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2,659 results on '"H. Maruyama"'

1. Postoperative decrease in Hounsfield unit values at adjacent vertebrae after thoraco-pelvic fusion as a risk factor of proximal junctional kyphosis and failure

Author: K. Tsuchiya, I. Okano, Y. Dodo, C. Hayakawa, R. Yamamura, H. Maruyama, T. Yasukawa, T. Shirahata, and Y. Kudo
Subjects: Neurology. Diseases of the nervous system, RC346-429
Published: 2024
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2. An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA’s analysis method

Author: Govinda Adhikari, Nelson Carlin, JaeJin Choi, Seonho Choi, Anthony Ezeribe, Luis Eduardo França, Chang Hyon Ha, In Sik Hahn, Sophia J. Hollick, Eunju Jeon, Jay Hyun Jo, Han Wool Joo, Woon Gu Kang, Matthew Kauer, Bongho Kim, Hongjoo Kim, Jinyoung Kim, Kyungwon Kim, SungHyun Kim, Sun Kee Kim, Won Kyung Kim, Yeongduk Kim, Yong-Hamb Kim, Young Ju Ko, Doo Hyok Lee, Eun Kyung Lee, Hyunseok Lee, Hyun Su Lee, Hye Young Lee, In Soo Lee, Jaison Lee, Jooyoung Lee, Moo Hyun Lee, Seo Hyun Lee, Seung Mok Lee, Yu Jin Lee, Douglas Leonard, Bruno B. Manzato, Reina H. Maruyama, Robert J. Neal, James A. Nikkel, Stephen L. Olsen, Byung Ju Park, Hyang Kyu Park, Hyeonseo Park, Kangsoon Park, Se Dong Park, Ricardo L. C. Pitta, Hafizh Prihtiadi, Sejin Ra, Carsten Rott, Keon Ah Shin, Andrew Scarff, Neil J. C. Spooner, William G. Thompson, Liang Yang, and Gyun Ho Yu
Subjects: Medicine, Science
Abstract: Abstract The DAMA/LIBRA collaboration has reported the observation of an annual modulation in the event rate that has been attributed to dark matter interactions over the last two decades. However, even though tremendous efforts to detect similar dark matter interactions were pursued, no definitive evidence has been observed to corroborate the DAMA/LIBRA signal. Many studies assuming various dark matter models have attempted to reconcile DAMA/LIBRA’s modulation signals and null results from other experiments, however no clear conclusion can be drawn. Apart from the dark matter hypothesis, several studies have examined the possibility that the modulation is induced by variations in detector’s environment or their specific analysis methods. In particular, a recent study presents a possible cause of the annual modulation from an analysis method adopted by the DAMA/LIBRA experiment in which the observed annual modulation could be reproduced by a slowly varying time-dependent background. Here, we study the COSINE-100 data using an analysis method similar to the one adopted by the DAMA/LIBRA experiment and observe a significant annual modulation, however the modulation phase is almost opposite to that of the DAMA/LIBRA data. Assuming the same background composition for COSINE-100 and DAMA/LIBRA, simulated experiments for the DAMA/LIBRA without dark matter signals also provide significant annual modulation with an amplitude similar to DAMA/LIBRA with opposite phase. Even though this observation does not directly explain the DAMA/LIBRA results directly, this interesting phenomenon motivates more profound studies of the time-dependent DAMA/LIBRA background data.
Published: 2023
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3. Optimization of the first CUPID detector module

Author: CUPID Collaboration, K. Alfonso, A. Armatol, C. Augier, F. T. Avignone, O. Azzolini, M. Balata, A. S. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, M. Bettelli, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Campani, C. Capelli, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, E. Celi, C. Chang, D. Chiesa, M. Clemenza, I. Colantoni, S. Copello, E. Craft, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’Addabbo, G. D’Imperio, S. Dabagov, I. Dafinei, F. A. Danevich, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, S. Di Lorenzo, T. Dixon, V. Dompè, A. Drobizhev, L. Dumoulin, G. Fantini, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, L. Foggetta, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, A. Gallas, J. Gascon, S. Ghislandi, A. Giachero, A. Gianvecchio, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, C. Grant, P. Gras, P. V. Guillaumon, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, D. L. Helis, H. Z. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. I. Konovalov, R. Kowalski, T. Langford, M. Lefevre, R. Liu, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, Ph. Mas, B. Mauri, D. Mayer, G. Mazzitelli, Y. Mei, S. Milana, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, S. Nisi, C. Nones, E. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, M. Olmi, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, L. Pattavina, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, O. G. Polischuk, I. Ponce, S. Pozzi, E. Previtali, A. Puiu, S. Quitadamo, A. Ressa, R. Rizzoli, C. Rosenfeld, P. Rosier, J. Scarpaci, B. Schmidt, V. Sharma, V. N. Shlegel, V. Singh, M. Sisti, P. Slocum, D. Speller, P. T. Surukuchi, L. Taffarello, C. Tomei, J. A. Torres, V. I. Tretyak, A. Tsymbaliuk, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, R. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. I. Umatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract CUPID will be a next generation experiment searching for the neutrinoless double $$\beta $$ β decay, whose discovery would establish the Majorana nature of the neutrino. Based on the experience achieved with the CUORE experiment, presently taking data at LNGS, CUPID aims to reach a background free environment by means of scintillating Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals coupled to light detectors. Indeed, the simultaneous heat and light detection allows us to reject the dominant background of $$\alpha $$ α particles, as proven by the CUPID-0 and CUPID-Mo demonstrators. In this work we present the results of the first test of the CUPID baseline module. In particular, we propose a new optimized detector structure and light sensors design to enhance the engineering and the light collection, respectively. We characterized the heat detectors, achieving an energy resolution of (5.9 ± 0.2) keV FWHM at the Q-value of $$^{100}$$ 100 Mo (about 3034 keV). We studied the light collection of the baseline CUPID design with respect to an alternative configuration which features gravity-assisted light detectors’ mounting. In both cases we obtained an improvement in the light collection with respect to past measures and we validated the particle identification capability of the detector, which ensures an $$\alpha $$ α particle rejection higher than 99.9%, fully satisfying the requirements for CUPID.
Published: 2022
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4. Background modeling for dark matter search with 1.7 years of COSINE-100 data

Author: G. Adhikari, E. Barbosa de Souza, N. Carlin, J. J. Choi, S. Choi, M. Djamal, A. C. Ezeribe, L. E. França, C. Ha, I. S. Hahn, E. J. Jeon, J. H. Jo, H. W. Joo, W. G. Kang, M. Kauer, H. Kim, H. J. Kim, K. W. Kim, S. H. Kim, S. K. Kim, W. K. Kim, Y. D. Kim, Y. H. Kim, Y. J. Ko, E. K. Lee, H. Lee, H. S. Lee, H. Y. Lee, I. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, S. H. Lee, S. M. Lee, D. S. Leonard, W. A. Lynch, B. B. Manzato, R. H. Maruyama, R. J. Neal, S. L. Olsen, B. J. Park, H. K. Park, H. S. Park, K. S. Park, R. L. C. Pitta, H. Prihtiadi, S. J. Ra, C. Rott, K. A. Shin, A. Scarff, N. J. C. Spooner, W. G. Thompson, L. Yang, G. H. Yu, and COSINE-100 Collaboration
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract We present a background model for dark matter searches using an array of NaI(Tl) crystals in the COSINE-100 experiment that is located in the Yangyang underground laboratory. The model includes background contributions from both internal and external sources, including cosmogenic radionuclides and surface $$^{210}$$ 210 Pb contamination. To build the model in the low energy region, with a threshold of 1 keV, we used a depth profile of $$^{210}$$ 210 Pb contamination in the surface of the NaI(Tl) crystals determined in a comparison between measured and simulated spectra. We also considered the effect of the energy scale errors propagated from the statistical uncertainties and the nonlinear detector response at low energies. The 1.7 years COSINE-100 data taken between October 21, 2016 and July 18, 2018 were used for this analysis. Our Monte Carlo simulation provides a non-Gaussian peak around 50 keV originating from beta decays of bulk $$^{210}$$ 210 Pb in a good agreement with the measured background. This model estimates that the activities of bulk $$^{210}$$ 210 Pb and $$^{3}$$ 3 H are dominating the background rate that amounts to an average level of $$2.85\pm 0.15$$ 2.85 ± 0.15 counts/day/keV/kg in the energy region of (1–6) keV, using COSINE-100 data with a total exposure of 97.7 kg $$\cdot $$ · years.
Published: 2021
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5. Identification of new isomers in $$^{228}$$ 228 Ac: impact on dark matter searches

Author: K. W. Kim, G. Adhikari, E. Barbosa de Souza, N. Carlin, J. J. Choi, S. Choi, M. Djamal, A. C. Ezeribe, L. E. França, C. Ha, I. S. Hahn, E. J. Jeon, J. H. Jo, W. G. Kang, M. Kauer, H. Kim, H. J. Kim, S. H. Kim, S. K. Kim, W. K. Kim, Y. D. Kim, Y. H. Kim, Y. J. Ko, E. K. Lee, H. Lee, H. S. Lee, H. Y. Lee, I. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, S. H. Lee, S. M. Lee, D. S. Leonard, B. B. Manzato, R. H. Maruyama, R. J. Neal, S. L. Olsen, B. J. Park, H. K. Park, H. S. Park, K. S. Park, R. L. C. Pitta, H. Prihtiadi, S. J. Ra, C. Rott, K. A. Shin, A. Scarff, N. J. C. Spooner, W. G. Thompson, L. Yang, G. H. Yu, and COSINE-100 Collaboration
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract We report the identification of metastable isomeric states of $$^{228}$$ 228 Ac at 6.28 keV, 6.67 keV and 20.19 keV, with lifetimes of an order of 100 ns. These states are produced by the $$\beta $$ β -decay of $$^{228}$$ 228 Ra, a component of the $$^{232}$$ 232 Th decay chain, with $$\beta $$ β Q-values of 39.52 keV, 39.13 keV and 25.61 keV, respectively. Due to the low Q-value of $$^{228}$$ 228 Ra as well as the relative abundance of $$^{232}$$ 232 Th and their progeny in low background experiments, these observations potentially impact the low-energy background modeling of dark matter search experiments.
Published: 2021
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6. Search for double-beta decay of $$\mathrm {^{130}Te}$$ 130 Te to the $$0^+$$ 0 + states of $$\mathrm {^{130}Xe}$$ 130 Xe with CUORE

Author: D. Q. Adams, C. Alduino, K. Alfonso, F. T. III Avignone, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, E. Celi, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D’Addabbo, I. Dafinei, C. J. Davis, S. Dell’Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, S. H. Fu, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, D. Mayer, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, A. Nucciotti, I. Nutini, T. O’Donnell, J. L. Ouellet, S. Pagan, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Sharma, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, F. Terranova, C. Tomei, K. J. Vetter, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, S. Zimmermann, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The CUORE experiment is a large bolometric array searching for the lepton number violating neutrino-less double beta decay ( $$0\nu \beta \beta $$ 0 ν β β ) in the isotope $$\mathrm {^{130}Te}$$ 130 Te . In this work we present the latest results on two searches for the double beta decay (DBD) of $$\mathrm {^{130}Te}$$ 130 Te to the first $$0^{+}_2$$ 0 2 + excited state of $$\mathrm {^{130}Xe}$$ 130 Xe : the $$0\nu \beta \beta $$ 0 ν β β decay and the Standard Model-allowed two-neutrinos double beta decay ( $$2\nu \beta \beta $$ 2 ν β β ). Both searches are based on a 372.5 kg $$\times $$ × yr TeO $$_2$$ 2 exposure. The de-excitation gamma rays emitted by the excited Xe nucleus in the final state yield a unique signature, which can be searched for with low background by studying coincident events in two or more bolometers. The closely packed arrangement of the CUORE crystals constitutes a significant advantage in this regard. The median limit setting sensitivities at 90% Credible Interval (C.I.) of the given searches were estimated as $$\mathrm {S^{0\nu }_{1/2} = 5.6 \times 10^{24} \, \mathrm {yr}}$$ S 1 / 2 0 ν = 5.6 × 10 24 yr for the $${0\nu \beta \beta }$$ 0 ν β β decay and $$\mathrm {S^{2\nu }_{1/2} = 2.1 \times 10^{24} \, \mathrm {yr}}$$ S 1 / 2 2 ν = 2.1 × 10 24 yr for the $${2\nu \beta \beta }$$ 2 ν β β decay. No significant evidence for either of the decay modes was observed and a Bayesian lower bound at $$90\%$$ 90 % C.I. on the decay half lives is obtained as: $$\mathrm {(T_{1/2})^{0\nu }_{0^+_2} > 5.9 \times 10^{24} \, \mathrm {yr}}$$ ( T 1 / 2 ) 0 2 + 0 ν > 5.9 × 10 24 yr for the $$0\nu \beta \beta $$ 0 ν β β mode and $$\mathrm {(T_{1/2})^{2\nu }_{0^+_2} > 1.3 \times 10^{24} \, \mathrm {yr}}$$ ( T 1 / 2 ) 0 2 + 2 ν > 1.3 × 10 24 yr for the $$2\nu \beta \beta $$ 2 ν β β mode. These represent the most stringent limits on the DBD of $$^{130}$$ 130 Te to excited states and improve by a factor $$\sim 5$$ ∼ 5 the previous results on this process.
Published: 2021
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7. Characterization of cubic Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals for the CUPID experiment

Author: The CUPID Collaboration, A. Armatol, E. Armengaud, W. Armstrong, C. Augier, F. T. Avignone, O. Azzolini, A. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, L. Bergé, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, A. Cazes, E. Celi, C. Chang, M. Chapellier, A. Charrier, D. Chiesa, M. Clemenza, I. Colantoni, F. Collamati, S. Copello, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’Addabbo, G. D’Imperio, I. Dafinei, F. A. Danevich, M. de Combarieu, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, V. Dompè, A. Drobizhev, L. Dumoulin, G. Fantini, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, J. Gascon, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, P. Gras, M. Gros, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, D. L. Helis, H. Z. Huang, R. G. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. Konovalov, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, R. Mariam, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, B. Mauri, D. Mayer, Y. Mei, S. Milana, D. Misiak, T. Napolitano, M. Nastasi, X. F. Navick, J. Nikkel, R. Nipoti, S. Nisi, C. Nones, E. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, C. Oriol, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, P. Pari, L. Pattavina, B. Paul, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, T. Polakovic, O. G. Polischuk, S. Pozzi, E. Previtali, A. Puiu, A. Ressa, R. Rizzoli, C. Rosenfeld, C. Rusconi, V. Sanglard, J. A. Scarpaci, B. Schmidt, V. Sharma, V. Shlegel, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, O. Tellier, C. Tomei, V. I. Tretyak, A. Tsymbaliuk, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. Yumatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of ( $$6.7\pm 0.6$$ 6.7 ± 0.6 ) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of $$\alpha $$ α particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this $$\alpha $$ α -induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector.
Published: 2021
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8. Double-beta decay of $$^{130}\hbox {Te}$$ 130Te to the first $$0^+$$ 0+ excited state of $$^{130}\hbox {Xe}$$ 130Xe with CUORE-0

Author: C. Alduino, K. Alfonso, D. R. Artusa, F. T. Avignone III, O. Azzolini, T. I. Banks, G. Bari, J. W. Beeman, F. Bellini, A. Bersani, M. Biassoni, C. Brofferio, C. Bucci, A. Camacho, A. Caminata, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Carbone, L. Cardani, P. Carniti, N. Casali, L. Cassina, D. Chiesa, N. Chott, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, J. S. Cushman, A. D’Addabbo, I. Dafinei, C. J. Davis, S. Dell’Oro, M. M. Deninno, S. Di Domizio, M. L. Di Vacri, A. Drobizhev, D. Q. Fang, M. Faverzani, J. Feintzeig, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, L. Gladstone, P. Gorla, C. Gotti, T. D. Gutierrez, E. E. Haller, K. Han, E. Hansen, K. M. Heeger, R. Hennings-Yeomans, K. P. Hickerson, H. Z. Huang, R. Kadel, G. Keppel, Yu. G. Kolomensky, A. Leder, C. Ligi, K. E. Lim, X. Liu, Y. G. Ma, M. Maino, L. Marini, M. Martinez, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, P. J. Mosteiro, T. Napolitano, C. Nones, E. B. Norman, A. Nucciotti, T. O’Donnell, F. Orio, J. L. Ouellet, C. E. Pagliarone, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, G. Piperno, C. Pira, S. Pirro, S. Pozzi, E. Previtali, C. Rosenfeld, C. Rusconi, S. Sangiorgio, D. Santone, N. D. Scielzo, V. Singh, M. Sisti, A. R. Smith, L. Taffarello, M. Tenconi, F. Terranova, C. Tomei, S. Trentalange, M. Vignati, S. L. Wagaarachchi, B. S. Wang, H. W. Wang, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, G. Q. Zhang, B. X. Zhu, S. Zimmermann, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract We report on a search for double beta decay of $$^{130}\hbox {Te}$$ 130Te to the first $$0^{+}$$ 0+ excited state of $$^{130}\hbox {Xe}$$ 130Xe using a $$9.8\,\hbox {kg}\cdot \hbox {yr}$$ 9.8kg·yr exposure of $$^{130}\hbox {Te}$$ 130Te collected with the CUORE-0 experiment. In this work we exploit different topologies of coincident events to search for both the neutrinoless and two-neutrino double beta decay modes. We find no evidence for either mode and place lower bounds on the half-lives: $$T^{0\nu }_{0^+_1}>7.9\cdot 10^{23}\hbox {yr}$$ T01+0ν>7.9·1023yr and $$T^{2\nu }_{0^+_1}>2.4\cdot 10^{23}\hbox {yr}$$ T01+2ν>2.4·1023yr ($$90\%\,\hbox {CL}$$ 90%CL ). Combining our results with those obtained by the CUORICINO experiment, we achieve the most stringent constraints available for these processes: $$T^{0\nu }_{0^+_1}>1.4\cdot 10^{24}\hbox {yr}$$ T01+0ν>1.4·1024yr and $$T^{2\nu }_{0^+_1}>2.5\cdot 10^{23}\hbox {yr}$$ T01+2ν>2.5·1023yr ($$90\%\,\hbox {CL}$$ 90%CL ).
Published: 2019
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9. Background model for the NaI(Tl) crystals in COSINE-100

Author: P. Adhikari, G. Adhikari, E. Barbosa de Souza, N. Carlin, S. Choi, W. Q. Choi, M. Djamal, A. C. Ezeribe, C. Ha, I. S. Hahn, A. J. F. Hubbard, E. J. Jeon, J. H. Jo, H. W. Joo, W. G. Kang, M. Kauer, W. S. Kang, B. H. Kim, H. Kim, H. J. Kim, K. W. Kim, M. C. Kim, N. Y. Kim, S. K. Kim, Y. D. Kim, Y. H. Kim, V. A. Kudryavtsev, H. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, D. S. Leonard, W. A. Lynch, R. H. Maruyama, F. Mouton, S. L. Olsen, H. K. Park, H. S. Park, J. S. Park, K. S. Park, W. Pettus, H. Prihtiadi, S. Ra, C. Rott, A. Scarff, N. J. C. Spooner, W. G. Thompson, L. Yang, and S. H. Yong
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The COSINE-100 dark matter search experiment is an array of NaI(Tl) crystal detectors located in the Yangyang Underground Laboratory (Y2L). To understand measured backgrounds in the NaI(Tl) crystals we have performed Monte Carlo simulations using the Geant4 toolkit and developed background models for each crystal that consider contributions from both internal and external sources, including cosmogenic nuclides. The background models are based on comparisons of measurement data with Monte Carlo simulations that are guided by a campaign of material assays and are used to evaluate backgrounds and identify their sources. The average background level for the six crystals (70 kg total mass) that are studied is 3.5 counts/day/keV/kg in the (2–6) keV energy interval. The dominant contributors in this energy region are found to be $$^{210}$$ 210 Pb and $$^3$$ 3 H.
Published: 2018
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10. Initial performance of the COSINE-100 experiment

Author: G. Adhikari, P. Adhikari, E. Barbosa de Souza, N. Carlin, S. Choi, W. Q. Choi, M. Djamal, A. C. Ezeribe, C. Ha, I. S. Hahn, A. J. F. Hubbard, E. J. Jeon, J. H. Jo, H. W. Joo, W. G. Kang, W. Kang, M. Kauer, B. H. Kim, H. Kim, H. J. Kim, K. W. Kim, M. C. Kim, N. Y. Kim, S. K. Kim, Y. D. Kim, Y. H. Kim, V. A. Kudryavtsev, H. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, D. S. Leonard, K. E. Lim, W. A. Lynch, R. H. Maruyama, F. Mouton, S. L. Olsen, H. K. Park, H. S. Park, J. S. Park, K. S. Park, W. Pettus, Z. P. Pierpoint, H. Prihtiadi, S. Ra, F. R. Rogers, C. Rott, A. Scarff, N. J. C. Spooner, W. G. Thompson, L. Yang, and S. H. Yong
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract COSINE is a dark matter search experiment based on an array of low background NaI(Tl) crystals located at the Yangyang underground laboratory. The assembly of COSINE-100 was completed in the summer of 2016 and the detector is currently collecting physics quality data aimed at reproducing the DAMA/LIBRA experiment that reported an annual modulation signal. Stable operation has been achieved and will continue for at least 2 years. Here, we describe the design of COSINE-100, including the shielding arrangement, the configuration of the NaI(Tl) crystal detection elements, the veto systems, and the associated operational systems, and we show the current performance of the experiment.
Published: 2018
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11. Brazilian porcupinepox virus infection in a free-ranging neotropical porcupine in Mato Grosso, Brazil

Author: David J. F. Silva, Janaina M. A. R. Moreira, Marlon Ribeiro, Fernanda H. Maruyama, Thaís O. Morgado, Luciano Nakazato, Valeria Dutra, Marcos A. Souza, and Edson M. Colodel
Subjects: General Veterinary
Abstract: Although the novel Brazilian porcupinepox virus (BPoPV) can infect wild porcupines, its lethality and zoonotic potential are not well-established. In May 2021, a free-ranging neotropical porcupine ( Coendou longicaudatus boliviensis) rescued from the natural savanna in the Brazilian Cerrado, Mato Grosso State, was presented with a lethal poxviral infection. Clinical signs and PCR detection of BPoPV supported the diagnosis. Poxviral lesions included erythema, exfoliative dermatitis, and erosions involving mainly the face, hindlimb, and vulva. Histologically, the lesions consisted of proliferative and necrotic dermatitis, intraepidermal and follicular pustules, and intracytoplasmic inclusion bodies in keratinocytes. Phylogenetic analysis revealed BPoPV strains closely related to other rodent-infecting poxviruses. This poxviral infection resulted in the death of a specimen of C. l. boliviensis; the effect on species conservation, and the potential of spillover into humans and other vertebrates remain unknown.
Published: 2023
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12. Low energy analysis techniques for CUORE

Author: C. Alduino, K. Alfonso, D. R. Artusa, F. T. Avignone, O. Azzolini, G. Bari, J. W. Beeman, F. Bellini, G. Benato, A. Bersani, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, A. Camacho, A. Caminata, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, L. Cassina, D. Chiesa, N. Chott, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, J. S. Cushman, A. D’Addabbo, D. D’Aguanno, I. Dafinei, C. J. Davis, S. Dell’Oro, M. M. Deninno, S. Di Domizio, M. L. Di Vacri, A. Drobizhev, D. Q. Fang, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, L. Gladstone, P. Gorla, C. Gotti, T. D. Gutierrez, E. E. Haller, K. Han, E. Hansen, K. M. Heeger, R. Hennings-Yeomans, H. Z. Huang, R. Kadel, G. Keppel, Yu. G. Kolomensky, A. Leder, C. Ligi, K. E. Lim, Y. G. Ma, M. Maino, L. Marini, M. Martinez, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, P. J. Mosteiro, T. Napolitano, M. Nastasi, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, T. O’Donnell, J. L. Ouellet, C. E. Pagliarone, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, G. Piperno, C. Pira, S. Pirro, S. Pozzi, E. Previtali, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, D. Santone, B. Schmidt, J. Schmidt, N. D. Scielzo, V. Singh, M. Sisti, A. R. Smith, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, H. W. Wang, B. Welliver, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, G. Q. Zhang, S. Zimmermann, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract CUORE is a tonne-scale cryogenic detector operating at the Laboratori Nazionali del Gran Sasso (LNGS) that uses tellurium dioxide bolometers to search for neutrinoless double-beta decay of $$^{130}$$ 130 Te. CUORE is also suitable to search for low energy rare events such as solar axions or WIMP scattering, thanks to its ultra-low background and large target mass. However, to conduct such sensitive searches requires improving the energy threshold to 10 keV. In this paper, we describe the analysis techniques developed for the low energy analysis of CUORE-like detectors, using the data acquired from November 2013 to March 2015 by CUORE-0, a single-tower prototype designed to validate the assembly procedure and new cleaning techniques of CUORE. We explain the energy threshold optimization, continuous monitoring of the trigger efficiency, data and event selection, and energy calibration at low energies in detail. We also present the low energy background spectrum of CUORE-0 below $$60 \, \mathrm {keV}$$ 60 keV . Finally, we report the sensitivity of CUORE to WIMP annual modulation using the CUORE-0 energy threshold and background, as well as an estimate of the uncertainty on the nuclear quenching factor from nuclear recoils inCUORE-0.
Published: 2017
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13. CUORE sensitivity to $$0\nu \beta \beta $$ 0 ν β β decay

Author: C. Alduino, K. Alfonso, D. R. Artusa, F. T. Avignone, O. Azzolini, T. I. Banks, G. Bari, J. W. Beeman, F. Bellini, G. Benato, A. Bersani, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, A. Camacho, A. Caminata, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Carbone, L. Cardani, P. Carniti, N. Casali, L. Cassina, D. Chiesa, N. Chott, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, J. S. Cushman, A. D’Addabbo, I. Dafinei, C. J. Davis, S. Dell’Oro, M. M. Deninno, S. Di Domizio, M. L. Di Vacri, A. Drobizhev, D. Q. Fang, M. Faverzani, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, L. Gladstone, P. Gorla, C. Gotti, T. D. Gutierrez, E. E. Haller, K. Han, E. Hansen, K. M. Heeger, R. Hennings-Yeomans, K. P. Hickerson, H. Z. Huang, R. Kadel, G. Keppel, Yu. G. Kolomensky, A. Leder, C. Ligi, K. E. Lim, Y. G. Ma, M. Maino, L. Marini, M. Martinez, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, P. J. Mosteiro, T. Napolitano, M. Nastasi, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, T. O’Donnell, J. L. Ouellet, C. E. Pagliarone, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, G. Piperno, C. Pira, S. Pirro, S. Pozzi, E. Previtali, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, D. Santone, B. Schmidt, J. Schmidt, N. D. Scielzo, V. Singh, M. Sisti, A. R. Smith, L. Taffarello, M. Tenconi, F. Terranova, C. Tomei, S. Trentalange, M. Vignati, S. L. Wagaarachchi, B. S. Wang, H. W. Wang, B. Welliver, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, G. Q. Zhang, B. X. Zhu, S. Zimmermann, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract We report a study of the CUORE sensitivity to neutrinoless double beta ( $$0\nu \beta \beta $$ 0 ν β β ) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the $$0\nu \beta \beta $$ 0 ν β β decay half-life ( $$T_{1/2}^{\,0\nu }$$ T 1 / 2 0 ν ) at $$90\%$$ 90 % credibility interval (CI) – i.e. the interval containing the true value of $$T_{1/2}^{\,0\nu }$$ T 1 / 2 0 ν with $$90\%$$ 90 % probability – and the $$3~\sigma $$ 3 σ discovery sensitivity. We consider various background levels and energy resolutions, and describe the influence of the data division in subsets with different background levels. If the background level and the energy resolution meet the expectation, CUORE will reach a $$90\%$$ 90 % CI exclusion sensitivity of $$2\cdot 10^{25}$$ 2 · 10 25 year with 3 months, and $$9\cdot 10^{25}$$ 9 · 10 25 year with 5 years of live time. Under the same conditions, the discovery sensitivity after 3 months and 5 years will be $$7\cdot 10^{24}$$ 7 · 10 24 year and $$4\cdot 10^{25}$$ 4 · 10 25 year, respectively.
Published: 2017
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14. The projected background for the CUORE experiment

Author: C. Alduino, K. Alfonso, D. R. Artusa, F. T. Avignone, O. Azzolini, T. I. Banks, G. Bari, J. W. Beeman, F. Bellini, G. Benato, A. Bersani, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, A. Camacho, A. Caminata, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Carbone, L. Cardani, P. Carniti, N. Casali, L. Cassina, D. Chiesa, N. Chott, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, J. S. Cushman, A. D’Addabbo, I. Dafinei, C. J. Davis, S. Dell’Oro, M. M. Deninno, S. Di Domizio, M. L. Di Vacri, A. Drobizhev, D. Q. Fang, M. Faverzani, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, L. Gladstone, P. Gorla, C. Gotti, T. D. Gutierrez, E. E. Haller, K. Han, E. Hansen, K. M. Heeger, R. Hennings-Yeomans, K. P. Hickerson, H. Z. Huang, R. Kadel, G. Keppel, Yu. G. Kolomensky, A. Leder, C. Ligi, K. E. Lim, Y. G. Ma, M. Maino, L. Marini, M. Martinez, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, P. J. Mosteiro, T. Napolitano, M. Nastasi, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, T. O’Donnell, J. L. Ouellet, C. E. Pagliarone, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, G. Piperno, C. Pira, S. Pirro, S. Pozzi, E. Previtali, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, D. Santone, B. Schmidt, J. Schmidt, N. D. Scielzo, V. Singh, M. Sisti, A. R. Smith, L. Taffarello, M. Tenconi, F. Terranova, C. Tomei, S. Trentalange, M. Vignati, S. L. Wagaarachchi, B. S. Wang, H. W. Wang, B. Welliver, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, G. Q. Zhang, B. X. Zhu, S. Zimmermann, S. Zucchelli, and M. Laubenstein
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The Cryogenic Underground Observatory for Rare Events (CUORE) is designed to search for neutrinoless double beta decay of $$^{130}$$ 130 Te with an array of 988 TeO $$_2$$ 2 bolometers operating at temperatures around 10 mK. The experiment is currently being commissioned in Hall A of Laboratori Nazionali del Gran Sasso, Italy. The goal of CUORE is to reach a 90% C.L. exclusion sensitivity on the $$^{130}$$ 130 Te decay half-life of 9 $$\times $$ × 10 $$^{25}$$ 25 years after 5 years of data taking. The main issue to be addressed to accomplish this aim is the rate of background events in the region of interest, which must not be higher than 10 $$^{-2}$$ - 2 counts/keV/kg/year. We developed a detailed Monte Carlo simulation, based on results from a campaign of material screening, radioassays, and bolometric measurements, to evaluate the expected background. This was used over the years to guide the construction strategies of the experiment and we use it here to project a background model for CUORE. In this paper we report the results of our study and our expectations for the background rate in the energy region where the peak signature of neutrinoless double beta decay of $$^{130}$$ 130 Te is expected.
Published: 2017
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15. Pulmonary Granuloma Is Not Always the Tuberculosis Hallmark: Pathology of Tuberculosis Stages in New World and Old World Monkeys Naturally Infected with the Mycobacterium tuberculosis Complex

Author: Asheley H.B. Pereira, Claudia A.A. Lopes, Thalita A. Pissinatti, Ana C.A. Pinto, Daniel R.A. Oliveira, Gabriel M. Leal, Luís C.M. Oliveira, Paulo Redner, Bruna E.P. Barbosa, Silvia B. Moreira, Alcides Pissinatti, Fernanda H. Maruyama, Luciano Nakazato, Valéria Dutra, and Daniel G. Ubiali
Subjects: Granuloma, General Veterinary, Animals, Tuberculosis, Cercopithecidae, Mycobacterium tuberculosis, Pneumonia, Macaca mulatta, Brazil, Pathology and Forensic Medicine
Abstract: We present the pathology of monkeys naturally infected with Mycobacterium tuberculosis complex from five different colonies in Rio de Janeiro, Brazil. On the basis of gross and histopathological findings, the lesions were classified into chronic-active, extrapulmonary, early-activation or latent-reactivation stages. Typical granulomatous pneumonia was seen in 46.6% of cases (six rhesus monkeys [Macaca mulatta] and one Uta Hick's bearded saki [Chiropotes utahickae]). The absence of pulmonary granulomas did not preclude a diagnosis of tuberculosis (TB): classical granulomatous pneumonia was observed in the chronic-active and latent-reactivation stages but not in the extrapulmonary and early-activation stages. The early-activation stage was characterized by interstitial pneumonia with a predominance of foamy macrophages and molecular and immunohistochemical evidence of M. tuberculosis complex infection. TB should be considered as a cause of interstitial pneumonia in New World Monkeys. We recommend the use of immunohistochemistry and molecular analysis for diagnosis of TB, even when typical macroscopic or histological changes are not observed.
Published: 2022
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16. Can the Appellate Body Be Saved?

Author: Warren H. Maruyama
Subjects: Economics and Econometrics, Political Science and International Relations, Law
Abstract: The ‘Walker Paper’ represents a commendable effort to find middle-ground on the World Trade Organization (WTO) Appellate Body, but does not address the US concerns about the Appellate Body’s overreaching in antidumping, countervailing duty, and General Agreement on Tariffs and Trade (GATT) Article XIX ‘escape clause’ disputes, and instead seizes on a series of half-hearted fixes to the long list of concerns in US Trade Representative’s (USTR’s) ‘Report on the Appellate Body of the World Trade Organization’. US concerns about overreaching date back to the Bush 43 and Obama Administrations and are rooted in the Appellate Body’s ‘zeroing’ line of cases. The concerns rest on the conviction of US trade officials who participated in the Uruguay Round negotiations and later served in the Bush 43, Obama, and Trump Administrations, that there was never a WTO agreement to abolish ‘zeroing’. This view was shared by the WTO Secretariat and WTO Panels and underpinned the contentious, decade-long impasse between USTR, the WTO Secretariat, and WTO Panels on the one hand, and the Appellate Body and Appellate Body Secretariat on the other. While the Appellate Body’s overreaching has multiple sources, one is its dismissive approach to negotiating history under Article 32 of the Vienna Convention, and obsessive reliance on the Oxford English Dictionary as a main source of meaning in interpreting the WTO Agreements. Had the Appellate Body taken a more respectful look at the Uruguay Round negotiating history, it would have found no support for efforts to read a broad prohibition on zeroing into terms that dated back to the Kennedy Round Antidumping Agreement, Tokyo Round Antidumping Code, and GATT 1947. The Appellate Body’s overreaching also appears to stem from hubris, as some Appellate Body Members have sought to make their mark on international jurisprudence or serve as saviours of the WTO system. While some in Geneva are clearly hoping the US concerns will disappear once the Biden Administration takes office, these concerns predated Ambassador Lighthizer by over a decade and are shared by both Republicans and Democratic Members of Congress. Accordingly, even if the new Administration were to seize on some variant of the Walker paper as an excuse to placate US allies and trading partners, it’s unlikely to offer a lasting solution, since the same problems will likely recur without serious systemic and structural reforms. World Trade Organization, WTO, Appellate Body, Dispute Settlement Understanding, Dispute Settlement, Antidumping Agreement, Zeroing
Published: 2021
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17. Electromagnetically-induced-transparency spectroscopy of high-lying Rydberg states in K39

Author: Yuqi Zhu, Sumita Ghosh, S. B. Cahn, M. J. Jewell, D. H. Speller, and Reina H. Maruyama
Published: 2022
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18. 1103P Drug-related pneumonitis induced by osimertinib as first-line treatment for EGFR-positive non-small cell lung cancer: A real-world setting

Author: Y. Sato, H. Sumikawa, R. Shibaki, T. Morimoto, Y. Sakata, Y. Oya, M. Tamiya, H. Suzuki, H. Matsumoto, T. Kijima, K. Hashimoto, H. Kobe, A. Hino, M. Inaba, Y. Tsukita, H. Ikeda, D. Arai, H. Maruyama, S. Sakata, and D. Fujimoto
Subjects: Oncology, Hematology
Published: 2022
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19. CUORE opens the door to tonne-scale cryogenics experiments

Author: L. Canonica, L. Marini, Kevin Hickerson, J. Schmidt, Massimiliano Clemenza, Carlo Cosmelli, S. Copello, L. Gladstone, M. Guerzoni, L. Ma, J. Johnston, A. Leder, M. Iannone, Irene Nutini, Paolo Carniti, Vladimir Datskov, R. J. Creswick, M. M. Deninno, G. Fantini, F. Bellini, I. C. Bandac, Yu-Gang Ma, D. Santone, V. Sharma, C. Brofferio, P. J. Mosteiro, A. Caminata, Ezio Previtali, B. Welliver, Evelyn Ferri, H. Z. Huang, G. Keppel, K. E. Lim, X. G. Cao, F. Bragazzi, Ettore Fiorini, V. Novati, C. Rusconi, N. Chott, T. Wise, C. Crescentini, R. Gaigher, L. Zanotti, Andrea Giachero, C. Maiano, N. Moggi, C. Martinez Amaya, S. S. Nagorny, A. Pelosi, G. Piperno, D. Q. Adams, L. Risegari, K. Alfonso, F. Terranova, Davide Chiesa, C. Rosenfeld, Deqing Fang, S. Pagan, S. Dell'Oro, M. L. Di Vacri, D. Mayer, Samuele Sangiorgio, Stefano Nisi, P. T. Surukuchi, S. Morganti, S. Zucchelli, J. Camilleri, A. Nucciotti, M. Sisti, P. Gorla, E. V. Hansen, F. Ferroni, C. Tomei, Elena Sala, L. Ioannucci, D. Speller, F. Alessandria, M. I. Martínez, Eugene E. Haller, C. Alduino, F. Rimondi, G. Ceruti, K. Wilson, L. Taffarello, Marisa Pedretti, R. Hennings-Yeomans, S. Pirro, Carlo Ligi, M. Faverzani, M. Beretta, Y. Mei, M. Tessaro, Jeffrey W. Beeman, M. Capodiferro, A. Bersani, N. D. Scielzo, M. Barucci, L. Cappelli, D. Biare, C. J. Davis, A. Camacho, Jonathan Ouellet, D. Conventi, J. Wallig, K. M. Heeger, L. Pagnanini, A. Giuliani, G. Bari, M. Cariello, Lindley Winslow, A. Campani, S. L. Wagaarachchi, M. Maino, Guoqiang Zhang, M. Carrettoni, R. Mazza, A. Branca, A. Bryant, J. Nikkel, C. Pira, H.W. Wang, M. Perego, T. I. Banks, S. Zimmermann, Ke Han, Reina H. Maruyama, S. Ghislandi, T. O'Donnell, S. Di Domizio, Simone Capelli, R. W. Kadel, Stuart J. Freedman, G. Ventura, A. Drobizhev, C. Bulfon, C. Zarra, Laura Cardani, V. Dompè, M. Balata, L. Di Paolo, A. D'Addabbo, L. Pattavina, B. K. Fujikawa, Stefano Pozzi, Alan R. Smith, D. Orlandi, Larissa M. Ejzak, M. Vignati, B. X. Zhu, V. Pettinacci, L. Kogler, E. Celi, L. Tatananni, S.H. Fu, E. Andreotti, M. A. Franceschi, R. Cereseto, I. Dafinei, M. Sakai, D. D'Aguanno, F. Stivanello, R. G. Huang, D. Schaeffer, C. Guandalini, F. Orio, Vasundhara Singh, B. Schmidt, B. S. Wang, O. Azzolini, Kai Vetter, M. Olcese, Jeremy S. Cushman, V. Palmieri, Eric B. Norman, M. Guetti, T. Napolitano, M. Biassoni, F. Del Corso, R. Faccini, Giovanni Benato, A. Buccheri, C. Salvioni, Yu. G. Kolomensky, R. Pedrotta, Lorenzo Cassina, C. Nones, A. Puiu, Marco Pallavicini, S. Quitadamo, G. Pessina, James R. Wilson, R. Liu, Massimiliano Nastasi, M. Pavan, E. Olivieri, L. Gironi, F. T. Avignone, Claudio Gotti, N. Casali, F. Reindl, Oliviero Cremonesi, J. Goett, M. Tenconi, C. Pagliarone, C. Rossi, A. Chiarini, C. Bucci, T. D. Gutierrez, Adams, D, Alduino, C, Alessandria, F, Alfonso, K, Andreotti, E, Avignone, F, Azzolini, O, Balata, M, Bandac, I, Banks, T, Bari, G, Barucci, M, Beeman, J, Bellini, F, Benato, G, Beretta, M, Bersani, A, Biare, D, Biassoni, M, Bragazzi, F, Branca, A, Brofferio, C, Bryant, A, Buccheri, A, Bucci, C, Bulfon, C, Camacho, A, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Capodiferro, M, Cappelli, L, Cardani, L, Cariello, M, Carniti, P, Carrettoni, M, Casali, N, Cassina, L, Celi, E, Cereseto, R, Ceruti, G, Chiarini, A, Chiesa, D, Chott, N, Clemenza, M, Conventi, D, Copello, S, Cosmelli, C, Cremonesi, O, Crescentini, C, Creswick, R, Cushman, J, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Datskov, V, Davis, C, Corso, F, Dell'Oro, S, Deninno, M, Di Domizio, S, Dompe, V, Di Vacri, M, Di Paolo, L, Drobizhev, A, Ejzak, L, Faccini, R, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fu, S, Fujikawa, B, Gaigher, R, Ghislandi, S, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Goett, J, Gorla, P, Gotti, C, Guandalini, C, Guerzoni, M, Guetti, M, Gutierrez, T, Haller, E, Han, K, Hansen, E, Heeger, K, Hennings-Yeomans, R, Hickerson, K, Huang, R, Huang, H, Iannone, M, Ioannucci, L, Johnston, J, Kadel, R, Keppel, G, Kogler, L, Kolomensky, Y, Leder, A, Ligi, C, Lim, K, Liu, R, Ma, L, Ma, Y, Maiano, C, Maino, M, Marini, L, Martinez, M, Amaya, C, Maruyama, R, Mayer, D, Mazza, R, Mei, Y, Moggi, N, Morganti, S, Mosteiro, P, Nagorny, S, Napolitano, T, Nastasi, M, Nikkel, J, Nisi, S, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Olcese, M, Olivieri, E, Orio, F, Orlandi, D, Ouellet, J, Pagan, S, Pagliarone, C, Pagnanini, L, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pedretti, M, Pedrotta, R, Pelosi, A, Perego, M, Pessina, G, Pettinacci, V, Piperno, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Quitadamo, S, Reindl, F, Rimondi, F, Risegari, L, Rosenfeld, C, Rossi, C, Rusconi, C, Sakai, M, Sala, E, Salvioni, C, Sangiorgio, S, Santone, D, Schaeffer, D, Schmidt, B, Schmidt, J, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Smith, A, Speller, D, Stivanello, F, Surukuchi, P, Taffarello, L, Tatananni, L, Tenconi, M, Terranova, F, Tessaro, M, Tomei, C, Ventura, G, Vetter, K, Vignati, M, Wagaarachchi, S, Wallig, J, Wang, B, Wang, H, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zarra, C, Zhang, G, Zhu, B, Zimmermann, S, Zucchelli, S, Adams D.Q., Alduino C., Alessandria F., Alfonso K., Andreotti E., Avignone F.T., Azzolini O., Balata M., Bandac I., Banks T.I., Bari G., Barucci M., Beeman J.W., Bellini F., Benato G., Beretta M., Bersani A., Biare D., Biassoni M., Bragazzi F., Branca A., Brofferio C., Bryant A., Buccheri A., Bucci C., Bulfon C., Camacho A., Camilleri J., Caminata A., Campani A., Canonica L., Cao X.G., Capelli S., Capodiferro M., Cappelli L., Cardani L., Cariello M., Carniti P., Carrettoni M., Casali N., Cassina L., Celi E., Cereseto R., Ceruti G., Chiarini A., Chiesa D., Chott N., Clemenza M., Conventi D., Copello S., Cosmelli C., Cremonesi O., Crescentini C., Creswick R.J., Cushman J.S., D'Addabbo A., D'Aguanno D., Dafinei I., Datskov V., Davis C.J., Del Corso F., Dell'Oro S., Deninno M.M., Di Domizio S., Dompe V., Di Vacri M.L., Di Paolo L., Drobizhev A., Ejzak L., Faccini R., Fang D.Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S.J., Fu S.H., Fujikawa B.K., Gaigher R., Ghislandi S., Giachero A., Gironi L., Giuliani A., Gladstone L., Goett J., Gorla P., Gotti C., Guandalini C., Guerzoni M., Guetti M., Gutierrez T.D., Haller E.E., Han K., Hansen E.V., Heeger K.M., Hennings-Yeomans R., Hickerson K.P., Huang R.G., Huang H.Z., Iannone M., Ioannucci L., Johnston J., Kadel R., Keppel G., Kogler L., Kolomensky Y.G., Leder A., Ligi C., Lim K.E., Liu R., Ma L., Ma Y.G., Maiano C., Maino M., Marini L., Martinez M., Amaya C.M., Maruyama R.H., Mayer D., Mazza R., Mei Y., Moggi N., Morganti S., Mosteiro P.J., Nagorny S.S., Napolitano T., Nastasi M., Nikkel J., Nisi S., Nones C., Norman E.B., Novati V., Nucciotti A., Nutini I., O'Donnell T., Olcese M., Olivieri E., Orio F., Orlandi D., Ouellet J.L., Pagan S., Pagliarone C.E., Pagnanini L., Pallavicini M., Palmieri V., Pattavina L., Pavan M., Pedretti M., Pedrotta R., Pelosi A., Perego M., Pessina G., Pettinacci V., Piperno G., Pira C., Pirro S., Pozzi S., Previtali E., Puiu A., Quitadamo S., Reindl F., Rimondi F., Risegari L., Rosenfeld C., Rossi C., Rusconi C., Sakai M., Sala E., Salvioni C., Sangiorgio S., Santone D., Schaeffer D., Schmidt B., Schmidt J., Scielzo N.D., Sharma V., Singh V., Sisti M., Smith A.R., Speller D., Stivanello F., Surukuchi P.T., Taffarello L., Tatananni L., Tenconi M., Terranova F., Tessaro M., Tomei C., Ventura G., Vetter K.J., Vignati M., Wagaarachchi S.L., Wallig J., Wang B.S., Wang H.W., Welliver B., Wilson J., Wilson K., Winslow L.A., Wise T., Zanotti L., Zarra C., Zhang G.Q., Zhu B.X., Zimmermann S., Zucchelli S., 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, and CUORE
Subjects: Cryostat, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, Cryogenic temperatures, Dilution refrigerator, Low temperature calorimeter, Neutrinoless double beta decay, Rare event searches, Ton-scale detector, Cryogenic temperatures, Neutrinoless double beta decay, Dilution refrigerator, Ton-scale detector, Low temperature calorimeter, Rare event searches, cryogenics, CUORE performance, Cryogenics, Rare event searche, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 7. Clean energy, 01 natural sciences, CUORE, double-beta decay: (0neutrino), Double beta decay, 0103 physical sciences, Cryogenic particle detectors, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), Aerospace engineering, 010306 general physics, Nuclear Experiment, activity report, Physics, 010308 nuclear & particles physics, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Cryogenic temperature, Instrumentation and Detectors (physics.ins-det), CUORE performance, Semiconductor detector, cryogenics: design, cryogenics, Neutrino, business, performance
Abstract: The past few decades have seen major developments in the design and operation of cryogenic particle detectors. This technology offers an extremely good energy resolution - comparable to semiconductor detectors - and a wide choice of target materials, making low temperature calorimetric detectors ideal for a variety of particle physics applications. Rare event searches have continued to require ever greater exposures, which has driven them to ever larger cryogenic detectors, with the CUORE experiment being the first to reach a tonne-scale, mK-cooled, experimental mass. CUORE, designed to search for neutrinoless double beta decay, has been operational since 2017 at a temperature of about 10 mK. This result has been attained by the use of an unprecedentedly large cryogenic infrastructure called the CUORE cryostat: conceived, designed and commissioned for this purpose. In this article the main characteristics and features of the cryogenic facility developed for the CUORE experiment are highlighted. A brief introduction of the evolution of the field and of the past cryogenic facilities are given. The motivation behind the design and development of the CUORE cryogenic facility is detailed as are the steps taken toward realization, commissioning, and operation of the CUORE cryostat. The major challenges overcome by the collaboration and the solutions implemented throughout the building of the cryogenic facility will be discussed along with the potential improvements for future facilities. The success of CUORE has opened the door to a new generation of large-scale cryogenic facilities in numerous fields of science. Broader implications of the incredible feat achieved by the CUORE collaboration on the future cryogenic facilities in various fields ranging from neutrino and dark matter experiments to quantum computing will be examined., Comment: 45 pages, 14 figures
Published: 2022
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20. Machine Learning Techniques for Pile-Up Rejection in Cryogenic Calorimeters

Author: G. Fantini, A. Armatol, E. Armengaud, W. Armstrong, C. Augier, F. T. Avignone, O. Azzolini, A. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, L. Bergé, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, A. Cazes, E. Celi, C. Chang, M. Chapellier, A. Charrier, D. Chiesa, M. Clemenza, I. Colantoni, F. Collamati, S. Copello, F. Cova, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’Addabbo, G. D’Imperio, I. Dafinei, F. A. Danevich, M. de Combarieu, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, V. Dompè, A. Drobizhev, L. Dumoulin, M. Fasoli, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, J. Gascon, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, P. Gras, M. Gros, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, D. L. Helis, H. Z. Huang, R. G. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. Konovalov, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, R. Mariam, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, B. Mauri, D. Mayer, Y. Mei, S. Milana, D. Misiak, T. Napolitano, M. Nastasi, X. F. Navick, J. Nikkel, R. Nipoti, S. Nisi, C. Nones, E. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, C. Oriol, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, P. Pari, L. Pattavina, B. Paul, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, T. Polakovic, O. G. Polischuk, S. Pozzi, E. Previtali, A. Puiu, A. Ressa, R. Rizzoli, C. Rosenfeld, C. Rusconi, V. Sanglard, J. Scarpaci, B. Schmidt, V. Sharma, V. Shlegel, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, O. Tellier, C. Tomei, V. I. Tretyak, A. Tsymbaliuk, A. Vedda, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. Yumatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, S. Zucchelli, Fantini, G, Armatol, A, Armengaud, E, Armstrong, W, Augier, C, Avignone, FT, Azzolini, O, Barabash, A, Bari, G, Barresi, A, Baudin, D, Bellini, F, Benato, G, Beretta, M, Berge, L, Biassoni, M, Billard, J, Boldrini, V, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cazes, A, Celi, E, Chang, C, Chapellier, M, Charrier, A, Chiesa, D, Clemenza, M, Colantoni, I, Collamati, F, Copello, S, Cova, F, Cremonesi, O, Creswick, RJ, Cruciani, A, D'Addabbo, A, D'Imperio, G, Dafinei, I, Danevich, FA, de Combarieu, M, De Jesus, M, de Marcillac, P, Dell'Oro, S, Di Domizio, S, Dompe, V, Drobizhev, A, Dumoulin, L, Fasoli, M, Faverzani, M, Ferri, E, Ferri, F, Ferroni, F, Formaggio, J, Franceschi, A, Fu, C, Fu, S, Fujikawa, BK, Gascon, J, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gras, P, Gros, M, Gutierrez, TD, Han, K, Hansen, EV, Heeger, KM, Helis, DL, Huang, HZ, Huang, RG, Imbert, L, Johnston, J, Juillard, A, Karapetrov, G, Keppel, G, Khalife, H, Kobychev, VV, Kolomensky, YG, Konovalov, S, Liu, Y, Loaiza, P, Ma, L, Madhukuttan, M, Mancarella, F, Mariam, R, Marini, L, Marnieros, S, Martinez, M, Maruyama, RH, Mauri, B, Mayer, D, Mei, Y, Milana, S, Misiak, D, Napolitano, T, Nastasi, M, Navick, XF, Nikkel, J, Nipoti, R, Nisi, S, Nones, C, Norman, EB, Novosad, V, Nutini, I, O'Donnell, T, Olivieri, E, Oriol, C, Ouellet, JL, Pagan, S, Pagliarone, C, Pagnanini, L, Pari, P, Pattavina, L, Paul, B, Pavan, M, Peng, H, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Poda, DV, Polakovic, T, Polischuk, OG, Pozzi, S, Previtali, E, Puiu, A, Ressa, A, Rizzoli, R, Rosenfeld, C, Rusconi, C, Sanglard, V, Scarpaci, J, Schmidt, B, Sharma, V, Shlegel, V, Singh, V, Sisti, M, Speller, D, Surukuchi, PT, Taffarello, L, Tellier, O, Tomei, C, Tretyak, VI, Tsymbaliuk, A, Vedda, A, Velazquez, M, Vetter, KJ, Wagaarachchi, SL, Wang, G, Wang, L, Welliver, B, Wilson, J, Wilson, K, Winslow, LA, Xue, M, Yan, L, Yang, J, Yefremenko, V, Yumatov, V, Zarytskyy, MM, Zhang, J, Zolotarova, A, Zucchelli, S, Laboratoire de Cryogénie (LC), Service de physique de l'état condensé (SPEC - UMR3680), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Institut Rayonnement Matière de Saclay (IRAMIS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Avignone, F, Bergé, L, Creswick, R, D’Addabbo, A, D’Imperio, G, Danevich, F, Dell’Oro, S, Domizio, S, Dompè, V, Figueroa-Feliciano, E, Fujikawa, B, Gutierrez, T, Hansen, E, Heeger, K, Helis, D, Huang, H, Huang, R, Kobychev, V, Kolomensky, Y, Maruyama, R, Navick, X, Norman, E, O’Donnell, T, Ouellet, J, Poda, D, Polischuk, O, Surukuchi, P, Tretyak, V, Vetter, K, Wagaarachchi, S, Winslow, L, and Zarytskyy, M
Subjects: neural network, Convolutional neural network, hierarchy, crystal, Cryogenic calorimeters, neutrino, Machine learning, CUPID, calorimeter, [INFO]Computer Science [cs], General Materials Science, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutrinoless double beta decay, neutrinoless, Pile-up, CUORE, background, double-beta decay, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, Gran Sasso, injection, cryogenics, efficiency, mass, readout, Convolutional neural networks, upgrade, Cryogenic calorimeter, performance, Majorana
Abstract: CUORE Upgrade with Particle IDentification (CUPID) is a foreseen ton-scale array of Li2MoO4 (LMO) cryogenic calorimeters with double readout of heat and light signals. Its scientific goal is to fully explore the inverted hierarchy of neutrino masses in the search for neutrinoless double beta decay of 100Mo. Pile-up of standard double beta decay of the candidate isotope is a relevant background. We generate pile-up heat events via injection of Joule heater pulses with a programmable waveform generator in a small array of LMO crystals operated underground in the Laboratori Nazionali del Gran Sasso, Italy. This allows to label pile-up pulses and control both time difference and underlying amplitudes of individual heat pulses in the data. We present the performance of supervised learning classifiers on data and the attained pile-up rejection efficiency.
Published: 2022
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21. Cosmogenic activation of sodium iodide

Author: R. Saldanha, W. G. Thompson, Y. Y. Zhong, L. J. Bignell, R. H. M. Tsang, S. J. Hollick, S. R. Elliott, G. J. Lane, R. H. Maruyama, and L. Yang
Subjects: High Energy Physics - Experiment (hep-ex), Physics - Instrumentation and Detectors, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Nuclear Experiment (nucl-ex), Nuclear Experiment, High Energy Physics - Experiment
Abstract: The production of radioactive isotopes by interactions of cosmic-ray particles with sodium iodide (NaI) crystals can produce radioactive backgrounds in detectors used to search for rare events. Through controlled irradiation of NaI crystals with a neutron beam that matches the cosmic-ray neutron spectrum, followed by direct counting and fitting the resulting spectrum across a broad range of energies, we determined the integrated production rate of several long-lived radioisotopes. The measurements were then extrapolated to determine the sea-level cosmogenic neutron activation rate, including the first experimental determination of the tritium production rate: $(80 \pm 21)$ atoms/kg/day. These results will help constrain background estimates and determine the maximum time that NaI-based detectors can remain unshielded above ground before cosmogenic backgrounds impact the sensitivity of next-generation experiments., Comment: 20 pages, 15 figures, 7 tables
Published: 2022
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22. New Trends in e-Business: From B2B to Web Services.

Author: H. Maruyama
Published: 2001
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23. Searching for dark photons with existing haloscope data

Author: M. J. Jewell, A. Leder, Reina H. Maruyama, Sumita Ghosh, and E. P. Ruddy
Subjects: Physics, Particle physics, Photon, 010308 nuclear & particles physics, Physics::Optics, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Phenomenology, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, 010306 general physics
Abstract: The dark (or hidden) photon is a massive U(1) gauge boson theorized as a dark force mediator and as a dark matter candidate. Dark photons can be detected with axion cavity haloscopes by probing for a power excess caused by the dark photon's kinetic mixing with Standard Model photons. Haloscope axion exclusion limits may therefore be converted into competitive dark photon parameter limits via the calculation of a corresponding dark photon to photon coupling factor. This calculation allows for an improvement in sensitivity of around four orders of magnitude relative to other dark photon exclusions and may be attained using existing data. We present how one converts haloscope axion search limits and a summary of relevant experimental parameters from published searches. In addition, we have included the code that can be used to generate our dark photon exclusion limits for the cases described in this paper. Finally, we present limits on the kinetic mixing coefficient between dark photons and the Standard Model photons based on existing haloscope axion searches., Comment: 4 pages of content plus 2 pages of bibliography, 1 figure; updated with code for a statistical analysis on the polarization of the dark photon; accepted for publication in PRD
Published: 2021
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24. Searching for Dark Matter from the Sun with the IceCube Detector

Author: Lisa Johanna Schumacher, Elisa Lohfink, Javier Gonzalez, Roxanne Turcotte, Catherine De Clercq, Michael DuVernois, Barbara Skrzypek, Larissa Paul, Naoko Kurahashi, Frank G. Schröder, Thomas McElroy, Erin O'Sullivan, S. Böser, Gerald Przybylski, Jakob van Santen, Shiqi Yu, Federica Bradascio, Alexander Burgman, Simeon Reusch, K. Meagher, Mehr Nisa, Benedikt Riedel, Stephanie Hickford, Delia Tosi, Sebastian Baur, Sebastian Fiedlschuster, Markus Ackermann, S. W. Barwick, Sreetama Goswami, Ken'ichi Kin, Ryan Burley, A. Steuer, Qinrui Liu, Martina Karl, Raamis Hussain, Aaron Fienberg, John Evans, Amirreza Raissi, U. Katz, Sally Robertson, Judith Schneider, Andres Medina, Donghwa Kang, Merlin Schaufel, Dawn Williams, Martin Pittermann, Chris Weaver, Stephanie Bron, K. Hoshina, Hrvoje Dujmovic, Jurgen Borowka, Benjamin Bastian, Anastasia Maria Barbano, Brian Clark, Sebastian Sanchez Herrera, Glenn Spiczak, Zelong Zhang, Michael Stamatikos, Jan Soedingrekso, P. Schlunder, John Hardin, Spencer Axani, Kael Hanson, Saskia Philippen, D. F. Cowen, A. Goldschmidt, Julia Becker Tjus, Markus Ahlers, Martin Unland Elorrieta, Shefali Shefali, C. Walck, Alfonso Garcia, Ankur Sharma, Jeffrey Lazar, Le Viet Nguyen, J. J. Beatty, Tianlu Yuan, Matthias Vraeghe, Torsten Schmidt, Abdul Rehman, Carsten Rott, Dave Nygren, Mohamed Rameez, Cyril Martin Alispach, Karen Andeen, Felix Henningsen, Tyler Anderson, Surujhdeo Seunarine, Thomas K. Gaisser, Timo Karg, Hermann Kolanoski, Carlos Arguelles, Lutz Kopke, Chiara Bellenghi, Thomas Kintscher, Maximilian Meier, Jessie Micallef, Juan Pablo Yanez, IceCube, Josh Peterson, Emma Kun, Paolo Desiati, Matthias Huber, Juanan Aguilar, Lenka Tomankova, Yosuke Ashida, A. R. Fazely, J. L. Kelley, Kenneth Clark, Aya Ishihara, Matthew Weiss, Yuiry Popovych, Kirill Filimonov, Pranav Dave, Maximilian Karl Scharf, Alejandro Diaz, Krijn de Vries, Stef Verpoest, Andreas Weindl, Jenni Adams, Xianwu Xu, Jay Gallagher, Minjin Jeong, K.-H. Becker, Ruth Hoffmann, Kwok Lung Fan, Alexander Fritz, Colin Turley, Erik Ganster, Najia Moureen Binte Amin, Uwe Naumann, T. Stanev, Yiqian Xu, Emma C. Hettinger, Matt Dunkman, Federico Bontempo, Nora Valtonen-Mattila, Marcos Santander, Francesco Lucarelli, Maria Liubarska, Ramesh Koirala, Dennis Soldin, Martin Ha Minh, Hans Dembinski, Erin Carnie-Bronca, Harald Schieler, K. Rawlins, Christian Glaser, Simona Toscano, Christian Spiering, Manuel Silva, Samvel Ter-Antonyan, Ben Jones, Alan Coleman, Gisela Anton, Maria Prado Rodriguez, Devyn Rysewyk Cantu, Gwenhaël de Wasseige, D. Z. Besson, Reina H. Maruyama, R. Halliday, Daniel Bindig, Georg Schwefer, L. Gerhardt, James Vincent Mead, Thomas Stuttard, Ryo Nagai, A. Olivas, E. Blaufuss, T. Stezelberger, Sarah Pieper, Markus Dittmer, Jannis Necker, Tetiana Kozynets, Neha Lad, Dirk Ryckbosch, Elizabeth Friedman, Chad Finley, Rasha Abbasi, Summer Blot, Matthias Boddenberg, Ibrahim Safa, Daria Pankova, Damian Pieloth, Ali Kheirandish, Sarah Mancina, Gerrit Roellinghoff, Stephan Meighen-Berger, Jannes Brostean-Kaiser, Kurt Woschnagg, Simon Hauser, Anna Franckowiak, Tobias Hoinka, Vedant Basu, James Madsen, Thorsten Glusenkamp, Massimiliano Lincetto, Lu Lu, Paul Evenson, S. Yoshida, I. Taboada, Dustin Hebecker, Nathan Whitehorn, Steve Sclafani, Klas Hultqvist, Joanna Kiryluk, Christoph Tönnis, Sally-Ann Browne, Brandom Pries, Mirco Hunnefeld, Marie Oehler, Segev BenZvi, Timothée Grégoire, Paras Koundal, Mike Richman, Colton Hill, Carlos Perez de los Heros, Gabriel Collin, Simone Garrappa, Dmitry Chirkin, Johan Wulff, Jan Weldert, Etienne Bourbeau, Spencer Klein, Julian Saffer, Chris Wendt, Sebastian Schindler, Michael Kovacevich, Pablo Correa, S. Tilav, Teresa Montaruli, Christoph Günther, Alexander Kappes, Michael Campana, Emily Dvorak, Cristian Jesus Lozano Mariscal, Kendall Mahn, K. Helbing, Elisa Bernardini, Tomas Kontrimas, Christian Dappen, Justin Vandenbroucke, Timothyblake Watson, Yijia Li, Sourav Sarkar, Benjamin Hokanson-Fasig, L. Halve, Philipp Eller, Christian Spannfellner, R. Morse, Frank McNally, Chunfai Tung, Olga Botner, Jakob Bottcher, Kara Hoffman, D. J. Koskinen, Antonio Augusto Alves Junior, Chujie Chen, Raffaela Busse, Anna Obertacke Pollmann, Yang Lyu, Joeran Stettner, Cristina Lagunas Gualda, Grant Parker, Philip Weigel, M. Plum, Mehmet Gunduz, Agnieszka Leszczyńska, R. C. Bay, Hershal Pandya, Martin Rongen, Wolfgang Rhode, Spencer Griswold, Maryon Ahrens, Joshua Hignight, Timo Sturwald, Frederik Tenholt, Wing Yan Ma, Feifei Huang, Hannah Erpenbeck, Konstancja Satalecka, Theo Glauch, Xinhua Bai, Austin Schneider, Abhishek Desai, Juan Carlos Diaz-Velez, Robert Stein, Maria Tselengidou, James DeLaunay, Marjon Moulai, Ava Ghadimi, Martin Wolf, Franziska Tischbein, Hans Niederhausen, Robert A. Cross, Frederik Hermann Lauber, Koun Choi, Andrew Ludwig, Justin Lanfranchi, Ben Smithers, Jean Pierre Twagirayezu, Jiwoong Lee, Rui An, Nahee Park, Darren Grant, Derek B Fox, Immacolata Carmen Rea, Sarah Nowicki, Andreas Haungs, Robert Snihur, C. H. Wiebusch, Kunal Deoskar, A. Karle, Ioana Codrina Maris, Sam De Ridder, Christoph Raab, Nadège Iovine, D. Berley, G. C. Hill, Bunheng Ty, Patrick Reichherzer, Ralph Engel, Moritz Kellermann, Giovanni Renzi, D. Seckel, Tyce DeYoung, George Japaridze, Roger Moore, Woosik Kang, Richard Naab, Marek Kowalski, Seongjin In, Elisa Resconi, Jan Conrad, K. Mase, Yuya Makino, Alessio Porcelli, Alexander A. Harnisch, Nick van Eijndhoven, Lew Classen, René Reimann, Leander Fischer, Thomas Ehrhardt, Christian Haack, Alexander Sandrock, Kirsten Tollefson, Kayla Leonard, Alexander Trettin, Sukeerthi Dharani, Francis Halzen, Lilly Peters, Juliana Stachurska, V Aswathi Balagopal, Gerrit Wrede, Johannes Werthebach, Thomas Huber, Ek Narayan Paudel, Michael J Larson, Allan Hallgren, Sandro Kopper, William Luszczak, M. Kauer, David Kappesser, Matti Jansson, P. Buford Price, Mark Weyrauch, Joakim Sandroos, Daniela Mockler, G. W. Sullivan, James E. Braun, Philipp Furst, Tim Ruhe, Paul Coppin, Andrea Turcati, Ella Roberts, Alex Pizzuto, Gary Binder, Xinyue Kang, Claudio Kopper, Subir Sarkar, and David Vannerom
Subjects: Physics, Dark matter, Detector, Astronomy
Published: 2021
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25. Domestic Birds as Source of Cryptococcus deuterogattii (AFLP6/VGII)

Author: Fernanda H. Maruyama, Nathan Pereira Siqueira, Olivia Cometti Favalessa, Valéria Dutra, Luciano Nakazato, Rosane Christine Hahn, Ferry Hagen, Westerdijk Fungal Biodiversity Institute, and Westerdijk Fungal Biodiversity Institute - Medical Mycology
Subjects: Antifungal Agents, Genotype, Veterinary (miscellaneous), Cryptococcus, Applied Microbiology and Biotechnology, Microbiology, biology.animal, medicine, Humans, Typing, Mycological Typing Techniques, Cryptococcus gattii, Cryptococcus neoformans, biology, Meningoencephalitis, Cryptococcosis, medicine.disease, biology.organism_classification, Passerine, Agronomy and Crop Science, Multilocus Sequence Typing
Abstract: Cryptococcosis is an infection caused by encapsulated basidiomycetous yeasts belonging to the Cryptococcus neoformans/Cryptococcus gattii species complexes. It is acquired through inhalation of infectious propagules, often resulting in meningitis and meningoencephalitis. The ecological niche of these agents is a wide variety of trees species, as well as pigeon, parrot and passerine excreta. The objective of this study was to isolate Cryptococcus yeasts from excreta of commercially traded parrots and passerines. The 237 samples were collected between October 2018 and April 2019 and processed using conventional methodologies. Nineteen colonies with a dark brown phenotype, caused by phenol oxidase activity, were isolated, suggesting the presence of pathogenic Cryptococcus yeasts. All isolates tested positive for urease activity. URA5-RFLP fingerprinting identified 14 isolates (68.4%) as C. neoformans (genotype AFLP1/VNI) and 5 (26.3%) as C. deuterogattii (genotype AFLP6/VGII). Multi-locus sequence typing was applied to investigate the relatedness of the C. deuterogattii isolates with those collected globally, showing that those originating from bird-excreta were genetically indistinguishable from some clinical isolates collected during the past two decades.
Published: 2021

26. Pulmonary granuloma is not always the tuberculosis hallmark: pathological findings of different tuberculosis stages in New and Old World Nonhuman Primates naturally infected with the Mycobacterium tuberculosis Complex

Author: Asheley Henrique Barbosa Pereira, Bruna E. P. Barbosa, Gabriel de Moraes Leal, Silvia Bahadian Moreira, Fernanda H. Maruyama, Daniel Rouede de Andrade Oliveira, Luciano Nakazato, Luiz Claudio Motta de Oliveira, Alcides Pissinatti, Daniel G. Ubiali, Valéria Dutra, Ana Cristina Araújo Pinto, Paulo Redner, Claudia A.A. Lopes, and Thalita A. Pissinatti
Subjects: Old World, Tuberculosis, Mycobacterium tuberculosis complex, biology, business.industry, Immunology, Medicine, PULMONARY GRANULOMA, business, medicine.disease, biology.organism_classification, Pathological
Abstract: Herein we present the pathological findings of different tuberculosis stages in Old and New World monkeys kept under human care in Rio de Janeiro, Brazil and naturally infected with Mycobacterium tuberculosis Complex. Fifteen nonhuman primates from five different colonies were incorporated into the study. There are 60% (9/15) Old World Monkeys and 40% (6/15) New World Monkeys. According to the gross and histopathologic findings, the lesions in nonhuman primates of this study are classified into the chronic-active, extrapulmonary, early-activation or latent-reactivation tuberculosis stage. Among the Old World Monkey, 66.7% (6/9) of nonhuman primates, all rhesus monkeys (Macaca mulatta), showed severe granulomatous pneumonia. In all Old World Monkeys cases, typical granulomas were seen in at least one organ regardless of the stage of the disease. In the New World Monkeys, the typical pulmonary granulomas were seen in 16.7% (1/6) of the cases, just in the latent-reactivation stage in Uta Hick’s Bearded Saki (Chiropotes utahickae). In this study, 66.7% (6/9) of Old World Monkeys (OWM) and 83.3% (5/6) of New World Monkeys (NWM) showed pulmonary changes at the histological evaluation. The tuberculosis diagnosis in the nonhuman primates in this study was based on pathological, immunohistochemical, molecular, and bacteriological culture. Although the typical presentation was observed in some cases, the absence of pulmonary granuloma did not exclude the tuberculosis occurrence in nonhuman primates of the Old and New World. Tuberculosis should be included as a cause of interstitial pneumonia with foamy macrophages infiltration in the New World nonhuman primates. Due to the high sensitivity of immunohistochemistry with Anti-Mycobacterium tuberculosis, we suggest the addition of this technique as a diagnostic tool of tuberculosis in the nonhuman primates even when the typical changes are not seen.
Published: 2021
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27. O.07 TDP43 accumulates in intramuscular nerve bundles of ALS patients

Author: T. Kurashige, H. Morino, T. Murao, Y. Izumi, T. Sugiura, K. Kuraoka, H. Kawakami, T. Torii, and H. Maruyama
Subjects: Neurology, Pediatrics, Perinatology and Child Health, Neurology (clinical), Genetics (clinical)
Published: 2022
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28. Optimization of a single module of CUPID

Author: Alberto Ressa, A. Armatol, E. Armengaud, W. Armstrong, C. Augier, F. T. Avignone, O. Azzolini, A. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, L. Bergé, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, A. Cazes, E. Celi, A. Chang, M. Chapellier, A. Charrier, D. Chiesa, M. Clemenza, I. Colantoni, F. Collamati, S. Copello, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’ Addabbo, G. D’ Imperio, I. Dafinei, F. A. Danevich, M. de Combarieu, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, V. Dompè, A. Drobizhev, L. Dumoulin, G. Fantini, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, J. Gascon, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, P. Gras, M. Gros, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, B. L. Helis, H.Z. Huang, R. G. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. Konovalov, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, R. Mariam, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, B. Mauri, D. Mayer, Y. Mei, S. Milana, D. Misiak, T. Napolitano, M. Nastasi, X. F. Navick, J. Nikkel, R. Nipoti, S. Nisi, C. Nones, C. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, C. Oriol, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, P. Pari, L. Pattavina, B. Paul, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, T. Polakovic, O. G. Polischuk, S. Pozzi, E. Previtali, A. Puiu, A. Ressa, R. Rizzoli, C. Rosenfeld, C. Rusconi, V. Sanglard, J. Scarpaci, B. Schmidt, V. Sharma, V. Shlegel, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, O. Tellier, C. Tomei, V. I. Tretyak, A. Tsymbaliuk, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. Yumatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, S. Zucchelli, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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 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), Science et Ingénierie des Matériaux et Procédés (SIMaP), Institut de Chimie du CNRS (INC)-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), and CUPID
Subjects: photon yield, History, tector design, helium background, energy resolution, lithium, molybdenum nuclide, molybdenum oxygen, scintillation counter, crystal bolometer, CUORE performance, photon yield, Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, energy resolution, helium background, molybdenum oxygen, CUORE performance, Computer Science Applications, Education, Gran Sasso, double-beta decay: (0neutrino), lithium, crystal bolometer, molybdenum nuclide, calorimeter: cryogenics, High Energy Physics::Experiment, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], activity report, scintillation counter, detector: design, performance, tector design
Abstract: CUPID is the next generation experiment which will use scintillating cryogenic calorimeters to search for the neutrinoless double β decay. This unobserved process would shed light on the nature of the neutrino, which up to our knowledge could be a Majorana or a Dirac particle, and would give us an important hint to explain the lack of antimatter in the universe. This ambitious search needs a detector with unique characteristics such as an extremely low background level and an excellent energy resolution. CUPID is now in advanced R&D state to optimize the detector design in order to completely exploit the potentialities of scintillating cryogenic calorimeters. In the following I will describe the test performed at the LNGS (Laboratori Nazionali del Gran Sasso) of a single module of the future CUPID detector. In this contribution we present the performance obtained with a novel assembly concept, proving that it matches the requirements for CUPID.
Published: 2021
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29. Expected sensitivity to $^{128}$Te neutrinoless double beta decay with the CUORE TeO$_2$ cryogenic bolometers

Author: V. Dompè, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Beretta, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, E. Celi, D. Chiesa, M. Clemenza, S. Copello, O. Cremonesi, R. J. Creswick, A. D’Addabbo, I. Dafinei, S. Dell’Oro, S. Di Domizio, S. Di Lorenzo, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, S. H. Fu, B. K. Fujikawa, S. Ghislandi, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu G. Kolomensky, R. Kowalski, C. Ligi, R. Liu, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, D. Mayer, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, A. Nucciotti, I. Nutini, T. O’Donnell, M. Olmi, J. L. Ouellet, S. Pagan, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, S. Quitadamo, A. Ressa, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Sharma, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, F. Terranova, C. Tomei, K. J. Vetter, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, S. Zimmermann, S. Zucchelli, 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Dompe, V, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Beretta, M, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Celi, E, Chiesa, D, Clemenza, M, Copello, S, Cremonesi, O, Creswick, R, D'Addabbo, A, Dafinei, I, Dell'Oro, S, Di Domizio, S, Di Lorenzo, S, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fu, S, Fujikawa, B, Ghislandi, S, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Hansen, E, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Kowalski, R, Ligi, C, Liu, R, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mayer, D, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Nucciotti, A, Nutini, I, O'Donnell, T, Olmi, M, Ouellet, J, Pagan, S, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Quitadamo, S, Ressa, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Speller, D, Surukuchi, P, Taffarello, L, Terranova, F, Tomei, C, Vetter, K, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zimmermann, S, Zucchelli, S, Adams, DQ, Avignone, FT, Cao, XG, Creswick, RJ, Fang, DQ, Franceschi, MA, Freedman, SJ, Fu, SH, Fujikawa, BK, Gutierrez, TD, Hansen, EV, Heeger, KM, Huang, RG, Huang, HZ, Kolomensky, YG, Ma, YG, Maruyama, RH, Norman, EB, Ouellet, JL, Pagliarone, CE, Scielzo, ND, Surukuchi, PT, Vetter, KJ, Wagaarachchi, SL, Wang, BS, and Winslow, LA
Subjects: CUORE, Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Condensed Matter Physics, Cryogenic bolometer, Atomic and Molecular Physics, and Optics, CUORE, Cryogenic Bolometers, Cryogenic bolometers, General Materials Science, High Energy Physics::Experiment, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutrinoless double beta decay, Tellurium, Nuclear Experiment, 128-Te
Abstract: The CUORE experiment is a ton-scale array of $$\hbox {TeO}_2$$ TeO 2 cryogenic bolometers located at the underground Laboratori Nazionali del Gran Sasso of Istituto Nazionale di Fisica Nucleare (INFN), in Italy. The CUORE detector consists of 988 crystals operated as source and detector at a base temperature of $$\sim 10$$ ∼ 10 mK. Such cryogenic temperature is reached and maintained by means of a custom built cryogen-free dilution cryostat, designed with the aim of minimizing the vibrational noise and the environmental radioactivity. The primary goal of CUORE is the search for neutrinoless double beta decay of $$^{130}\hbox {Te}$$ 130 Te , but thanks to its large target mass and ultra-low background it is suitable for the study of other rare processes as well, such as the neutrinoless double beta decay of $$^{128}\hbox {Te}$$ 128 Te . This tellurium isotope is an attractive candidate for the search of this process, due to its high natural isotopic abundance of 31.75%. The transition energy at (866.7 ± 0.7) keV lies in a highly populated region of the energy spectrum, dominated by the contribution of the two-neutrino double beta decay of $$^{130}\hbox {Te}$$ 130 Te . As the first ton-scale infrastructure operating cryogenic $$\hbox {TeO}_2$$ TeO 2 bolometers in stable conditions, CUORE is able to achieve a factor $$>10$$ > 10 higher sensitivity to the neutrinoless double beta decay of this isotope with respect to past direct experiments.
Published: 2021
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30. A Convolutional Neural Network based Cascade Reconstruction for the IceCube Neutrino Observatory

Author: J. Werthebach, A. Franckowiak, Chujie Chen, Ioana Codrina Maris, K. Hoshina, A. Steuer, A. Weindl, Maryon Ahrens, P. Schlunder, Saskia Philippen, Glenn Spiczak, G. Momenté, Segev BenZvi, Spencer Klein, M. Rameez, Sam De Ridder, Frederik Tenholt, R. Nagai, D. F. Cowen, Martin Unland Elorrieta, Stephen L. Hauser, Christoph Raab, Nadège Iovine, Barbara Skrzypek, Kara Hoffman, Sarah Mancina, N. van Eijndhoven, U. Naumann, Raamis Hussain, D. Berley, G. C. Hill, Tobias Hoinka, Vedant Basu, Steve Sclafani, J. Kiryluk, B. J. P. Jones, Andres Medina, D. Mockler, Bunheng Ty, Ralph Engel, Moritz Kellermann, U. Katz, Emily Dvorak, Timo Karg, K. Andeen, D. R. Nygren, Marek Kowalski, D. Kang, Giovanni Renzi, K. D. de Vries, M. Stamatikos, Hershal Pandya, Wolfgang Rhode, Robert Stein, A.A. Alves, Pablo Correa, D. Seckel, S. Fahey, Javier Gonzalez, Roxanne Turcotte, Maximilian Karl Scharf, Alexander Trettin, P. B. Price, I. Taboada, Gisela Anton, Michael O. Wolf, Lenka Tomankova, Max Renschler, Y. Makino, Matthias Vraeghe, Tyce DeYoung, K. Tollefson, D. J. Koskinen, K. Rawlins, Nathan Whitehorn, C. Weaver, T. Anderson, B. A. Clark, Francesco Lucarelli, Brandom Pries, L. Schumacher, Devyn Rysewyk Cantu, P. Peiffer, J. Kim, Daria Pankova, E. Friedman, M. Kauer, Alan Coleman, John Hardin, Shefali Shefali, Nora Valtonen-Mattila, M. E. Huber, D. B. Fox, Alexander Fritz, D. Z. Besson, T. O. B. Schmidt, E. Bourbeau, Suyong Choi, M. Silva, Najia Moureen Binte Amin, J. P. Lazar, Sebastian Böser, R. Morse, Spencer Griswold, Jakob Bottcher, T. Montaruli, David A. Williams, A. Goldschmidt, K. Mase, Abdul Rehman, David Kappesser, Kurt Woschnagg, Paul Evenson, Clara E. Hill, Le Viet Nguyen, Sebastian Sanchez Herrera, Marcos Santander, Carsten Rott, L. Gerhardt, Y. Popovych, J. Evans, Maria Tselengidou, D. Soldin, J. B. Tjus, Chiara Bellenghi, Alexander A. Harnisch, Benjamin Bastian, Anastasia Maria Barbano, Markus Ackermann, S. W. Barwick, Matti Jansson, Immacolata Carmen Rea, P. Eller, Simone Garrappa, H. Schieler, Dmitry Chirkin, Kael Hanson, A. Kyriacou, A. Olivas, Hermann Kolanoski, Simeon Reusch, A. O. Pollmann, Elisa Bernardini, K. Meagher, S. Hickford, J. C. Gallagher, Kirill Filimonov, Mehmet Gunduz, Agnieszka Leszczyńska, R. C. Bay, Alexander Kappes, Pranav Dave, Jan Soedingrekso, K. Krings, Xianwu Xu, J. Sandroos, James Madsen, Lu Lu, M. J. Weiss, Stef Verpoest, H. Dujmovic, Austin Schneider, Juan Carlos Diaz-Velez, Jenni Adams, K.-H. Becker, Yiqian Xu, M. Plum, A. Wallace, Katharina Morik, J. Stettner, Daniel Bindig, Ramesh Koirala, Gerrit Wrede, C.P. de los Heros, Thomas Huber, Ek Narayan Paudel, Allan Hallgren, Matt Dunkman, R. Joppe, T. Stezelberger, Colin Turley, S. Kopper, Christian Glaser, Paolo Desiati, S. Sarker, C. Alispach, Damian Pieloth, R. G. Stokstad, Ali Kheirandish, Sreetama Goswami, Minjin Jeong, Martin Ha Minh, T. Glüsenkamp, Janet Conrad, G. Krückl, Jannis Necker, Sebastian Baur, R. Cross, Sebastian Fiedlschuster, Surujhdeo Seunarine, Ken'ichi Kin, Jannes Brostean-Kaiser, Chunfai Tung, Alejandro Diaz, M. J. Larson, M. U. Nisa, Tim Ruhe, E. O'Sullivan, René Reimann, Chad Finley, Federica Bradascio, A. V. Balagopal, Alexander Burgman, M. Meier, Michael Campana, F. Huang, Christoph Tönnis, Benjamin Hokanson-Fasig, E. Blaufuss, Leander Fischer, Gerrit Roellinghoff, Mirco Hunnefeld, Marie Oehler, Thomas Stuttard, William Luszczak, G. H. Collin, Sarah Pieper, Dirk Ryckbosch, S. Robertson, R. Snihur, A. Ludwig, Wing Yan Ma, Yang Lyu, Grant Parker, L. Köpke, Karl J. Clark, Juanan Aguilar, I. Safa, Merlin Schaufel, James DeLaunay, Marjon Moulai, Olga Botner, Cristian Jesus Lozano Mariscal, Kendall Mahn, L. Classen, Johan Wulff, K. Wiebe, Timothyblake Watson, J. J. Beatty, Tianlu Yuan, Stephan Meighen-Berger, S. Yoshida, Kayla Leonard, A. Ishihara, V. Baum, H. Niederhausen, Won Nam Kang, Joshua Hignight, A. Sharma, Sukeerthi Dharani, Francis Halzen, J. Merz, Paras Koundal, Mike Richman, X. Bai, Konstancja Satalecka, F. McNally, Emma C. Hettinger, I. Ansseau, Michael Kovacevich, Theo Glauch, Juliana Stachurska, H. Dembinski, Reina H. Maruyama, Frank G. Schröder, Summer Blot, Thomas Ehrhardt, D. Tosi, D. van Eijk, Mark Weyrauch, Spencer Axani, Elisa Lohfink, Aaron Fienberg, Amirreza Raissi, S. Tilav, Michael DuVernois, Carlos Arguelles, Jessie Micallef, Stephanie Bron, R. S. Busse, Y. L. Li, J. P. Yanez, Gerald Przybylski, Christian Haack, Christopher Wiebusch, R. Halliday, Kunal Deoskar, K. Helbing, Alexander Sandrock, N. Kurahashi, Todor Stanev, Benedikt Riedel, Cristina Lagunas Gualda, C. Wendt, G. W. Sullivan, A. Karle, James E. Braun, Philipp Furst, D. Hebecker, G. de Wasseige, George Japaridze, Roger Moore, Paul Coppin, Andrea Turcati, T. Gregoire, J. van Santen, R. Hoffmann, Alex Pizzuto, Gary Binder, J. Bourbeau, Richard Naab, Zhedong Zhang, C. Walck, Thomas K. Gaisser, Ava Ghadimi, Franziska Tischbein, Seongjin In, Elisa Resconi, Alessio Porcelli, P. Mallik, Catherine De Clercq, M. Rongen, Qinrui Liu, Martina Karl, Jochen M. Schneider, Christian Spiering, Justin Vandenbroucke, Maria Prado Rodriguez, Abhishek Desai, Xinyue Kang, Claudio Kopper, S. C. Nowicki, Subir Sarkar, T. Kintscher, Frederik Hermann Lauber, Justin Lanfranchi, David Vannerom, Ben Smithers, Jean Pierre Twagirayezu, A. Haungs, Rui An, Nahee Park, K. Hultqvist, Darren Grant, T. Stürwald, Z. Griffith, Felix Henningsen, A. R. Fazely, Simona Toscano, J. L. Kelley, Markus Ahlers, Erik Ganster, Samvel Ter-Antonyan, Rasha Abbasi, B. J. Whelan, Jan Weldert, L. Halve, Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, Elementary Particle Physics, and collaboration, The IceCube
Subjects: FOS: Computer and information sciences, Computer Science - Machine Learning, Astrophysics::High Energy Astrophysical Phenomena, cs.LG, Data analysis, FOS: Physical sciences, Fitting methods, 01 natural sciences, Convolutional neural network, Calibration, Cluster finding, Neutrino detectors, Pattern recognition, High Energy Physics - Experiment, IceCube Neutrino Observatory, Machine Learning (cs.LG), High Energy Physics - Experiment (hep-ex), 0103 physical sciences, 010303 astronomy & astrophysics, Instrumentation, Mathematical Physics, 010308 nuclear & particles physics, business.industry, hep-ex, Deep learning, Detector, Neutrino detector, Computer engineering, Orders of magnitude (time), 13. Climate action, Cascade, Pattern recognition (psychology), Artificial intelligence, business
Abstract: Continued improvements on existing reconstruction methods are vital to the success of high-energy physics experiments, such as the IceCube Neutrino Observatory. In IceCube, further challenges arise as the detector is situated at the geographic South Pole where computational resources are limited. However, to perform real-time analyses and to issue alerts to telescopes around the world, powerful and fast reconstruction methods are desired. Deep neural networks can be extremely powerful, and their usage is computationally inexpensive once the networks are trained. These characteristics make a deep learning-based approach an excellent candidate for the application in IceCube. A reconstruction method based on convolutional architectures and hexagonally shaped kernels is presented. The presented method is robust towards systematic uncertainties in the simulation and has been tested on experimental data. In comparison to standard reconstruction methods in IceCube, it can improve upon the reconstruction accuracy, while reducing the time necessary to run the reconstruction by two to three orders of magnitude., Comment: 39 pages, 15 figures, submitted to Journal of Instrumentation; added references
Published: 2021

31. Measurement of the 2νββ Decay Half-Life of Te130 with CUORE

Author: V. Sharma, D. Speller, Deqing Fang, S. Morganti, J. Nikkel, S. H. Fu, P. T. Surukuchi, S. Zimmermann, Carlo Ligi, R. J. Creswick, A. Campani, L. Gironi, I. Nutini, C. Rosenfeld, J. Camilleri, Oliviero Cremonesi, Kai Vetter, P. Gorla, F. Ferroni, C. Tomei, Massimiliano Clemenza, Carlo Cosmelli, Monica Sisti, F. T. Avignone, B. S. Wang, A. Giuliani, Emanuele Ferri, C. Pagliarone, N. D. Scielzo, C. Brofferio, L. Pattavina, C. J. Davis, Silvia Capelli, S. Pozzi, F. Terranova, C. Nones, A. Puiu, Massimiliano Nastasi, S. Di Domizio, K. Wilson, Davide Chiesa, Lucia Canonica, A. Caminata, Ezio Previtali, Marco Pallavicini, C. Rusconi, B. Welliver, V. Dompè, F. Bellini, Jonathan Ouellet, G. Bari, H. Z. Huang, S. Pagan, Y. Mei, A. D'Addabbo, C. Bucci, L. Marini, T. D. Gutierrez, T. O'Donnell, J. Johnston, S. Copello, N. Moggi, Laura Cardani, Yu. G. Kolomensky, Luigi Cappelli, B. K. Fujikawa, Xiangyu Cao, G. Keppel, Samuele Sangiorgio, K. M. Heeger, A. Nucciotti, C. Alduino, S. Pirro, B. Schmidt, Stefano Zucchelli, S. Dell'Oro, Ke Han, Paolo Carniti, Reina H. Maruyama, Claudio Gotti, Stuart J. Freedman, M. Sakai, O. Azzolini, T. Napolitano, M. Pavan, N. Casali, James R. Wilson, G. Pessina, S. L. Wagaarachchi, V. Pettinacci, M. Vignati, M. Biassoni, I. Dafinei, E. Fiorini, Giovanni Benato, Yudi Ma, L. Pagnanini, Eric B. Norman, L. Taffarello, D. Q. Adams, K. Alfonso, D. Mayer, M. Faverzani, Lindley Winslow, Virendra Singh, L. Ma, C. Pira, G. Fantini, R. G. Huang, A. Branca, M. A. Franceschi, and A. Giachero
Subjects: Physics, Nuclear physics, CUORE, Double beta decay, 0103 physical sciences, General Physics and Astronomy, Half-life, High Energy Physics::Experiment, 010306 general physics, 01 natural sciences, Spectral line
Abstract: We measured two-neutrino double beta decay of $^{130}$Te using an exposure of 300.7 kg$\cdot$yr accumulated with the CUORE detector. Using a Bayesian analysis to fit simulated spectra to experimental data, it was possible to disentangle all the major background sources and precisely measure the two-neutrino contribution. The half-life is in agreement with past measurements with a strongly reduced uncertainty: $T^{2\nu}_{1/2} = 7.71^{+0.08}_{-0.06}\mathrm{(stat.)}^{+0.12}_{-0.15}\mathrm{(syst.)}\times10^{20}$ yr. This measurement is the most precise determination of the $^{130}$Te 2$\nu\beta\beta$ decay half-life to date.
Published: 2021
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32. Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target

Author: Bruno B. Manzato, M. Kauer, N. J. C. Spooner, Govinda Adhikari, Woon Gu Kang, Estella Barbosa de Souza, Moo Hyun Lee, Y. J. Ko, Joo Young Lee, Gyun Ho Yu, Hye Young Lee, Hyunseok Lee, Sun Kee Kim, A. Scarff, Ricardo L. C. Pitta, H. Prihtiadi, Hyun Su Lee, C. Ha, Liang Yang, D. S. Leonard, W. G. Thompson, N. Carlin, A. C. Ezeribe, Seo Hyun Lee, Robert J. Neal, Mitra Djamal, K. A. Shin, Hyang Kyu Park, Seonho Choi, Eunju Jeon, Stephen L. Olsen, J. H. Jo, Sung Hyun Kim, Carsten Rott, Won Kyung Kim, Luis E. França, Yong-Hamb Kim, K. W. Kim, Jongmin Lee, Jae Jin Choi, Yeongduk Kim, Han Wool Joo, Hongjoo Kim, In Sik Hahn, Kangsoon Park, Eun Kyung Lee, S. J. Ra, Seung Mok Lee, Hyeonseo Park, Byung Ju Park, H. Kim, Reina H. Maruyama, and In Soo Lee
Subjects: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Multidisciplinary, 010308 nuclear & particles physics, Dark matter, Analytical chemistry, SciAdv r-articles, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), chemistry.chemical_compound, chemistry, Sodium iodide, 0103 physical sciences, Physical and Materials Sciences, 010306 general physics, Research Article, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Description, Dark matter interpretations of the DAMA signals are excluded by COSINE-100 with the same NaI(Tl) target for various models., We present new constraints on dark matter interactions using 1.7 years of COSINE-100 data. The COSINE-100 experiment, consisting of 106 kg of tallium-doped sodium iodide [NaI(Tl)] target material, is aimed to test DAMA’s claim of dark matter observation using the same NaI(Tl) detectors. Improved event selection requirements, a more precise understanding of the detector background, and the use of a larger dataset considerably enhance the COSINE-100 sensitivity for dark matter detection. No signal consistent with the dark matter interaction is identified and rules out model-dependent dark matter interpretations of the DAMA signals in the specific context of standard halo model with the same NaI(Tl) target for various interaction hypotheses.
Published: 2021
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33. Search for Double-Beta Decay of $\mathrm{^{130}Te}$ to the $0^+$ States of $\mathrm{^{130}Xe}$ with CUORE

Author: Davide Chiesa, S. Di Domizio, Laura Cardani, B. K. Fujikawa, Stefano Pozzi, M. Vignati, Massimiliano Clemenza, Carlo Cosmelli, A. Giuliani, Monica Sisti, C. Pagliarone, V. Sharma, S. Zimmermann, A. Branca, Deqing Fang, S. Dell'Oro, B. Schmidt, L. Pattavina, L. Pagnanini, B. S. Wang, C. Brofferio, Marco Pallavicini, Lindley Winslow, F. Terranova, S. Morganti, O. Azzolini, S. Copello, S. Pagan, Kai Vetter, G. Pessina, Paolo Carniti, C. Rusconi, Carlo Ligi, L. Taffarello, L. Ma, Virendra Singh, Yudi Ma, H. Z. Huang, C. Rosenfeld, S. Pirro, A. Campani, C. Pira, Ettore Fiorini, S. L. Wagaarachchi, Andrea Giachero, P. Gorla, F. Ferroni, J. Camilleri, Xiangyu Cao, C. Tomei, Ke Han, Reina H. Maruyama, Stuart J. Freedman, L. Canonica, L. Marini, D. Q. Adams, Simone Capelli, K. Alfonso, G. Keppel, D. Speller, D. Mayer, C. J. Davis, Y. Mei, C. Nones, A. Puiu, I. Dafinei, Irene Nutini, J. Johnston, V. Pettinacci, A. Caminata, V. Dompè, A. D'Addabbo, J. Nikkel, G. Fantini, K. M. Heeger, Ezio Previtali, P. T. Surukuchi, T. O'Donnell, Yu. G. Kolomensky, N. D. Scielzo, R. G. Huang, B. Welliver, K. Wilson, Jonathan Ouellet, G. Bari, E. Celi, M. A. Franceschi, S. Zucchelli, M. Faverzani, Evelyn Ferri, N. Moggi, Eric B. Norman, L. Cappelli, M. Sakai, T. Napolitano, Samuele Sangiorgio, Oliviero Cremonesi, A. Nucciotti, M. Biassoni, C. Alduino, Claudio Gotti, N. Casali, Giovanni Benato, C. Bucci, T. D. Gutierrez, L. Gironi, F. T. Avignone, F. Bellini, R. J. Creswick, M. Pavan, Massimiliano Nastasi, James R. Wilson, S. H. Fu, 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), Département de Physique des Particules (ex SPP) (DPP), 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, CUORE, and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: Particle physics, experimental methods, Physics and Astronomy (miscellaneous), FOS: Physical sciences, Dirac Neutrino, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Neutrinoless Double Beta Decay, 7. Clean energy, 01 natural sciences, Bayesian, decay modes, crystal, CUORE, background: low, bolometer, Double beta decay, Neutrino, 0103 physical sciences, excited state, double-beta decay: (2neutrino), Beta (velocity), Sensitivity (control systems), bayesian analysis, Nuclear Experiment (nucl-ex), Particle Physics, 010306 general physics, Engineering (miscellaneous), Nuclear Experiment, lepton number: violation, excited states, Physics, 010308 nuclear & particles physics, Majorana Neutrino, Gamma ray, sensitivity, Lepton number, gamma ray: emission, Excited state, Double beta decay, excited states, bayesian analysis, CUORE, Neutrinoless Double Beta Decay, Particle Physics, Neutrino, Majorana Neutrino, Dirac Neutrino
Abstract: The CUORE experiment is a large bolometric array searching for the lepton number violating neutrino-less double beta decay ($0\nu\beta\beta$) in the isotope $\mathrm{^{130}Te}$. In this work we present the latest results on two searches for the double beta decay (DBD) of $\mathrm{^{130}Te}$ to the first $0^{+}_2$ excited state of $\mathrm{^{130}Xe}$: the $0\nu\beta\beta$ decay and the Standard Model-allowed two-neutrinos double beta decay ($2\nu\beta\beta$). Both searches are based on a 372.5 kg$\times$yr TeO$_2$ exposure. The de-excitation gamma rays emitted by the excited Xe nucleus in the final state yield a unique signature, which can be searched for with low background by studying coincident events in two or more bolometers. The closely packed arrangement of the CUORE crystals constitutes a significant advantage in this regard. The median limit setting sensitivities at 90\% Credible Interval (C.I.) of the given searches were estimated as $\mathrm{S^{0\nu}_{1/2} = 5.6 \times 10^{24} \: \mathrm{yr}}$ for the ${0\nu\beta\beta}$ decay and $\mathrm{S^{2\nu}_{1/2} = 2.1 \times 10^{24} \: \mathrm{yr}}$ for the ${2\nu\beta\beta}$ decay. No significant evidence for either of the decay modes was observed and a Bayesian lower bound at $90\%$ C.I. on the decay half lives is obtained as: $\mathrm{(T_{1/2})^{0\nu}_{0^+_2} > 5.9 \times 10^{24} \: \mathrm{yr}}$ for the $0\nu\beta\beta$ mode and $\mathrm{(T_{1/2})^{2\nu}_{0^+_2} > 1.3 \times 10^{24} \: \mathrm{yr}}$ for the $2\nu\beta\beta$ mode. These represent the most stringent limits on the DBD of $^{130}$Te to excited states and improve by a factor $\sim5$ the previous results on this process., Comment: 13 pages, 6 figures
Published: 2021
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34. Characterization of cubic Li 2100 MoO 4 crystals for the CUPID experiment

Author: Federico Ferri, Stefano Dell'Oro, J. Camilleri, V. Shlegel, N. Casali, R. Rizzoli, F. Bellini, A. Ressa, J. A. Scarpaci, C. Augier, Goran Karapetrov, G. Fantini, P. Gras, M. I. Martínez, F.A. Danevich, L. Pagnanini, P. T. Surukuchi, A. Drobizhev, S. H. Fu, C. Oriol, I. Dafinei, T. O'Donnell, E. Figueroa-Feliciano, P. Loaiza, Jie Yang, S. Copello, Haiping Peng, Oliviero Cremonesi, L. Wang, A. Franceschi, C. Pagliarone, Davide Chiesa, Paolo Carniti, A. Juillard, Andrea Barresi, V.I. Tretyak, E. V. Hansen, M. Xue, S. Zucchelli, C. Pira, O. G. Polischuk, X. F. Navick, R. J. Creswick, L. Marini, K. Wilson, I. Colantoni, D. Misiak, C. Rusconi, J. Billard, D. V. Poda, J. Johnston, Jonathan Ouellet, A. Charrier, A. Cruciani, S. L. Wagaarachchi, G. Bari, F. Collamati, V. Yumatov, J. Gascon, C. C. Chang, Stefano Nisi, Changbo Fu, G. Pessina, S. Pirro, L. Pattavina, S. Marnieros, Jie Zhang, G. Wang, G. D'Imperio, A. Cazes, Yuting Liu, E. Celi, Massimiliano Clemenza, A. Tsymbaliuk, Monica Sisti, Valentyn Novosad, I. Nutini, S. Milana, R. Nipoti, C. Nones, A. Puiu, M. Chapellier, H. Z. Huang, V. G. Yefremenko, R. Mariam, B. Schmidt, G. Keppel, Yu. G. Kolomensky, Luigi Cappelli, D. Mayer, O. Tellier, L. Ma, Y. Mei, R. G. Huang, F. Mancarella, M. Faverzani, L. Dumoulin, M. Madhukuttan, H. Khalife, M. Gros, Kai Vetter, S. Di Domizio, D. Baudin, P. Pari, A. Armatol, Giovanni Benato, M. Beretta, Tomas Polakovic, L. Taffarello, Virendra Singh, Danielle Speller, Laura Cardani, K. M. Heeger, B. K. Fujikawa, E. Olivieri, Eric B. Norman, L. Yan, T. Napolitano, S. Pagan, M. Biassoni, B. Mauri, V. Pettinacci, M. de Combarieu, O. Azzolini, M. M. Zarytskyy, A. Giachero, Claudio Gotti, S. I. Konovalov, L. Gironi, Lindley Winslow, M. Pavan, James Nikkel, F. T. Avignone, Whitney Armstrong, V. Sanglard, L. Imbert, C. Bucci, T. D. Gutierrez, C. Brofferio, A. S. Barabash, Ezio Previtali, B. Welliver, P. de Marcillac, D. L. Helis, A. S. Zolotarova, Ke Han, Reina H. Maruyama, B. Paul, A. Giuliani, Silvia Capelli, Massimiliano Nastasi, James R. Wilson, M. De Jesus, E. Armengaud, V. Sharma, Matias Velázquez, V. V. Kobychev, L. Bergé, A. Branca, C. Rosenfeld, V. Boldrini, P. Gorla, F. Ferroni, C. Tomei, Emanuele Ferri, Joseph A. Formaggio, S. Pozzi, V. Dompè, A. D'Addabbo, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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 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), Institut Rayonnement Matière de Saclay (IRAMIS), Service de physique de l'état condensé (SPEC - UMR3680), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Science et Ingénierie des Matériaux et Procédés (SIMaP), Institut de Chimie du CNRS (INC)-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), CUPID, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Armatol A., Armengaud E., Armstrong W., Augier C., Avignone F.T., Azzolini O., Barabash A., Bari G., Barresi A., Baudin D., Bellini F., Benato G., Beretta M., Berge L., Biassoni M., Billard J., Boldrini V., Branca A., Brofferio C., Bucci C., Camilleri J., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Cazes A., Celi E., Chang C., Chapellier M., Charrier A., Chiesa D., Clemenza M., Colantoni I., Collamati F., Copello S., Cremonesi O., J.Creswick R., Cruciani A., D'Addabbo A., D'Imperio G., Dafinei I., A.Danevich F., deCombarieu M., DeJesus M., deMarcillac P., Dell'Oro S., DiDomizio S., Dompe V., Drobizhev A., Dumoulin L., Fantini G., Faverzani M., Ferri E., Ferri F., Ferroni F., Figueroa-Feliciano E., Formaggio J., Franceschi A., Fu C., Fu S., Fujikawa B.K., Gascon J., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gras P., Gros M., Gutierrez T.D., Han K., Hansen E.V., Heeger K.M., Helis D.L., Huang H.Z., Huang R.G., Imbert L., Johnston J., Juillard A., Karapetrov G., Keppel G., Khalife H., Kobychev V.V., Kolomensky Y.G., Konovalov S., Liu Y., Loaiza P., Ma L., Madhukuttan M., Mancarella F., Mariam R., Marini L., Marnieros S., Martinez M., Maruyama R.H., Mauri B., Mayer D., Mei Y., Milana S., Misiak D., Napolitano T., Nastasi M., Navick X.F., Nikkel J., Nipoti R., Nisi S., Nones C., Norman E.B., Novosad V., Nutini I., O'Donnell T., Olivieri E., Oriol C., Ouellet J.L., Pagan S., Pagliarone C., Pagnanini L., Pari P., Pattavina L., Paul B., Pavan M., Peng H., Pessina G., Pettinacci V., Pira C., Pirro S., V.Poda D., Polakovic T., Polischuk O.G., Pozzi S., Previtali E., Puiu A., Ressa A., Rizzoli R., Rosenfeld C., Rusconi C., Sanglard V., Scarpaci J.A., Schmidt B., Sharma V., Shlegel V., Singh V., Sisti M., Speller D., Surukuchi P.T., Taffarello L., Tellier O., Tomei C., Tretyak V.I., Tsymbaliuk A., Velazquez M., Vetter K.J., Wagaarachchi S.L., Wang G., Wang L., Welliver B., Wilson J., Wilson K., Winslow L.A., Xue M., Yan L., Yang J., Yefremenko V., Yumatov V., Zarytskyy M.M., Zhang J., Zolotarova A., Zucchelli S., Armatol, A, Armengaud, E, Armstrong, W, Augier, C, Avignone, F, Azzolini, O, Barabash, A, Bari, G, Barresi, A, Baudin, D, Bellini, F, Benato, G, Beretta, M, Berge, L, Biassoni, M, Billard, J, Boldrini, V, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cazes, A, Celi, E, Chang, C, Chapellier, M, Charrier, A, Chiesa, D, Clemenza, M, Colantoni, I, Collamati, F, Copello, S, Cremonesi, O, J. Creswick, R, Cruciani, A, D'Addabbo, A, D'Imperio, G, Dafinei, I, A. Danevich, F, Decombarieu, M, Dejesus, M, Demarcillac, P, Dell'Oro, S, Didomizio, S, Dompe, V, Drobizhev, A, Dumoulin, L, Fantini, G, Faverzani, M, Ferri, E, Ferri, F, Ferroni, F, Figueroa-Feliciano, E, Formaggio, J, Franceschi, A, Fu, C, Fu, S, Fujikawa, B, Gascon, J, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gras, P, Gros, M, Gutierrez, T, Han, K, Hansen, E, Heeger, K, Helis, D, Huang, H, Huang, R, Imbert, L, Johnston, J, Juillard, A, Karapetrov, G, Keppel, G, Khalife, H, Kobychev, V, Kolomensky, Y, Konovalov, S, Liu, Y, Loaiza, P, Ma, L, Madhukuttan, M, Mancarella, F, Mariam, R, Marini, L, Marnieros, S, Martinez, M, Maruyama, R, Mauri, B, Mayer, D, Mei, Y, Milana, S, Misiak, D, Napolitano, T, Nastasi, M, Navick, X, Nikkel, J, Nipoti, R, Nisi, S, Nones, C, Norman, E, Novosad, V, Nutini, I, O'Donnell, T, Olivieri, E, Oriol, C, Ouellet, J, Pagan, S, Pagliarone, C, Pagnanini, L, Pari, P, Pattavina, L, Paul, B, Pavan, M, Peng, H, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, V. Poda, D, Polakovic, T, Polischuk, O, Pozzi, S, Previtali, E, Puiu, A, Ressa, A, Rizzoli, R, Rosenfeld, C, Rusconi, C, Sanglard, V, Scarpaci, J, Schmidt, B, Sharma, V, Shlegel, V, Singh, V, Sisti, M, Speller, D, Surukuchi, P, Taffarello, L, Tellier, O, Tomei, C, Tretyak, V, Tsymbaliuk, A, Velazquez, M, Vetter, K, Wagaarachchi, S, Wang, G, Wang, L, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Xue, M, Yan, L, Yang, J, Yefremenko, V, Yumatov, V, Zarytskyy, M, Zhang, J, Zolotarova, A, and Zucchelli, S
Subjects: Mo-100, Physics - Instrumentation and Detectors, Physics and Astronomy (miscellaneous), background: induced, Physics::Instrumentation and Detectors, Monte Carlo method, measurement methods, bolometers, neutrinoless double beta decay, energy resolution, Parameter space, 01 natural sciences, Nuclear Experiment (nucl-ex), Double Beta Decay, Nuclear Experiment, background: suppression, Physics, Detector, Instrumentation and Detectors (physics.ins-det), Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators), molybdenum: oxygen, Double-beta decay detector, Low Temperature Detector, lithium, Scintillation counter, Neutrino, photon: yield, numerical calculations: Monte Carlo, bolometers, FOS: Physical sciences, Cryogenic detector, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], neutrinoless double beta decay, Particle identification method, double-beta decay: (0neutrino), Double beta decay, CUPID, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Engineering (miscellaneous), scintillation counter, Scintillation, molybdenum: nuclide, 010308 nuclear & particles physics, bibliography, crystal: geometry, Computational physics, efficiency, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE, Energy (signal processing)
Abstract: The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li$$_{2}$$ 2 $$^{100}$$ 100 MoO$$_4$$ 4 crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of ($$6.7\pm 0.6$$ 6.7 ± 0.6 ) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of $$\alpha $$ α particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this $$\alpha $$ α -induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector.
Published: 2021
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35. Novel technique for the study of pileup events in cryogenic bolometers

Author: Valentyn Novosad, Andrea Giachero, R. Nipoti, Jie Zhang, H. Z. Huang, V. G. Yefremenko, G. Keppel, D. Mayer, C. Nones, A. Puiu, S. Nisi, A. Armatol, K. Wilson, I. Colantoni, A. Barresi, P. Loaiza, C. Oriol, G. Pessina, V. Sanglard, L. Imbert, M. Faverzani, M. Beretta, S. Copello, C. Pagliarone, F.A. Danevich, A. Branca, Jonathan Ouellet, T. O'Donnell, Paolo Carniti, Massimiliano Clemenza, G. Bari, S. Di Domizio, Kai Vetter, C. Rosenfeld, D. L. Helis, Monica Sisti, Federico Ferri, H. Khalife, V. Boldrini, P. Gorla, P. Pari, F. Ferroni, Tomas Polakovic, B. Schmidt, Stefano Dell'Oro, A. Charrier, J. Billard, C. Tomei, S. H. Fu, N. Casali, Laura Cardani, G. Wang, Jie Yang, B. K. Fujikawa, R. J. Creswick, Davide Chiesa, P. Gras, M. Chapellier, C. Pira, Joseph A. Formaggio, L. Pagnanini, P. T. Surukuchi, C. Brofferio, L. Wang, Massimiliano Nastasi, Stefano Pozzi, E. Figueroa-Feliciano, Haiping Peng, V. Shlegel, V. Sharma, E. V. Hansen, A. S. Barabash, B. Paul, M. Gros, Evelyn Ferri, Oliviero Cremonesi, S. Zucchelli, James Nikkel, Ezio Previtali, J. Gascon, R. Mariam, C. C. Chang, L. Ma, Yu. G. Kolomensky, Luigi Cappelli, L. Taffarello, B. Welliver, A. Giuliani, M. Madhukuttan, Matias Velázquez, C. Augier, S. Marnieros, V. Yumatov, Goran Karapetrov, G. Fantini, A. Cazes, Danielle Speller, James R. Wilson, A. Cruciani, X. F. Navick, S. Pirro, V. V. Kobychev, J. Camilleri, A. Franceschi, Changbo Fu, C. Rusconi, J. A. Scarpaci, A. Juillard, L. Bergé, R. Rizzoli, M. M. Zarytskyy, V. Dompè, G. D'Imperio, Irene Nutini, A. D'Addabbo, P. de Marcillac, M. De Jesus, O. G. Polischuk, F. Bellini, A. Ressa, D. Baudin, M. Xue, M. Pavan, Lindley Winslow, A. Drobizhev, I. Dafinei, S. L. Wagaarachchi, F. Collamati, V. Pettinacci, Simone Capelli, E. Olivieri, S. I. Konovalov, Eric B. Norman, L. Pattavina, M. I. Martínez, T. Napolitano, L. Marini, V.I. Tretyak, D. Misiak, D. V. Poda, J. Johnston, M. Biassoni, E. Armengaud, Vasundhara Singh, S. Milana, O. Azzolini, L. Gironi, F. T. Avignone, Whitney Armstrong, Y. Liu, C. Bucci, T. D. Gutierrez, R. G. Huang, F. Mancarella, L. Yan, S. Pagan, B. Mauri, M. de Combarieu, E. Celi, C. Gotti, A. S. Zolotarova, Ke Han, Reina H. Maruyama, A. Tsymbaliuk, Y. Mei, K. M. Heeger, O. Tellier, L. Dumoulin, Giovanni Benato, Armatol A., Armengaud E., Armstrong W., Augier C., Avignone F.T., Azzolini O., Barabash A., Bari G., Barresi A., Baudin D., Bellini F., Benato G., Beretta M., Berge L., Biassoni M., Billard J., Boldrini V., Branca A., Brofferio C., Bucci C., Camilleri J., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Cazes A., Celi E., Chang C., Chapellier M., Charrier A., Chiesa D., Clemenza M., Colantoni I., Collamati F., Copello S., Cremonesi O., Creswick R.J., Cruciani A., D'Addabbo A., D'Imperio G., Dafinei I., Danevich F.A., De Combarieu M., De Jesus M., De Marcillac P., Dell'Oro S., Di Domizio S., Dompe V., Drobizhev A., Dumoulin L., Fantini G., Faverzani M., Ferri E., Ferri F., Ferroni F., Figueroa-Feliciano E., Formaggio J., Franceschi A., Fu C., Fu S., Fujikawa B.K., Gascon J., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gras P., Gros M., Gutierrez T.D., Han K., Hansen E.V., Heeger K.M., Helis D.L., Huang H.Z., Huang R.G., Imbert L., Johnston J., Juillard A., Karapetrov G., Keppel G., Khalife H., Kobychev V.V., Kolomensky Y.G., Konovalov S., Liu Y., Loaiza P., Ma L., Madhukuttan M., Mancarella F., Mariam R., Marini L., Marnieros S., Martinez M., Maruyama R.H., Mauri B., Mayer D., Mei Y., Milana S., Misiak D., Napolitano T., Nastasi M., Navick X.F., Nikkel J., Nipoti R., Nisi S., Nones C., Norman E.B., Novosad V., Nutini I., O'Donnell T., Olivieri E., Oriol C., Ouellet J.L., Pagan S., Pagliarone C., Pagnanini L., Pari P., Pattavina L., Paul B., Pavan M., Peng H., Pessina G., Pettinacci V., Pira C., Pirro S., Poda D.V., Polakovic T., Polischuk O.G., Pozzi S., Previtali E., Puiu A., Ressa A., Rizzoli R., Rosenfeld C., Rusconi C., Sanglard V., Scarpaci J., Schmidt B., Sharma V., Shlegel V., Singh V., Sisti M., Speller D., Surukuchi P.T., Taffarello L., Tellier O., Tomei C., Tretyak V.I., Tsymbaliuk A., Velazquez M., Vetter K.J., Wagaarachchi S.L., Wang G., Wang L., Welliver B., Wilson J., Wilson K., Winslow L.A., Xue M., Yan L., Yang J., Yefremenko V., Yumatov V., Zarytskyy M.M., Zhang J., Zolotarova A., Zucchelli S., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-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), Institut Rayonnement Matière de Saclay (IRAMIS), Science et Ingénierie des Matériaux et Procédés (SIMaP), Institut de Chimie du CNRS (INC)-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), CUPID, 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), Centre National de la Recherche Scientifique (CNRS)-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)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Armatol, A, Armengaud, E, Armstrong, W, Augier, C, Avignone, F, Azzolini, O, Barabash, A, Bari, G, Barresi, A, Baudin, D, Bellini, F, Benato, G, Beretta, M, Berge, L, Biassoni, M, Billard, J, Boldrini, V, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cazes, A, Celi, E, Chang, C, Chapellier, M, Charrier, A, Chiesa, D, Clemenza, M, Colantoni, I, Collamati, F, Copello, S, Cremonesi, O, Creswick, R, Cruciani, A, D'Addabbo, A, D'Imperio, G, Dafinei, I, Danevich, F, De Combarieu, M, De Jesus, M, De Marcillac, P, Dell'Oro, S, Di Domizio, S, Dompe, V, Drobizhev, A, Dumoulin, L, Fantini, G, Faverzani, M, Ferri, E, Ferri, F, Ferroni, F, Figueroa-Feliciano, E, Formaggio, J, Franceschi, A, Fu, C, Fu, S, Fujikawa, B, Gascon, J, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gras, P, Gros, M, Gutierrez, T, Han, K, Hansen, E, Heeger, K, Helis, D, Huang, H, Huang, R, Imbert, L, Johnston, J, Juillard, A, Karapetrov, G, Keppel, G, Khalife, H, Kobychev, V, Kolomensky, Y, Konovalov, S, Liu, Y, Loaiza, P, Ma, L, Madhukuttan, M, Mancarella, F, Mariam, R, Marini, L, Marnieros, S, Martinez, M, Maruyama, R, Mauri, B, Mayer, D, Mei, Y, Milana, S, Misiak, D, Napolitano, T, Nastasi, M, Navick, X, Nikkel, J, Nipoti, R, Nisi, S, Nones, C, Norman, E, Novosad, V, Nutini, I, O'Donnell, T, Olivieri, E, Oriol, C, Ouellet, J, Pagan, S, Pagliarone, C, Pagnanini, L, Pari, P, Pattavina, L, Paul, B, Pavan, M, Peng, H, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Poda, D, Polakovic, T, Polischuk, O, Pozzi, S, Previtali, E, Puiu, A, Ressa, A, Rizzoli, R, Rosenfeld, C, Rusconi, C, Sanglard, V, Scarpaci, J, Schmidt, B, Sharma, V, Shlegel, V, Singh, V, Sisti, M, Speller, D, Surukuchi, P, Taffarello, L, Tellier, O, Tomei, C, Tretyak, V, Tsymbaliuk, A, Velazquez, M, Vetter, K, Wagaarachchi, S, Wang, G, Wang, L, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Xue, M, Yan, L, Yang, J, Yefremenko, V, Yumatov, V, Zarytskyy, M, Zhang, J, Zolotarova, A, and Zucchelli, S
Subjects: data analysis method, double beta decay, nuclear tests of fundamental interactions, Particle decays, Physics - Instrumentation and Detectors, double beta decay, FOS: Physical sciences, Cryogenics, MESH: numerical calculation, 01 natural sciences, law.invention, benchmark, bolometer, double-beta decay: (0neutrino), law, Double beta decay, 0103 physical sciences, Electronic engineering, MESH: benchmark, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], numerical calculations, 010306 general physics, time resolution, nuclear tests of fundamental interactions, Physics, Signal generator, 010308 nuclear & particles physics, Bolometer, Detector, Time resolution, MESH: data analysis method, Instrumentation and Detectors (physics.ins-det), MESH: bolometer, Gran Sasso, Neutrinoless Double Beta decay, Neutrino Physics, MESH: cryogenics, efficiency, cryogenics, pile-up, Rise time, MESH: Gran Sasso, Benchmark (computing), MESH: double-beta decay: (0neutrino), Neutrinoless double-beta decay, MESH: efficiency, Particle decays, MESH: time resolution, MESH: pile-up
Abstract: International audience; Precise characterization of detector time resolution is of crucial importance for next-generation cryogenic-bolometer experiments searching for neutrinoless double-beta decay, such as CUPID, in order to reject background due to pile-up of two-neutrino double-beta decay events. In this paper, we describe a technique developed to study the pile-up rejection capability of cryogenic bolometers. Our approach, which consists of producing controlled pile-up events with a programmable waveform generator, has the benefit that we can reliably and reproducibly control the time separation and relative energy of the individual components of the generated pile-up events. The resulting data allow us to optimize and benchmark analysis strategies to discriminate between individual and pile-up pulses. We describe a test of this technique performed with a small array of detectors at the Laboratori Nazionali del Gran Sasso, in Italy; we obtain a 90% rejection efficiency against pulser-generated pile-up events with rise time of ~15 ms down to time separation between the individual events of 2 ms.
Published: 2021
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36. A CUPID Li$_2$ $^{100} $MoO$_4$ scintillating bolometer tested in the CROSS underground facility

Author: A. S. Barabash, V. Yumatov, G. D'Imperio, M. De Deo, Ezio Previtali, J. M. Calvo-Mozota, Evelyn Ferri, B. Welliver, L. Gironi, L. Marini, E. Guerard, D. Misiak, D. V. Poda, J. Johnston, V. Dompè, F. T. Avignone, Whitney Armstrong, A. Charrier, O. Tellier, I. Colantoni, A. D'Addabbo, S. Di Domizio, P. Pari, Tomas Polakovic, Massimiliano Clemenza, V. Shlegel, R. Mariam, Yu. G. Kolomensky, Luigi Cappelli, Monica Sisti, M. Pavan, S. Zucchelli, Laura Cardani, P. de Marcillac, C. Augier, Goran Karapetrov, X.-F. Navick, B. K. Fujikawa, Stefano Pozzi, L. Pagnanini, P. T. Surukuchi, O. Azzolini, G. Fantini, Federico Ferri, B. Schmidt, C. Oriol, C. Pagliarone, E. Celi, T. O'Donnell, S. H. Fu, S. Dell'Oro, Giovanni Benato, M. Xue, Yuting Liu, Ch. Bourgeois, C. C. Chang, Stefano Nisi, James R. Wilson, S. Milana, G. Olivier, A. Cruciani, A. Franceschi, Changbo Fu, I. Dafinei, M. Chapellier, C. Gotti, S. Copello, C. Brofferio, S. Pirro, Jie Yang, V. Sharma, D. L. Helis, A. Barresi, J. Camilleri, R. Rizzoli, L. Ma, L. Dumoulin, Davide Chiesa, A. S. Zolotarova, Paolo Carniti, V. Pettinacci, A. Juillard, A. Candela, M. Gros, M. Madhukuttan, I. C. Bandac, M. De Jesus, E. V. Hansen, O. G. Polischuk, A. Drobizhev, Ke Han, F. Bellini, A. Ressa, Reina H. Maruyama, V.I. Tretyak, F.A. Danevich, J. A. Scarpaci, C. Bucci, T. D. Gutierrez, M. Faverzani, Matias Velázquez, P. Loaiza, Kai Vetter, Massimiliano Nastasi, S. I. Konovalov, L. Taffarello, D. Reynet, V. V. Kobychev, L. Bergé, J. Gascon, V. Sanglard, L. Yan, L. Imbert, Virendra Singh, M. M. Zarytskyy, Valentyn Novosad, C. Rosenfeld, Danielle Speller, Andrea Giachero, N. Casali, A. Branca, L. Pattavina, A. Ianni, E. Olivieri, R. J. Creswick, Eric B. Norman, V. Boldrini, P. Gras, K. Wilson, S. Pagan, J. Billard, S. Marnieros, Li Wang, T. Napolitano, R. Nipoti, A. Cazes, P. Gorla, F. Ferroni, E. Figueroa-Feliciano, C. Tomei, C. Pira, Haiping Peng, Oliviero Cremonesi, M. Biassoni, D. Mayer, Jonathan Ouellet, G. Bari, Lindley Winslow, M. de Combarieu, Joseph A. Formaggio, A. Tsymbaliuk, Y. Mei, A. Armatol, K. M. Heeger, R. G. Huang, F. Mancarella, B. Paul, M. I. Martínez, G. Pessina, Jie Zhang, C. Nones, A. Puiu, A. Giuliani, B. Mauri, James Nikkel, Irene Nutini, G. Wang, H. Z. Huang, V. G. Yefremenko, G. Keppel, H. Khalife, E. Armengaud, D. Baudin, M. Beretta, S. L. Wagaarachchi, F. Collamati, Simone Capelli, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-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), Institut Rayonnement Matière de Saclay (IRAMIS), Science et Ingénierie des Matériaux et Procédés (SIMaP), 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), CUPID, CROSS, 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), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Armatol A., Armengaud E., Armstrong W., Augier C., Iii F.T.A., Azzolini O., Bandac I.C., Barabash A.S., Bari G., Barresi A., Baudin D., Bellini F., Benato G., Beretta M., Berge L., Bourgeois C., Biassoni M., Billard J., Boldrini V., Branca A., Brofferio C., Bucci C., Calvo-Mozota J.M., Camilleri J., Candela A., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Cazes A., Celi E., Chang C., Chapellier M., Charrier A., Chiesa D., Clemenza M., Colantoni I., Collamati F., Copello S., Cremonesi O., Creswick R.J., Cruciani A., D'Addabbo A., D'Imperio G., Dafinei I., Danevich F.A., De Combarieu M., Deo M.D., Jesus M.D., De Marcillac P., Dell'Oro S., Domizio S.D., Dompe V., Drobizhev A., Dumoulin L., Fantini G., Faverzani M., Ferri E., Ferri F., Ferroni F., Figueroa-Feliciano E., Formaggio J., Franceschi A., Fu C., Fu S., Fujikawa B.K., Gascon J., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gras P., Gros M., Guerard E., Gutierrez T.D., Han K., Hansen E.V., Heeger K.M., Helis D.L., Huang H.Z., Huang R.G., Ianni A., Imbert L., Johnston J., Juillard A., Karapetrov G., Keppel G., Khalife H., Kobychev V.V., Kolomensky Y.G., Konovalov S.I., Liu Y., Loaiza P., Ma L., Madhukuttan M., Mancarella F., Mariam R., Marini L., Marnieros S., Martinez M., Maruyama R.H., Mauri B., Mayer D., Mei Y., Milana S., Misiak D., Napolitano T., Nastasi M., Navick X.-F., Nikkel J., Nipoti R., Nisi S., Nones C., Norman E.B., Novosad V., Nutini I., O'Donnell T., Olivier G., Olivieri E., Oriol C., Ouellet J.L., Pagan S., Pagliarone C., Pagnanini L., Pari P., Pattavina L., Paul B., Pavan M., Peng H., Pessina G., Pettinacci V., Pira C., Pirro S., Poda D.V., Polakovic T., Polischuk O.G., Pozzi S., Previtali E., Puiu A., Ressa A., Reynet D., Rizzoli R., Rosenfeld C., Sanglard V., Scarpaci J.A., Schmidt B., Sharma V., Shlegel V.N., Singh V., Sisti M., Speller D., Surukuchi P.T., Taffarello L., Tellier O., Tomei C., Tretyak V.I., Tsymbaliuk A., Velazquez M., Vetter K.J., Wagaarachchi S.L., Wang G., Wang L., Welliver B., Wilson J., Wilson K., Winslow L.A., Xue M., Yan L., Yang J., Yefremenko V., Yumatov V.I., Zarytskyy M.M., Zhang J., Zolotarova A.S., Zucchelli S., Armatol, A, Armengaud, E, Armstrong, W, Augier, C, Avignone F. T., I, Azzolini, O, Bandac, I, Barabash, A, Bari, G, Barresi, A, Baudin, D, Bellini, F, Benato, G, Beretta, M, Berge, L, Bourgeois, C, Biassoni, M, Billard, J, Boldrini, V, Branca, A, Brofferio, C, Bucci, C, Calvo-Mozota, J, Camilleri, J, Candela, A, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cazes, A, Celi, E, Chang, C, Chapellier, M, Charrier, A, Chiesa, D, Clemenza, M, Colantoni, I, Collamati, F, Copello, S, Cremonesi, O, Creswick, R, Cruciani, A, D'Addabbo, A, D'Imperio, G, Dafinei, I, Danevich, F, De Combarieu, M, Deo, M, Jesus, M, De Marcillac, P, Dell'Oro, S, Domizio, S, Dompe, V, Drobizhev, A, Dumoulin, L, Fantini, G, Faverzani, M, Ferri, E, Ferri, F, Ferroni, F, Figueroa-Feliciano, E, Formaggio, J, Franceschi, A, Fu, C, Fu, S, Fujikawa, B, Gascon, J, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gras, P, Gros, M, Guerard, E, Gutierrez, T, Han, K, Hansen, E, Heeger, K, Helis, D, Huang, H, Huang, R, Ianni, A, Imbert, L, Johnston, J, Juillard, A, Karapetrov, G, Keppel, G, Khalife, H, Kobychev, V, Kolomensky, Y, Konovalov, S, Liu, Y, Loaiza, P, Ma, L, Madhukuttan, M, Mancarella, F, Mariam, R, Marini, L, Marnieros, S, Martinez, M, Maruyama, R, Mauri, B, Mayer, D, Mei, Y, Milana, S, Misiak, D, Napolitano, T, Nastasi, M, Navick, X, Nikkel, J, Nipoti, R, Nisi, S, Nones, C, Norman, E, Novosad, V, Nutini, I, O'Donnell, T, Olivier, G, Olivieri, E, Oriol, C, Ouellet, J, Pagan, S, Pagliarone, C, Pagnanini, L, Pari, P, Pattavina, L, Paul, B, Pavan, M, Peng, H, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Poda, D, Polakovic, T, Polischuk, O, Pozzi, S, Previtali, E, Puiu, A, Ressa, A, Reynet, D, Rizzoli, R, Rosenfeld, C, Sanglard, V, Scarpaci, J, Schmidt, B, Sharma, V, Shlegel, V, Singh, V, Sisti, M, Speller, D, Surukuchi, P, Taffarello, L, Tellier, O, Tomei, C, Tretyak, V, Tsymbaliuk, A, Velazquez, M, Vetter, K, Wagaarachchi, S, Wang, G, Wang, L, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Xue, M, Yan, L, Yang, J, Yefremenko, V, Yumatov, V, Zarytskyy, M, Zhang, J, Zolotarova, A, and Zucchelli, S
Subjects: gas and liquid scintillators), Physics - Instrumentation and Detectors, Accurate estimation, Physics::Instrumentation and Detectors, Bolometer, Analytical chemistry, Double-beta decay, FOS: Physical sciences, Cryogenic detector, Radiopurity, 01 natural sciences, 030218 nuclear medicine & medical imaging, law.invention, Particle identification, Particle identification methods, 03 medical and health sciences, Particle identification method, 0302 clinical medicine, CUORE, law, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Detector array, Instrumentation, Mathematical Physics, Event triggered, Physics, Lithium molybdate, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators), Double-beta decay detectors, scintillation and light emission processes (solid, Double-beta decay detector, Cryogenic detectors, Scintillators, Crystal scintillator, Energy (signal processing)
Abstract: A scintillating bolometer based on a large cubic Li$_{2}$$^{100}$MoO$_4$ crystal (45 mm side) and a Ge wafer (scintillation detector) has been operated in the CROSS cryogenic facility at the Canfranc underground laboratory in Spain. The dual-readout detector is a prototype of the technology that will be used in the next-generation $0\nu2\beta$ experiment CUPID. The measurements were performed at 18 and 12 mK temperature in a pulse tube dilution refrigerator. This setup utilizes the same technology as the CUORE cryostat that will host CUPID and so represents an accurate estimation of the expected performance. The Li$_{2}$$^{100}$MoO$_4$ bolometer shows a high energy resolution of 6 keV FWHM at the 2615 keV $\gamma$ line. The detection of scintillation light for each event triggered by the Li$_{2}$$^{100}$MoO$_4$ bolometer allowed for a full separation ($\sim$8$\sigma$) between $\gamma$($\beta$) and $\alpha$ events above 2 MeV. The Li$_{2}$$^{100}$MoO$_4$ crystal also shows a high internal radiopurity with $^{228}$Th and $^{226}$Ra activities of less than 3 and 8 $\mu$Bq/kg, respectively. Taking also into account the advantage of a more compact and massive detector array, which can be made of cubic-shaped crystals (compared to the cylindrical ones), this test demonstrates the great potential of cubic Li$_{2}$$^{100}$MoO$_4$ scintillating bolometers for high-sensitivity searches for the $^{100}$Mo $0\nu2\beta$ decay in CROSS and CUPID projects., Comment: 19 pages, 7 figures, 1 table
Published: 2021
Full Text: View/download PDF

37. Lowering the energy threshold in COSINE-100 dark matter searches

Author: A. C. Ezeribe, S. Choi, Sun-Whe Kim, K.W. Kim, N. J. C. Spooner, David Leonard, S. L. Olsen, G. H. Yu, Carsten Rott, L. E. França, R. L. C. Pitta, J. H. Jo, L. Yang, N. Carlin, J.H. Lee, Hyo-Suk Lee, M. Kauer, J.J. Choi, Kangsoon Park, Hansoo Park, W. G. Thompson, B. B. Manzato, H. Prihtiadi, E.K. Lee, Govinda Adhikari, Hyunghoon Kim, R. J. Neal, A. Scarff, Reina H. Maruyama, Yong Hamb Kim, Y. D. Kim, E. Barbosa de Souza, H. J. Kim, Woosik Kang, K. A. Shin, Insik Hahn, Mitra Djamal, Y. J. Ko, C. Ha, S. J. Ra, B. J. Park, Eunju Jeon, J.Y. Lee, Hyangkyu Park, Moo Hyun Lee, and S.H. Lee
Subjects: Physics, Physics - Instrumentation and Detectors, MATÉRIA ESCURA, 010308 nuclear & particles physics, Dark matter, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Electron, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 7. Clean energy, High Energy Physics - Experiment, Nuclear physics, Event selection, High Energy Physics - Experiment (hep-ex), Modulation, 0103 physical sciences, Underground laboratory, Trigonometric functions, 010303 astronomy & astrophysics, Energy (signal processing)
Abstract: COSINE-100 is a dark matter detection experiment that uses NaI(Tl) crystal detectors operating at the Yangyang underground laboratory in Korea since September 2016. Its main goal is to test the annual modulation observed by the DAMA/LIBRA experiment with the same target medium. Recently DAMA/LIBRA has released data with an energy threshold lowered to 1 keV, and the persistent annual modulation behavior is still observed at 9.5 σ . By lowering the energy threshold for electron recoils to 1 keV, COSINE-100 annual modulation results can be compared to those of DAMA/LIBRA in a model-independent way. Additionally, the event selection methods provide an access to a few to sub-GeV dark matter particles using constant rate studies. In this article, we discuss the COSINE-100 event selection algorithm, its validation, and efficiencies near the threshold.
Published: 2021

38. Searching for New Physics in two-neutrino double beta decay with CUPID

Author: A Armatol, E Armengaud, W Armstrong, C Augier, F T Avignone, O Azzolini, A Barabash, G Bari, A Barresi, D Baudin, F Bellini, G Benato, M Beretta, L Bergé, M Biassoni, J Billard, V Boldrini, A Branca, C Brofferio, C Bucci, J Camilleri, S Capelli, L Cappelli, L Cardani, P Carniti, N Casali, A Cazes, E Celi, C Chang, M Chapellier, A Charrier, D Chiesa, M Clemenza, I Colantoni, F Collamati, S Copello, O Cremonesi, R J Creswick, A Cruciani, A D’ Addabbo, G D’ Imperio, I Dafinei, F A Danevich, M de Combarieu, M De Jesus, P de Marcillac, S Dell’Oro, S Di Domizio, V Dompè, A Drobizhev, L Dumoulin, G Fantini, M Faverzani, E Ferri, F Ferri, F Ferroni, E Figueroa-Feliciano, J Formaggio, A Franceschi, C Fu, S Fu, B K Fujikawa, J Gascon, S Ghislandi, A Giachero, L Gironi, A Giuliani, P Gorla, C Gotti, P Gras, M Gros, T D Gutierrez, K Han, E V Hansen, K M Heeger, D L Helis, H Z Huang, R G Huang, L Imbert, J Johnston, A Juillard, G Karapetrov, G Keppel, H Khalife, V V Kobychev, J Kotila, Yu G Kolomensky, S Konovalov, Y Liu, P Loaiza, L Ma, M Madhukuttan, F Mancarella, R Mariam, L Marini, S Marnieros, M Martinez, R H Maruyama, B Mauri, D Mayer, Y Mei, S Milana, D Misiak, T Napolitano, M Nastasi, X F Navick, J Nikkel, R Nipoti, S Nisi, C Nones, E B Norman, V Novosad, I Nutini, T O’Donnell, E Olivieri, C Oriol, J L Ouellet, S Pagan, C Pagliarone, L Pagnanini, P Pari, L Pattavina, B Paul, M Pavan, H Peng, G Pessina, V Pettinacci, C Pira, S Pirro, D V Poda, T Polakovic, O G Polischuk, S Pozzi, E Previtali, A Puiu, S Quitadamo, A Ressa, R Rizzoli, C Rosenfeld, C Rusconi, V Sanglard, J Scarpaci, B Schmidt, V Sharma, V Shlegel, V Singh, M Sisti, D Speller, P T Surukuchi, L Taffarello, O Tellier, C Tomei, V I Tretyak, A Tsymbaliuk, M Velazquez, K J Vetter, S L Wagaarachchi, G Wang, L Wang, B Welliver, J Wilson, K Wilson, L A Winslow, M Xue, L Yan, J Yang, V Yefremenko, V Yumatov, M M Zarytskyy, J Zhang, A Zolotarova, S Zucchelli, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, 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 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), Institut Rayonnement Matière de Saclay (IRAMIS), Science et Ingénierie des Matériaux et Procédés (SIMaP), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), and Université Grenoble Alpes (UGA)
Subjects: CUPID, Neutrinoless Double Beta Decay, LNGS, Particle Physics, Neutrino, Majorana Neutrino, History, LNGS, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], hiukkasfysiikka, Neutrinoless Double Beta Decay, Education, crystal, CUPID, Neutrino, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], double-beta decay: (2neutrino), Particle Physics, scintillation counter, symmetry: violation, background, new physics: search for, Majorana Neutrino, neutriinot, sensitivity, violation: Lorentz, Majoron, Computer Science Applications, calorimeter: cryogenics, electron: energy spectrum, symmetry: Lorentz, ydinfysiikka
Abstract: In the past few years, attention has been drawn to the fact that a precision analysis of two-neutrino double beta decay (2υββ) allows the study of interesting physics cases like the emission of Majoron bosons and possible Lorentz symmetry violation. These processes modify the summed-energy distribution of the two electrons emitted in 2υββ. CUPID is a next-generation experiment aiming to exploit 100Mo-enriched scintillating Li2MoO4 crystals, operating as cryogenic calorimeters. Given the relatively fast half-life of 100Mo 2υββ and the large exposure that can be reached by CUPID, we expect to measure with very high precision the 100Mo 2υββ spectrum shape, reaching great sensitivities in the search for distortions induced by the physics beyond the Standard Model. In this contribution, we present the CUPID exclusion sensitivity for such New Physics processes, as well as the preliminary projected background of CUPID.
Published: 2021
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39. EV-Scale Sterile Neutrino Search Using Eight Years of Atmospheric Muon Neutrino Data from the IceCube Neutrino Observatory

Author: K. Tollefson, Albrecht Karle, U. Katz, R. S. Busse, G. H. Collin, Christopher Wiebusch, Kunal Deoskar, Thomas Ehrhardt, P. Schlunder, R. Hellauer, Spencer Axani, D. B. Fox, Kayla Leonard, R. Maunu, Alan Coleman, Sukeerthi Dharani, Francis Halzen, J. Merz, S. Hickford, R. Joppe, A. Wallace, Delia Tosi, Sebastian Baur, M. G. Aartsen, Carlos Arguelles, David Vannerom, I. Ansseau, Hermann Kolanoski, Juliana Stachurska, H. Dembinski, Stef Verpoest, Jessie Micallef, Matthias Vraeghe, George Japaridze, Roger Moore, Tim Ruhe, N. Kurahashi, Todor Stanev, C. Wendt, Ioana Codrina Maris, H. Bagherpour, Johan Wulff, Sebastian Böser, Olga Botner, J. Kim, Elisa Bernardini, A. Ludwig, Christoph Raab, Nadège Iovine, Timothyblake Watson, D. Heereman, Gisela Anton, M. Stamatikos, J. Bourbeau, K. Rawlins, G. de Wasseige, Won Nam Kang, V. Baum, Jenni Adams, D. Berley, G. C. Hill, H. Niederhausen, A. Steuer, C. Alispach, Bunheng Ty, Stephen L. Hauser, Raamis Hussain, Janet Conrad, B. Relethford, Jan Soedingrekso, Ralph Engel, Moritz Kellermann, Z. Griffith, Y. Makino, Seongjin In, R. Hoffmann, James Madsen, Konstancja Satalecka, Benjamin Bastian, Theo Glauch, Anastasia Maria Barbano, Saskia Philippen, F. Jonske, R. Cross, M. J. Larson, Lu Lu, T. Kittler, X. Bai, G. Neer, Alexander Fritz, A. Goldschmidt, D. van Eijk, Lenka Tomankova, Giovanni Renzi, D. Seckel, S. Fahey, Elisa Resconi, Alessio Porcelli, Claudio Kopper, Daniel Bindig, G. Krückl, Alejandro Diaz, C. Pérez de los Heros, E. O’Sullivan, Le Viet Nguyen, Wing Yan Ma, James DeLaunay, Marjon Moulai, R. G. Stokstad, K. Krings, M. Plum, P. B. Price, William Luszczak, M. Kauer, Suyong Choi, David Kappesser, S. E. Sanchez Herrera, Francesco Lucarelli, T. O. B. Schmidt, Tyce DeYoung, Chad Finley, Nathan Whitehorn, Immacolata Carmen Rea, Matti Jansson, D. Z. Besson, C. Walck, Thomas K. Gaisser, G. B. Yodh, A. Kyriacou, M. Silva, Najia Moureen Binte Amin, K.-H. Becker, Yiqian Xu, Qinrui Liu, J. Becker Tjus, T. Glüsenkamp, Subir Sarkar, Martina Karl, Matt Dunkman, Kendall Mahn, Christoph Tönnis, F. Huang, K. Meagher, Jochen M. Schneider, J. Stettner, T. R. Wood, Kurt Woschnagg, Paul Evenson, T. Palczewski, S. De Ridder, Y. L. Li, G. W. Sullivan, J. J. Beatty, Tianlu Yuan, Jeffrey Lazar, Chunfai Tung, James E. Braun, Alexander Trettin, E. Cheung, J. Werthebach, Thomas Stuttard, Mirco Hunnefeld, Marie Oehler, Alexander Sandrock, Elisa Lohfink, Thomas Meures, N. L. Strotjohann, M. A. Unland Elorrieta, M. Wallraff, Michael DuVernois, Benjamin Hokanson-Fasig, Felix Henningsen, Karl J. Clark, Simone Garrappa, Dmitry Chirkin, Sarah Pieper, D. Hebecker, Anatoli Fedynitch, K. Helbing, Chujie Chen, Dirk Ryckbosch, Joshua Hignight, M. Zöcklein, T. Grégoire, Timo Sturwald, J. C. Gallagher, Timo Karg, Gerald Przybylski, Federica Bradascio, Yang Lyu, Alexander Kappes, Alexander Burgman, M. Song, T. L. Carver, Paras Koundal, Mike Richman, Sarah Mancina, Paul Coppin, Anna Franckowiak, Tobias Hoinka, Vedant Basu, Steve Sclafani, F. McNally, A. R. Fazely, M. Usner, Grant Parker, R. Halliday, Stephan Meighen-Berger, K. D. de Vries, Gerrit Wrede, Andrea Turcati, J. van Santen, K. Hoshina, Glenn Spiczak, Thomas Huber, G. Momenté, Merlin Schaufel, A. Stößl, J. Kiryluk, K. Andeen, D. R. Nygren, Marek Kowalski, A. Weindl, Maryon Ahrens, Frederik Tenholt, R. Nagai, M. Medici, M. Rameez, Javier Gonzalez, Roxanne Turcotte, Alex Pizzuto, D. F. Cowen, Reina H. Maruyama, E. Pinat, N. Kulacz, U. Naumann, Martin Rongen, Ek Narayan Paudel, Allan Hallgren, Giorgio Maggi, K. Wiebe, A. Balagopal, Gary Binder, Zhedong Zhang, E. Unger, Simona Toscano, J. Auffenberg, Pablo Correa, Summer Blot, Brian Clark, C. De Clercq, P. Heix, K. Mase, P. Mallik, M. E. Huber, A. O'Murchadha, Marcos Santander, Ramesh Koirala, David A. Williams, L. Schumacher, Benedikt Riedel, S. Tilav, Max Renschler, D. Kang, D. J. Koskinen, Markus Ackermann, S. W. Barwick, L. Gerhardt, M. J. Weiss, E. Bourbeau, J. P. Yanez, Ben Smithers, Colin Turley, A. Olivas, S. Kopper, Spencer Griswold, I. Taboada, Michael O. Wolf, René Reimann, A. Haungs, M. Prado Rodriguez, Maria Tselengidou, D. Soldin, Nahee Park, Pranav Dave, K. Hultqvist, Darren Grant, E. Blaufuss, Mehmet Gunduz, Agnieszka Leszczyńska, R. C. Bay, M. Günder, Austin Schneider, Steven Robertson, Juan Carlos Diaz-Velez, Shefali Shefali, L. Classen, T. Stezelberger, Abdul Rehman, Carsten Rott, Y. Popovych, T. Kintscher, Frederik Hermann Lauber, Xianwu Xu, A. Terliuk, J. Sandroos, C. Bohm, Justin Lanfranchi, Christian Spiering, Justin Vandenbroucke, Abhishek Desai, S. C. Nowicki, Rasha Abbasi, B. J. Whelan, Jan Weldert, L. Halve, Philipp Eller, J. Felde, J. Buscher, D. Rysewyk Cantu, A. Obertacke Pollmann, J. L. Kelley, Markus Ahlers, Erik Ganster, Samvel Ter-Antonyan, Frank G. Schröder, J. Lünemann, N. van Eijndhoven, C. Haack, Emily Dvorak, Aaron Fienberg, Amirreza Raissi, Minjin Jeong, Chris Weaver, Stephanie Bron, C. J. Lozano Mariscal, H. Dujmovic, L. Rauch, S. Yoshida, Surujhdeo Seunarine, R. Snihur, Juanan Aguilar, Kael Hanson, A. Ishihara, Maximilian Meier, Paolo Desiati, Segev BenZvi, Spencer Klein, B. J. P. Jones, Andres Medina, Kara Hoffman, D. Mockler, Hershal Pandya, Daria Pankova, E. Friedman, Wolfgang Rhode, Robert Stein, L. Wills, P. Muth, R. Morse, Jakob Bottcher, T. Montaruli, Maximilian Karl Scharf, P. Peiffer, Ibrahim Safa, Damian Pieloth, Ali Kheirandish, W. Van Driessche, Jannes Brostean-Kaiser, M. U. Nisa, L. Köpke, T. Anderson, John Hardin, H. Schieler, Kirill Filimonov, Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, and Elementary Particle Physics
Subjects: Sterile neutrino, Physics::Instrumentation and Detectors, General Physics and Astronomy, sterile [neutrino], 01 natural sciences, Cosmology, IceCube, High Energy Physics - Experiment, Subatomär fysik, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), Astronomi, astrofysik och kosmologi, Subatomic Physics, TOOL, Astronomy, Astrophysics and Cosmology, atmosphere [muon], Muon neutrino, Physics, oscillation [neutrino], Astrophysics::Instrumentation and Methods for Astrophysics, hep-ph, neutrino: sterile, mass difference [neutrino], ddc, muon: atmosphere, observatory, High Energy Physics - Phenomenology, Physique des particules élémentaires, signature, Particle physics, data analysis method, Scale (ratio), Astrophysics::High Energy Astrophysical Phenomena, neutrino: mass difference, FOS: Physical sciences, IceCube Neutrino Observatory, statistical analysis, 0103 physical sciences, OSCILLATIONS, ddc:530, 010306 general physics, hep-ex, ICE, High Energy Physics::Phenomenology, neutrino: mixing angle, CONVERSION, Physics and Astronomy, COSMOLOGY, High Energy Physics::Experiment, neutrino: oscillation, BAYESIAN-INFERENCE, mixing angle [neutrino], experimental results
Abstract: Physical review letters 125(14), 141801 (1-11) (2020). doi:10.1103/PhysRevLett.125.141801, The results of a 3+1 sterile neutrino search using eight years of data from the IceCube Neutrino Observatory are presented. A total of 305 735 muon neutrino events are analyzed in reconstructed energy-zenith space to test for signatures of a matter-enhanced oscillation that would occur given a sterile neutrino state with a mass-squared differences between 0.01 and 100 eV$^2$. The best-fit point is found to be at sin$^2$($2θ_{24}$)=0.10 and $Δm_{41}^2$=4.5 eV$^2$, which is consistent with the no sterile neutrino hypothesis with a $p$ value of 8.0%., Published by APS, College Park, Md.
Published: 2020
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40. IceCube-Gen2: The Window to the Extreme Universe

Author: J. Kim, A. Gartner, A. Obertacke Pollmann, B. Hoffmann, J. L. Kelley, Markus Ahlers, Jenni Adams, Akimichi Taketa, D. van Eijk, Daniel Bindig, G. H. Collin, T. C. Arlen, Robert Lahmann, J. J. Beatty, Tianlu Yuan, U. Nauman, Azadeh Keivani, Y. L. Li, Karl J. Clark, T. Kintscher, M. Song, T. L. Carver, Paras Koundal, Michael Kovacevich, Christian Glaser, Frederik Hermann Lauber, T. Huege, Erik Ganster, Benedikt Riedel, D. Seckel, Anna Nelles, R. G. Stokstad, F. McNally, R. Maunu, M. Prado Rodriguez, Kayla Leonard, N. Kurahashi, James E. Braun, Amy Connolly, Samvel Ter-Antonyan, A. Terliuk, Justin Lanfranchi, Pranav Dave, Jannis Necker, C. Wendt, S. Wren, A. Sharma, Sukeerthi Dharani, David Vannerom, M. H. Shaevitz, Alexander Trettin, Reina H. Maruyama, Francis Halzen, J. Merz, K. Krings, Rasha Abbasi, Ben Smithers, Qinrui Liu, M. J. Larson, T. Anderson, Summer Blot, G. de Wasseige, I. Ansseau, D. Hebecker, Jorge Torres, Killian Holzapfel, Martina Karl, C. J. Lozano Mariscal, John Hardin, Jean Pierre Twagirayezu, Daniel García-Fernández, T. Stezelberger, S. Mandalia, E. O'Sullivan, R. Hoffmann, M. Plum, Juliana Stachurska, H. Dembinski, C. Pérez de los Heros, S. Márka, G. WSullivan, A. Haungs, Paul Coppin, Z. Griffith, J. C. Gallagher, Saskia Philippen, Federica Bradascio, Jochen M. Schneider, Srubabati Goswami, Andrea Turcati, Wing Yan Ma, Nahee Park, Y. Makino, Sarah Mancina, C. Walck, M. Kauer, Suyong Choi, Anna Franckowiak, Tobias Hoinka, Chad Finley, David Kappesser, T. Gregoire, Ella Roberts, J. van Santen, S. De Ridder, Jan Weldert, Chunfai Tung, F. Jonske, Ken'ichi Kin, L. Halve, Philipp Eller, K. Hultqvist, N. L. Strotjohann, H. Dujmovic, Vedant Basu, M. A. Unland Elorrieta, Alex Pizzuto, K. D. de Vries, I. CMariş, Gerrit Wrede, R. Gernhaeuser, Thomas Huber, Matti Jansson, Thomas K. Gaisser, M. Richman, Christoph Tönnis, James DeLaunay, Gary Binder, K.-H. Becker, Ek Narayan Paudel, Allan Hallgren, U. Latif, Hiroyuki Tanaka, I. Safa, Steve Sclafani, J. Kiryluk, K. Andeen, P. B. Price, H. Schieler, Kirill Filimonov, Segev BenZvi, Alexander Fritz, D. Z. Besson, Darren Grant, Marjon Moulai, Yiqian Xu, Felix Henningsen, S. Robertson, Aswathi Balagopal, Francesco Lucarelli, Pisin Chen, Matt Dunkman, Merlin Schaufel, Patrick Allison, Spencer Klein, Cosmin Deaconu, Tim Ruhe, A. Ludwig, George Japaridze, Javier Gonzalez, C. B. Krauss, Roxanne Turcotte, T. O. B. Schmidt, Simona Toscano, Roger Moore, P. Heix, R. S. Busse, Chujie Chen, Pablo Correa, L. Gerhard, S. De Kockere, J. Felde, Surujhdeo Seunarine, R. Snihur, J. Buscher, D. Rysewyk Cantu, A. Weindl, R. Hellauer, Giorgio Maggi, H. Niederhausen, Mauricio Bustamante, D. Southall, Julia Böttcher, J. Bourbeau, Lenka Tomankova, Maryon Ahrens, A. Burgman, Christopher Wiebusch, Darko Veberič, Juanan Aguilar, T. R. Wood, Christian Spiering, Frederik Tenholt, R. Nagai, L. Schumacher, C. De Clercq, Benjamin Hokanson-Fasig, L. V. Nguyen, C. Lagunas Gualda, K. Hughes, Kara Hoffman, C. Alispach, J. M. LoSecco, Joshua Hignight, K. Helbing, Timo Sturwald, Xinyue Kang, Richard Naab, Kunal Deoskar, Janet Conrad, Zackary Meyers, K. Meagher, Mehmet Gunduz, Agnieszka Leszczyńska, R. C. Bay, David A. Williams, Kurt Woschnagg, M. Zöcklein, M. Silva, Claudio Kopper, Eric Oberla, Ramesh Koirala, E. Cheung, Thomas Stuttard, Martin Rongen, Najia Moureen Binte Amin, R. Cross, Paul Evenson, A. Karle, Sebastian Böser, Seongjin In, Johannes Werthebach, J. P. Lazar, Markus Ackermann, Austin Schneider, Yang Lyu, Justin Vandenbroucke, Juan Carlos Diaz-Velez, Beverley A. Clark, Timo Karg, Sarah Pieper, Hershal Pandya, Wolfgang Rhode, Zhedong Zhang, P. Schlunder, A. Ishihara, Elisa Resconi, Subir Sarkar, William Luszczak, Clara E. Hill, Ava Ghadimi, Alessio Porcelli, Alan Coleman, J. Auffenberg, Grant Parker, Robert Stein, Dirk Ryckbosch, Benjamin Bastian, Anastasia Maria Barbano, Abhishek Desai, T. Kittler, J. Nam, P. Mallik, E. Blaufuss, S. Zierke, T. Stanev, M. Bohmer, Stephan Meighen-Berger, Simone Garrappa, P. Muth, Dmitry Chirkin, M. E. Huber, Marcos Santander, Christoph Raab, Nadège Iovine, J. Becker Tjus, L. Classen, Colin Turley, S. C. Nowicki, K. Farrag, M. Kleifges, O. Kalekin, A. Olivas, Alexander Kappes, D. Berley, G. C. Hill, Abigail G. Vieregg, Frank G. Schröder, D. Heinen, Erin Carnie-Bronca, N. Kulacz, D. Tosi, J. C. Hanson, Bunheng Ty, Ralph Engel, Moritz Kellermann, Gisela Anton, Elisa Lohfink, Elisa Bernardini, Damian Pieloth, Ali Kheirandish, Jan Soedingrekso, Giovanni Renzi, Michael DuVernois, Jannes Brostean-Kaiser, K. Wiebe, S. Fahey, A. R. Fazely, Tyce DeYoung, J. Lünemann, Thomas Ehrhardt, Nathan Whitehorn, Immacolata Carmen Rea, M. U. Nisa, Aaron Fienberg, Gerald Przybylski, G. Krückl, L. Papp, Amirreza Raissi, L. Köpke, Chris Weaver, R. Halliday, Alejandro Diaz, Stephanie Bron, S. Söldner-Rembold, James Pinfold, Ryan Burley, M. Riegel, H. Bagherpour, Stephanie Wissel, Olga Botner, Y. Pan, A. Steuer, S. Tilav, D. Kang, M. deWith, V. Baum, J. P. Yanez, I. Taboada, Stephen L. Hauser, Raamis Hussain, Michael O. Wolf, M. Stamatikos, John Evans, Shefali Shefali, Christoph Welling, Abdul Rehman, Carsten Rott, K. Tollefson, A. Goldschmidt, Y. Popovych, Troels Petersen, S. E. Sanchez Herrera, Simeon Reusch, S. Hickford, Xianwu Xu, J. Sandroos, C. Bohm, R. Joppe, Spencer Axani, Sebastian Baur, Carlos Arguelles, Jessie Micallef, Teppei Katori, K. Rawlins, James Madsen, Lu Lu, M. G. Aartsen, T. Glüsenkamp, M. Meier, Michael Campana, P. Sandstrom, Kendall Mahn, B. J. P. Jones, K. Hoshina, Glenn Spiczak, Andres Medina, G. Momenté, D. Mockler, M. Rameez, D. F. Cowen, Daria Pankova, E. Friedman, R. Morse, T. Montaruli, E. Unger, Maximilian Karl Scharf, P. Peiffer, J. Stettner, Gerrit Roellinghoff, Mirco Hunnefeld, Marie Oehler, Max Renschler, D. J. Koskinen, E. Bourbeau, Spencer Griswold, Maria Tselengidou, D. Soldin, Z. Márka, Minjin Jeong, L. Rauch, S. Yoshida, N. van Eijndhoven, C. Haack, Emily Dvorak, D. R. Nygren, Marek Kowalski, Kael Hanson, Paolo Desiati, J. Haugen, Lars Steffen Weinstock, Johan Wulff, Won Nam Kang, Timothyblake Watson, X. Bai, G. Neer, Konstancja Satalecka, Theo Glauch, U. Katz, Alexander Sandrock, Ilse Plaisier, K. Mase, D. B. Fox, Hermann Kolanoski, M. J. Weiss, Stef Verpoest, Imre Bartos, David J. Smith, S. Kopper, René Reimann, Leander Fischer, F. Huang, Matthias Vraeghe, Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, and Elementary Particle Physics
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Nuclear and High Energy Physics, Active galactic nucleus, 010308 nuclear & particles physics, High-energy astronomy, Gravitational wave, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, FOS: Physical sciences, Cosmic ray, 01 natural sciences, Universe, Neutron star, 0103 physical sciences, Neutrino, Neutrino astronomy, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, media_common
Abstract: The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. The discovery of cosmic neutrinos with IceCube has opened this new window on the universe. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the universe at the highest energies. IceCube-Gen2 is designed to: 1) Resolve the high-energy neutrino sky from TeV to EeV energies; 2) Investigate cosmic particle acceleration through multi-messenger observations; 3) Reveal the sources and propagation of the highest energy particles in the universe; 4) Probe fundamental physics with high-energy neutrinos. IceCube-Gen2 will increase the annual rate of observed cosmic neutrinos by a factor of ten compared to IceCube, and will be able to detect sources five times fainter than its predecessor. Furthermore, through the addition of a radio array, IceCube-Gen2 will extend the energy range by several orders of magnitude compared to IceCube. Construction will take 8 years and cost about \$350M. The goal is to have IceCube-Gen2 fully operational by 2033. IceCube-Gen2 will play an essential role in shaping the new era of multi-messenger astronomy, fundamentally advancing our knowledge of the high-energy universe. This challenging mission can be fully addressed only in concert with the new survey instruments across the electromagnetic spectrum and gravitational wave detectors which will be available in the coming years., Comment: 56 pages, 29 figures
Published: 2020
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41. IceCube Search for High-Energy Neutrino Emission from TeV Pulsar Wind Nebulae

Author: C. Haack, Immacolata Carmen Rea, Emily Dvorak, K.-H. Becker, K. Hoshina, Yiqian Xu, Matt Dunkman, K. Mase, Yuya Makino, Minjin Jeong, Timothyblake Watson, Thomas Meures, B. Relethford, E. Cheung, Saskia Philippen, M. J. Weiss, Konstancja Satalecka, Theo Glauch, L. Rauch, U. Katz, Thomas Stuttard, S. De Ridder, Jeffrey Lazar, P. B. Price, D. Heereman, S. Yoshida, D. B. Fox, S. Kopper, Sarah Pieper, K. Jero, N. L. Strotjohann, Hermann Kolanoski, Dirk Ryckbosch, Stef Verpoest, Colin Turley, Felix Henningsen, M. Zöcklein, René Reimann, C. Alispach, Lenka Tomankova, T. Grégoire, Timo Karg, A. Steuer, Stephan Meighen-Berger, Janet Conrad, Thomas Ehrhardt, Frank G. Schröder, A. R. Fazely, M. Silva, Francesco Lucarelli, Raamis Hussain, R. Cross, A. Obertacke Pollmann, E. Pinat, T. O. B. Schmidt, Johannes Werthebach, M. Usner, Kael Hanson, Karl J. Clark, Maximilian Meier, S. Hickford, R. Joppe, Delia Tosi, Sebastian Baur, Chujie Chen, A. Weindl, Maryon Ahrens, Frederik Tenholt, R. Nagai, K. Helbing, Won Nam Kang, X. Bai, G. Neer, Simona Toscano, P. Heix, R. Maunu, J. Lünemann, William Luszczak, S. Tilav, M. Medici, Christian Spiering, L. Wills, P. Muth, P. Schlunder, Daria Pankova, E. Friedman, R. S. Busse, M. Song, T. L. Carver, Mike Richman, Amirreza Raissi, Federica Bradascio, Alexander Burgman, T. R. Wood, Ramesh Koirala, J. P. Yanez, Karim Ghorbani, Spencer Axani, Christopher Wiebusch, Kunal Deoskar, Paolo Desiati, Chris Weaver, Stephanie Bron, Kurt Woschnagg, C. J. Lozano Mariscal, G. Merino, Tim Ruhe, Justin Vandenbroucke, H. Bagherpour, Alexander Sandrock, J. L. Kelley, Markus Ahlers, Martin Rongen, George Japaridze, Roger Moore, A. Ludwig, Olga Botner, Paul Evenson, M. G. Aartsen, N. Wandkowsky, H. Dujmovic, Merlin Schaufel, M. Stamatikos, E. Blaufuss, Ioana Codrina Maris, L. Wille, H. Niederhausen, Carlos Arguelles, Ibrahim Safa, V. Baum, Jessie Micallef, L. Classen, Damian Pieloth, Ali Kheirandish, N. Kurahashi, J. Bourbeau, D. Kang, Todor Stanev, K. Tollefson, Surujhdeo Seunarine, Albrecht Karle, D. van Eijk, Christoph Raab, Nadège Iovine, P. Mallik, Simone Garrappa, Dmitry Chirkin, S. C. Nowicki, W. Van Driessche, C. Wendt, Alexander Kappes, Erik Ganster, K. Mallot, R. Morse, James W. Wood, Z. Griffith, Jakob Bottcher, D. Berley, G. C. Hill, Bunheng Ty, R. Snihur, T. Montaruli, Jannes Brostean-Kaiser, Juanan Aguilar, G. de Wasseige, G. W. Sullivan, K. Rawlins, Donglian Xu, Seongjin In, B. J. P. Jones, Ralph Engel, Moritz Kellermann, Elisa Resconi, I. Taboada, Samvel Ter-Antonyan, Elisa Lohfink, James E. Braun, Gisela Anton, James Madsen, Lu Lu, Alessio Porcelli, T. Kintscher, Frederik Hermann Lauber, Giovanni Renzi, A. Goldschmidt, D. Hebecker, Qinrui Liu, R. Hoffmann, T. Glüsenkamp, Le Viet Nguyen, L. Köpke, D. Seckel, S. Fahey, Michael O. Wolf, Alexander Fritz, D. Z. Besson, Martina Karl, A. Wallace, A. Terliuk, Paul Coppin, Andrea Turcati, Justin Lanfranchi, J. van Santen, Mehr Nisa, Jochen M. Schneider, B. J. Whelan, Claudio Kopper, A. Ishihara, Tyce DeYoung, Andres Medina, Alexander Trettin, Nathan Whitehorn, Alex Pizzuto, D. R. Nygren, Gerald Przybylski, S. E. Sanchez Herrera, M. A. Unland Elorrieta, Gary Binder, R. Halliday, A. Haungs, C. Pérez de los Heros, K. Krings, D. Mockler, Nahee Park, K. Hultqvist, M. Wallraff, Darren Grant, Kendall Mahn, C. Walck, Alan Coleman, E. O’Sullivan, T. Anderson, Marek Kowalski, J. C. Gallagher, M. Plum, Subir Sarkar, Jan Weldert, Thomas K. Gaisser, G. B. Yodh, A. Kyriacou, Gerrit Wrede, K. Meagher, L. Halve, Philipp Eller, Thomas Huber, Allan Hallgren, Benjamin Hokanson-Fasig, Yang Lyu, Elisa Bernardini, J. Auffenberg, Chunfai Tung, J. Becker Tjus, J. Felde, J. Buscher, D. Rysewyk Cantu, Jenni Adams, P. Peiffer, Joshua Hignight, Timo Sturwald, H. Schieler, Kirill Filimonov, K. Wiebe, Steven Robertson, R. G. Stokstad, Segev BenZvi, Shefali Shefali, Spencer Klein, Abdul Rehman, Carsten Rott, Kara Hoffman, Javier Gonzalez, Roxanne Turcotte, Giorgio Maggi, Matthias Vraeghe, C. De Clercq, Hershal Pandya, Wolfgang Rhode, David A. Williams, Xianwu Xu, Robert Stein, J. Sandroos, Markus Ackermann, S. W. Barwick, C. Bohm, J. Kim, Daniel Bindig, K. D. de Vries, N. Kulacz, Brian Clark, Chad Finley, Christoph Tönnis, Pranav Dave, M. Günder, T. Stezelberger, G. H. Collin, Sarah Mancina, Anna Franckowiak, Tobias Hoinka, Kayla Leonard, Steve Sclafani, Jan Soedingrekso, Francis Halzen, J. Kiryluk, K. Andeen, I. Ansseau, G. Krückl, Juliana Stachurska, Alejandro Diaz, Pablo Correa, H. Dembinski, M. Kauer, Suyong Choi, David Kappesser, R. Hellauer, Matti Jansson, T. Palczewski, Sebastian Böser, Benjamin Bastian, Anastasia Maria Barbano, T. Kittler, B. Eberhardt, M. E. Huber, Marcos Santander, L. Gerhardt, A. Olivas, M. J. Larson, Wing Yan Ma, James DeLaunay, Marjon Moulai, J. J. Beatty, Tianlu Yuan, F. McNally, A. Stößl, Reina H. Maruyama, Summer Blot, F. Jonske, L. Schumacher, F. Huang, Mehmet Gunduz, Agnieszka Leszczyńska, R. C. Bay, Austin Schneider, Juan Carlos Diaz-Velez, Glenn Spiczak, G. Momenté, M. Rameez, D. F. Cowen, U. Naumann, E. Unger, A. O'Murchadha, Max Renschler, D. J. Koskinen, E. Bourbeau, Spencer Griswold, Maria Tselengidou, D. Soldin, J. Stettner, Mirco Hunnefeld, Marie Oehler, N. van Eijndhoven, Physics, Faculty of Sciences and Bioengineering Sciences, Vriendenkring VUB, and Elementary Particle Physics
Subjects: 010504 meteorology & atmospheric sciences, High-energy astronomy, Astrophysics::High Energy Astrophysical Phenomena, Neutrino astronomy, High energy astrophysics, FOS: Physical sciences, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, Pulsar, 0103 physical sciences, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Astronomy and Astrophysics, Galactic plane, COSMIC-RAYS, CRAB-NEBULA, Crab Nebula, Physics and Astronomy, 13. Climate action, Space and Planetary Science, GALACTIC SOURCES, DISCOVERY, Physique des particules élémentaires, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, GAMMA-RAY EMISSION, Lepton
Abstract: Pulsar wind nebulae (PWNe) are the main gamma-ray emitters in the Galactic plane. They are diffuse nebulae that emit nonthermal radiation. Pulsar winds, relativistic magnetized outflows from the central star, shocked in the ambient medium produce a multiwavelength emission from the radio through gamma-rays. Although the leptonic scenario is able to explain most PWNe emission, a hadronic contribution cannot be excluded. A possible hadronic contribution to the high-energy gamma-ray emission inevitably leads to the production of neutrinos. Using 9.5 yr of all-sky IceCube data, we report results from a stacking analysis to search for neutrino emission from 35 PWNe that are high-energy gamma-ray emitters. In the absence of any significant correlation, we set upper limits on the total neutrino emission from those PWNe and constraints on hadronic spectral components., SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2020
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42. A quantum enhanced search for dark matter axions

Author: K M, Backes, D A, Palken, S Al, Kenany, B M, Brubaker, S B, Cahn, A, Droster, Gene C, Hilton, Sumita, Ghosh, H, Jackson, S K, Lamoreaux, A F, Leder, K W, Lehnert, S M, Lewis, M, Malnou, R H, Maruyama, N M, Rapidis, M, Simanovskaia, Sukhman, Singh, D H, Speller, I, Urdinaran, Leila R, Vale, E C, van Assendelft, K, van Bibber, and H, Wang
Abstract: The manipulation of quantum states of light
Published: 2020

43. Improved Limit on Neutrinoless Double-Beta Decay in Te130 with CUORE

Author: Yudi Ma, Massimiliano Clemenza, C. Pagliarone, Carlo Cosmelli, B. S. Wang, Silvia Capelli, Massimiliano Nastasi, S. Pirro, N. Chott, C. Brofferio, C. Rosenfeld, V. Novati, Davide Chiesa, A. Caminata, L. Ma, V. Dompè, Ezio Previtali, Marco Pallavicini, A. D'Addabbo, P. Gorla, F. Ferroni, C. Tomei, James R. Wilson, B. Welliver, K. Wilson, Emanuele Ferri, Carlo Ligi, A. Campani, R. G. Huang, I. Nutini, D. Q. Adams, I. Dafinei, M. Sakai, Jonathan Ouellet, G. Bari, K. Alfonso, Giovanni Benato, N. D. Scielzo, C. Nones, E. Fiorini, C. Bucci, Lucia Canonica, S. Di Domizio, A. Puiu, T. D. Gutierrez, C. Rusconi, M. Faverzani, Deqing Fang, C. J. Davis, Laura Cardani, B. K. Fujikawa, L. Zanotti, F. Bellini, S. Morganti, Stefano Dell'Oro, A. Branca, L. Marini, M. Vignati, S. L. Wagaarachchi, S. Pozzi, J. Johnston, L. Pattavina, A. Giachero, V. Sharma, R. J. Creswick, L. Cappelli, B. Schmidt, T. Napolitano, G. Pessina, N. Moggi, A. Giuliani, Stefano Zucchelli, O. Azzolini, M. Biassoni, V. Pettinacci, Samuele Sangiorgio, A. Nucciotti, M. Sisti, S. Copello, C. Alduino, G. Fantini, S. Zimmermann, D. D'Aguanno, L. Pagnanini, L. Gironi, F. T. Avignone, Paolo Carniti, M. A. Franceschi, Eric B. Norman, M. Pavan, J. Nikkel, P. T. Surukuchi, Lindley Winslow, T. O'Donnell, F. Terranova, H. Z. Huang, Y. Mei, Xiangyu Cao, G. Keppel, Oliviero Cremonesi, K. M. Heeger, Ke Han, Reina H. Maruyama, Stuart J. Freedman, N. Casali, Yu. G. Kolomensky, Claudio Gotti, C. Pira, L. Taffarello, Virendra Singh, and Danielle Speller
Subjects: Physics, Semileptonic decay, Particle physics, General Physics and Astronomy, 01 natural sciences, Lower limit, MAJORANA, CUORE, Double beta decay, 0103 physical sciences, Limit (mathematics), Sensitivity (control systems), Neutrino, 010306 general physics
Abstract: We report new results from the search for neutrinoless double-beta decay in ^{130} Te with the CUORE detector. This search benefits from a fourfold increase in exposure, lower trigger thresholds, and analysis improvements relative to our previous results. We observe a background of (1.38±0.07)×10^{-2} counts/(keV kg yr)) in the 0νββ decay region of interest and, with a total exposure of 372.5 kg yr, we attain a median exclusion sensitivity of 1.7×10^{25} yr. We find no evidence for 0νββ decay and set a 90% credibility interval Bayesian lower limit of 3.2×10^{25} yr on the ^{130} Te half-life for this process. In the hypothesis that 0νββ decay is mediated by light Majorana neutrinos, this results in an upper limit on the effective Majorana mass of 75-350 meV, depending on the nuclear matrix elements used.
Published: 2020
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44. LeptonInjector and LeptonWeighter: A neutrino event generator and weighter for neutrino observatories

Author: Janet Conrad, R. Cross, D. Hebecker, William Luszczak, K.-H. Becker, Yiqian Xu, Matt Dunkman, Ioana Codrina Maris, Thomas Stuttard, Christian Spiering, Thomas Ehrhardt, Sarah Pieper, A. Kyriacou, Ken'ichi Kin, Christoph Raab, Nadège Iovine, Dirk Ryckbosch, S. De Ridder, Stephan Meighen-Berger, D. Berley, G. C. Hill, Bunheng Ty, Paul Coppin, Justin Vandenbroucke, Andrea Turcati, J. Becker Tjus, J. J. Beatty, Christian Haack, Tianlu Yuan, M. J. Larson, Ralph Engel, Moritz Kellermann, F. McNally, Wing Yan Ma, Emma C. Hettinger, Reina H. Maruyama, A. Obertacke Pollmann, Summer Blot, Frank G. Schröder, U. Katz, Giovanni Renzi, Damian Pieloth, Ali Kheirandish, T. Gregoire, James DeLaunay, Marjon Moulai, S. Fahey, M. Kauer, Tyce DeYoung, Abhishek Desai, J. Werthebach, D. B. Fox, J. van Santen, J. L. Kelley, Markus Ahlers, Suyong Choi, Alex Pizzuto, Jannes Brostean-Kaiser, Nathan Whitehorn, Immacolata Carmen Rea, David Kappesser, Jan Soedingrekso, Brandom Pries, L. Schumacher, Maximilian Karl Scharf, S. C. Nowicki, Gary Binder, Karl J. Clark, D. van Eijk, Shefali Shefali, P. B. Price, Matti Jansson, A. Franckowiak, Hermann Kolanoski, M. U. Nisa, Mehmet Gunduz, Agnieszka Leszczyńska, R. C. Bay, Abdul Rehman, Francesco Lucarelli, Carsten Rott, Chujie Chen, Austin Schneider, George Japaridze, Juan Carlos Diaz-Velez, Roger Moore, L. Köpke, Mark Weyrauch, Stef Verpoest, Aaron Fienberg, Timo Karg, D. Tosi, Y. L. Li, Amirreza Raissi, T. O. B. Schmidt, Paras Koundal, Mike Richman, N. van Eijndhoven, Erik Ganster, Y. Makino, P. Peiffer, Johan Wulff, A. Weindl, Segev BenZvi, Elisa Lohfink, Timothyblake Watson, J. Bourbeau, Nora Valtonen-Mattila, Michael Kovacevich, M. E. Huber, Spencer Klein, Javier Gonzalez, Roxanne Turcotte, Maryon Ahrens, Samvel Ter-Antonyan, Kurt Woschnagg, Marcos Santander, Richard Naab, S. Tilav, Daria Pankova, L. Gerhardt, G. Krückl, Konstancja Satalecka, A. Olivas, Alexander Fritz, D. Z. Besson, Stephanie Bron, E. Friedman, Paul Evenson, Frederik Tenholt, R. Nagai, C. De Clercq, C. Lagunas Gualda, Y. Popovych, C. J. Lozano Mariscal, C. Weaver, Martin Rongen, Theo Glauch, Alejandro Diaz, Michael DuVernois, Seongjin In, Elisa Resconi, Alessio Porcelli, H. Dujmovic, Matthias Vraeghe, Rasha Abbasi, B. J. Whelan, Kara Hoffman, J. Kim, G. W. Sullivan, James E. Braun, T. Kintscher, Simone Garrappa, Xianwu Xu, J. Sandroos, Dmitry Chirkin, Alexander Kappes, K. Rawlins, J. P. Yanez, G. H. Collin, J. Evans, Alan Coleman, David A. Williams, Markus Ackermann, S. W. Barwick, Philipp Furst, Zhedong Zhang, Ava Ghadimi, F. Huang, Emily Dvorak, Hershal Pandya, Frederik Hermann Lauber, R. S. Busse, Surujhdeo Seunarine, R. Snihur, K. Tollefson, E. O'Sullivan, R. Morse, Jakob Bottcher, T. Montaruli, Jan Weldert, Wolfgang Rhode, Robert Stein, Alexander Trettin, N. Kurahashi, Christopher Wiebusch, Kunal Deoskar, Juanan Aguilar, L. Halve, Franziska Tischbein, Justin Lanfranchi, M. Ha Minh, C. Wendt, P. Mallik, M. Stamatikos, K. Meagher, C. Pérez de los Heros, Gerald Przybylski, A. Karle, James Madsen, Chad Finley, Daniel Bindig, R. Halliday, B. J. P. Jones, G. de Wasseige, A. Wallace, Kayla Leonard, Ben Smithers, P. Eller, Simeon Reusch, Lu Lu, T. Anderson, J. C. Gallagher, A. Sharma, Sukeerthi Dharani, Christoph Tönnis, R. Hoffmann, John Hardin, Jean Pierre Twagirayezu, A. Ishihara, Tim Ruhe, A. Haungs, Rui An, Nahee Park, A. Ludwig, Francis Halzen, J. Merz, D. Rysewyk Cantu, C. Walck, Elisa Bernardini, Gerrit Wrede, T. Stanev, K. Hultqvist, Benedikt Riedel, D. Seckel, K. Mase, Andres Medina, Darren Grant, Benjamin Hokanson-Fasig, I. Ansseau, D. Mockler, Thomas Huber, Thomas K. Gaisser, Chiara Bellenghi, Yang Lyu, T. Glüsenkamp, Grant Parker, Jenni Adams, M. Meier, Michael Campana, H. Niederhausen, H. Schieler, Ek Narayan Paudel, Allan Hallgren, Colin Turley, Saskia Philippen, Juliana Stachurska, H. Dembinski, K. Helbing, A. Steuer, Kendall Mahn, A. Goldschmidt, Alexander A. Harnisch, Kirill Filimonov, Kael Hanson, Spencer Axani, Christian Glaser, K. Wiebe, Barbara Skrzypek, S. E. Sanchez Herrera, Stephen L. Hauser, M. J. Weiss, R. G. Stokstad, Lenka Tomankova, Carlos Arguelles, Jessie Micallef, Jannis Necker, Raamis Hussain, D. Kang, M. Silva, I. Taboada, Najia Moureen Binte Amin, Federica Bradascio, Alexander Burgman, J. P. Lazar, Michael O. Wolf, M. Prado Rodriguez, Clara E. Hill, S. Kopper, Paolo Desiati, K. D. de Vries, S. Hickford, I. Safa, Pranav Dave, René Reimann, Merlin Schaufel, Minjin Jeong, Leander Fischer, Qinrui Liu, R. Joppe, Martina Karl, Jochen M. Schneider, Srubabati Goswami, M. A. Unland Elorrieta, Sebastian Baur, Sebastian Fiedlschuster, D. R. Nygren, Marek Kowalski, Olga Botner, V. Baum, T. Stezelberger, S. Yoshida, Won Nam Kang, Sarah Mancina, X. Bai, Tobias Hoinka, Vedant Basu, Steve Sclafani, J. Kiryluk, K. Andeen, A.A. Alves, Alexander Sandrock, Pablo Correa, B. A. Clark, P. Schlunder, Sebastian Böser, Benjamin Bastian, Anastasia Maria Barbano, Gisela Anton, Max Renschler, Chunfai Tung, D. J. Koskinen, S. Robertson, E. Bourbeau, Joshua Hignight, Spencer Griswold, Maria Tselengidou, D. Soldin, Ramesh Koirala, E. Blaufuss, L. Classen, K. Hoshina, Glenn Spiczak, G. Momenté, M. Rameez, D. F. Cowen, U. Naumann, David Vannerom, Le Viet Nguyen, K. Krings, J. Stettner, M. Plum, Gerrit Roellinghoff, Mirco Hunnefeld, Marie Oehler, Z. Griffith, Xinyue Kang, Claudio Kopper, Subir Sarkar, Felix Henningsen, A. R. Fazely, Simona Toscano, C. Alispach, Physics, Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, and Vriendenkring VUB
Subjects: Particle physics, Physics::Instrumentation and Detectors, Computer science, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, General Physics and Astronomy, CHERENKOV LIGHT YIELD, Weighting, 01 natural sciences, High Energy Physics - Experiment, 010305 fluids & plasmas, Standard Model, High Energy Physics - Experiment (hep-ex), Neutrino interaction, High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, 010306 general physics, Cherenkov radiation, Event generator, Neutrino generator, Neutrino simulation, Generator (computer programming), hep-ex, Event (computing), ICE, High Energy Physics::Phenomenology, Detector, hep-ph, Computational Physics (physics.comp-ph), Quantitative Biology::Genomics, High Energy Physics - Phenomenology, physics.comp-ph, Hardware and Architecture, High Energy Physics::Experiment, Neutrino, Physics - Computational Physics, Lepton
Abstract: We present a high-energy neutrino event generator, called LeptonInjector, alongside an event weighter, called LeptonWeighter. Both are designed for large-volume Cherenkov neutrino telescopes such as IceCube. The neutrino event generator allows for quick and flexible simulation of neutrino events within and around the detector volume, and implements the leading Standard Model neutrino interaction processes relevant for neutrino observatories: neutrino-nucleon deep-inelastic scattering and neutrino-electron annihilation. In this paper, we discuss the event generation algorithm, the weighting algorithm, and the main functions of the publicly available code, with examples., Comment: 28 pages, 10 figures, 3 tables
Published: 2021
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45. The IceCube realtime alert system

Author: B. J. P. Jones, Chris Wendt, S. Hickford, D. Tosi, M. Day, R. Konietz, M. Vehring, S. Coenders, Joshua Hignight, Francis Halzen, Karim Ghorbani, S. Seunarine, G. Merino, Spencer Axani, I. Ansseau, N. Wandkowsky, S. Schoenen, J. Kiryluk, M. Wolf, F. Bos, A. Terliuk, Sally Robertson, G. Krückl, Carlos Arguelles, M. Song, T. L. Carver, Mike Richman, H. Dembinski, Sebastian Böser, D. Heereman, P. Schlunder, R. Nahnhauer, M. Lesiak-Bzdak, Gisela Anton, V. di Lorenzo, Allan Hallgren, J. Tatar, M. J. Larson, Jae Yool Kim, M. Kauer, L. Classen, Kurt Woschnagg, T. Menne, Paul Evenson, L. Brayeur, C. Finley, Juanan Aguilar, Jenni Adams, Hrvoje Dujmovic, Janet Conrad, B. Relethford, Ignacio Taboada, A. Obertacke Pollmann, K. Rawlins, M. G. Aartsen, Michael Sutherland, K. Mase, T. Kittler, S. Flis, P. Peiffer, R. Cross, K. D. de Vries, George Japaridze, S. De Ridder, Dirk Lennarz, Konstancja Satalecka, Theo Glauch, M. Rongen, Gabriel Collin, Dmitry Chirkin, A. Franckowiak, D. Z. Besson, Marjon Moulai, James Madsen, Lu Lu, R. Maunu, E. Friedman, Alexander Kappes, R. G. Stokstad, Markus Ahlers, J. Kunnen, Jay Gallagher, T. Ehrhardt, N. van Eijndhoven, M. N. Tobin, A. Meli, C.-C. Fösig, M. van Rossem, M. Vraeghe, C. Haack, K. Meagher, Elisa Resconi, A. Steuer, Teresa Montaruli, M. J. Weiss, N. Kurahashi, B. J. Whelan, Todor Stanev, R. Hellauer, D. Bose, Kendall Mahn, N. L. Strotjohann, J. P. Dumm, M. Relich, A. Olivas, K. Helbing, T. Palczewski, H. Pandya, M. Bissok, K. Jero, A. Wallace, R. Reimann, E. Vogel, Maryon Ahrens, U. Katz, J. C. Díaz-Vélez, S. Kopper, E. Woolsey, G. Binder, Joshua Pepper, H. Niederhausen, Dawn Williams, F. Huang, M. Leuermann, G. de Wasseige, A. Turcati, U. Naumann, E. Hansen, M. E. Huber, B. Eberhardt, M. S. Kim, Samvel Ter-Antonyan, Aya Ishihara, D. Bindig, E. Jacobi, Elisa Bernardini, Segev BenZvi, G. Maggi, T. Schmidt, L. Wille, Y. Xu, J. Lünemann, M. Kowalski, S. E. Sanchez Herrera, Azadeh Keivani, Frederik Tenholt, M. Rameez, M. Medici, L. Gerhardt, D. F. Cowen, Albrecht Karle, S. Euler, T. Fuchs, T. Karg, Ch. Weaver, Alexander Burgman, W. Kang, Z. Griffith, S. Miarecki, J. van Santen, Kael Hanson, Thomas Meures, K. Krings, K. Clark, D. V. Pankova, F. McNally, G. W. Sullivan, M. Casier, B. Riedel, D. R. Nygren, S. Bron, Steven W. Barwick, M. Tselengidou, Thomas K. Gaisser, G. B. Yodh, Spencer Klein, A. Stasik, Stijn Vanheule, Philipp Eller, Maximilian Meier, T. Ruhe, S. Wickmann, J. Auffenberg, D. Hebecker, Paolo Desiati, A. Sandrock, T. Glüsenkamp, Gerald Przybylski, Minjin Jeong, G. Neer, T. Kintscher, Hermann Kolanoski, M. Labare, M. Quinnan, M. Dunkman, J. Felde, H. Taavola, Stijn Blot, Christian Spiering, S. Yoshida, Xinhua Bai, T. Hansmann, R. Hoffmann, Javier Gonzalez, M. Mandelartz, E. Blaufuss, Kara Hoffman, E. Pinat, Olga Botner, K. Wiebe, P. B. Price, V. Baum, D. J. Koskinen, D. Ryckbosch, Simona Toscano, M. Voge, Markus Ackermann, Donglian Xu, J. Becker Tjus, Ö. Penek, D. Soldin, L. Rädel, J. Stettner, Justin Vandenbroucke, K. Hoshina, E. del Pino Rosendo, Subir Sarkar, Glenn Spiczak, S. Schöneberg, K. H. Becker, E. Unger, D. Berley, W. Giang, J. L. Lanfranchi, Wolfgang Rhode, J. L. Kelley, S. In, S. C. Nowicki, L. Gladstone, R. Koirala, Darren Grant, J. P. A. M. de André, C. Walck, Sarah Mancina, Frederik Hermann Lauber, M. Börner, Klas Hultqvist, M. Zoll, K. Andeen, S. Westerhoff, A. Christov, M. Wallraff, T. Stezelberger, E. Cheung, M. Usner, L. Sabbatini, B. Eichmann, H.-P. Bretz, S. Tilav, Christian Bohm, Aongus O'Murchadha, J. P. Yanez, Christoph Raab, G. C. Hill, L. Schumacher, C. Krüger, A. Goldschmidt, R. C. Bay, D. Seckel, S. Fahey, S. Kunwar, M. Archinger, A. R. Fazely, Tyce DeYoung, P. A. Toale, M. Kroll, C. Kopper, J. Braun, T. R. Wood, J. J. Beatty, A. Bernhard, D. Rysewyk, A. Stößl, Reina H. Maruyama, Christopher Wiebusch, J. Feintzeig, Carsten Rott, Xianwu Xu, J. Sandroos, D. Altmann, C. Pérez de los Heros, R. Ström, T. Kuwabara, L. Wills, Damian Pieloth, Ali Kheirandish, L. Köpke, G. Kohnen, T. Anderson, C. De Clercq, G. Tešić, Kirill Filimonov, Physics, Elementary Particle Physics, Faculty of Sciences and Bioengineering Sciences, and Vriendenkring VUB
Subjects: HIGH-ENERGY NEUTRINOS, TELESCOPE, Astrophysics::High Energy Astrophysical Phenomena, Multi-messenger astronomy, Neutrino astronomy, Neutrino detectors, Transient sources, Astronomy and Astrophysics, pole, FOS: Physical sciences, 01 natural sciences, IceCube, law.invention, IceCube Neutrino Observatory, Telescope, SEARCHES, CORE-COLLAPSE SUPERNOVAE, law, Observatory, 0103 physical sciences, site, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, background, Event (computing), Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, PERFORMANCE, sensitivity, observatory, Identification (information), electromagnetic, Physics and Astronomy, Neutrino detector, ddc:540, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, FOLLOW-UP
Abstract: Following the detection of high-energy astrophysical neutrinos in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the IceCube neutrino observatory. Several analyses selecting neutrinos of astrophysical origin are now operating in realtime at the detector site in Antarctica and are producing alerts to the community to enable rapid follow-up observations. The goal of these observations is to locate the astrophysical objects responsible for these neutrino signals. This paper highlights the infrastructure in place both at the South Pole detector site and at IceCube facilities in the north that have enabled this fast follow-up program to be developed. Additionally, this paper presents the first realtime analyses to be activated within this framework, highlights their sensitivities to astrophysical neutrinos and background event rates, and presents an outlook for future discoveries., Comment: 33 pages, 9 figures, Published in Astroparticle Physics
Published: 2017
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46. A quantum-enhanced search for dark matter axions

Author: S. Al Kenany, A. Leder, Alex Droster, Sumita Ghosh, Sukhman Singh, Nicholas M. Rapidis, Samantha M. Lewis, Leila R. Vale, Gene C. Hilton, H. E. Jackson, Danielle Speller, B. M. Brubaker, Daniel Palken, Steve K. Lamoreaux, Maria Simanovskaia, E. C. van Assendelft, I. Urdinaran, Konrad Lehnert, K. van Bibber, Reina H. Maruyama, Maxime Malnou, Sidney Cahn, K. M. Backes, and Hang Wang
Subjects: Physics, Particle physics, Quantum Physics, Multidisciplinary, Uncertainty principle, 010308 nuclear & particles physics, Quantum limit, Dark matter, FOS: Physical sciences, Observable, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Quantum state, 0103 physical sciences, 010306 general physics, Quantum Physics (quant-ph), Quantum, Axion, Squeezed coherent state
Abstract: In dark matter axion searches, quantum uncertainty manifests as a fundamental noise source, limiting the measurement of the quadrature observables used for detection. We use vacuum squeezing to circumvent the quantum limit in a search for a new particle. By preparing a microwave-frequency electromagnetic field in a squeezed state and near-noiselessly reading out only the squeezed quadrature, we double the search rate for axions over a mass range favored by recent theoretical projections. We observe no signature of dark matter axions in the combined $16.96-17.12$ and $17.14-17.28\space\mu\text{eV}/c^2$ mass window for axion-photon couplings above $g_{\gamma} = 1.38\times g_{\gamma}^\text{KSVZ}$, reporting exclusion at the 90% level., Comment: 7 pages, 4 figures
Published: 2020
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47. Perspectives of lowering CUORE thresholds with Optimum Trigger

Author: Monica Sisti, A. Bersani, C. Brofferio, G. Fantini, A. Caminata, Marco Pallavicini, B. Welliver, C. Pagliarone, R. G. Huang, M. Faverzani, Y. u. G. Kolomensky, H. Z. Huang, G. Keppel, Massimiliano Nastasi, Yudi Ma, S. Pozzi, S. L. Wagaarachchi, C. Cosmelli, A. Giuliani, C. Pira, C. Rusconi, Ke Han, A. Branca, N. D. Scielzo, Reina H. Maruyama, N. Casali, Stefano Dell'Oro, Lucia Canonica, F. Bellini, I. Dafinei, V. Novati, T. Wise, V. Pettinacci, Davide Chiesa, Stefano Zucchelli, Laura Cardani, L. Gironi, M. Pavan, B. K. Fujikawa, Y. Mei, V. Singh, D. D'Aguanno, F. T. Avignone, L. Taffarello, R. J. Creswick, C. Rosenfeld, P. Gorla, Danielle Speller, F. Ferroni, C. Tomei, M. Vignati, E. Previtali, Simone Capelli, D. Q. Adams, L. Marini, C. J. Davis, K. Alfonso, T. O'Donnell, B. Schmidt, N. Chott, C. Nones, A. Puiu, Lindley Winslow, S. Zimmermann, Oliviero Cremonesi, J. Johnston, L. Pattavina, Irene Nutini, S. Copello, C. Bucci, Miriam Lucio Martinez, Paolo Carniti, Sergio Di Domizio, S. Pirro, Xi-Guang Cao, E. Fiorini, S. J. Freedman, K. M. Heeger, Luigi Cappelli, T. D. Gutierrez, F. Terranova, K. Wilson, G. Pessina, B. S. Wang, Jonathan Ouellet, G. Bari, O. Azzolini, Evelyn Ferri, N. Moggi, Samuele Sangiorgio, A. Nucciotti, C. Alduino, Jeremy S. Cushman, S. Morganti, L. Zanotti, Carlo Ligi, A. Campani, V. Dompè, A. D'Addabbo, A. Leder, J. S. Wilson, Franceschi, Eric B. Norman, M. Sakai, T. Napolitano, M. Biassoni, Giovanni Benato, A. Drobizhev, C. Gotti, A. Giachero, D. Q. Fang, Massimiliano Clemenza, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), 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 de Recherches sur les lois Fondamentales de l'Univers (IRFU), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Subjects: Physics, History, CUORE, 010308 nuclear & particles physics, Physics::Instrumentation and Detectors, WIMP nucleus: scattering, trigger: programming, 01 natural sciences, Large target, tellurium: oxygen, Computer Science Applications, Education, Combinatorics, energy: threshold, Low energy, double-beta decay: (0neutrino), 0103 physical sciences, High Energy Physics::Experiment, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, activity report, energy: low
Abstract: Author(s): Dompe, V; Adams, DQ; Alduino, C; Alfonso, K; Avignone, FT; Azzolini, O; Bari, G; Bellini, F; Benato, G; Bersani, A; Biassoni, M; Branca, A; Brofferio, C; Bucci, C; Caminata, A; Campani, A; Canonica, L; Cao, XG; Capelli, S; Cappelli, L; Cardani, L; Carniti, P; Casali, N; Chiesa, D; Chott, N; Clemenza, M; Copello, S; Cosmelli, C; Cremonesi, O; Creswick, RJ; Cushman, JS; D'Addabbo, A; D'Aguanno, D; Dafinei, I; Davis, CJ; Dell'Oro, S; Domizio, SD; Drobizhev, A; Fang, DQ; Fantini, G; Faverzani, M; Ferri, E; Ferroni, F; Fiorini, E; Franceschi, MA; Freedman, SJ; Fujikawa, BK; Giachero, A; Gironi, L; Giuliani, A; Gorla, P; Gotti, C; Gutierrez, TD; Han, K; Heeger, KM; Huang, RG; Huang, HZ; Johnston, J; Keppel, G; Kolomensky, YG; Leder, A; Ligi, C; Ma, YG; Marini, L; Martinez, M; Maruyama, RH; Mei, Y; Moggi, N; Morganti, S; Napolitano, T; Nastasi, M; Nones, C; Norman, EB; Novati, V; Nucciotti, A; Nutini, I; O'Donnell, T; Ouellet, JL; Pagliarone, CE; Pallavicini, M; Pattavina, L; Pavan, M; Pessina, G; Pettinacci, V; Pira, C | Abstract: CUORE is a cryogenic experiment that focuses on the search of neutrinoless double beta decay in 130Te and it is located at the Gran Sasso National Laboratories. Its detector consists of 988 TeO2 crystals operating at a base temperature of ∼10 mK. It is the first ton-scale bolometric experiment ever realized for this purpose. Thanks to its large target mass and ultra-low background, the CUORE detector is also suitable for the search of other rare phenomena. In particular the low energy part of the spectra is interesting for the detection of WIMP-nuclei scattering reactions. One of the most important requirements to perform these studies is represented by the achievement of a stable energy threshold lower than 10 keV. Here, the CUORE capability to accomplish this purpose using a low energy software trigger will be presented and described.
Published: 2020
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48. A search for time-dependent astrophysical neutrino emission with IceCube data from 2012 to 2017

Author: Alexander Trettin, J. C. Gallagher, Gerrit Wrede, Federica Bradascio, S. Tilav, K. Rawlins, Alexander Burgman, C. J. Lozano Mariscal, K. Helbing, Thomas Huber, Ek Narayan Paudel, Allan Hallgren, J. P. Yanez, H. Dujmovic, D. Tosi, James Madsen, Lu Lu, P. Schlunder, Rasha Abbasi, B. J. Whelan, Won Nam Kang, D. Kang, Elisa Lohfink, X. Bai, I. Safa, A. Wallace, Surujhdeo Seunarine, R. Snihur, Juanan Aguilar, I. Taboada, Michael DuVernois, P. B. Price, Francesco Lucarelli, Merlin Schaufel, Michael O. Wolf, T. O. B. Schmidt, Sarah Mancina, Minjin Jeong, T. Glüsenkamp, Kurt Woschnagg, Simon Hauser, Paul Evenson, K. D. de Vries, Simone Garrappa, M. Meier, David Vannerom, Michael Campana, Dmitry Chirkin, Gerald Przybylski, Alexander Kappes, Jan Weldert, L. Halve, M. Ha Minh, Tobias Hoinka, R. Halliday, Antonio Augusto Alves Jr., A. Ishihara, K. Tollefson, A. Desai, Vedant Basu, Steve Sclafani, M. Stamatikos, B. J. P. Jones, Thomas Ehrhardt, J. Kiryluk, Alexander Sandrock, Kendall Mahn, Gisela Anton, Karl J. Clark, K. Andeen, Christian Haack, C. Pérez de los Heros, Jan Soedingrekso, Frank G. Schröder, Paras Koundal, Mike Richman, Andres Medina, Z. Griffith, A. Goldschmidt, George Japaridze, Saskia Philippen, Pablo Correa, D. Mockler, Simeon Reusch, Michael Kovacevich, Roger Moore, S. Yoshida, B. A. Clark, G. Krückl, Benjamin Hokanson-Fasig, D. Rysewyk Cantu, A. Obertacke Pollmann, U. Katz, K. Hoshina, D. Hebecker, J. Bourbeau, D. R. Nygren, Yang Lyu, Richard Naab, Grant Parker, Lenka Tomankova, Alejandro Diaz, N. van Eijndhoven, D. F. Cowen, Glenn Spiczak, Marek Kowalski, J. L. Kelley, Markus Ahlers, Spencer Axani, Aaron Fienberg, Daria Pankova, E. Friedman, M. Silva, Seongjin In, Elisa Resconi, Alessio Porcelli, E. O'Sullivan, Lisa Johanna Schumacher, Najia Moureen Binte Amin, C. Alispach, Amirreza Raissi, Janet Conrad, Stephanie Bron, Felix Henningsen, M. J. Larson, Le Viet Nguyen, Emily Dvorak, G. Momenté, M. Rameez, M. Prado Rodriguez, Pranav Dave, Carlos Arguelles, K. Wiebe, J. P. Lazar, Clara E. Hill, Erik Ganster, Shefali Shefali, Samvel Ter-Antonyan, A. Steuer, Chunfai Tung, D. B. Fox, Jessie Micallef, Chad Finley, Christoph Tönnis, Raamis Hussain, Abdul Rehman, Carsten Rott, Y. Popovych, K. Krings, Jenni Adams, K. Mase, Alexander A. Harnisch, S. Robertson, Joshua Hignight, R. Cross, Johannes Werthebach, Wing Yan Ma, James DeLaunay, Marjon Moulai, Simona Toscano, Benedikt Riedel, D. Seckel, M. Plum, Y. Makino, Alexander Fritz, D. Z. Besson, Javier Gonzalez, Roxanne Turcotte, M. J. Weiss, R. Morse, Jakob Bottcher, T. Montaruli, S. De Ridder, Xianwu Xu, J. Sandroos, Matthias Vraeghe, Christian Glaser, Brandom Pries, S. Hickford, Paul Coppin, Maximilian Karl Scharf, Xinyue Kang, Olga Botner, S. Kopper, J. Kim, René Reimann, Hermann Kolanoski, R. G. Stokstad, A. V. Balagopal, Andrea Turcati, J. Evans, C. De Clercq, Kael Hanson, U. Naumann, Claudio Kopper, A. Franckowiak, T. Stezelberger, Timo Karg, V. Baum, Leander Fischer, R. Joppe, Stef Verpoest, Jannis Necker, C. Lagunas Gualda, Chujie Chen, T. Gregoire, A. Weindl, Maryon Ahrens, Subir Sarkar, K. Meagher, William Luszczak, P. Peiffer, Daniel Bindig, G. H. Collin, Frederik Tenholt, R. Nagai, Johan Wulff, Timothyblake Watson, Paolo Desiati, C. Weaver, M. E. Huber, Sebastian Baur, Marcos Santander, Ramesh Koirala, Sebastian Fiedlschuster, Alan Coleman, David A. Williams, J. van Santen, J. Stettner, L. Gerhardt, A. Olivas, Konstancja Satalecka, E. Blaufuss, Alex Pizzuto, Markus Ackermann, Theo Glauch, S. W. Barwick, Elisa Bernardini, A. Kyriacou, L. Classen, Gary Binder, D. van Eijk, Sebastian Böser, F. Huang, Gerrit Roellinghoff, J. Becker Tjus, Mark Weyrauch, Kayla Leonard, Y. L. Li, Sukeerthi Dharani, Francis Halzen, J. Merz, Mirco Hunnefeld, Marie Oehler, I. Ansseau, Benjamin Bastian, Anastasia Maria Barbano, Juliana Stachurska, H. Dembinski, G. W. Sullivan, Max Renschler, James E. Braun, D. J. Koskinen, M. Kauer, Suyong Choi, E. Bourbeau, David Kappesser, Matti Jansson, N. Kurahashi, Spencer Griswold, Todor Stanev, C. Wendt, Maria Tselengidou, D. Soldin, Philipp Furst, Mehmet Gunduz, G. de Wasseige, R. Hoffmann, C. Walck, Thomas K. Gaisser, Agnieszka Leszczyńska, R. C. Bay, Tim Ruhe, Austin Schneider, A. Ludwig, H. Niederhausen, Juan Carlos Diaz-Velez, Ken'ichi Kin, J. J. Beatty, Tianlu Yuan, F. McNally, Emma C. Hettinger, Reina H. Maruyama, Summer Blot, Segev BenZvi, Spencer Klein, Kara Hoffman, Hershal Pandya, Wolfgang Rhode, Robert Stein, T. Anderson, John Hardin, Chiara Bellenghi, H. Schieler, Kirill Filimonov, Damian Pieloth, Ali Kheirandish, Jannes Brostean-Kaiser, Ben Smithers, M. U. Nisa, L. Köpke, Jean Pierre Twagirayezu, A. Haungs, Nahee Park, K. Hultqvist, Darren Grant, T. Kintscher, Frederik Hermann Lauber, Justin Lanfranchi, Christian Spiering, Justin Vandenbroucke, S. C. Nowicki, S. E. Sanchez Herrera, K.-H. Becker, Yiqian Xu, Matt Dunkman, Thomas Stuttard, Sarah Pieper, Dirk Ryckbosch, Stephan Meighen-Berger, Qinrui Liu, Martina Karl, Jochen M. Schneider, Srubabati Goswami, M. A. Unland Elorrieta, Martin Rongen, Zhedong Zhang, Ava Ghadimi, Franziska Tischbein, P. Mallik, P. Eller, Colin Turley, R. S. Busse, Christopher Wiebusch, Kunal Deoskar, A. Karle, Ioana Codrina Maris, Christoph Raab, Nadège Iovine, D. Berley, G. C. Hill, Bunheng Ty, Ralph Engel, Moritz Kellermann, Giovanni Renzi, S. Fahey, A. R. Fazely, Tyce DeYoung, Nathan Whitehorn, Immacolata Carmen Rea, Physics, Faculty of Sciences and Bioengineering Sciences, Elementary Particle Physics, and Vriendenkring VUB
Subjects: 010504 meteorology & atmospheric sciences, High-energy astronomy, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, model [emission], FOS: Physical sciences, Cosmic ray, Astrophysics, 01 natural sciences, law.invention, IceCube Neutrino Observatory, IceCube, blazar, law, emission [gamma ray], 0103 physical sciences, Cosmic ray sources, High-energy astrophysics, Particle astrophysics, energy: high [neutrino], Blazar, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, media_common, High Energy Astrophysical Phenomena (astro-ph.HE), astro-ph.HE, Astroparticle physics, Physics, background, Astronomy and Astrophysics, Universe, messenger, observatory, Space and Planetary Science, ddc:520, time dependence, acceleration [cosmic radiation], Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Flare
Abstract: High-energy neutrinos are unique messengers of the high-energy universe, tracing the processes of cosmic ray acceleration. This paper presents analyses focusing on time-dependent neutrino point-source searches. A scan of the whole sky, making no prior assumption about source candidates, is performed, looking for a space and time clustering of high-energy neutrinos in data collected by the IceCube Neutrino Observatory between 2012 and 2017. No statistically significant evidence for a time-dependent neutrino signal is found with this search during this period, as all results are consistent with the background expectation. Within this study period, the blazar 3C 279, showed strong variability, inducing a very prominent gamma-ray flare observed in 2015 June. This event motivated a dedicated study of the blazar, which consists of searching for a time-dependent neutrino signal correlated with the gamma-ray emission. No evidence for a time-dependent signal is found. Hence, an upper limit on the neutrino fluence is derived, allowing us to constrain a hadronic emission model.
Published: 2020
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49. Results from the CUORE experiment

Author: D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, and Zucchelli, S
Subjects: neutrinoless double beta decay
Published: 2020

50. Lowering the Energy Threshold of the CUORE Experiment: Benefits in the Surface Alpha Events Reconstruction: Comparison Between Optimum Trigger and Derivative Trigger Performance in the Search for 0 νββ

Author: L. Pattavina, Marco Pallavicini, L. Canonica, L. Marini, S. Di Domizio, C. Bucci, T. D. Gutierrez, G. Pessina, K. Wilson, Stefano Dell'Oro, Jonathan Ouellet, J. Johnston, G. Bari, Laura Cardani, L. Zanotti, J. Nikkel, L. Gironi, F. T. Avignone, H. Z. Huang, B. K. Fujikawa, G. Keppel, Stefano Pozzi, Y. G. Ma, Massimiliano Clemenza, Carlo Cosmelli, Davide Chiesa, C. Nones, A. Puiu, V. Pettinacci, S. Zucchelli, N. D. Scielzo, L. Pagnanini, C. Brofferio, T. O'Donnell, D. Q. Fang, Claudio Gotti, Ke Han, Reina H. Maruyama, M. Vignati, C. Rusconi, Stuart J. Freedman, D. D'Aguanno, Ettore Fiorini, V. Novati, James R. Wilson, Andrea Giachero, C. Rosenfeld, P. Gorla, F. Ferroni, C. Tomei, M. A. Franceschi, C. Pagliarone, D. Q. Adams, R. G. Huang, N. Casali, F. Terranova, Vasundhara Singh, K. Alfonso, C. J. Davis, Monica Sisti, B. Schmidt, Eric B. Norman, B. S. Wang, L. Ma, O. Azzolini, Y. Mei, Lindley Winslow, V. Sharma, T. Napolitano, S. Copello, I. Dafinei, M. Sakai, Paolo Carniti, Silvia Capelli, Xi-Guang Cao, Massimiliano Nastasi, K. M. Heeger, F. Bellini, S. Pirro, L. Cappelli, Oliviero Cremonesi, M. Biassoni, R. J. Creswick, G. Fantini, M. Pavan, V. Dompè, Giovanni Benato, A. D'Addabbo, C. Pira, A. Caminata, Ezio Previtali, S. Morganti, B. Welliver, Carlo Ligi, Evelyn Ferri, N. Moggi, Samuele Sangiorgio, A. Campani, A. Nucciotti, C. Alduino, M. Faverzani, Yu. G. Kolomensky, A. Branca, L. Taffarello, A. Giuliani, Danielle Speller, S. L. Wagaarachchi, N. Chott, Irene Nutini, S. Zimmermann, Campani, A, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Dell'Oro, S, Di Domizio, S, Dompe, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, Y, Ma, L, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, Campani A., Adams D.Q., Alduino C., Alfonso K., Avignone F.T., Azzolini O., Bari G., Bellini F., Benato G., Biassoni M., Branca A., Brofferio C., Bucci C., Caminata A., Canonica L., Cao X.G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R.J., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C.J., Dell'Oro S., Di Domizio S., Dompe V., Fang D.Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S.J., Fujikawa B.K., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gutierrez T.D., Han K., Heeger K.M., Huang R.G., Huang H.Z., Johnston J., Keppel G., Kolomensky Y.G., Ligi C., Ma Y.G., Ma L., Marini L., Maruyama R.H., Mei Y., Moggi N., Morganti S., Napolitano T., Nastasi M., Nikkel J., Nones C., Norman E.B., Novati V., Nucciotti A., Nutini I., O'Donnell T., Ouellet J.L., Pagliarone C.E., Pagnanini L., Pallavicini M., Pattavina L., Pavan M., Pessina G., Pettinacci V., Pira C., Pirro S., Pozzi S., Previtali E., Puiu A., Rosenfeld C., Rusconi C., Sakai M., Sangiorgio S., Schmidt B., Scielzo N.D., Sharma V., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S.L., Wang B.S., Welliver B., Wilson J., Wilson K., Winslow L.A., Zanotti L., Zimmermann S., and Zucchelli S.
Subjects: Particle physics, Bolometers for dark matter research, Physics::Instrumentation and Detectors, trigger algorithm, 01 natural sciences, Coincidence, law.invention, CUORE, WIMP, law, Double beta decay, 0103 physical sciences, General Materials Science, Neutrinoless double beta decay, 010306 general physics, Axion, Physics, 010308 nuclear & particles physics, Scattering, Bolometer, Astrophysics::Instrumentation and Methods for Astrophysics, Trigger algorithms, Condensed Matter Physics, Digital signal processing, Atomic and Molecular Physics, and Optics, Energy (signal processing)
Abstract: CUORE is a tonne-scale cryogenic experiment located at the Laboratori Nazionali del Gran Sasso that exploits bolometric technique to search for neutrinoless double beta decay of 130Te. Thanks to its very low background and large mass, CUORE is also a powerful tool to study a broad class of phenomena, such as solar axions and WIMP scattering. The ability to conduct such sensitive searches crucially depends on the energy threshold, which has to be kept as low as possible. In this contribution, we show how the trigger algorithm affects the sensitivity to low-energy phenomena and the interpretation of the energy spectrum. In particular, we focus on the impact that the trigger algorithm has on the identification of the coincidence events among different crystals and, consequently, on the reconstruction of the background.
Published: 2020

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