson, S., Stern, N., Stevens, A., Stiegler, T. M., Stifter, K., Studley, R., Sumner, T. J., Sundarnath, K., Sutcliffe, P., Swanson, N., Szydagis, M., Tan, M., Taylor, W. C., Taylor, R., Taylor, D. J., Temples, D., Tennyson, B. P., Terman, P. A., Thomas, K. J., Thomson, J. A., Tiedt, D. R., Timalsina, M., To, W. H., Tomás, A., Tope, T. E., Tripathi, M., Tronstad, D. R., Tull, C. E., Turner, W., Tvrznikova, L., Utes, M., Utku, U., Uvarov, S., Va’vra, J., Vacheret, A., Vaitkus, A., Verbus, J. R., Vietanen, T., Voirin, E., Vuosalo, C. O., Walcott, S., Waldron, W. L., Walker, K., Wang, J. J., Wang, R., Wang, L., Wang, W., Wang, Y., Watson, J. R., Migneault, J., Weatherly, S., Webb, R. C., Wei, W.-Z., While, M., White, R. G., White, J. T., White, D. T., Whitis, T. J., Wisniewski, W. J., Wilson, K., Witherell, M. S., Wolfs, F. L. H., Wolfs, J. D., Woodward, D., Worm, S. D., Xiang, X., Xiao, Q., Xu, J., Yeh, M., Yin, J., Young, I., Zhang, C., and Zarzhitsky, P.
Published: 2022
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77. Snowmass CF1 Summary: WIMP Dark Matter Direct Detection

Author: Cushman, P., Galbiati, C., McKinsey, D. N., Robertson, H., Tait, T. M. P., Bauer, D., Borgland, A., Cabrera, B., Calaprice, F., Cooley, J., Empl, T., Essig, R., Figueroa-Feliciano, E., Gaitskell, R., Golwala, S., Hall, J., Hill, R., Hime, A., Hoppe, E., Hsu, L., Hungerford, E., Jacobsen, R., Kelsey, M., Lang, R. F., Lippincott, W. H., Loer, B., Luitz, S., Mandic, V., Mardon, J., Maricic, J., Maruyama, R., Mahapatra, R., Nelson, H., Orrell, J., Palladino, K., Pantic, E., Partridge, R., Ryd, A., Saab, T., Sadoulet, B., Schnee, R., Shepherd, W., Sonnenschein, A., Sorensen, P., Szydagis, M., Volansky, T., Witherell, M., Wright, D., and Zurek, K.
Subjects: High Energy Physics - Experiment, Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors
Abstract: As part of the Snowmass process, the Cosmic Frontier WIMP Direct Detection subgroup (CF1) has drawn on input from the Cosmic Frontier and the broader Particle Physics community to produce this document. The charge to CF1 was (a) to summarize the current status and projected sensitivity of WIMP direct detection experiments worldwide, (b) motivate WIMP dark matter searches over a broad parameter space by examining a spectrum of WIMP models, (c) establish a community consensus on the type of experimental program required to explore that parameter space, and (d) identify the common infrastructure required to practically meet those goals., Comment: Snowmass CF1 Final Summary Report: 47 pages and 28 figures with a 5 page appendix on instrumentation R&D
Published: 2013

78. Antarctic Radio Frequency Albedo and Implications for Cosmic Ray Reconstruction

Author: Besson, D. Z., Stockham, J., Sullivan, M., Allison, P., Barwick, S. W., Baughman, B. M., Beatty, J. J., Belov, K., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., De Marco, D., Dowkontt, P. F., DuVernois, M., Goldstein, D., Gorham, P. W., Grashorn, E. W., Hill, B., Hoover, S., Huang, M., Israel, M. H., Javaid, A., Kowalski, J., Learned, J., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Naudet, C. J., Nichol, R. J., Palladino, K., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Shang, R. Y., Stockham, M., Varner, G. S., Vieregg, A. G., and Wang, Y.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: From an elevation of ~38 km, the balloon-borne ANtarctic Impulsive Transient Antenna (ANITA) is designed to detect the up-coming radio frequency (RF) signal resulting from a sub-surface neutrino-nucleon collision. Although no neutrinos have been discovered thus far, ANITA is nevertheless the only experiment to self-trigger on radio frequency emissions from cosmic-ray induced atmospheric air showers. In the majority of those cases, down-coming RF signals are observed via their reflection from the Antarctic ice sheet and back up to the ANITA interferometer. Estimating the energy scale of the incident cosmic rays therefore requires an estimate of the fractional power reflected at the air-ice interface. Similarly, inferring the energy of neutrinos interacting in-ice from observations of the upwards-directed signal refracting out to ANITA also requires consideration of signal coherence across the interface. By comparing the direct Solar RF signal intensity measured with ANITA to the surface-reflected Solar signal intensity, as a function of incident elevation angle relative to the surface {\Theta}, we estimate the power reflection coefficients R({\Theta}). We find general consistency between our average measurements and the values of R({\Theta}) expected from the Fresnel equations, separately for horizontal- vs. vertical-polarizations., Comment: final version as accepted for publication by Radio Science
Published: 2013

79. The First Limits on the Ultra-high Energy Neutrino Fluence from Gamma-ray Bursts

Author: Vieregg, A. G., Palladino, K., Allison, P., Baughman, B. M., Beatty, J. J., Belov, K., Besson, D. Z., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Detrixhe, M., De Marco, D., Dowkontt, P. F., DuVernois, M., Gorham, P. W., Grashorn, E. W., Hill, B., Hoover, S., Huang, M., Israel, M. H., Javaid, A., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Nichol, R. J., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G. S., and Wang, Y.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We set the first limits on the ultra-high energy (UHE) neutrino fluence at energies greater than 10^9 GeV from gamma-ray bursts (GRBs) based on data from the second flight of the ANtarctic Impulsive Transient Antenna (ANITA). During the 31 day flight of ANITA-II, 26 GRBs were recorded by Swift or Fermi. Of these, we analyzed the 12 GRBs which occurred during quiet periods when the payload was away from anthropogenic activity. In a blind analysis, we observe 0 events on a total background of 0.0044 events in the combined prompt window for all 12 low-background bursts. We also observe 0 events from the remaining 14 bursts. We place a 90% confidence level limit on the E^-4 prompt neutrino fluence of 2.5x10^17 GeV^3/cm^2 between 10^8 and 10^12 GeV from GRB090107A. This is the first reported limit on the UHE neutrino fluence from GRBs above 10^9 GeV, and the strongest limit above 10^8 GeV., Comment: 4 pages, 2 figures, submitted to ApJ
Published: 2011
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80. Erratum: Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment

Author: Gorham, P. W., Allison, P., Baughman, B. M., Beatty, J. J., Belov, K., Besson, D. Z., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Detrixhe, M., De Marco, D., Dowkontt, P. F., DuVernois, M., Grashorn, E. W., Hill, B., Hoover, S., Huang, M., Israel, M. H., Javaid, A., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Nichol, R. J., Palladino, K., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Shang, R. Y., Varner, G. S., Vieregg, A. G., and Wang, Y.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: This is an erratum to our paper in Physical Review D82:022004,2010, corresponding to preprint: arXiv:1003.2961 ., Comment: 2 pages, 1 figure, 1 table. Erratum
Published: 2010
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81. Ultra-Relativistic Magnetic Monopole Search with the ANITA-II Balloon-borne Radio Interferometer

Author: Detrixhe, M., Besson, D., Gorham, P. W., Allison, P., Baughmann, B., Beatty, J. J., Belov, K., Bevan, S., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., DeMarco, D., Dowkontt, P. F., Duvernois, M. A., Frankenfeld, C., Grashorn, E. W., Hogan, D. P., Griffith, N., Hill, B., Hoover, S., Israel, M. H., Javaid, A., Liewer, K. M., Matsuno, S., Mercurio, B. C., Miki, C., Mottram, M., Nam, J., Nichol, R. J., Palladino, K., Romero-Wolf, A., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G. S., Vieregg, A. G., and Wang, Y.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We have conducted a search for extended energy deposition trails left by ultra-relativistic magnetic monopoles interacting in Antarctic ice. The non-observation of any satisfactory candidates in the 31 days of accumulated ANITA-II flight data results in an upper limit on the diffuse flux of relativistic monopoles. We obtain a 90% C.L. limit of order 10^{-19}/(cm^2-s-sr) for values of Lorentz boost factor 10^{10}
Published: 2010
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82. Observation of Ultra-high-energy Cosmic Rays with the ANITA Balloon-borne Radio Interferometer

Author: Hoover, S., Nam, J., Gorham, P. W., Grashorn, E., Allison, P., Barwick, S. W., Beatty, J. J., Belov, K., Besson, D. Z., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Dowkontt, P. F., DuVernois, M. A., Field, R. C., Goldstein, D., Vieregg, A. G., Hast, C., Hebert, C. L., Israel, M. H., Javaid, A., Kowalski, J., Learned, J. G., Liewer, K. M., Link, J. T., Lusczek, E., Matsuno, S., Mercurio, B. C., Miki, C., Miočinović, P., Naudet, C. J., Ng, J., Nichol, R. J., Palladino, K., Reil, K., Romero-Wolf, A., Rosen, M., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G. S., Walz, D., and Wu, F.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We report the observation of sixteen cosmic ray events of mean energy of 1.5 x 10^{19} eV, via radio pulses originating from the interaction of the cosmic ray air shower with the Antarctic geomagnetic field, a process known as geosynchrotron emission. We present the first ultra-wideband, far-field measurements of the radio spectral density of geosynchrotron emission in the range from 300-1000 MHz. The emission is 100% linearly polarized in the plane perpendicular to the projected geomagnetic field. Fourteen of our observed events are seen to have a phase-inversion due to reflection of the radio beam off the ice surface, and two additional events are seen directly from above the horizon., Comment: 5 pages, 5 figures, new figure added
Published: 2010
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83. New Limits on the Ultra-high Energy Cosmic Neutrino Flux from the ANITA Experiment

Author: ANITA collaboration, Gorham, P., Allison, P., Barwick, S., Beatty, J., Besson, D., Binns, W., Chen, C., Chen, P., Clem, J., Connolly, A., Dowkontt, P., DuVernois, M., Field, R., Goldstein, D., Goodhue, A., Hast, C., Hebert, C., Hoover, S., Israel, M., Kowalski, J., Learned, J., Liewer, K., Link, J., Lusczek, E., Matsuno, S., Mercurio, B., Miki, C., Miocinovic, P., Nam, J., Naudet, C., Nichol, R., Palladino, K., Reil, K., Romero-Wolf, A., Rosen, M., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G., Walz, D., Wang, Y., and Wu, F.
Subjects: Astrophysics
Abstract: We report initial results of the first flight of the Antarctic Impulsive Transient Antenna (ANITA-1) 2006-2007 Long Duration Balloon flight, which searched for evidence of a diffuse flux of cosmic neutrinos above energies of 3 EeV. ANITA-1 flew for 35 days looking for radio impulses due to the Askaryan effect in neutrino-induced electromagnetic showers within the Antarctic ice sheets. We report here on our initial analysis, which was performed as a blind search of the data. No neutrino candidates are seen, with no detected physics background. We set model-independent limits based on this result. Upper limits derived from our analysis rule out the highest cosmogenic neutrino models. In a background horizontal-polarization channel, we also detect six events consistent with radio impulses from ultra-high energy extensive air showers., Comment: 4 pages, 2 tables
Published: 2008
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84. The Antarctic Impulsive Transient Antenna Ultra-high Energy Neutrino Detector Design, Performance, and Sensitivity for 2006-2007 Balloon Flight

Author: ANITA collaboration, Gorham, P., Allison, P., Barwick, S., Beatty, J., Besson, D., Binns, W., Chen, C., Chen, P., Clem, J., Connolly, A., Dowkontt, P., DuVernois, M., Field, R., Goldstein, D., Goodhue, A., Hast, C., Hebert, C., Hoover, S., Israel, M., Kowalski, J., Learned, J., Liewer, K., Link, J., Lusczek, E., Matsuno, S., Mercurio, B., Miki, C., Miocinovic, P., Nam, J., Naudet, C., Nichol, R., Palladino, K., Reil, K., Romero-Wolf, A., Rosen, M., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G., Walz, D., Wang, Y., and Wu, F.
Subjects: Astrophysics, High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract: We present a detailed report on the experimental details of the Antarctic Impulsive Transient Antenna (ANITA) long duration balloon payload, including the design philosophy and realization, physics simulations, performance of the instrument during its first Antarctic flight completed in January of 2007, and expectations for the limiting neutrino detection sensitivity. Neutrino physics results will be reported separately., Comment: 50 pages, 49 figures, in preparation for PRD
Published: 2008
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85. In situ radioglaciological measurements near Taylor Dome, Antarctica and implications for UHE neutrino astronomy

Author: Besson, D., Jenkins, J., Matsuno, S., Nam, J., Smith, M., Barwick, S. W., Beatty, J. J., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Dowkontt, P. F., DuVernois, M. A., Field, R. C., Goldstein, D., Gorham, P. W., Goodhue, A., Hast, C., Hebert, C. L., Hoover, S., Israel, M. H., Kowalski, J., Learned, J. G., Liewer, K. M., Link, J. T., Lusczek, E., Mercurio, B., Miki, C., Miocinovic, P., Naudet, C. J., Ng, J., Nichol, R., Palladino, K., Reil, K., Romero-Wolf, A., Rosen, M., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G. S., Walz, D., and Wu, F.
Subjects: Astrophysics
Abstract: Radiowave detection of the Cherenkov radiation produced by neutrino-ice collisions requires an understanding of the radiofrequency (RF) response of cold polar ice. We herein report on a series of radioglaciological measurements performed approximately 10 km north of Taylor Dome Station, Antarctica from Dec. 6, 2006 - Dec. 16, 2006. Using RF signals broadcast from: a) an englacial discone, submerged to a depth of 100 meters and broadcasting to a surface dual polarization horn receiver, and b) a dual-polarization horn antenna on the surface transmitting signals which reflect off the underlying bed and back up to the surface receiver, we have made time-domain estimates of both the real (index-of-refraction) and imaginary (attenuation length) components of the complex ice dielectric constant. We have also measured the uniformity of ice response along two orthogonal axes in the horizontal plane. We observe a wavespeed asymmetry of order 0.1%, projected onto the vertical propagation axis, consistent with some previous measurements, but somewhat lower than others., Comment: replacement of previous arXiv version with published version
Published: 2007
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86. Observations of the Askaryan Effect in Ice

Author: ANITA collaboration, Gorham, P. W., Barwick, S. W., Beatty, J. J., Besson, D. Z., Binns, W. R., Chen, C., Chen, P., Clem, J. M., Connolly, A., Dowkontt, P. F., DuVernois, M. A., Field, R. C., Goldstein, D., Goodhue, A., Hast, C., Hebert, C. L., Hoover, S., Israel, M. H., Kowalski, J., Learned, J. G., Liewer, K. M., Link, J. T., Lusczek, E., Matsuno, S., Mercurio, B., Miki, C., Miocinovic, P., Nam, J., Naudet, C. J., Ng, J., Nichol, R., Palladino, K., Reil, K., Romero-Wolf, A., Rosen, M., Saltzberg, D., Seckel, D., Varner, G. S., Walz, D., and Wu, F.
Subjects: High Energy Physics - Experiment, Astrophysics, Physics - Instrumentation and Detectors
Abstract: We report on the first observations of the Askaryan effect in ice: coherent impulsive radio Cherenkov radiation from the charge asymmetry in an electromagnetic (EM) shower. Such radiation has been observed in silica sand and rock salt, but this is the first direct observation from an EM shower in ice. These measurements are important since the majority of experiments to date that rely on the effect for ultra-high energy neutrino detection are being performed using ice as the target medium. As part of the complete validation process for the Antarctic Impulsive Transient Antenna (ANITA) experiment, we performed an experiment at the Stanford Linear Accelerator Center (SLAC) in June 2006 using a 7.5 metric ton ice target, yielding results fully consistent with theoretical expectations., Comment: 4 pages, 5 figures, minor corrections
Published: 2006
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87. Constraints on Cosmic Neutrino Fluxes from the ANITA Experiment

Author: ANITA collaboration, Barwick, S. W., Beatty, J. J., Besson, D. Z., Binns, W. R., Cai, B., Clem, J. M., Connolly, A., Cowen, D. F., Dowkontt, P. F., DuVernois, M. A., Evenson, P. A., Goldstein, D., Gorham, P. W., Hebert, C. L., Israel, M. H., Learned, J. G., Liewer, K. M., Link, J. T., Matsuno, S., Miocinovic, P., Nam, J., Naudet, C. J., Nichol, R., Palladino, K., Rosen, M., Saltzberg, D., Seckel, D., Silvestri, A., Stokes, B. T., Varner, G. S., and Wu, F.
Subjects: Astrophysics
Abstract: We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Transient Antenna (ANITA) experiment, which completed an 18.4 day flight of a prototype long-duration balloon payload, called ANITA-lite, in early 2004. We search for impulsive events that could be associated with ultra-high energy neutrino interactions in the ice, and derive limits that constrain several models for ultra-high energy neutrino fluxes. We rule out the long-standing Z-burst model as the source for the ultra-high energy cosmic rays., Comment: 4 pages, 3 figures, accepted to PRL
Published: 2005
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88. Tuning into UHE Neutrinos in Antarctica - The ANITA Experiment

Author: Miocinovic, P., Barwick, S. W., Beatty, J. J., Besson, D. Z., Binns, W. R., Cai, B., Clem, J. M., Connolly, A., Coutu, S., Cowen, D. F., Dowkontt, P. F., DuVernois, M. A., Evenson, P. A., Goldstein, D., Gorham, P. W., Hebert, C. L., Israel, M. H., Learned, J. G., Liewer, K. M., Link, J. T., Matsuno, S., Nam, J. W., Naudet, C. J., Nichol, R., Palladino, K. J., Rosen, M., Saltzberg, D., Seckel, D., Silvestri, A., Varner, G. S., and Williams, D.
Subjects: Astrophysics
Abstract: The Antarctic Impulsive Transient Antenna (ANITA) experiment is being developed to search for ultra-high-energy (UHE) neutrino interactions ($>3\times10^{18}$ eV) in the Antarctic ice cap. A neutrino interaction in the ice will produce a radio pulse by the means of the Askaryan effect. The large radio transparency of ice allows for such a pulse to be recorded by a cluster of balloon-borne antennas. The details of the ANITA instrument, now in a construction phase, and the science we hope to achieve is discussed. In order to prepare for the main mission, we have flown ANITA-lite during the 2003/04 austral season. ANITA-lite consisted of two quad-ridge horn antennas and a prototype RF (radio frequency) triggering and recording system. Here we present the results of an impulsive RF background survey of Antarctica, as well as proof-of-principle gain, tracking, and timing calibrations conducted by observing solar radio emissions and calibration radio-pulses. A preliminary UHE neutrino flux limit based on ANITA-lite data is also presented., Comment: Presented at 22nd Texas Symposium on Relativistic Astrophysics at Stanford, Palo Alto, 13-17 December 2004, (TSRA04-2516) 6 pages, LaTeX, 10 eps figures
Published: 2005

89. Snowmass CF1 Summary: WIMP Dark Matter Direct Detection

Author: Cushman, P, Galbiati, C, McKinsey, DN, Robertson, H, Tait, TMP, Bauer, D, Borgland, A, Cabrera, B, Calaprice, F, Cooley, J, Empl, T, Essig, R, Figueroa-Feliciano, E, Gaitskell, R, Golwala, S, Hall, J, Hill, R, Hime, A, Hoppe, E, Hsu, L, Hungerford, E, Jacobsen, R, Kelsey, M, Lang, RF, Lippincott, WH, Loer, B, Luitz, S, Mandic, V, Mardon, J, Maricic, J, Maruyama, R, Mahapatra, R, Nelson, H, Orrell, J, Palladino, K, Pantic, E, Partridge, R, Ryd, A, Saab, T, Sadoulet, B, Schnee, R, Shepherd, W, Sonnenschein, A, Sorensen, P, Szydagis, M, Volansky, T, Witherell, M, Wright, D, and Zurek, K
Subjects: hep-ex, astro-ph.CO, astro-ph.HE, astro-ph.IM, physics.ins-det
Abstract: As part of the Snowmass process, the Cosmic Frontier WIMP Direct Detectionsubgroup (CF1) has drawn on input from the Cosmic Frontier and the broaderParticle Physics community to produce this document. The charge to CF1 was (a)to summarize the current status and projected sensitivity of WIMP directdetection experiments worldwide, (b) motivate WIMP dark matter searches over abroad parameter space by examining a spectrum of WIMP models, (c) establish acommunity consensus on the type of experimental program required to explorethat parameter space, and (d) identify the common infrastructure required topractically meet those goals.
Published: 2013

90. Background determination for the LUX-ZEPLIN dark matter experiment

Author: Aalbers, J., Akerib, D. S., Musalhi, A. K. Al, Alder, F., Alsum, S. K., Amarasinghe, C. S., Ames, A., Anderson, T. J., Angelides, N., Araújo, H. M., Armstrong, J. E., Arthurs, M., Baker, A., Bang, J., Bargemann, J. W., Baxter, A., Beattie, K., Beltrame, P., Bernard, E. P., Bhatti, A., Biekert, A., Biesiadzinski, T. P., Birch, H. J., Blockinger, G. M., Boxer, B., Brew, C. A. J., Brás, P., Burdin, S., Buuck, M., Cabrita, R., Carmona-Benitez, M. C., Chan, C., Chawla, A., Chen, H., Chiang, A. P. S., Chott, N. I., Converse, M. V., Cottle, A., Cox, G., Creaner, O., Dahl, C. E., David, A., Dey, S., de Viveiros, L., Ding, C., Dobson, J. E. Y., Druszkiewicz, E., Eriksen, S. R., Fan, A., Fearon, N. M., Fiorucci, S., Flaecher, H., Fraser, E. D., Fruth, T., Gaitskell, R. J., Genovesi, J., Ghag, C., Gibbons, R., Gilchriese, M. G. D., Gokhale, S., Green, J., van der Grinten, M. G. D., Gwilliam, C. B., Hall, C. R., Han, S., Hartigan-O’Connor, E., Haselschwardt, S. J., Hertel, S. A., Heuermann, G., Horn, M., Huang, D. Q., Hunt, D., Ignarra, C. M., Jacobsen, R. G., Jahangir, O., James, R. S., Johnson, J., Kaboth, A. C., Kamaha, A. C., Khaitan, D., Khurana, I., Kirk, R., Kodroff, D., Korley, L., Korolkova, E. V., Kraus, H., Kravitz, S., Kreczko, L., Krikler, B., Kudryavtsev, V. A., Leason, E. A., Lee, J., Leonard, D. S., Lesko, K. T., Levy, C., Lin, J., Lindote, A., Linehan, R., Lippincott, W. H., Liu, X., Lopes, M. I., Asamar, E. Lopez, Paredes, B. López, Lorenzon, W., Lu, C., Luitz, S., Majewski, P. A., Manalaysay, A., Mannino, R. L., Marangou, N., McCarthy, M. E., McKinsey, D. N., McLaughlin, J., Miller, E. H., Mizrachi, E., Monte, A., Monzani, M. E., Mendoza, J. D. Morales, Morrison, E., Mount, B. J., Murdy, M., Murphy, A. St. J., Naim, D., Naylor, A., Nedlik, C., Nelson, H. N., Neves, F., Nguyen, A., Nikoleyczik, J. A., Olcina, I., Oliver-Mallory, K. C., Orpwood, J., Palladino, K. J., Palmer, J., Parveen, N., Patton, S. J., Penning, B., Pereira, G., Perry, E., Pershing, T., Piepke, A., Porzio, D., Poudel, S., Qie, Y., Reichenbacher, J., Rhyne, C. A., Riffard, Q., Rischbieter, G. R. C., Riyat, H. S., Rosero, R., Rossiter, P., Rushton, T., Santone, D., Sazzad, A. B. M. R., Schnee, R. W., Shaw, S., Shutt, T., Silk, J. J., Silva, C., Sinev, G., Smith, R., Solmaz, M., Solovov, V. N., Sorensen, P., Soria, J., Stancu, I., Stevens, A., Stifter, K., Suerfu, B., Sumner, T. J., Swanson, N., Szydagis, M., Taylor, R., Taylor, W. C., Temples, D. J., Terman, P. A., Tiedt, D. R., Timalsina, M., Tong, Z., Tovey, D. R., Tranter, J., Trask, M., Tripathi, M., Tronstad, D. R., Turner, W., Utku, U., Vaitkus, A. C., Wang, A., Wang, J. J., Wang, W., Wang, Y., Watson, J. R., Webb, R. C., Whitis, T. J., Williams, M., Wolfs, F. L. H., Woodford, S., Woodward, D., Wright, C. J., Xia, Q., Xiang, X., Xu, J., and Yeh, M.
Abstract: The LUX-ZEPLIN experiment recently reported limits on WIMP-nucleus interactions from its initial science run, down to 9.2×10−48 cm2 for the spin-independent interaction of a 36 GeV/c2 WIMP at 90% confidence level. In this paper, we present a comprehensive analysis of the backgrounds important for this result and for other upcoming physics analyses, including neutrinoless double-beta decay searches and effective field theory interpretations of LUX-ZEPLIN data. We confirm that the in-situ determinations of bulk and fixed radioactive backgrounds are consistent with expectations from the ex-situ assays. The observed background rate after WIMP search criteria were applied was (6.3±0.5)×10−5 events/keVee/kg/day in the low-energy region, approximately 60 times lower than the equivalent rate reported by the LUX experiment.
Published: 2023

91. A next-generation liquid xenon observatory for dark matter and neutrino physics

Author: Aalbers, J, AbdusSalam, S S, Abe, K, Aerne, V, Agostini, F, Ahmed Maouloud, S, Akerib, D S, Akimov, D Y, Akshat, J, Al Musalhi, A K, Alder, F, Alsum, S K, Althueser, L, Amarasinghe, C S, Amaro, F D, Ames, A, Anderson, T J, Andrieu, B, Angelides, N, Angelino, E, Angevaare, J, Antochi, V C, Antón Martin, D, Antunovic, B, Aprile, E, Araújo, H M, Armstrong, J E, Arneodo, F, Arthurs, M, Asadi, P, Baek, S, Bai, X, Bajpai, D, Baker, A, Balajthy, J, Balashov, S, Balzer, M, Bandyopadhyay, A, Bang, J, Barberio, E, Bargemann, J W, Baudis, L, Bauer, D, Baur, D, Baxter, A, Baxter, A L, Bazyk, M, Beattie, K, Behrens, J, Bell, N F, Bellagamba, L, Beltrame, P, Benabderrahmane, M, Bernard, E P, Bertone, G F, Bhattacharjee, P, Bhatti, A, Biekert, A, Biesiadzinski, T P, Binau, A R, Biondi, R, Biondi, Y, Birch, H J, Bishara, F, Bismark, A, Blanco, C, Blockinger, G M, Bodnia, E, Boehm, C, Bolozdynya, A I, Bolton, P D, Bottaro, S, Bourgeois, C, Boxer, B, Brás, P, Breskin, A, Breur, P A, Brew, C A J, Brod, J, Brookes, E, Brown, A, Brown, E, Bruenner, S, Bruno, G, Budnik, R, Bui, T K, Burdin, S, Buse, S, Busenitz, J K, Buttazzo, D, Buuck, M, Buzulutskov, A, Cabrita, R, Cai, C, Cai, D, Capelli, C, Cardoso, J M R, Carmona-Benitez, M C, Cascella, M, Catena, R, Chakraborty, S, Chan, C, Chang, S, Chauvin, A, Chawla, A, Chen, H, Chepel, V, Chott, N I, Cichon, D, Cimental Chavez, A, Cimmino, B, Clark, M, Co, R T, Colijn, A P, Conrad, J, Converse, M V, Costa, M, Cottle, A, Cox, G, Creaner, O, Cuenca Garcia, J J, Cussonneau, J P, Cutter, J E, Dahl, C E, D’Andrea, V, David, A, Decowski, M P, Dent, J B, Deppisch, F F, de Viveiros, L, Di Gangi, P, Di Giovanni, A, Di Pede, S, Dierle, J, Diglio, S, Dobson, J E Y, Doerenkamp, M, Douillet, D, Drexlin, G, Druszkiewicz, E, Dunsky, D, Eitel, K, Elykov, A, Emken, T, Engel, R, Eriksen, S R, Fairbairn, M, Fan, A, Fan, J J, Farrell, S J, Fayer, S, Fearon, N M, Ferella, A, Ferrari, C, Fieguth, A, Fiorucci, S, Fischer, H, Flaecher, H, Flierman, M, Florek, T, Foot, R, Fox, P J, Franceschini, R, Fraser, E D, Frenk, C S, Frohlich, S, Fruth, T, Fulgione, W, Fuselli, C, Gaemers, P, Gaior, R, Gaitskell, R J, Galloway, M, Gao, F, Garcia Garcia, I, Genovesi, J, Ghag, C, Ghosh, S, Gibson, E, Gil, W, Giovagnoli, D, Girard, F, Glade-Beucke, R, Glück, F, Gokhale, S, de Gouvêa, A, Gráf, L, Grandi, L, Grigat, J, Grinstein, B, van der Grinten, M G D, Grössle, R, Guan, H, Guida, M, Gumbsheimer, R, Gwilliam, C B, Hall, C R, Hall, L J, Hammann, R, Han, K, Hannen, V, Hansmann-Menzemer, S, Harata, R, Hardin, S P, Hardy, E, Hardy, C A, Harigaya, K, Harnik, R, Haselschwardt, S J, Hernandez, M, Hertel, S A, Higuera, A, Hils, C, Hochrein, S, Hoetzsch, L, Hoferichter, M, Hood, N, Hooper, D, Horn, M, Howlett, J, Huang, D Q, Huang, Y, Hunt, D, Iacovacci, M, Iaquaniello, G, Ide, R, Ignarra, C M, Iloglu, G, Itow, Y, Jacquet, E, Jahangir, O, Jakob, J, James, R S, Jansen, A, Ji, W, Ji, X, Joerg, F, Johnson, J, Joy, A, Kaboth, A C, Kalhor, L, Kamaha, A C, Kanezaki, K, Kar, K, Kara, M, Kato, N, Kavrigin, P, Kazama, S, Keaveney, A W, Kellerer, J, Khaitan, D, Khazov, A, Khundzakishvili, G, Khurana, I, Kilminster, B, Kleifges, M, Ko, P, Kobayashi, M, Kodroff, D, Koltmann, G, Kopec, A, Kopmann, A, Kopp, J, Korley, L, Kornoukhov, V N, Korolkova, E V, Kraus, H, Krauss, L M, Kravitz, S, Kreczko, L, Kudryavtsev, V A, Kuger, F, Kumar, J, López Paredes, B, LaCascio, L, Laha, R, Laine, Q, Landsman, H, Lang, R F, Leason, E A, Lee, J, Leonard, D S, Lesko, K T, Levinson, L, Levy, C, Li, I, Li, S C, Li, T, Liang, S, Liebenthal, C S, Lin, J, Lin, Q, Lindemann, S, Lindner, M, Lindote, A, Linehan, R, Lippincott, W H, Liu, X, Liu, K, Liu, J, Loizeau, J, Lombardi, F, Long, J, Lopes, M I, Lopez Asamar, E, Lorenzon, W, Lu, C, Luitz, S, Ma, Y, Machado, P A N, Macolino, C, Maeda, T, Mahlstedt, J, Majewski, P A, Manalaysay, A, Mancuso, A, Manenti, L, Manfredini, A, Mannino, R L, Marangou, N, March-Russell, J, Marignetti, F, Marrodán Undagoitia, T, Martens, K, Martin, R, Martinez-Soler, I, Masbou, J, Masson, D, Masson, E, Mastroianni, S, Mastronardi, M, Matias-Lopes, J A, McCarthy, M E, McFadden, N, McGinness, E, McKinsey, D N, McLaughlin, J, McMichael, K, Meinhardt, P, Menéndez, J, Meng, Y, Messina, M, Midha, R, Milisavljevic, D, Miller, E H, Milosevic, B, Milutinovic, S, Mitra, S A, Miuchi, K, Mizrachi, E, Mizukoshi, K, Molinario, A, Monte, A, Monteiro, C M B, Monzani, M E, Moore, J S, Morå, K, Morad, J A, Morales Mendoza, J D, Moriyama, S, Morrison, E, Morteau, E, Mosbacher, Y, Mount, B J, Mueller, J, Murphy, A St J, Murra, M, Naim, D, Nakamura, S, Nash, E, Navaieelavasani, N, Naylor, A, Nedlik, C, Nelson, H N, Neves, F, Newstead, J L, Ni, K, Nikoleyczik, J A, Niro, V, Oberlack, U G, Obradovic, M, Odgers, K, O’Hare, C A J, Oikonomou, P, Olcina, I, Oliver-Mallory, K, Oranday, A, Orpwood, J, Ostrovskiy, I, Ozaki, K, Paetsch, B, Pal, S, Palacio, J, Palladino, K J, Palmer, J, Panci, P, Pandurovic, M, Parlati, A, Parveen, N, Patton, S J, Pěč, V, Pellegrini, Q, Penning, B, Pereira, G, Peres, R, Perez-Gonzalez, Y, Perry, E, Pershing, T, Petrossian-Byrne, R, Pienaar, J, Piepke, A, Pieramico, G, Pierre, M, Piotter, M, Pizzella, V, Plante, G, Pollmann, T, Porzio, D, Qi, J, Qie, Y, Qin, J, Quevedo, F, Raj, N, Rajado Silva, M, Ramanathan, K, Ramírez García, D, Ravanis, J, Redard-Jacot, L, Redigolo, D, Reichard, S, Reichenbacher, J, Rhyne, C A, Richards, A, Riffard, Q, Rischbieter, G R C, Rocchetti, A, Rosenfeld, S L, Rosero, R, Rupp, N, Rushton, T, Saha, S, Salucci, P, Sanchez, L, Sanchez-Lucas, P, Santone, D, dos Santos, J M F, Sarnoff, I, Sartorelli, G, Sazzad, A B M R, Scheibelhut, M, Schnee, R W, Schrank, M, Schreiner, J, Schulte, P, Schulte, D, Schulze Eissing, H, Schumann, M, Schwemberger, T, Schwenk, A, Schwetz, T, Scotto Lavina, L, Scovell, P R, Sekiya, H, Selvi, M, Semenov, E, Semeria, F, Shagin, P, Shaw, S, Shi, S, Shockley, E, Shutt, T A, Si-Ahmed, R, Silk, J J, Silva, C, Silva, M C, Simgen, H, Šimkovic, F, Sinev, G, Singh, R, Skulski, W, Smirnov, J, Smith, R, Solmaz, M, Solovov, V N, Sorensen, P, Soria, J, Sparmann, T J, Stancu, I, Steidl, M, Stevens, A, Stifter, K, Strigari, L E, Subotic, D, Suerfu, B, Suliga, A M, Sumner, T J, Szabo, P, Szydagis, M, Takeda, A, Takeuchi, Y, Tan, P-L, Taricco, C, Taylor, W C, Temples, D J, Terliuk, A, Terman, P A, Thers, D, Thieme, K, Thümmler, T, Tiedt, D R, Timalsina, M, To, W H, Toennies, F, Tong, Z, Toschi, F, Tovey, D R, Tranter, J, Trask, M, Trinchero, G C, Tripathi, M, Tronstad, D R, Trotta, R, Tsai, Y D, Tunnell, C D, Turner, W G, Ueno, R, Urquijo, P, Utku, U, Vaitkus, A, Valerius, K, Vassilev, E, Vecchi, S, Velan, V, Vetter, S, Vincent, A C, Vittorio, L, Volta, G, von Krosigk, B, von Piechowski, M, Vorkapic, D, Wagner, C E M, Wang, A M, Wang, B, Wang, Y, Wang, W, Wang, J J, Wang, L-T, Wang, M, Watson, J R, Wei, Y, Weinheimer, C, Weisman, E, Weiss, M, Wenz, D, West, S M, Whitis, T J, Williams, M, Wilson, M J, Winkler, D, Wittweg, C, Wolf, J, Wolf, T, Wolfs, F L H, Woodford, S, Woodward, D, Wright, C J, Wu, V H S, Wu, P, Wüstling, S, Wurm, M, Xia, Q, Xiang, X, Xing, Y, Xu, J, Xu, Z, Xu, D, Yamashita, M, Yamazaki, R, Yan, H, Yang, L, Yang, Y, Ye, J, Yeh, M, Young, I, Yu, H B, Yu, T T, Yuan, L, Zavattini, G, Zerbo, S, Zhang, Y, Zhong, M, Zhou, N, Zhou, X, Zhu, T, Zhu, Y, Zhuang, Y, Zopounidis, J P, Zuber, K, Zupan, J, Aalbers, J, AbdusSalam, S S, Abe, K, Aerne, V, Agostini, F, Ahmed Maouloud, S, Akerib, D S, Akimov, D Y, Akshat, J, Al Musalhi, A K, Alder, F, Alsum, S K, Althueser, L, Amarasinghe, C S, Amaro, F D, Ames, A, Anderson, T J, Andrieu, B, Angelides, N, Angelino, E, Angevaare, J, Antochi, V C, Antón Martin, D, Antunovic, B, Aprile, E, Araújo, H M, Armstrong, J E, Arneodo, F, Arthurs, M, Asadi, P, Baek, S, Bai, X, Bajpai, D, Baker, A, Balajthy, J, Balashov, S, Balzer, M, Bandyopadhyay, A, Bang, J, Barberio, E, Bargemann, J W, Baudis, L, Bauer, D, Baur, D, Baxter, A, Baxter, A L, Bazyk, M, Beattie, K, Behrens, J, Bell, N F, Bellagamba, L, Beltrame, P, Benabderrahmane, M, Bernard, E P, Bertone, G F, Bhattacharjee, P, Bhatti, A, Biekert, A, Biesiadzinski, T P, Binau, A R, Biondi, R, Biondi, Y, Birch, H J, Bishara, F, Bismark, A, Blanco, C, Blockinger, G M, Bodnia, E, Boehm, C, Bolozdynya, A I, Bolton, P D, Bottaro, S, Bourgeois, C, Boxer, B, Brás, P, Breskin, A, Breur, P A, Brew, C A J, Brod, J, Brookes, E, Brown, A, Brown, E, Bruenner, S, Bruno, G, Budnik, R, Bui, T K, Burdin, S, Buse, S, Busenitz, J K, Buttazzo, D, Buuck, M, Buzulutskov, A, Cabrita, R, Cai, C, Cai, D, Capelli, C, Cardoso, J M R, Carmona-Benitez, M C, Cascella, M, Catena, R, Chakraborty, S, Chan, C, Chang, S, Chauvin, A, Chawla, A, Chen, H, Chepel, V, Chott, N I, Cichon, D, Cimental Chavez, A, Cimmino, B, Clark, M, Co, R T, Colijn, A P, Conrad, J, Converse, M V, Costa, M, Cottle, A, Cox, G, Creaner, O, Cuenca Garcia, J J, Cussonneau, J P, Cutter, J E, Dahl, C E, D’Andrea, V, David, A, Decowski, M P, Dent, J B, Deppisch, F F, de Viveiros, L, Di Gangi, P, Di Giovanni, A, Di Pede, S, Dierle, J, Diglio, S, Dobson, J E Y, Doerenkamp, M, Douillet, D, Drexlin, G, Druszkiewicz, E, Dunsky, D, Eitel, K, Elykov, A, Emken, T, Engel, R, Eriksen, S R, Fairbairn, M, Fan, A, Fan, J J, Farrell, S J, Fayer, S, Fearon, N M, Ferella, A, Ferrari, C, Fieguth, A, Fiorucci, S, Fischer, H, Flaecher, H, Flierman, M, Florek, T, Foot, R, Fox, P J, Franceschini, R, Fraser, E D, Frenk, C S, Frohlich, S, Fruth, T, Fulgione, W, Fuselli, C, Gaemers, P, Gaior, R, Gaitskell, R J, Galloway, M, Gao, F, Garcia Garcia, I, Genovesi, J, Ghag, C, Ghosh, S, Gibson, E, Gil, W, Giovagnoli, D, Girard, F, Glade-Beucke, R, Glück, F, Gokhale, S, de Gouvêa, A, Gráf, L, Grandi, L, Grigat, J, Grinstein, B, van der Grinten, M G D, Grössle, R, Guan, H, Guida, M, Gumbsheimer, R, Gwilliam, C B, Hall, C R, Hall, L J, Hammann, R, Han, K, Hannen, V, Hansmann-Menzemer, S, Harata, R, Hardin, S P, Hardy, E, Hardy, C A, Harigaya, K, Harnik, R, Haselschwardt, S J, Hernandez, M, Hertel, S A, Higuera, A, Hils, C, Hochrein, S, Hoetzsch, L, Hoferichter, M, Hood, N, Hooper, D, Horn, M, Howlett, J, Huang, D Q, Huang, Y, Hunt, D, Iacovacci, M, Iaquaniello, G, Ide, R, Ignarra, C M, Iloglu, G, Itow, Y, Jacquet, E, Jahangir, O, Jakob, J, James, R S, Jansen, A, Ji, W, Ji, X, Joerg, F, Johnson, J, Joy, A, Kaboth, A C, Kalhor, L, Kamaha, A C, Kanezaki, K, Kar, K, Kara, M, Kato, N, Kavrigin, P, Kazama, S, Keaveney, A W, Kellerer, J, Khaitan, D, Khazov, A, Khundzakishvili, G, Khurana, I, Kilminster, B, Kleifges, M, Ko, P, Kobayashi, M, Kodroff, D, Koltmann, G, Kopec, A, Kopmann, A, Kopp, J, Korley, L, Kornoukhov, V N, Korolkova, E V, Kraus, H, Krauss, L M, Kravitz, S, Kreczko, L, Kudryavtsev, V A, Kuger, F, Kumar, J, López Paredes, B, LaCascio, L, Laha, R, Laine, Q, Landsman, H, Lang, R F, Leason, E A, Lee, J, Leonard, D S, Lesko, K T, Levinson, L, Levy, C, Li, I, Li, S C, Li, T, Liang, S, Liebenthal, C S, Lin, J, Lin, Q, Lindemann, S, Lindner, M, Lindote, A, Linehan, R, Lippincott, W H, Liu, X, Liu, K, Liu, J, Loizeau, J, Lombardi, F, Long, J, Lopes, M I, Lopez Asamar, E, Lorenzon, W, Lu, C, Luitz, S, Ma, Y, Machado, P A N, Macolino, C, Maeda, T, Mahlstedt, J, Majewski, P A, Manalaysay, A, Mancuso, A, Manenti, L, Manfredini, A, Mannino, R L, Marangou, N, March-Russell, J, Marignetti, F, Marrodán Undagoitia, T, Martens, K, Martin, R, Martinez-Soler, I, Masbou, J, Masson, D, Masson, E, Mastroianni, S, Mastronardi, M, Matias-Lopes, J A, McCarthy, M E, McFadden, N, McGinness, E, McKinsey, D N, McLaughlin, J, McMichael, K, Meinhardt, P, Menéndez, J, Meng, Y, Messina, M, Midha, R, Milisavljevic, D, Miller, E H, Milosevic, B, Milutinovic, S, Mitra, S A, Miuchi, K, Mizrachi, E, Mizukoshi, K, Molinario, A, Monte, A, Monteiro, C M B, Monzani, M E, Moore, J S, Morå, K, Morad, J A, Morales Mendoza, J D, Moriyama, S, Morrison, E, Morteau, E, Mosbacher, Y, Mount, B J, Mueller, J, Murphy, A St J, Murra, M, Naim, D, Nakamura, S, Nash, E, Navaieelavasani, N, Naylor, A, Nedlik, C, Nelson, H N, Neves, F, Newstead, J L, Ni, K, Nikoleyczik, J A, Niro, V, Oberlack, U G, Obradovic, M, Odgers, K, O’Hare, C A J, Oikonomou, P, Olcina, I, Oliver-Mallory, K, Oranday, A, Orpwood, J, Ostrovskiy, I, Ozaki, K, Paetsch, B, Pal, S, Palacio, J, Palladino, K J, Palmer, J, Panci, P, Pandurovic, M, Parlati, A, Parveen, N, Patton, S J, Pěč, V, Pellegrini, Q, Penning, B, Pereira, G, Peres, R, Perez-Gonzalez, Y, Perry, E, Pershing, T, Petrossian-Byrne, R, Pienaar, J, Piepke, A, Pieramico, G, Pierre, M, Piotter, M, Pizzella, V, Plante, G, Pollmann, T, Porzio, D, Qi, J, Qie, Y, Qin, J, Quevedo, F, Raj, N, Rajado Silva, M, Ramanathan, K, Ramírez García, D, Ravanis, J, Redard-Jacot, L, Redigolo, D, Reichard, S, Reichenbacher, J, Rhyne, C A, Richards, A, Riffard, Q, Rischbieter, G R C, Rocchetti, A, Rosenfeld, S L, Rosero, R, Rupp, N, Rushton, T, Saha, S, Salucci, P, Sanchez, L, Sanchez-Lucas, P, Santone, D, dos Santos, J M F, Sarnoff, I, Sartorelli, G, Sazzad, A B M R, Scheibelhut, M, Schnee, R W, Schrank, M, Schreiner, J, Schulte, P, Schulte, D, Schulze Eissing, H, Schumann, M, Schwemberger, T, Schwenk, A, Schwetz, T, Scotto Lavina, L, Scovell, P R, Sekiya, H, Selvi, M, Semenov, E, Semeria, F, Shagin, P, Shaw, S, Shi, S, Shockley, E, Shutt, T A, Si-Ahmed, R, Silk, J J, Silva, C, Silva, M C, Simgen, H, Šimkovic, F, Sinev, G, Singh, R, Skulski, W, Smirnov, J, Smith, R, Solmaz, M, Solovov, V N, Sorensen, P, Soria, J, Sparmann, T J, Stancu, I, Steidl, M, Stevens, A, Stifter, K, Strigari, L E, Subotic, D, Suerfu, B, Suliga, A M, Sumner, T J, Szabo, P, Szydagis, M, Takeda, A, Takeuchi, Y, Tan, P-L, Taricco, C, Taylor, W C, Temples, D J, Terliuk, A, Terman, P A, Thers, D, Thieme, K, Thümmler, T, Tiedt, D R, Timalsina, M, To, W H, Toennies, F, Tong, Z, Toschi, F, Tovey, D R, Tranter, J, Trask, M, Trinchero, G C, Tripathi, M, Tronstad, D R, Trotta, R, Tsai, Y D, Tunnell, C D, Turner, W G, Ueno, R, Urquijo, P, Utku, U, Vaitkus, A, Valerius, K, Vassilev, E, Vecchi, S, Velan, V, Vetter, S, Vincent, A C, Vittorio, L, Volta, G, von Krosigk, B, von Piechowski, M, Vorkapic, D, Wagner, C E M, Wang, A M, Wang, B, Wang, Y, Wang, W, Wang, J J, Wang, L-T, Wang, M, Watson, J R, Wei, Y, Weinheimer, C, Weisman, E, Weiss, M, Wenz, D, West, S M, Whitis, T J, Williams, M, Wilson, M J, Winkler, D, Wittweg, C, Wolf, J, Wolf, T, Wolfs, F L H, Woodford, S, Woodward, D, Wright, C J, Wu, V H S, Wu, P, Wüstling, S, Wurm, M, Xia, Q, Xiang, X, Xing, Y, Xu, J, Xu, Z, Xu, D, Yamashita, M, Yamazaki, R, Yan, H, Yang, L, Yang, Y, Ye, J, Yeh, M, Young, I, Yu, H B, Yu, T T, Yuan, L, Zavattini, G, Zerbo, S, Zhang, Y, Zhong, M, Zhou, N, Zhou, X, Zhu, T, Zhu, Y, Zhuang, Y, Zopounidis, J P, Zuber, K, and Zupan, J
Abstract: The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector.
Published: 2023

92. Update on the MiniCLEAN Dark Matter Experiment

Author: Rielage, K., Akashi-Ronquest, M., Bodmer, M., Bourque, R., Buck, B., Butcher, A., Caldwell, T., Chen, Y., Coakley, K., Flores, E., Formaggio, J.A., Gastler, D., Giuliani, F., Gold, M., Grace, E., Griego, J., Guerrero, N., Guiseppe, V., Henning, R., Hime, A., Jaditz, S., Kachulis, C., Kearns, E., Kelsey, J., Klein, J.R., Latorre, A., Lawson, I., Linden, S., Lopez, F., McKinsey, D.N., MacMullin, S., Mastbaum, A., Mei, D.-M., Monroe, J., Nikkel, J.A., Oertel, J., Gann, G.D. Orebi, Palladino, K., Perumpilly, G., Rodriguez, L., Schnee, R., Seibert, S., Walding, J., Wang, B., Wang, J., and Zhang, C.
Published: 2015
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93. An interferometric analysis method for radio impulses from ultra-high energy particle showers

Author: Romero-Wolf, A., Hoover, S., Vieregg, A.G., Gorham, P.W., Allison, P., Barwick, S.W., Baughman, B.M., Beatty, J.J., Belov, K., Besson, D.Z., Bevan, S., Binns, W.R., Chen, C., Chen, P., Clem, J.M., Connolly, A., Detrixhe, M., De Marco, D., Dowkontt, P.F., DuVernois, M., Goldstein, D., Grashorn, E.W., Hill, B., Huang, M., Israel, M.H., Javaid, A., Kowalski, J., Learned, J., Liewer, K.M., Matsuno, S., Mercurio, B.C., Miki, C., Mottram, M., Nam, J., Naudet, C.J., Nichol, R.J., Palladino, K., Ruckman, L., Saltzberg, D., Seckel, D., Shang, R.Y., Stockham, J., Stockham, M., Varner, G.S., and Wang, Y.
Published: 2015
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94. A next-generation liquid xenon observatory for dark matter and neutrino physics

Author: Aalbers, J, primary, AbdusSalam, S S, additional, Abe, K, additional, Aerne, V, additional, Agostini, F, additional, Ahmed Maouloud, S, additional, Akerib, D S, additional, Akimov, D Y, additional, Akshat, J, additional, Al Musalhi, A K, additional, Alder, F, additional, Alsum, S K, additional, Althueser, L, additional, Amarasinghe, C S, additional, Amaro, F D, additional, Ames, A, additional, Anderson, T J, additional, Andrieu, B, additional, Angelides, N, additional, Angelino, E, additional, Angevaare, J, additional, Antochi, V C, additional, Antón Martin, D, additional, Antunovic, B, additional, Aprile, E, additional, Araújo, H M, additional, Armstrong, J E, additional, Arneodo, F, additional, Arthurs, M, additional, Asadi, P, additional, Baek, S, additional, Bai, X, additional, Bajpai, D, additional, Baker, A, additional, Balajthy, J, additional, Balashov, S, additional, Balzer, M, additional, Bandyopadhyay, A, additional, Bang, J, additional, Barberio, E, additional, Bargemann, J W, additional, Baudis, L, additional, Bauer, D, additional, Baur, D, additional, Baxter, A, additional, Baxter, A L, additional, Bazyk, M, additional, Beattie, K, additional, Behrens, J, additional, Bell, N F, additional, Bellagamba, L, additional, Beltrame, P, additional, Benabderrahmane, M, additional, Bernard, E P, additional, Bertone, G F, additional, Bhattacharjee, P, additional, Bhatti, A, additional, Biekert, A, additional, Biesiadzinski, T P, additional, Binau, A R, additional, Biondi, R, additional, Biondi, Y, additional, Birch, H J, additional, Bishara, F, additional, Bismark, A, additional, Blanco, C, additional, Blockinger, G M, additional, Bodnia, E, additional, Boehm, C, additional, Bolozdynya, A I, additional, Bolton, P D, additional, Bottaro, S, additional, Bourgeois, C, additional, Boxer, B, additional, Brás, P, additional, Breskin, A, additional, Breur, P A, additional, Brew, C A J, additional, Brod, J, additional, Brookes, E, additional, Brown, A, additional, Brown, E, additional, Bruenner, S, additional, Bruno, G, additional, Budnik, R, additional, Bui, T K, additional, Burdin, S, additional, Buse, S, additional, Busenitz, J K, additional, Buttazzo, D, additional, Buuck, M, additional, Buzulutskov, A, additional, Cabrita, R, additional, Cai, C, additional, Cai, D, additional, Capelli, C, additional, Cardoso, J M R, additional, Carmona-Benitez, M C, additional, Cascella, M, additional, Catena, R, additional, Chakraborty, S, additional, Chan, C, additional, Chang, S, additional, Chauvin, A, additional, Chawla, A, additional, Chen, H, additional, Chepel, V, additional, Chott, N I, additional, Cichon, D, additional, Cimental Chavez, A, additional, Cimmino, B, additional, Clark, M, additional, Co, R T, additional, Colijn, A P, additional, Conrad, J, additional, Converse, M V, additional, Costa, M, additional, Cottle, A, additional, Cox, G, additional, Creaner, O, additional, Cuenca Garcia, J J, additional, Cussonneau, J P, additional, Cutter, J E, additional, Dahl, C E, additional, D’Andrea, V, additional, David, A, additional, Decowski, M P, additional, Dent, J B, additional, Deppisch, F F, additional, de Viveiros, L, additional, Di Gangi, P, additional, Di Giovanni, A, additional, Di Pede, S, additional, Dierle, J, additional, Diglio, S, additional, Dobson, J E Y, additional, Doerenkamp, M, additional, Douillet, D, additional, Drexlin, G, additional, Druszkiewicz, E, additional, Dunsky, D, additional, Eitel, K, additional, Elykov, A, additional, Emken, T, additional, Engel, R, additional, Eriksen, S R, additional, Fairbairn, M, additional, Fan, A, additional, Fan, J J, additional, Farrell, S J, additional, Fayer, S, additional, Fearon, N M, additional, Ferella, A, additional, Ferrari, C, additional, Fieguth, A, additional, Fiorucci, S, additional, Fischer, H, additional, Flaecher, H, additional, Flierman, M, additional, Florek, T, additional, Foot, R, additional, Fox, P J, additional, Franceschini, R, additional, Fraser, E D, additional, Frenk, C S, additional, Frohlich, S, additional, Fruth, T, additional, Fulgione, W, additional, Fuselli, C, additional, Gaemers, P, additional, Gaior, R, additional, Gaitskell, R J, additional, Galloway, M, additional, Gao, F, additional, Garcia Garcia, I, additional, Genovesi, J, additional, Ghag, C, additional, Ghosh, S, additional, Gibson, E, additional, Gil, W, additional, Giovagnoli, D, additional, Girard, F, additional, Glade-Beucke, R, additional, Glück, F, additional, Gokhale, S, additional, de Gouvêa, A, additional, Gráf, L, additional, Grandi, L, additional, Grigat, J, additional, Grinstein, B, additional, van der Grinten, M G D, additional, Grössle, R, additional, Guan, H, additional, Guida, M, additional, Gumbsheimer, R, additional, Gwilliam, C B, additional, Hall, C R, additional, Hall, L J, additional, Hammann, R, additional, Han, K, additional, Hannen, V, additional, Hansmann-Menzemer, S, additional, Harata, R, additional, Hardin, S P, additional, Hardy, E, additional, Hardy, C A, additional, Harigaya, K, additional, Harnik, R, additional, Haselschwardt, S J, additional, Hernandez, M, additional, Hertel, S A, additional, Higuera, A, additional, Hils, C, additional, Hochrein, S, additional, Hoetzsch, L, additional, Hoferichter, M, additional, Hood, N, additional, Hooper, D, additional, Horn, M, additional, Howlett, J, additional, Huang, D Q, additional, Huang, Y, additional, Hunt, D, additional, Iacovacci, M, additional, Iaquaniello, G, additional, Ide, R, additional, Ignarra, C M, additional, Iloglu, G, additional, Itow, Y, additional, Jacquet, E, additional, Jahangir, O, additional, Jakob, J, additional, James, R S, additional, Jansen, A, additional, Ji, W, additional, Ji, X, additional, Joerg, F, additional, Johnson, J, additional, Joy, A, additional, Kaboth, A C, additional, Kalhor, L, additional, Kamaha, A C, additional, Kanezaki, K, additional, Kar, K, additional, Kara, M, additional, Kato, N, additional, 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additional, Liang, S, additional, Liebenthal, C S, additional, Lin, J, additional, Lin, Q, additional, Lindemann, S, additional, Lindner, M, additional, Lindote, A, additional, Linehan, R, additional, Lippincott, W H, additional, Liu, X, additional, Liu, K, additional, Liu, J, additional, Loizeau, J, additional, Lombardi, F, additional, Long, J, additional, Lopes, M I, additional, Lopez Asamar, E, additional, Lorenzon, W, additional, Lu, C, additional, Luitz, S, additional, Ma, Y, additional, Machado, P A N, additional, Macolino, C, additional, Maeda, T, additional, Mahlstedt, J, additional, Majewski, P A, additional, Manalaysay, A, additional, Mancuso, A, additional, Manenti, L, additional, Manfredini, A, additional, Mannino, R L, additional, Marangou, N, additional, March-Russell, J, additional, Marignetti, F, additional, Marrodán Undagoitia, T, additional, Martens, K, additional, Martin, R, additional, Martinez-Soler, I, additional, Masbou, J, additional, Masson, D, additional, Masson, E, additional, Mastroianni, S, additional, Mastronardi, M, additional, Matias-Lopes, J A, additional, McCarthy, M E, additional, McFadden, N, additional, McGinness, E, additional, McKinsey, D N, additional, McLaughlin, J, additional, McMichael, K, additional, Meinhardt, P, additional, Menéndez, J, additional, Meng, Y, additional, Messina, M, additional, Midha, R, additional, Milisavljevic, D, additional, Miller, E H, additional, Milosevic, B, additional, Milutinovic, S, additional, Mitra, S A, additional, Miuchi, K, additional, Mizrachi, E, additional, Mizukoshi, K, additional, Molinario, A, additional, Monte, A, additional, Monteiro, C M B, additional, Monzani, M E, additional, Moore, J S, additional, Morå, K, additional, Morad, J A, additional, Morales Mendoza, J D, additional, Moriyama, S, additional, Morrison, E, additional, Morteau, E, additional, Mosbacher, Y, additional, Mount, B J, additional, Mueller, J, additional, Murphy, A St J, additional, Murra, M, additional, Naim, D, additional, Nakamura, S, additional, Nash, E, additional, Navaieelavasani, N, additional, Naylor, A, additional, Nedlik, C, additional, Nelson, H N, additional, Neves, F, additional, Newstead, J L, additional, Ni, K, additional, Nikoleyczik, J A, additional, Niro, V, additional, Oberlack, U G, additional, Obradovic, M, additional, Odgers, K, additional, O’Hare, C A J, additional, Oikonomou, P, additional, Olcina, I, additional, Oliver-Mallory, K, additional, Oranday, A, additional, Orpwood, J, additional, Ostrovskiy, I, additional, Ozaki, K, additional, Paetsch, B, additional, Pal, S, additional, Palacio, J, additional, Palladino, K J, additional, Palmer, J, additional, Panci, P, additional, Pandurovic, M, additional, Parlati, A, additional, Parveen, N, additional, Patton, S J, additional, Pěč, V, additional, Pellegrini, Q, additional, Penning, B, additional, Pereira, G, additional, Peres, R, additional, Perez-Gonzalez, Y, additional, Perry, E, additional, Pershing, T, additional, Petrossian-Byrne, R, additional, Pienaar, J, additional, Piepke, A, additional, Pieramico, G, additional, Pierre, M, additional, Piotter, M, additional, Pizzella, V, additional, Plante, G, additional, Pollmann, T, additional, Porzio, D, additional, Qi, J, additional, Qie, Y, additional, Qin, J, additional, Quevedo, F, additional, Raj, N, additional, Rajado Silva, M, additional, Ramanathan, K, additional, Ramírez García, D, additional, Ravanis, J, additional, Redard-Jacot, L, additional, Redigolo, D, additional, Reichard, S, additional, Reichenbacher, J, additional, Rhyne, C A, additional, Richards, A, additional, Riffard, Q, additional, Rischbieter, G R C, additional, Rocchetti, A, additional, Rosenfeld, S L, additional, Rosero, R, additional, Rupp, N, additional, Rushton, T, additional, Saha, S, additional, Salucci, P, additional, Sanchez, L, additional, Sanchez-Lucas, P, additional, Santone, D, additional, dos Santos, J M F, additional, Sarnoff, I, additional, Sartorelli, G, additional, Sazzad, A B M R, additional, Scheibelhut, M, additional, Schnee, R W, additional, Schrank, M, additional, Schreiner, J, additional, Schulte, P, additional, Schulte, D, additional, Schulze Eissing, H, additional, Schumann, M, additional, Schwemberger, T, additional, Schwenk, A, additional, Schwetz, T, additional, Scotto Lavina, L, additional, Scovell, P R, additional, Sekiya, H, additional, Selvi, M, additional, Semenov, E, additional, Semeria, F, additional, Shagin, P, additional, Shaw, S, additional, Shi, S, additional, Shockley, E, additional, Shutt, T A, additional, Si-Ahmed, R, additional, Silk, J J, additional, Silva, C, additional, Silva, M C, additional, Simgen, H, additional, Šimkovic, F, additional, Sinev, G, additional, Singh, R, additional, Skulski, W, additional, Smirnov, J, additional, Smith, R, additional, Solmaz, M, additional, Solovov, V N, additional, Sorensen, P, additional, Soria, J, additional, Sparmann, T J, additional, Stancu, I, additional, Steidl, M, additional, Stevens, A, additional, Stifter, K, additional, Strigari, L E, additional, Subotic, D, additional, Suerfu, B, additional, Suliga, A M, additional, Sumner, T J, additional, Szabo, P, additional, Szydagis, M, additional, Takeda, A, additional, Takeuchi, Y, additional, Tan, P-L, additional, Taricco, C, additional, Taylor, W C, additional, Temples, D J, additional, Terliuk, A, additional, Terman, P A, additional, Thers, D, additional, Thieme, K, additional, Thümmler, T, additional, Tiedt, D R, additional, Timalsina, M, additional, To, W H, additional, Toennies, F, additional, Tong, Z, additional, Toschi, F, additional, Tovey, D R, additional, Tranter, J, additional, Trask, M, additional, Trinchero, G C, additional, Tripathi, M, additional, Tronstad, D R, additional, Trotta, R, additional, Tsai, Y D, additional, Tunnell, C D, additional, Turner, W G, additional, Ueno, R, additional, Urquijo, P, additional, Utku, U, additional, Vaitkus, A, additional, Valerius, K, additional, Vassilev, E, additional, Vecchi, S, additional, Velan, V, additional, Vetter, S, additional, Vincent, A C, additional, Vittorio, L, additional, Volta, G, additional, von Krosigk, B, additional, von Piechowski, M, additional, Vorkapic, D, additional, Wagner, C E M, additional, Wang, A M, additional, Wang, B, additional, Wang, Y, additional, Wang, W, additional, Wang, J J, additional, Wang, L-T, additional, Wang, M, additional, Watson, J R, additional, Wei, Y, additional, Weinheimer, C, additional, Weisman, E, additional, Weiss, M, additional, Wenz, D, additional, West, S M, additional, Whitis, T J, additional, Williams, M, additional, Wilson, M J, additional, Winkler, D, additional, Wittweg, C, additional, Wolf, J, additional, Wolf, T, additional, Wolfs, F L H, additional, Woodford, S, additional, Woodward, D, additional, Wright, C J, additional, Wu, V H S, additional, Wu, P, additional, Wüstling, S, additional, Wurm, M, additional, Xia, Q, additional, Xiang, X, additional, Xing, Y, additional, Xu, J, additional, Xu, Z, additional, Xu, D, additional, Yamashita, M, additional, Yamazaki, R, additional, Yan, H, additional, Yang, L, additional, Yang, Y, additional, Ye, J, additional, Yeh, M, additional, Young, I, additional, Yu, H B, additional, Yu, T T, additional, Yuan, L, additional, Zavattini, G, additional, Zerbo, S, additional, Zhang, Y, additional, Zhong, M, additional, Zhou, N, additional, Zhou, X, additional, Zhu, T, additional, Zhu, Y, additional, Zhuang, Y, additional, Zopounidis, J P, additional, Zuber, K, additional, and Zupan, J, additional
Published: 2022
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95. High Energy Physics Opportunities Using Reactor Antineutrinos

Author: Awe, C., Barbeau, P. S., Haghighat, A., Huber, P., Li, S. C., Link, J. M., Mascolino, V., Subedi, T., Walkup, K., Aguilar-Arevalo, A., Bertou, X., Bonifazi, C., Cancelo, G., Cervantes-Vergara, B. A., Chavez, C., D Olivo, J. C., Egea, J. M., Dos Anjos, J. C., Estrada, J., Neto, A. R. F., Fernandez-Moroni, G., Foguel, A., Ford, R., Gasanego, J., Gollo, V., Izraelevitch, F., Kilminster, B., Lima, Jr H. P., Makler, M., Mendes, L. H., Molina, J., Mota, P., Nasteva, I., Paolini, E., Romero, C., Sarkis, Y., Haro, M. S., Soto, A., Stalder, D., Tiffenberg, J., Torres, C., Lindner, M., An, F. P., Balantekin, A. B., Band, H. R., Bishai, M., Blyth, S., Cao, G. F., Cao, J., Chang, J. F., Chang, Y., Chen, H. S., Chen, S. M., Chen, Y., Chen, Y. X., Cheng, J., Cheng, Z. K., Cherwinka, J. J., Chu, M. C., Cummings, J. P., Dalager, O., Deng, F. S., Ding, Y. Y., Diwan, M. V., Dohnal, T., Dove, J., Dvořák, M., Dwyer, D. A., Gallo, J. P., Gonchar, M., Gong, G. H., Gong, H., Gu, W. Q., Guo, J. Y., Guo, L., Guo, X. H., Guo, Y. H., Guo, Z., Hackenburg, R. W., Hans, S., He, M., Heeger, K. M., Heng, Y. K., Higuera, A., Hor, Y. K., Hsiung, Y. B., Hu, B. Z., Hu, J. R., Hu, T., Hu, Z. J., Huang, H. X., Huang, X. T., Jaffe, D. E., Jen, K. L., Ji, X. L., Ji, X. P., Johnson, R. A., Jones, D., Kang, L., Kettell, S. H., Kohn, S., Kramer, M., Langford, T. J., Lee, J., Lee, J. H. C., Lei, R. T., Leitner, R., Leung, J. K. C., Li, F., Li, H. L., Li, J. J., Li, Q. J., Li, S., Li, W. D., Li, X. N., Li, X. Q., Li, Y. F., Li, Z. B., Liang, H., Lin, C. J., Lin, G. L., Lin, S., Ling, J. J., Littenberg, L., Littlejohn, B. R., Liu, J. C., Liu, J. L., Lu, C., Lu, H. Q., Lu, J. S., Luk, K. B., Ma, X. B., Ma, X. Y., Ma, Y. Q., Mandujano, R. C., Marshall, C., Martinez Caicedo, D. A., Mcdonald, K. T., Mckeown, R. D., Meng, Y., Napolitano, J., Naumov, D., Naumova, E., Ochoa-Ricoux, J. P., Olshevskiy, A., Pan, H. -R, Park, J., Patton, S., Peng, J. C., Pun, C. S. J., Qi, F. Z., Qi, M., Qian, X., Raper, N., Ren, J., Reveco, C. Morales, Rosero, R., Roskovec, B., Ruan, X. C., Steiner, H., Sun, J. L., Tmej, T., Treskov, K., Tse, W. -H, Tull, C. E., Viren, B., Vorobel, V., Wang, C. H., Wang, J., Wang, M., Wang, N. Y., Wang, R. G., Wang, W., Wang, X., Wang, Y., Wang, Y. F., Wang, Z., Wang, Z. M., Wei, H. Y., Wei, L. H., Wen, L. J., Whisnant, K., White, C. G., Wong, H. L. H., Worcester, E., Wu, D. R., Wu, F. L., Wu, Q., Wenjie Wu, Xia, D. M., Xie, Z. Q., Xing, Z. Z., Xu, J. L., Xu, T., Xue, T., Yang, C. G., Yang, L., Yang, Y. Z., Yao, H. F., Ye, M., Yeh, M., Young, B. L., Yu, H. Z., Yu, Z. Y., Yue, B. B., Zeng, S., Zeng, Y., Zhan, L., Zhang, C., Zhang, F. Y., Zhang, H. H., Zhang, J. W., Zhang, Q. M., Zhang, X. T., Zhang, Y. M., Zhang, Y. X., Zhang, Y. Y., Zhang, Z. J., Zhang, Z. P., Zhang, Z. Y., Zhao, J., Zhou, L., Zhuang, H. L., Zou, J. H., Abusleme, A., Adam, T., Ahmad, S., Ahmed, R., Aiello, S., An, G. P., An, Q., Andronico, G., Anfimov, N., Antonelli, V., Antoshkina, T., Asavapibhop, B., André, J. P. A. M., Auguste, D., Babic, A., Baldini, W., Barresi, A., Baussan, E., Bellato, M., Bergnoli, A., Bernieri, E., Birkenfeld, T., Blin, S., Blum, D., Bolshakova, A., Bongrand, M., Bordereau, C., Breton, D., Brigatti, A., Brugnera, R., Bruno, R., Budano, A., Buesken, M., Buscemi, M., Busto, Jose, Butorov, I., Cabrera, A., Cai, H., Cai, X., Cai, Y. K., Cai, Z. Y., Cammi, A., Campeny, A., Cao, C. Y., Caruso, R., Cerna, C., Chakaberia, I., Chen, P. P., Chen, P. A., Chen, S., Chen, X., Chen, Y. W., Chen, Z., Cheng, Y., Chiesa, D., Chimenti, P., Chukanov, A., Chuvashova, A., Claverie, G., Clementi, C., Clerbaux, B., Di Lorenzo, S., Corti, D., Costa, S., Corso, F. D., La Taille, C., Deng, J., Deng, Z., Deng, Z. Y., Depnering, W., Diaz, M., Ding, X. F., Dirgantara, B., Dmitrievsky, S., Donchenko, G., Dong, J. M., Dornic, D., Doroshkevich, E., Dracos, M., Druillole, F., Du, S. X., Dusini, S., Dvorak, M., Enqvist, T., Enzmann, H., Fabbri, A., Fajt, L., Fan, D. H., Fan, L., Fang, C., Fang, J., Fang, W. X., Fargetta, M., Fatkina, A., Fedoseev, D., Fekete, V., Feng, L. C., Feng, Q. C., Formozov, A., Fournier, A., Gan, H. N., Gao, F., Garfagnini, A., Göttel, A., Genster, C., Giammarchi, M., Giaz, A., Giudice, N., Gong, G., Gorchakov, O., Gornushkin, Y., Grassi, M., Grewing, C., Gromov, V., Gu, M., Gu, X., Gu, Y., Guan, M. Y., Guardone, N., Gul, M., Guo, C., Guo, W. L., Hackspacher, P., Hagner, C., Han, R., Han, Y., Hassan, M., He, W., Heinz, T., Hellmuth, P., Herrera, R., Hong, D. J., Hou, S. J., Hsiung, Y., Hu, H., Hu, J., Hu, S. Y., Huang, C. H., Huang, G. H., Huang, Q. H., Huang, W. H., Huang, X., Huang, Y. B., Hui, J. Q., Huo, L., Huo, W., Huss, C., Hussain, S., Insolia, A., Ioannisian, A., Isocrate, R., Ji, X. Z., Jia, H. H., Jia, J. J., Jian, S. Y., Jiang, D., Jiang, X. S., Jin, R. Y., Jing, X. 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M., Ma, S., Maalmi, J., Malyshkin, Y., Mantovani, F., Manzali, F., Mao, X., Mao, Y. J., Mari, S. M., Marini, F., Marium, S., Martellini, C., Martin-Chassard, G., Martini, A., Mayilyan, D., Müller, A., Mednieks, I., Meregaglia, A., Meroni, E., Meyhöfer, D., Mezzetto, M., Miller, J., Miramonti, L., Monforte, S., Montini, P., Montuschi, M., Morozov, N., Muhammad, A., Muralidharan, P., Nastasi, M., Naumov, D. V., Nemchenok, I., Ning, F. P., Ning, Z., Nunokawa, H., Oberauer, L., Orestano, D., Ortica, F., Pan, H. R., Paoloni, A., Parkalian, N., Parmeggiano, S., Payupol, T., Pei, Y., Pelliccia, N., Peng, A., Peng, H., Perrot, F., Petitjean, P. A., Petrucci, F., Piñeres Rico, L. F., Pilarczyk, O., Popov, A., Poussot, P., Pratumwan, W., Previtali, E., Qi, F., Qian, S., Qian, X. H., Qiao, H., Qin, Z. H., Qiu, S. K., Rajput, M., Ranucci, G., Re, A., Rebber, H., Rebii, A., Ren, B., Rezinko, T., Ricci, B., Robens, M., Roche, M., Rodphai, N., Romani, A., Roth, C., Ruan, X., Rujirawat, S., Rybnikov, A., Sadovsky, A., Saggese, P., Salamanna, G., Sanfilippo, S., Sangka, A., Sanguansak, N., Sawangwit, U., Sawatzki, J., Sawy, F., Schever, M., Schuler, J., Schwab, C., Schweizer, K., Selivanov, D., Selyunin, A., Serafini, A., Settanta, G., Settimo, M., Shao, Z., Sharov, V., Shi, J., Shutov, V., Sidorenkov, A., Simkovic, F., Sirignano, C., Siripak, J., Sisti, M., Slupecki, M., Smirnov, M., Smirnov, O., Sogo-Bezerra, T., Songwadhana, J., Soonthornthum, B., Sotnikov, A., Sramek, O., Sreethawong, W., Stahl, A., Stanco, L., Stankevich, K., Stefanik, D., Steiger, H., Steinmann, J., Sterr, T., Stock, M. R., Strati, V., Studenikin, A., Sun, G. X., Sun, S. F., Sun, X. L., Sun, Y. J., Sun, Y. Z., Suwonjandee, N., Szelezniak, M., Tang, J., Tang, Q., Tang, X., Tietzsch, A., Tkachev, I., Triossi, A., Troni, G., Trzaska, W., Tuve, C., Ushakov, N., Waasen, S., Boom, J. Vanden, Vanroyen, G., Vassilopoulos, N., Vedin, V., Verde, G., Vialkov, M., Viaud, B., Volpe, C., Voronin, D., Votano, L., Walker, P., Wang, C., Wang, E., Wang, G., Wang, K. Y., Wang, L., Wang, M. F., Wang, S. G., Wang, W. S., Wang, X. Y., Wang, Y. G., Wang, Y. Q., Wang, Z. Y., Waqas, M., Watcharangkool, A., Wei, W., Wei, Y. D., Wiebusch, C., Wong, S. C. F., Wonsak, B., Wu, D., Wu, W. J., Wu, Z., Wurm, M., Wurtz, J., Wysotzki, C., Xi, Y. F., Xie, Y. G., Xu, B., Xu, C., Xu, D. L., Xu, F. R., Xu, H. K., Xu, J., Xu, M. H., Xu, Y., Yan, B. J., Yan, T., Yan, W. Q., Yan, X. B., Yan, Y. P., Yang, A. B., Yang, H., Yang, J., Yang, X. Y., Yang, Y., Yang, Y. F., Yasin, Z., Ye, J. X., Ye, Z. P., Yegin, U., Yermia, F., Yi, P. H., Yin, X. W., You, Z. Y., Yu, B. X., Yu, C. Y., Yu, C. X., Yu, M., Yu, X. H., Yuan, C. Z., Yuan, Y., Yuan, Z. X., Yuan, Z. Y., Zafar, N., Zambanini, A., Zeng, T. X., Zeng, Y. D., Zhang, G. Q., Zhang, H. Q., Zhang, J., Zhang, J. B., Zhang, P., Zhang, S., Zhang, T., Zhang, X. M., Zhang, Y., Zhang, Y. H., Zhang, Y. P., Zhao, F. Y., Zhao, R., Zhao, S. J., Zhao, T. C., Zheng, D. Q., Zheng, H., Zheng, M. S., Zheng, Y. H., Zhong, W. R., Zhou, J., Zhou, N., Zhou, S., Zhou, X., Zhu, J., Zhu, K. J., Zhuang, B., Zong, L., Rasco, B. C., Han, B. Y., Jeon, E. J., Jeong, Y., Jo, H. S., Kim, D. K., Kim, J. Y., Kim, J. G., Kim, Y. D., Ko, Y. J., Lee, H. M., Lee, M. H., Moon, C. S., Oh, Y. M., Park, H. K., Park, K. S., Seo, S. H., Siyeon, K., Sun, G. M., Yoon, Y. S., Yu, I., Borusinski, M. J., Dorrill, R., Druetzler, A., Learned, J., Li, V., Markoff, D., Maricic, J., Matsuno, S., Mumm, H. P., Nishimura, K., Irani, A., Pitt, M., Rasco, C., Thibodeau, B., Varner, G., Vogelaar, B., Wright, T., Andriamirado, M., Bass, C. D., Bergeron, D. E., Berish, D., Bowden, N. S., Brodsky, J. P., Bryan, C. D., Carr, R., Classen, T., Conant, A. J., Deichert, G., Dolinski, M. J., Erickson, A., Foust, B. T., Gaison, J. K., Galindo-Uribarri, A., Gilbert, C. E., Grant, C., Hackett, B. T., Hansell, A. B., Ji, X., Jones, D. C., Kyzylova, O., Lane, C. E., Larosa, J., Lu, X., Mendenhall, M. P., Meyer, A. M., Milincic, R., Mitchell, I., Mueller, P. E., Nave, C., Neilson, R., Nikkel, J. A., Norcini, D., Nour, S., Palomino, J. L., Pushin, D. A., Romero-Romero, E., Surukuchi, P. T., Tyra, M. A., Varner, R. L., Venegas-Vargas, D., Weatherly, P. B., White, C., Wilhelmi, J., Woolverton, A., Zhang, A., Zhang, X., Choi, J. H., Jang, H. I., Jang, J. S., Jeon, S. H., Joo, K. K., Ju, K., Jung, D. E., Kim, J. H., Kim, S. B., Kim, S. Y., Kim, W., Kwon, E., Lee, D. H., Lee, H. G., Lim, I. T., Moon, D. H., Pac, M. Y., Seo, H., Seo, J. W., Shin, C. D., Yang, B. S., Yoo, J., Yoon, S. G., Yeo, I. S., Chang, C., Bergé, L., Broniatowski, A., Dumoulin, L., Giuliani, A., Chapellier, M., Marcillac, P., Marnieros, S., Olivieri, E., Poda, D., Calvo, M., Goupy, J., Monfardini, A., Arnaud, Q., Augier, C., Billard, J., Cazes, A., Colas, J., Filippini, J., Gascon, J., Jesus, M., Lattaud, H., Juillard, A., Salagnac, T., Soldner, T., Lubashevskiy, A., Yakushev, E., Rozov, S., Lamblin, J., Mom, B., Stutz, A., Formaggio, J. A., Mayer, D. W., Johnston, J., Harrington, P., Heine, S., Sibille, V., Chen, R., Figueroa-Feliciano, E., Ziqing, H., Hertel, S., Patel, P., Pinckney, D., Serafin, A., Shilcusky, A., Decheine, N., Palladino, K., Weber, S., Hirjibehedin, C., Akindele, O. A., Carman, L., Dazeley, S., Ford, M., Jovanovic, I., Sutanto, F., Zaitseva, N., Beaumont, W., Binet, S., Bolognino, I., Borg, J., Buridon, V., Chanal, H., Coupé, B., Crochet, P., Cussans, D., Roeck, A., Durand, D., Fallot, M., Galbinski, D., Gallego, S., Giot, L., Guillon, B., Henaff, D., Hayashida, S., Hosseini, B., Kalcheva, S., Lehaut, G., Michiels, I., Monteil, S., Newbold, D., Roy, N., Ryckbosch, D., Sfar, H. Rejeb, Simard, L., Vacheret, A., Vandierendonck, G., Dyck, S., Remortel, N., Vercaemer, S., Verstraeten, M., Weber, A., Yeresko, M., Bonhomme, A., Buck, C., Del Amo Sanchez, P., El Atmani, I., Labit, L., Letourneau, A., Lhuillier, D., Licciardi, M., Materna, T., Pessard, H., Rogly, R., Savu, V., Schoppmann, S., Vialat, M., Algora, A., Beloeuvre, A., Estienne, M., Kean, R., Porta, A., Tain, J. L., Sidelnik, I., Anderson, T., Askins, M., Bagdasarian, Z., Baldoni, A., Barna, A., Benson, T., Bergevin, M., Bernstein, A., Birrittella, B., Bogetic, S., Boissevain, J., Borusinki, J., Boyd, S., Brooks, T., Budsworth, Mat, Burns, J., Calle, M., Camilo, C., Carroll, A., Coleman, J., Collins, R., Connor, C., Cowen, D., Crow, B., Curry, J., Dalnoki-Veress, F., Danielson, D., Diwan, M., Dixon, S., Drakopoulou, L., Duron, J., Dye, S., Fargher, S., Fienberg, A., Fischer, V., Foster, R., Frankiewicz, Kat, Gamble, T., Gooding, D., Gokhale, S., Gregorio, R., Gribble, J., Griskevich, J., Hadley, D., He, J., Healey, K., Hecla, J., Holt, G., Jabbari, C., Jewkes, K., Kaiser, R., Keenan, M., Keener, P., Kneale, Liz, Kudryavtsev, V., Kunkle, P., Litchfield, P., Liu, X. Ran, Lynch, G., Malek, M., Marr-Laundrie, P., Masic, B., Mauger, C., Mccauley, N., Metelko, C., Mills, R., Mitra, A., Muheim, F., Mullen, A., Murphy, A., Needham, M., Neights, E., Ogren, K., Orebi Gann, G., Oxborough, L., Paling, S., Papatyi, A., Paulos, B., Pershing, T., Pickard, L., Quillin, S., Resoro, R., Richards, B., Sabarots, L., Scarff, A., Schnellbach, Yan-Jie, Scovell, P., Seitz, B., Shea, O., Shebalin, V., Smith, G., Smy, M., Song, H., Spooner, N., Stanton, C., Stone, O., Svoboda, R., Szoldos, S., Thompson, L., Thomson, F., Toth, C., Vagins, M., Berg, Rick, Ventura, S., Walsh, B., Webster, J., Weiss, M., Westphal, D., Wetstein, M., Wilson, T., Wilson, S., Wolcott, S., Wright, M., Berryman, J. M., Collar, J. I., Erlandson, A., Gariazzo, S., Garzelli, M. V., Giunti, C., Goldblum, B. L., Hayes, A., Hedges, S., Mariani, C., Minic, D., Mougeot, X., Naim, D., Newby, J., Ni, K., O Donnell, T., Ozturk, S., Périssé, L., Pestes, R., Sonzogni, A. A., Tabrizi, Z., Vivier, M., Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-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), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Neutrino de Champagne Ardenne (LNCA - UMS 3263), 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-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST), Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Cryogénie (NEEL - Cryo), Institut Néel (NEEL), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Hélium : du fondamental aux applications (NEEL - HELFA), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut Laue-Langevin (ILL), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Département de Physique Nucléaire (ex SPhN) (DPHN), 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, CHANDLER, CONNIE, CONUS, Daya Bay, JUNO, MTAS, NEOS, NuLat, PROSPECT, RENO, Ricochet, ROADSTR Near-Field Working Group, SoLid, Stereo, Valencia-Nantes TAGS, vIOLETA, WATCHMAN, and HEP, INSPIRE
Subjects: High Energy Physics - Experiment (hep-ex), [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], hep-ex, neutrino: energy spectrum, antineutrino: nuclear reactor, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], FOS: Physical sciences, neutrino: oscillation, neutrino: nuclear reactor, Particle Physics - Experiment, neutrino: flux, High Energy Physics - Experiment
Abstract: Nuclear reactors are uniquely powerful, abundant, and flavor-pure sources of antineutrinos that continue to play a vital role in the US neutrino physics program. The US reactor antineutrino physics community is a diverse interest group encompassing many detection technologies and many particle physics topics, including Standard Model and short-baseline oscillations, BSM physics searches, and reactor flux and spectrum modeling. The community's aims offer strong complimentary with numerous aspects of the wider US neutrino program and have direct relevance to most of the topical sub-groups composing the Snowmass 2021 Neutrino Frontier. Reactor neutrino experiments also have a direct societal impact and have become a strong workforce and technology development pipeline for DOE National Laboratories and universities. This white paper, prepared as a submission to the Snowmass 2021 community organizing exercise, will survey the state of the reactor antineutrino physics field and summarize the ways in which current and future reactor antineutrino experiments can play a critical role in advancing the field of particle physics in the next decade., Contribution to Snowmass 2021
Published: 2022

96. Improved Dark Matter Search Sensitivity Resulting from LUX Low-Energy Nuclear Recoil Calibration

Author: LUX Collaboration, Akerib, D. S., Alsum, S., Araújo, H. M., Bai, X., Balajthy, J., Bang, J., Baxter, A., Bernard, E. P., Bernstein, A., Biesiadzinski, T. P., Boulton, E. M., Boxer, B., Brás, P., Burdin, S., Byram, D., Carmona-Benitez, M. C., Chan, C., Cutter, J. E., de Viveiros, L., Druszkiewicz, E., Fan, A., Fiorucci, S., Gaitskell, R. J., Ghag, C., Gilchriese, M. G. D., Gwilliam, C., Hall, C. R., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Jahangir, O., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Korolkova, E. V., Kravitz, S., Kudryavtsev, V. A., Leason, E., Lesko, K. T., Liao, J., Lin, J., Lindote, A., Lopes, M. I., Manalaysay, A., Mannino, R. L., Marangou, N., McKinsey, D. N., Mei, D. -M., Morad, J. A., Murphy, A. St. J., Naylor, A., Nehrkorn, C., Nelson, H. N., Neves, F., Nilima, A., Oliver-Mallory, K. C., Palladino, K. J., Rhyne, C., Riffard, Q., Rischbieter, G. R. C., Rossiter, P., Shaw, S., Shutt, T. A., Silva, C., Solmaz, M., Solovov, V. N., Sorensen, P., Sumner, T. J., Swanson, N., Szydagis, M., Taylor, D. J., Taylor, R., Taylor, W. C., Tennyson, B. P., Terman, P. A., Tiedt, D. R., To, W. H., Tvrznikova, L., Utku, U., Vacheret, A., Vaitkus, A., Velan, V., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Woodward, D., Xiang, X., Xu, J., and Zhang, C.
Subjects: High Energy Physics - Experiment (hep-ex), Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics - Instrumentation and Detectors, hep-ex, astro-ph.CO, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), physics.ins-det, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Experiment
Abstract: Dual-phase xenon time projection chamber (TPC) detectors have demonstrated superior search sensitivities to dark matter over a wide range of particle masses. To extend their sensitivity to include low-mass dark matter interactions, it is critical to characterize both the light and charge responses of liquid xenon to sub-keV nuclear recoils. In this work, we report a new nuclear recoil calibration in the LUX detector $\textit{in situ}$ using neutron events from a pulsed Adelphi Deuterium-Deuterium neutron generator. We demonstrate direct measurements of light and charge yields down to 0.45 keV (1.4 scintillation photons) and 0.27 keV (1.3 ionization electrons), respectively, approaching the physical limit of liquid xenon detectors. We discuss the implication of these new measurements on the physics reach of dual-phase xenon TPCs for nuclear-recoil-based low-mass dark matter detection.
Published: 2022

97. Cosmogenic production of <math><mrow><mmultiscripts><mrow><mi>Ar</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>37</mn></mrow></mmultiscripts></mrow></math> in the context of the LUX-ZEPLIN experiment

Author: Aalbers, J., Akerib, D. S., Al Musalhi, A. K., Alder, F., Alsum, S. K., Amarasinghe, C. S., Ames, A., Anderson, T. J., Angelides, N., Araújo, H. M., Armstrong, J. E., Arthurs, M., Bai, X., Baker, A., Balajthy, J., Balashov, S., Bang, J., Bargemann, J. W., Bauer, D., Baxter, A., Beattie, K., Bernard, E. P., Bhatti, A., Biekert, A., Biesiadzinski, T. P., Birch, H. J., Blockinger, G. M., Bodnia, E., Boxer, B., Brew, C. A. J., Brás, P., Burdin, S., Busenitz, J. K., Buuck, M., Cabrita, R., Carmona-Benitez, M. C., Cascella, M., Chan, C., Chawla, A., Chen, H., Chott, N. I., Cole, A., Converse, M. V., Cottle, A., Cox, G., Creaner, O., Cutter, J. E., Dahl, C. E., David, A., de Viveiros, L., Dobson, J. E. Y., Druszkiewicz, E., Eriksen, S. R., Fan, A., Fayer, S., Fearon, N. M., Fiorucci, S., Flaecher, H., Fraser, E. D., Fruth, T., Gaitskell, R. J., Genovesi, J., Ghag, C., Gibson, E., Gilchriese, M. G. D., Gokhale, S., van der Grinten, M. G. D., Gwilliam, C. B., Hall, C. R., Haselschwardt, S. J., Hertel, S. A., Horn, M., Huang, D. Q., Hunt, D., Ignarra, C. M., Jahangir, O., James, R. S., Ji, W., Johnson, J., Kaboth, A. C., Kamaha, A. C., Kamdin, K., Khaitan, D., Khazov, A., Khurana, I., Kodroff, D., Korley, L., Korolkova, E. V., Kraus, H., Kravitz, S., Kreczko, L., Kudryavtsev, V. A., Leason, E. A., Leonard, D. S., Lesko, K. T., Levy, C., Lee, J., Lin, J., Lindote, A., Linehan, R., Lippincott, W. H., Liu, X., Lopes, M. I., Lopez Asamar, E., Lopez-Paredes, B., Lorenzon, W., Luitz, S., Majewski, P. A., Manalaysay, A., Manenti, L., Mannino, R. L., Marangou, N., McCarthy, M. E., McKinsey, D. N., McLaughlin, J., Miller, E. H., Mizrachi, E., Monte, A., Monzani, M. E., Morad, J. A., Morales Mendoza, J. D., Morrison, E., Mount, B. J., Murphy, A. St. J., Naim, D., Naylor, A., Nedlik, C., Nelson, H. N., Neves, F., Nikoleyczik, J. A., Nilima, A., Olcina, I., Oliver-Mallory, K., Pal, S., Palladino, K. J., Palmer, J., Parveen, N., Patton, S. J., Pease, E. K., Penning, B., Pereira, G., Perry, E., Pershing, J., Piepke, A., Porzio, D., Qie, Y., Reichenbacher, J., Rhyne, C. A., Richards, A., Riffard, Q., Rischbieter, G. R. C., Rosero, R., Rossiter, P., Rushton, T., Santone, D., Sazzad, A. B. M. R., Schnee, R. W., Scovell, P. R., Shaw, S., Shutt, T. A., Silk, J. J., Silva, C., Sinev, G., Smith, R., Solmaz, M., Solovov, V. N., Sorensen, P., Soria, J., Stancu, I., Stevens, A., Stifter, K., Suerfu, B., Sumner, T. J., Swanson, N., Szydagis, M., Taylor, W. C., Taylor, R., Temples, D. J., Terman, P. A., Tiedt, D. R., Timalsina, M., To, W. H., Tong, Z., Tovey, D. R., Trask, M., Tripathi, M., Tronstad, D. R., Turner, W., Utku, U., Vaitkus, A., Wang, B., Wang, Y., Wang, J. J., Wang, W., Watson, J. R., Webb, R. C., White, R. G., Whitis, T. J., Williams, M., Wolfs, F. L. H., Woodford, S., Woodward, D., Wright, C. J., Xia, Q., Xiang, X., Xu, J., and Yeh, M.
Abstract: We estimate the amount of Ar37 produced in natural xenon via cosmic-ray-induced spallation, an inevitable consequence of the transportation and storage of xenon on the Earth’s surface. We then calculate the resulting Ar37 concentration in a 10-tonne payload (similar to that of the LUX-ZEPLIN experiment) assuming a representative schedule of xenon purification, storage, and delivery to the underground facility. Using the spallation model by Silberberg and Tsao, the sea-level production rate of Ar37 in natural xenon is estimated to be 0.024 atoms/kg/day. Assuming the xenon is successively purified to remove radioactive contaminants in 1-tonne batches at a rate of 1 tonne/month, the average Ar37 activity after 10 tons are purified and transported underground is 0.058−0.090 μBq/kg, depending on the degree of argon removal during above-ground purification. Such cosmogenic Ar37 will appear as a noticeable background in the early science data, while decaying with a 35-day half-life. This newly noticed production mechanism of Ar37 should be considered when planning for future liquid-xenon-based experiments.
Published: 2022

98. Observation of ultra-high-energy cosmic rays with the ANITA balloon-borne radio interferometer

Author: Romero-Wolf, A., Hoover, S., Nam, J., Gorham, P.W., Grashorn, E., Allison, P., Barwick, S.W., Beatty, J.J., Belov, K., Besson, D.Z., Binns, W.R., Chen, C., Chen, P., Clem, J.M., Connolly, A., Dowkontt, P.F., DuVernois, M.A., Field, R.C., Goldstein, D., Vieregg, A.G., Hast, C., Hebert, C.L., Israel, M.H., Javaid, A., Kowalski, J., Learned, J.G., Liewer, K.M., Link, J.T., Lusczek, E., Matsuno, S., Mercurio, B.C., Miki, C., Miočinović, P., Naudet, C.J., Ng, J., Nichol, R.J., Palladino, K., Reil, K., Rosen, M., Ruckman, L., Saltzberg, D., Seckel, D., Varner, G.S., Walz, D., and Wu, F.
Published: 2010
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99. Projected sensitivities of the LUX-ZEPLIN experiment to new physics via low-energy electron recoils

Author: The LZ Collaboration, Akerib, D. S., Musalhi, A. K. Al, Alsum, S. K., Amarasinghe, C. S., Ames, A., Anderson, T. J., Angelides, N., Araújo, H. M., Armstrong, J. E., Arthurs, M., Bai, X., Balajthy, J., Balashov, S., Bang, J., Bargemann, J. W., Bauer, D., Baxter, A., Beltrame, P., Bernard, E. P., Bernstein, A., Bhatti, A., Biekert, A., Biesiadzinski, T. P., Birch, H. J., Blockinger, G. M., Bodnia, E., Boxer, B., Brew, C. A. J., Brás, P., Burdin, S., Busenitz, J. K., Buuck, M., Cabrita, R., Carmona-Benitez, M. C., Cascella, M., Chan, C., Chott, N. I., Cole, A., Converse, M. V., Cottle, A., Cox, G., Creaner, O., Cutter, J. E., Dahl, C. E., de Viveiros, L., Dobson, J. E. Y., Druszkiewicz, E., Eriksen, S. R., Fan, A., Fayer, S., Fearon, N. M., Fiorucci, S., Flaecher, H., Fraser, E. D., Fruth, T., Gaitskell, R. J., Genovesi, J., Ghag, C., Gibson, E., Gokhale, S., van der Grinten, M. G. D., Gwilliam, C. B., Hall, C. R., Hardy, C. A., Haselschwardt, S. J., Hertel, S. A., Horn, M., Huang, D. Q., Ignarra, C. M., Jahangir, O., James, R. S., Ji, W., Johnson, J., Kaboth, A. C., Kamaha, A. C., Kamdin, K., Kazkaz, K., Khaitan, D., Khazov, A., Khurana, I., Kodroff, D., Korley, L., Korolkova, E. V., Kraus, H., Kravitz, S., Kreczko, L., Krikler, B., Kudryavtsev, V. A., Leason, E. A., Lee, J., Leonard, D. S., Lesko, K. T., Levy, C., Li, J., Liao, J., Lindote, A., Linehan, R., Lippincott, W. H., Liu, X., Lopes, M. I., Asamar, E. Lopez, Paredes, B. López, Lorenzon, W., Luitz, S., Majewski, P. A., Manalaysay, A., Manenti, L., Mannino, R. L., Marangou, N., McCarthy, M. E., McKinsey, D. N., McLaughlin, J., Miller, E. H., Mizrachi, E., Monte, A., Monzani, M. E., Morad, J. A., Mendoza, J. D. Morales, Morrison, E., Mount, B. J., Murphy, A. St. J., Naim, D., Naylor, A., Nedlik, C., Nelson, H. N., Neves, F., Nikoleyczik, J. A., Nilima, A., Nguyen, A., Olcina, I., Oliver-Mallory, K. C., Pal, S., Palladino, K. J., Palmer, J., Patton, S., Parveen, N., Pease, E. K., Penning, B., Pereira, G., Piepke, A., Qie, Y., Reichenbacher, J., Rhyne, C. A., Richards, A., Riffard, Q., Rischbieter, G. R. C., Rosero, R., Rossiter, P., Santone, D., Sazzad, A. B. M. R., Schnee, R. W., Scovell, P. R., Shaw, S., Shutt, T. A., Silk, J. J., Silva, C., Smith, R., Solmaz, M., Solovov, V. N., Sorensen, P., Soria, J., Stancu, I., Stevens, A., Stifter, K., Suerfu, B., Sumner, T. J., Swanson, N., Szydagis, M., Taylor, W. C., Taylor, R., Temples, D. J., Terman, P. A., Tiedt, D. R., Timalsina, M., To, W. H., Tovey, D. R., Tripathi, M., Tronstad, D. R., Turner, W., Utku, U., Vaitkus, A., Wang, B., Wang, J. J., Wang, W., Watson, J. R., Webb, R. C., White, R. G., Whitis, T. J., Williams, M., Wolfs, F. L. H., Woodward, D., Wright, C. J., Xiang, X., Xu, J., Yeh, M., and Zarzhitsky, P.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Science & Technology, Physics::Instrumentation and Detectors, hep-ex, Physics, FOS: Physical sciences, XMASS, hep-ph, Astronomy & Astrophysics, High Energy Physics - Experiment, Physics, Particles & Fields, MODEL, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology, LIMITS, High Energy Physics - Phenomenology (hep-ph), SOLAR AXIONS, SEARCH, Physical Sciences, DARK-MATTER, astro-ph.CO, NEUTRINO, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear recoils with a ~7-tonne xenon target mass. This manuscript presents sensitivity projections to several low-energy signals of the complementary electron recoil signal type: 1) an effective neutrino magnetic moment and 2) an effective neutrino millicharge, both for pp-chain solar neutrinos, 3) an axion flux generated by the Sun, 4) axion-like particles forming the galactic dark matter, 5) hidden photons, 6) mirror dark matter, and 7) leptophilic dark matter. World-leading sensitivities are expected in each case, a result of the large 5.6t 1000d exposure and low expected rate of electron recoil backgrounds in the $, Comment: v2 updates exclusion sensitivities from single-sided to two-sided
Published: 2021

100. Projected sensitivities of the LUX-ZEPLIN experiment to new physics via low-energy electron recoils

Author: Akerib, D. S., primary, Al Musalhi, A. K., additional, Alsum, S. K., additional, Amarasinghe, C. S., additional, Ames, A., additional, Anderson, T. J., additional, Angelides, N., additional, Araújo, H. M., additional, Armstrong, J. E., additional, Arthurs, M., additional, Bai, X., additional, Balajthy, J., additional, Balashov, S., additional, Bang, J., additional, Bargemann, J. W., additional, Bauer, D., additional, Baxter, A., additional, Beltrame, P., additional, Bernard, E. P., additional, Bernstein, A., additional, Bhatti, A., additional, Biekert, A., additional, Biesiadzinski, T. P., additional, Birch, H. J., additional, Blockinger, G. M., additional, Bodnia, E., additional, Boxer, B., additional, Brew, C. A. J., additional, Brás, P., additional, Burdin, S., additional, Busenitz, J. K., additional, Buuck, M., additional, Cabrita, R., additional, Carmona-Benitez, M. C., additional, Cascella, M., additional, Chan, C., additional, Chott, N. I., additional, Cole, A., additional, Converse, M. V., additional, Cottle, A., additional, Cox, G., additional, Creaner, O., additional, Cutter, J. E., additional, Dahl, C. E., additional, de Viveiros, L., additional, Dobson, J. E. Y., additional, Druszkiewicz, E., additional, Eriksen, S. R., additional, Fan, A., additional, Fayer, S., additional, Fearon, N. M., additional, Fiorucci, S., additional, Flaecher, H., additional, Fraser, E. D., additional, Fruth, T., additional, Gaitskell, R. J., additional, Genovesi, J., additional, Ghag, C., additional, Gibson, E., additional, Gokhale, S., additional, van der Grinten, M. G. D., additional, Gwilliam, C. B., additional, Hall, C. R., additional, Hardy, C. A., additional, Haselschwardt, S. J., additional, Hertel, S. A., additional, Horn, M., additional, Huang, D. Q., additional, Ignarra, C. M., additional, Jahangir, O., additional, James, R. S., additional, Ji, W., additional, Johnson, J., additional, Kaboth, A. C., additional, Kamaha, A. C., additional, Kamdin, K., additional, Kazkaz, K., additional, Khaitan, D., additional, Khazov, A., additional, Khurana, I., additional, Kodroff, D., additional, Korley, L., additional, Korolkova, E. V., additional, Kraus, H., additional, Kravitz, S., additional, Kreczko, L., additional, Krikler, B., additional, Kudryavtsev, V. A., additional, Leason, E. A., additional, Lee, J., additional, Leonard, D. S., additional, Lesko, K. T., additional, Levy, C., additional, Li, J., additional, Liao, J., additional, Lindote, A., additional, Linehan, R., additional, Lippincott, W. H., additional, Liu, X., additional, Lopes, M. I., additional, Lopez Asamar, E., additional, López Paredes, B., additional, Lorenzon, W., additional, Luitz, S., additional, Majewski, P. A., additional, Manalaysay, A., additional, Manenti, L., additional, Mannino, R. L., additional, Marangou, N., additional, McCarthy, M. E., additional, McKinsey, D. N., additional, McLaughlin, J., additional, Miller, E. H., additional, Mizrachi, E., additional, Monte, A., additional, Monzani, M. E., additional, Morad, J. A., additional, Morales Mendoza, J. D., additional, Morrison, E., additional, Mount, B. J., additional, Murphy, A. St. J., additional, Naim, D., additional, Naylor, A., additional, Nedlik, C., additional, Nelson, H. N., additional, Neves, F., additional, Nikoleyczik, J. A., additional, Nilima, A., additional, Nguyen, A., additional, Olcina, I., additional, Oliver-Mallory, K. C., additional, Pal, S., additional, Palladino, K. J., additional, Palmer, J., additional, Patton, S., additional, Parveen, N., additional, Pease, E. K., additional, Penning, B., additional, Pereira, G., additional, Piepke, A., additional, Qie, Y., additional, Reichenbacher, J., additional, Rhyne, C. A., additional, Richards, A., additional, Riffard, Q., additional, Rischbieter, G. R. C., additional, Rosero, R., additional, Rossiter, P., additional, Santone, D., additional, Sazzad, A. B. M. R., additional, Schnee, R. W., additional, Scovell, P. R., additional, Shaw, S., additional, Shutt, T. A., additional, Silk, J. J., additional, Silva, C., additional, Smith, R., additional, Solmaz, M., additional, Solovov, V. N., additional, Sorensen, P., additional, Soria, J., additional, Stancu, I., additional, Stevens, A., additional, Stifter, K., additional, Suerfu, B., additional, Sumner, T. J., additional, Swanson, N., additional, Szydagis, M., additional, Taylor, W. C., additional, Taylor, R., additional, Temples, D. J., additional, Terman, P. A., additional, Tiedt, D. R., additional, Timalsina, M., additional, To, W. H., additional, Tovey, D. R., additional, Tripathi, M., additional, Tronstad, D. R., additional, Turner, W., additional, Utku, U., additional, Vaitkus, A., additional, Wang, B., additional, Wang, J. J., additional, Wang, W., additional, Watson, J. R., additional, Webb, R. C., additional, White, R. G., additional, Whitis, T. J., additional, Williams, M., additional, Wolfs, F. L. H., additional, Woodward, D., additional, Wright, C. J., additional, Xiang, X., additional, Xu, J., additional, Yeh, M., additional, and Zarzhitsky, P., additional
Published: 2021
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