Author: "MacLellan R" - Searchworks@Jio Institute Digital Library Search Results

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291 results on '"MacLellan R"'

1. Imaging of single barium atoms in a second matrix site in solid xenon for barium tagging in a $^{136}$Xe double beta decay experiment

Author: Yvaine, M., Fairbank, D., Soderstrom, J., Taylor, C., Stanley, J., Walton, T., Chambers, C., Iverson, A., Fairbank, W., Kharusi, S. Al, Amy, A., Angelico, E., Anker, A., Arnquist, I. J., Atencio, A., Bane, J., Belov, V., Bernard, E. P., Bhatta, T., Bolotnikov, A., Breslin, J., Breur, P. A., Brodsky, J. P., Brown, E., Brunner, T., Caden, E., Cao, G. F., Cesmecioglu, D., Chambers, E., Chana, B., Chernyak, D., Chiu, M., Collister, R., Cvitan, M., Daniels, T., Darroch, L., DeVoe, R., di Vacri, M. L., Dolinski, M. J., Eckert, B., Elbeltagi, M., Elmansali, R., Fatemighomi, N., Foust, B., Fu, Y. S., Gallacher, D., Gallice, N., Giacomini, G., Gillis, W., Gingras, C., Gornea, R., Gratta, G., Hardy, C. A., Hedges, S., Hein, E., Holt, J. D., Hoppe, E. W., Karelin, A., Keblbeck, D., Kotov, I., Kuchenkov, A., Kumar, K. S., Kwiatkowski, A. A., Larson, A., Latif, M. B., Leach, K. G., Lennarz, A., Leonard, D. S., Lewis, H., Li, G., Li, Z., Licciardi, C., Lindsay, R., MacLellan, R., Majidi, S., Malbrunot, C., Masbou, J., McMichael, K., Peregrina, M. Medina, Moe, M., Mong, B., Moore, D. C., Natzke, C. R., Ngwadla, X. E., Ni, K., Nolan, A., Nowicki, S. C., Ondze, J. C. Nzobadila, Odian, A., Orrell, J. L., Ortega, G. S., Overman, C. T., Pagani, L., Smalley, H. Peltz, Perna, A., Pocar, A., Radeka, V., Raguzin, E., Rasiwala, H., Ray, D., Rescia, S., Richardson, G., Ross, R., Rowson, P. C., Saldanha, R., Sangiorgio, S., Schwartz, S., Sekula, S., Si, L., Soma, A. K., Spadoni, F., Stekhanov, V., Sun, X. L., Thibado, S., Tidball, A., Totev, T., Triambak, S., Tsang, T., Tyuka, O. A., van Bruggen, E., Vidal, M., Walent, M., Wamba, K., Wang, H. W., Wang, Q. D., Wang, W., Wang, Y. G., Watts, M., Wehrfritz, M., Wen, L. J., Wichoski, U., Wilde, S., Worcester, M., Xu, H., Yang, L., Yu, M., and Zeldovich, O.
Subjects: Physics - Atomic Physics, High Energy Physics - Experiment, Nuclear Experiment
Abstract: Neutrinoless double beta decay is one of the most sensitive probes for new physics beyond the Standard Model of particle physics. One of the isotopes under investigation is $^{136}$Xe, which would double beta decay into $^{136}$Ba. Detecting the single $^{136}$Ba daughter provides a sort of ultimate tool in the discrimination against backgrounds. Previous work demonstrated the ability to perform single atom imaging of Ba atoms in a single-vacancy site of a solid xenon matrix. In this paper, the effort to identify signal from individual barium atoms is extended to Ba atoms in a hexa-vacancy site in the matrix and is achieved despite increased photobleaching in this site. Abrupt fluorescence turn-off of a single Ba atom is also observed. Significant recovery of fluorescence signal lost through photobleaching is demonstrated upon annealing of Ba deposits in the Xe ice. Following annealing, it is observed that Ba atoms in the hexa-vacancy site exhibit antibleaching while Ba atoms in the tetra-vacancy site exhibit bleaching. This may be evidence for a matrix site transfer upon laser excitation. Our findings offer a path of continued research toward tagging of Ba daughters in all significant sites in solid xenon., Comment: 9 pages, 8 figures
Published: 2024

2. Supernova Electron-Neutrino Interactions with Xenon in the nEXO Detector

Author: nEXO Collaboration, Hedges, S., Kharusi, S. Al, Angelico, E., Brodsky, J. P., Richardson, G., Wilde, S., Amy, A., Anker, A., Arnquist, I. J., Arsenault, P., Atencio, A., Badhrees, I., Bane, J., Belov, V., Bernard, E. P., Bhatta, T., Bolotnikov, A., Breslin, J., Breur, P. A., Brown, E., Brunner, T., Caden, E., Cao, G. F., Cao, L. Q., Cesmecioglu, D., Chambers, E., Chana, B., Charlebois, S. A., Chernyak, D., Chiu, M., Collister, R., Cvitan, M., Dalmasson, J., Daniels, T., Darroch, L., DeVoe, R., di Vacri, M. L., Ding, Y. Y., Dolinski, M. J., Eckert, B., Elbeltagi, M., Elmansali, R., Fabris, L., Fairbank, W., Farine, J., Fatemighomi, N., Foust, B., Fu, Y. S., Gallacher, D., Gallice, N., Gillis, W., Goeldi, D., Gorham, A., Gornea, R., Gratta, G., Guan, Y. D., Hardy, C. A., Heffner, M., Hein, E., Holt, J. D., Hoppe, E. W., House, A., Hunt, W., Iverson, A., Kachru, P., Karelin, A., Keblbeck, D., Kuchenkov, A., Kumar, K. S., Larson, A., Latif, M. B., Leach, K. G., Lenardo, B. G., Leonard, D. S., Lewis, H., Li, G., Li, Z., Licciardi, C., Lindsay, R., MacLellan, R., Majidi, S., Malbrunot, C., Martel-Dion, P., Masbou, J., McMichael, K., Medina-Peregrina, M., Mong, B., Moore, D. C., Nattress, J., Natzke, C. R., Ngwadla, X. E., Ni, K., Nolan, A., Nowicki, S. C., Ondze, J. C. Nzobadila, Orrell, J. L., Ortega, G. S., Overman, C. T., Pagani, L., Smalley, H. Peltz, Perna, A., Piepke, A., Franco, T. Pinto, Pocar, A., Pratte, J. -F., Rasiwala, H., Ray, D., Raymond, K., Rescia, S., Riot, V., Ross, R., Saldanha, R., Sangiorgio, S., Schwartz, S., Sekula, S., Soderstrom, J., Soma, A. K., Spadoni, F., Sun, X. L., Thibado, S., Tidball, A., Totev, T., Triambak, S., Tsang, R. H. M., Tyuka, O. A., van Bruggen, E., Vidal, M., Viel, S., Walent, M., Wang, Q. D., Wang, W., Wang, Y. G., Watts, M., Wehrfritz, M., Wei, W., Wen, L. J., Wichoski, U., Wu, X. M., Xu, H., Yang, H. B., Yang, L., Yu, M., Yvaine, M., Zeldovich, O., and Zhao, J.
Subjects: High Energy Physics - Phenomenology, High Energy Physics - Experiment, Nuclear Theory
Abstract: Electron-neutrino charged-current interactions with xenon nuclei were modeled in the nEXO neutrinoless double-beta decay detector (~5-tonne, 90% ${}^{136}$Xe, 10% ${}^{134}$Xe) to evaluate its sensitivity to supernova neutrinos. Predictions for event rates and detectable signatures were modeled using the MARLEY event generator. We find good agreement between MARLEY's predictions and existing theoretical calculations of the inclusive cross sections at supernova neutrino energies. The interactions modeled by MARLEY were simulated within the nEXO simulation framework and were run through an example reconstruction algorithm to determine the detector's efficiency for reconstructing these events. The simulated data, incorporating the detector response, were used to study the ability of nEXO to reconstruct the incident electron-neutrino spectrum and these results were extended to a larger xenon detector of the same isotope enrichment. We estimate that nEXO will be able to observe electron-neutrino interactions with xenon from supernovae as far as 5 to 8 kpc from earth, while the ability to reconstruct incident electron-neutrino spectrum parameters from observed interactions in nEXO is limited to closer supernovae., Comment: 17 pages, 16 figures
Published: 2024

3. An integrated online radioassay data storage and analytics tool for nEXO

Author: Tsang, R. H. M., Piepke, A., Kharusi, S. Al, Angelico, E., Arnquist, I. J., Atencio, A., Badhrees, I., Bane, J., Belov, V., Bernard, E. P., Bhat, A., Bhatta, T., Bolotnikov, A., Breur, P. A., Brodsky, J. P., Brown, E., Brunner, T., Caden, E., Cao, G. F., Cao, L. Q., Cesmecioglu, D., Chambers, C., Chambers, E., Chana, B., Charlebois, S. A., Chernyak, D., Chiu, M., Cleveland, B., Cohen, J. R., Collister, R., Cvitan, M., Dalmasson, J., Darroch, L., Deslandes, K., DeVoe, R., di Vacri, M. L., Ding, Y. Y., Dolinski, M. J., Echevers, J., Eckert, B., Elbeltagi, M., Elmansali, R., Fabris, L., Fairbank, W., Farine, J., Fu, Y. S., Gallacher, D., Gallina, G., Gautam, P., Giacomini, G., Gillis, W., Gingras, C., Goeldi, D., Gornea, R., Gratta, G., Guan, Y. D., Hardy, C. A., Hedges, S., Heffner, M., Hein, E., Holt, J., Hoppe, E. W., House, A., Hunt, W., Iverson, A., Jamil, A., Jiang, X. S., Karelin, A., Kaufman, L. J., Kotov, I., Krücken, R., Kuchenkov, A., Kumar, K. S., Larson, A., Leach, K. G., Lenardo, B. G., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lindsay, R., MacLellan, R., Mahtab, M., Majidi, S., Malbrunot, C., Martel-Dion, P., Masbou, J., Massacret, N., McMichael, K., Mong, B., Moore, D. C., Murray, K., Nattress, J., Natzke, C. R., Ngwadla, X. E., Ni, K., Nolan, A., Nowicki, S. C., Ondze, J. C. Nzobadila, Orrell, J. L., Ortega, G. S., Overman, C. T., Peltz-Smalley, H., Perna, A., Franco, T. Pinto, Pocar, A., Pratte, J. -F., Radeka, V., Raguzin, E., Rasiwala, H., Ray, D., Rebeiro, B., Rescia, S., Retière, F., Richardson, G., Ringuette, J., Riot, V., Rowson, P. C., Roy, N., Rudolph, L., Saldanha, R., Sangiorgio, S., Schwartz, S., Soderstrom, J., Soma, A. K., Spadoni, F., Stekhanov, V., Sun, X. L., Barakoohi, E. Teimoori, Thibado, S., Tidball, A., Totev, T., Triambak, S., Tsang, T., Tyuka, O. A., Underwood, R., van Bruggen, E., Veeraraghavan, V., Vidal, M., Viel, S., Walent, M., Wamba, K., Wang, Q. D., Wang, W., Wang, Y. G., Watts, M., Wei, W., Wen, L. J., Wichoski, U., Wilde, S., Worcester, M., Wu, S., Wu, X. M., Yang, H., Yang, L., Yvaine, M., Zeldovich, O., Zhao, J., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract: Large-scale low-background detectors are increasingly used in rare-event searches as experimental collaborations push for enhanced sensitivity. However, building such detectors, in practice, creates an abundance of radioassay data especially during the conceptual phase of an experiment when hundreds of materials are screened for radiopurity. A tool is needed to manage and make use of the radioassay screening data to quantitatively assess detector design options. We have developed a Materials Database Application for the nEXO experiment to serve this purpose. This paper describes this database, explains how it functions, and discusses how it streamlines the design of the experiment.
Published: 2023

4. Fundamental Symmetries, Neutrons, and Neutrinos (FSNN): Whitepaper for the 2023 NSAC Long Range Plan

Author: Acharya, B., Adams, C., Aleksandrova, A. A., Alfonso, K., An, P., Baeßler, S., Balantekin, A. B., Barbeau, P. S., Bellini, F., Bellini, V., Beminiwattha, R. S., Bernauer, J. C., Bhattacharya, T., Bishof, M., Bolotnikov, A. E., Breur, P. A., Brodeur, M., Brodsky, J. P., Broussard, L. J., Brunner, T., Burdette, D. P., Caylor, J., Chiu, M., Cirigliano, V., Clark, J. A., Clayton, S. M., Daniels, T. V., Darroch, L., Davoudi, Z., de Gouvêa, A., Dekens, W., Demarteau, M., DeMille, D., Deshpande, A., Detwiler, J. A., Dodson, G. W., Dolinski, M. J., Elliott, S. R., Engel, J., Erler, J., Filippone, B. W., Fomin, N., Formaggio, J. A., Friesen, F. Q. L., Fry, J., Fujikawa, B. K., Fuller, G., Fuyuto, K., Gallant, A. T., Gallina, G., Ruiz, A. Garcia, Ruiz, R. F. Garcia, Gardner, S., Gonzalez, F. M., Gratta, G., Gruszko, J., Gudkov, V., Guiseppe, V. E., Gutierrez, T. D., Hansen, E. V., Hardy, C. A., Haxton, W. C., Hayen, L., Hedges, S., Heeger, K. M., Heffner, M., Heise, J., Henning, R., Hergert, H., Hertzog, D. W., Aguilar, D. Hervas, Holt, J. D., Hoogerheide, S. F., Hoppe, E. W., Horoi, M., Howell, C. R., Huang, M., Hutzler, N. R., Imam, K., Ito, T. M., Jamil, A., Janssens, R. V., Jayich, A. M., Jones, B. J. P., Kammel, P., Liu, K. F., Khachatryan, V., King, P. M., Klein, J. R., Kneller, J. P., Kolomensky, Yu. G., Korsch, W., Krücken, R., Kumar, K. S., Launey, K. D., Lawrence, D., Leach, K. G., Lehnert, B., Lenardo, B. G., Li, Z., Lin, H. -W., Longfellow, B., Lopez-Caceres, S., Lunardini, C., MacLellan, R., Markoff, D. M., Maruyama, R. H., Mathews, D. G., Melconian, D., Mereghetti, E., Mohanmurthy, P., Moore, D. C., Mueller, P. E., Mumm, H. P., Nazarewicz, W., Newby, J., Nicholson, A. N., Novitski, E., Ondze, J. C. Nzobadila, O'Donnell, T., Gann, G. D. Orebi, Orrell, J. L., Ouellet, J. L., Parno, D. S., Paschke, K. D., Pastore, S., Pattie Jr, R. W., Petrov, A. A., Pitt, M. L., Plaster, B., Pocanic, D., Pocar, A., Poon, A. W. P., Radford, D. C., Rahangdale, H., Rasco, B. C., Rasiwala, H., Redwine, R. P., Ritz, A., Rogers, L., Ron, G., Saldanha, R., Sangiorgio, S., Sargsyan, G. H., Saunders, A., Savard, G., Schaper, D. C., Scholberg, K., Scielzo, N. D., Seng, C. -Y., Shindler, A., Singh, J. T., Singh, M., Singh, V., Snow, W. M., Soma, A. K., Souder, P. A., Speller, D. H., Stachurska, J., Surukuchi, P. T., Oregui, B. Tapia, Tomalak, O., Torres, J. A., Tyuka, O. A., VanDevender, B. A., Varriano, L., Vogt, R., Walker-Loud, A., Wamba, K., Watkins, S. L., Wietfeldt, F. E., Williams, W. D., Wilson, J. T., Winslow, L., Yan, X. L., Yang, L., Young, A. R., Zheng, X., and Zhou, Y.
Subjects: Nuclear Experiment, Nuclear Theory
Abstract: This whitepaper presents the research priorities decided on by attendees of the 2022 Town Meeting for Fundamental Symmetries, Neutrons and Neutrinos, which took place December 13-15, 2022 in Chapel Hill, NC, as part of the Nuclear Science Advisory Committee (NSAC) 2023 Long Range Planning process. A total of 275 scientists registered for the meeting. The whitepaper makes a number of explicit recommendations and justifies them in detail.
Published: 2023

5. Generative Adversarial Networks for Scintillation Signal Simulation in EXO-200

Author: Li, S., Ostrovskiy, I., Li, Z., Yang, L., Kharusi, S. Al, Anton, G., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Daniels, T., Darroch, L., Daugherty, S. J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Echevers, J., Fairbank Jr., W., Fairbank, D., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fu, Y. S., Fudenberg, D., Gautam, P., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Karelin, A., Kaufman, L. J., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Li, G. S., Licciardi, C., Lin, Y. H., MacLellan, R., McElroy, T., Michel, T., Mong, B., Moore, D. C., Murray, K., Njoya, O., Nusair, O., Odian, A., Perna, A., Piepke, A., Pocar, A., Retière, F., Robinson, A. L., Rowson, P. C., Runge, J., Schmidt, S., Sinclair, D., Skarpaas, K., Soma, A. K., Stekhanov, V., Tarka, M., Thibado, S., Todd, J., Tolba, T., Totev, T. I., and Tsang, R.
Subjects: High Energy Physics - Experiment, Computer Science - Machine Learning, Physics - Instrumentation and Detectors
Abstract: Generative Adversarial Networks trained on samples of simulated or actual events have been proposed as a way of generating large simulated datasets at a reduced computational cost. In this work, a novel approach to perform the simulation of photodetector signals from the time projection chamber of the EXO-200 experiment is demonstrated. The method is based on a Wasserstein Generative Adversarial Network - a deep learning technique allowing for implicit non-parametric estimation of the population distribution for a given set of objects. Our network is trained on real calibration data using raw scintillation waveforms as input. We find that it is able to produce high-quality simulated waveforms an order of magnitude faster than the traditional simulation approach and, importantly, generalize from the training sample and discern salient high-level features of the data. In particular, the network correctly deduces position dependency of scintillation light response in the detector and correctly recognizes dead photodetector channels. The network output is then integrated into the EXO-200 analysis framework to show that the standard EXO-200 reconstruction routine processes the simulated waveforms to produce energy distributions comparable to that of real waveforms. Finally, the remaining discrepancies and potential ways to improve the approach further are highlighted., Comment: As accepted by JINST
Published: 2023
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6. Search for Two-neutrino Double-Beta Decay of $^{136}\rm Xe$ to the $0^+_1$ excited state of $^{136}\rm Ba$ with the Complete EXO-200 Dataset

Author: Collaboration, EXO-200, Kharusi, S. Al, Anton, G., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Daniels, T., Darroch, L., Daugherty, S. J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Echevers, J., Fairbank Jr., W., Fairbank, D., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fu, Y. S., Fudenberg, D., Gautam, P., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Karelin, A., Kaufman, L. J., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Li, G. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., McElroy, T., Michel, T., Mong, B., Moore, D. C., Murray, K., Njoya, O., Nusair, O., Odian, A., Ostrovskiy, I., Perna, A., Piepke, A., Pocar, A., Retière, F., Robinson, A. L., Rowson, P. C., Runge, J., Schmidt, S., Sinclair, D., Skarpaas, K., Soma, A. K., Stekhanov, V., Tarka, M., Thibado, S., Todd, J., Tolba, T., Totev, T. I., Tsang, R., Veenstra, B., Veeraraghavan, V., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Watkins, J., Weber, M., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Xia, Q., Yahne, D. R., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., and Ziegler, T.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: A new search for two-neutrino double-beta ($2\nu\beta\beta$) decay of $^{136}\rm Xe$ to the $0^+_1$ excited state of $^{136}\rm Ba$ is performed with the full EXO-200 dataset. A deep learning-based convolutional neural network is used to discriminate signal from background events. Signal detection efficiency is increased relative to previous searches by EXO-200 by more than a factor of two. With the addition of the Phase II dataset taken with an upgraded detector, the median 90$\%$ confidence level half-life sensitivity of $2\nu\beta\beta$ decay to the $0^+_1$ state of $^{136}\rm Ba$ is $2.9 \times 10^{24}~\rm yr$ using a total $^{136}\rm Xe$ exposure of $234.1~\rm kg~yr$. No statistically significant evidence for $2\nu\beta\beta$ decay to the $0^+_1$ state is observed, leading to a lower limit of $T^{2\nu}_{1/2}(0^+ \rightarrow 0^+_1) > 1.4\times10^{24}~\rm yr$ at 90$\%$ confidence level, improved by 70$\%$ relative to the current world's best constraint., Comment: 9 pages, 7 figures, 2 tables
Published: 2023
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7. Neutrinoless Double Beta Decay

Author: Adams, C., Alfonso, K., Andreoiu, C., Angelico, E., Arnquist, I. J., Asaadi, J. A. A., Avignone, F. T., Axani, S. N., Barabash, A. S., Barbeau, P. S., Baudis, L., Bellini, F., Beretta, M., Bhatta, T., Biancacci, V., Biassoni, M., Bossio, E., Breur, P. A., Brodsky, J. P., Brofferio, C., Brown, E., Brugnera, R., Brunner, T., Burlac, N., Caden, E., Calgaro, S., Cao, G. F., Cao, L., Capelli, C., Cardani, L., Fernandez, R. Castillo, Cattadori, C. M., Chana, B., Chernyak, D., Christofferson, C. D., Chu, P. -H., Church, E., Cirigliano, V., Collister, R., Comellato, T., Dalmasson, J., D'Andrea, V., Daniels, T., Darroch, L., Decowski, M. P., Demarteau, M., Peixoto, S. De Meireles, Detwiler, J. A., DeVoe, R. G., Di Domizio, S., Di Marco, N., di Vacri, M. L., Dolinski, M. J., Efremenko, Yu., Elbeltagi, M., Elliott, S. R., Engel, J., Fabris, L., Fairbank, W. M., Farine, J., Febbraro, M., Figueroa-Feliciano, E., Fields, D. E., Formaggio, J. A., Foust, B. T., Franke, B., Fu, Y., Fujikawa, B. K., Gallacher, D., Gallina, G., Garfagnini, A., Gingras, C., Gironi, L., Giuliani, A., Gold, M., Gornea, R., Grant, C., Gratta, G., Green, M. P., Grinyer, G. F., Gruszko, J., Guan, Y., Guinn, I. S., Guiseppe, V. E., Gutierrez, T. D., Hansen, E. V., Hardy, C. A., Hauptman, J., Heffner, M., Heeger, K. M., Henning, R., Hergert, H., Aguilar, D. Hervas, Hodak, R., Holt, J. D., Hoppe, E. W., Horoi, M., Huang, H. Z., Inoue, K., Jamil, A., Jochum, J., Jones, B. J. P., Kaizer, J., Karapetrov, G., Kharusi, S. Al, Kidd, M. F., Kishimoto, Y., Klein, J. R., Kolomensky, Yu. G., Kontul, I., Kornoukhov, V. N., Krause, P., Krucken, R., Kumar, K. S., Lang, K., Leach, K. G., Lenardo, B. G., Leonhardt, A., Li, A., Li, G., Li, Z., Licciardi, C., Lindsay, R., Lippi, I., Liu, J., Macko, M., MacLellan, R., Macolino, C., Majidi, S., Mamedov, F., Masbou, J., Massarczyk, R., Mastbaum, A. T., Mayer, D., Mazumdar, A., Mei, D. M., Mei, Y., Meijer, S. J., Mereghetti, E., Mertens, S., Mistry, K., Mitsui, T., Moore, D. C., Morella, M., Nattress, J. T., Neuberger, M., Ngwadla, X. E., Nones, C., Novosad, V., Nygren, D. R., Ondze, J. C. Nzobadila, O'Donnell, T., Gann, G. D. Orebi, Orrell, J. L., Ortega, G. S., Ouellet, J. L., Overman, C., Pagani, L., Palusova, V., Para, A., Pavan, M., Perna, A., Pertoldi, L., Pettus, W., Piepke, A., Piseri, P., Pocar, A., Povinec, P., Psihas, F., Pullia, A., Radford, D. C., Ramonnye, G. J, Rasiwala, H., Redchuk, M., Riboldi, S., Richardson, G., Rielage, K., Rogers, L., Rowson, P. C., Rukhadze, E., Saakyan, R., Sada, C., Salamanna, G., Salamida, F., Saldanha, R., Salvat, D. J., Sangiorgio, S., Schaper, D. C., Schoenert, S., Schwarz, M., Schwartz, S. E., Shitov, Y., Simkovic, F., Singh, V., Slavickova, M., Sousa, A. C., Spadoni, F. L., Speller, D. H., Stekl, I., Sumathi, R. R., Surukuchi, P. T., Tayloe, R., Tornow, W., Torres, J. A., Totev, T. I., Triambak, S., Tyuka, O. A., Vasilyev, S. I., Velazquez, M., Viel, S., Vogl, C., von Strum, K., Wang, Q., Waters, D., Watkins, S. L., Watts, M., Wei, W. -Z., Welliver, B., Wen, Liangjian, Wichoski, U., Wilde, S., Wilkerson, J. F., Winslow, L., Wiseman, C., Wu, X., Xu, W., Yang, H., Yang, L., Yu, C. H., Zeman, J., Zennamo, J., and Zuzel, G.
Subjects: Nuclear Experiment, Nuclear Theory
Abstract: This White Paper, prepared for the Fundamental Symmetries, Neutrons, and Neutrinos Town Meeting related to the 2023 Nuclear Physics Long Range Plan, makes the case for double beta decay as a critical component of the future nuclear physics program. The major experimental collaborations and many theorists have endorsed this white paper., Comment: white paper submitted for the Fundamental Symmetries, Neutrons, and Neutrinos Town Meeting in support of the US Nuclear Physics Long Range Planning Process
Published: 2022

8. Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO

Author: Gallina, G., Guan, Y., Retiere, F., Cao, G., Bolotnikov, A., Kotov, I., Rescia, S., Soma, A. K., Tsang, T., Darroch, L., Brunner, T., Bolster, J., Cohen, J. R., Franco, T. Pinto, Gillis, W. C., Smalley, H. Peltz, Thibado, S., Pocar, A., Bhat, A., Jamil, A., Moore, D. C., Adhikari, G., Kharusi, S. Al, Angelico, E., Arnquist, I. J., Arsenault, P., Badhrees, I., Bane, J., Belov, V., Bernard, E. P., Bhatta, T., Brodsky, J. P., Brown, E., Caden, E., Cao, L., Chambers, C., Chana, B., Charlebois, S. A., Chernyak, D., Chiu, M., Cleveland, B., Collister, R., Cvitan, M., Dalmasson, J., Daniels, T., Deslandes, K., DeVoe, R., di Vacri, M. L., Ding, Y., Dolinski, M. J., Dragone, A., Echevers, J., Eckert, B., Elbeltagi, M., Fabris, L., Fairbank, W., Farine, J., Fu, Y. S., Gallacher, D., Gautam, P., Giacomini, G., Gingras, C., Goeldi, D., Gornea, R., Gratta, G., Hardy, C. A., Hedges, S., Heffner, M., Hein, E., Holt, J., Hoppe, E. W., Hößl, J., House, A., Hunt, W., Iverson, A., Jiang, X. S., Karelin, A., Kaufman, L. J., Krücken, R., Kuchenkov, A., Kumar, K. S., Larson, A., Leach, K. G., Lenardo, B. G., Leonard, D. S., Lessard, G., Li, G., Li, S., Li, Z., Licciardi, C., Lindsay, R., MacLellan, R., Mahtab, M., Majidi, S., Malbrunot, C., Margetak, P., Martel-Dion, P., Martin, L., Masbou, J., Massacret, N., McMichael, K., Mong, B., Murray, K., Nattress, J., Natzke, C. R., Ngwadla, X. E., Ondze, J. C. Nzobadila, Odian, A., Orrell, J. L., Ortega, G. S., Overman, C. T., Parent, S., Perna, A., Piepke, A., Pletskova, N., Pratte, J. F., Radeka, V., Raguzin, E., Ramonnye, G. J., Rao, T., Rasiwala, H., Raymond, K., Rebeiro, B. M., Richardson, G., Ringuette, J., Riot, V., Rossignol, T., Rowson, P. C., Rudolph, L., Saldanha, R., Sangiorgio, S., Shang, X., Spadoni, F., Stekhanov, V., Sun, X. L., Tidball, A., Totev, T., Triambak, S., Tsang, R. H. M., Tyuka, O. A., Vachon, F., Vidal, M., Viel, S., Visser, G., Wagenpfeil, M., Walent, M., Wamba, K., Wang, Q., Wang, W., Wang, Y., Watts, M., Wei, W., Wen, L. J., Wichoski, U., Wilde, S., Worcester, M., Wu, W. H., Wu, X., Xie, L., Yan, W., Yang, H., Yang, L., Zeldovich, O., Zhao, J., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors
Abstract: Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0$\nu \beta \beta$), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0$\nu \beta \beta$ of \ce{^{136}Xe} with projected half-life sensitivity of $1.35\times 10^{28}$~yr. To reach this sensitivity, the design goal for nEXO is $\leq$1\% energy resolution at the decay $Q$-value ($2458.07\pm 0.31$~keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163~K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay $Q$-value for the nEXO design.
Published: 2022
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9. Search for MeV Electron Recoils from Dark Matter in EXO-200

Author: Collaboration, EXO-200, Kharusi, S. Al, Anton, G., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Daniels, T., Darroch, L., Daugherty, S. J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Echevers, J., Fairbank Jr., W., Fairbank, D., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fu, Y. S., Fudenberg, D., Gautam, P., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Karelin, A., Kaufman, L. J., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Li, G. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., McElroy, T., Michel, T., Mong, B., Moore, D. C., Murray, K., Njoya, O., Nusair, O., Odian, A., Ostrovskiy, I., Perna, A., Piepke, A., Pocar, A., Retière, F., Robinson, A. L., Rowson, P. C., Ruddell, D., Runge, J., Schmidt, S., Sinclair, D., Skarpaas, K., Soma, A. K., Stekhanov, V., Tarka, M., Thibado, S., Todd, J., Tolba, T., Totev, T. I., Tsang, R. H. M., Veenstra, B., Veeraraghavan, V., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Watkins, J., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Xia, Q., Yahne, D. R., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., and Ziegler, T.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: We present a search for electron-recoil signatures from the charged-current absorption of fermionic dark matter using the EXO-200 detector. We report an average electron recoil background rate of $6.8 \times 10^{-4}\, \mathrm{cts}\,\mathrm{kg}^{-1}\mathrm{yr}^{-1}\mathrm{keV}^{-1}$ above $4\,\mathrm{MeV}$ and find no statistically significant excess over our background projection. Using a total ${}^{136}\mathrm{Xe}$ exposure of $234.1\,\mathrm{kg}\,\mathrm{yr}$ we exclude new parameter space for the charged-current absorption cross-section for dark matter masses between $m_\chi = 2.6\,\mathrm{MeV} - 11.6\,\mathrm{MeV}$ with a minimum of $6\times 10^{-51}\,\mathrm{cm}^2$ at $8.3\,\mathrm{MeV}$ at the $90\%$ confidence level., Comment: 9 pages, 6 figures, 1 table
Published: 2022
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10. Development of a $^{127}$Xe calibration source for nEXO

Author: Lenardo, B. G., Hardy, C. A., Tsang, R. H. M., Ondze, J. C. Nzobadila, Piepke, A., Triambak, S., Jamil, A., Adhikari, G., Kharusi, S. Al, Angelico, E., Arnquist, I. J., Belov, V., Bernard, E. P., Bhat, A., Bhatta, T., Bolotnikov, A., Breur, P. A., Brodsky, J. P., Brown, E., Brunner, T., Caden, E., Cao, G. F., Cao, L., Chana, B., Charlebois, S. A., Chernyak, D., Chiu, M., Cohen, J. R., Collister, R., Dalmasson, J., Daniels, T., Darroch, L., DeVoe, R., di Vacri, M. L., Ding, Y. Y., Dolinski, M. J., Echevers, J., Eckert, B., Elbeltagi, M., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Fu, Y. S., Gallina, G., Gautam, P., Giacomini, G., Gillis, W., Gingras, C., Gornea, R., Gratta, G., Harouaka, K., Heffner, M., Hein, E., Hößl, J., House, A., Iverson, A., Jiang, X. S., Karelin, A., Kaufman, L. J., Krücken, R., Kuchenkov, A., Kumar, K. S., Larson, A., Leach, K. G., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lindsay, R., MacLellan, R., Masbou, J., McMichael, K., Peregrina, M. Medina, Mong, B., Moore, D. C., Murray, K., Nattress, J., Natzke, C. R., Ngwadla, X. E., Ni, K., Ning, Z., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Perna, A., Franco, T. Pinto, Pocar, A., Pratte, J. F., Priel, N., Raguzin, E., Ramonnye, G. J., Rasiwala, H., Raymond, K., Richardson, G., Richman, M., Ringuette, J., Rowson, P. C., Saldanha, R., Sangiorgio, S., Shang, X., Soma, A. K., Spadoni, F., Stekhanov, V., Sun, X. L., Thibado, S., Tidball, A., Todd, J., Totev, T., Tyuka, O. A., Vachon, F., Veeraraghavan, V., Viel, S., Wamba, K., Wang, Y., Wang, Q., Wei, W., Wen, L. J., Wichoski, U., Wilde, S., Wu, W. H., Yan, W., Yang, L., Zeldovich, O., Zhao, J., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract: We study a possible calibration technique for the nEXO experiment using a $^{127}$Xe electron capture source. nEXO is a next-generation search for neutrinoless double beta decay ($0\nu\beta\beta$) that will use a 5-tonne, monolithic liquid xenon time projection chamber (TPC). The xenon, used both as source and detection medium, will be enriched to 90% in $^{136}$Xe. To optimize the event reconstruction and energy resolution, calibrations are needed to map the position- and time-dependent detector response. The 36.3 day half-life of $^{127}$Xe and its small $Q$-value compared to that of $^{136}$Xe $0\nu\beta\beta$ would allow a small activity to be maintained continuously in the detector during normal operations without introducing additional backgrounds, thereby enabling in-situ calibration and monitoring of the detector response. In this work we describe a process for producing the source and preliminary experimental tests. We then use simulations to project the precision with which such a source could calibrate spatial corrections to the light and charge response of the nEXO TPC., Comment: 24 pages, 16 figures
Published: 2022
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11. Search for Majoron-emitting modes of $^{136}$Xe double beta decay with the complete EXO-200 dataset

Author: Kharusi, S. Al, Anton, G., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Daniels, T., Darroch, L., Daugherty, S. J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Echevers, J., Fairbank Jr., W., Fairbank, D., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fudenberg, D., Gautam, P., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Karelin, A., Kaufman, L. J., Koffas, T., Krucken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Li, G. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., McElroy, T., Michel, T., Mong, B., Moore, D. C., Murray, K., Njoya, O., Nusair, O., Odian, A., Ostrovskiy, I., Perna, A., Piepke, A., Pocar, A., Retiere, F., Robinson, A. L., Rowson, P. C., Rudde, D., Runge, J., Schmidt, S., Sinclair, D., Skarpaas, K., Soma, A. K., Stekhanov, V., Tarka, M., Thibado, S., Todd, J., Tolba, T., Totev, T. I., Tsang, R., Veenstra, B., Veeraraghavan, V., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Watkins, J., Weber, M., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Xia, Q., Yahne, D. R., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., and Ziegler, T.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: A search for Majoron-emitting modes of the neutrinoless double-beta decay of $^{136}$Xe is performed with the full EXO-200 dataset. This dataset consists of a total $^{136}$Xe exposure of 234.1 kg$\cdot$yr, and includes data with detector upgrades that have improved the energy threshold relative to previous searches. A lower limit of T$_{1/2}^{\rm{^{136}Xe}}>$4.3$\cdot$10$^{24}$ yr at 90\% C.L. on the half-life of the spectral index $n=1$ Majoron decay was obtained, a factor of 3.6 more stringent than the previous limit from EXO-200, corresponding to a constraint on the Majoron-neutrino coupling constant of $|\langle g_{ee}^{M}\rangle|$$<(0.4$-$0.9)\cdot10^{-5}$. The lower threshold and the additional data taken resulted in a factor 8.4 improvement for the $n=7$ mode compared to the previous EXO search. This search provides the most stringent limits to-date on the Majoron-emitting decays of $^{136}$Xe with spectral indices $n=1,2,3,$ and 7.
Published: 2021
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12. The EXO-200 detector, part II: Auxiliary Systems

Author: Ackerman, N., Albert, J., Auger, M., Auty, D. J., Badhrees, I., Barbeau, P. S., Bartoszek, L., Baussan, E., Belov, V., Benitez-Medina, C., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Conley, R., Cook, S., Coon, M., Craddock, W., Craycraft, A., Cree, W., Daniels, T., Darroch, L., Daugherty, S. J., Daughhetee, J., Davis, C. G., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., deVoe, R., Didberidze, T., Dilling, J., Dobi, A., Dolgolenko, A. G., Dolinski, M. J., Dunford, M., Echevers, J., Espic, L., Fairbank Jr., W., Fairbank, D., Farine, J., Feldmeier, W., Feyzbakhsh, S., Fierlinger, P., Fouts, K., Franco, D., Freytag, D., Fudenberg, D., Gautam, P., Giroux, G., Gornea, R., Graham, K., Gratta, G., Hagemann, C., Hall, C., Hall, K., Haller, G., Hansen, E. V., Hargrove, C., Herbst, R., Herrin, S., Hodgson, J., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Johnson, T. N., Johnston, S., Karelin, A., Kaufman, L. J., Killick, R., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leonard, D. S., Leonard, F., LePort, F., Li, G. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., Mackay, D., MacLellan, R., Marino, M., Martin, J. -M., Martin, Y., McElroy, T., McFarlane, K., Michel, T., Mong, B., Moore, D. C., Murray, K., Neilson, R., Njoya, O., Nusair, O., O'Sullivan, K., Odian, A., Ostrovskiy, I., Ouellet, C., Piepke, A., Pocar, A., Prescott, C. Y., Pushkin, K., Retiere, F., Rivas, A., Robinson, A. L., Rollin, E., Rowson, P. C., Rozo, M. P., Runge, J., Russell, J. J., Schmidt, S., Schubert, A., Sinclair, D., Skarpaas, K., Slutsky, S., Smith, E., Soma, A. K., Stekhanov, V., Strickland, V., Swift, M., Tarka, M., Todd, J., Tolba, T., Tosi, D., Totev, T. I., Tsang, R., Twelker, K., Veenstra, B., Veeraraghavan, V., Vuilleumier, J. -L., Vuilleumier, J. -M., Wagenpfeil, M., Waite, A., Walton, J., Walton, T., Wamba, K., Watkins, J., Weber, M., Wen, L. J., Wichoski, U., Wittgen, M., Wodin, J., Wood, J., Wrede, G., Wu, S. X., Xia, Q., Yang, L., Yen, Y. -R., Zeldovich, O. Ya, and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment, Nuclear Experiment
Abstract: The EXO-200 experiment searched for neutrinoless double-beta decay of $^{136}$Xe with a single-phase liquid xenon detector. It used an active mass of 110 kg of 80.6%-enriched liquid xenon in an ultra-low background time projection chamber with ionization and scintillation detection and readout. This paper describes the design and performance of the various support systems necessary for detector operation, including cryogenics, xenon handling, and controls. Novel features of the system were driven by the need to protect the thin-walled detector chamber containing the liquid xenon, to achieve high chemical purity of the Xe, and to maintain thermal uniformity across the detector., Comment: Manuscript updated in response to JINST reviewer comments
Published: 2021
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13. NEXO: Neutrinoless double beta decay search beyond $10^{28}$ year half-life sensitivity

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

Author: Wagenpfeil, M., Ziegler, T., Schneider, J., Fieguth, A., Murra, M., Schulte, D., Althueser, L., Huhmann, C., Weinheimer, C., Michel, T., Anton, G., Adhikari, G., Kharusi, S. Al, Angelico, E., Arnquist, I. J., Badhrees, I., Bane, J., Beck, D., Belov, V., Bhatta, T., Bolotnikov, A., Breur, P. A., Brodsky, J. P., Brown, E., Brunner, T., Caden, E., Cao, G. F., Chambers, C., Chana, B., Charlebois, S. A., Chernyak, D., Chiu, M., Cleveland, B., Craycraft, A., Daniels, T., Darroch, L., Der Mesrobian-Kabakian, A., Croix, A. de St, Deslandes, K., DeVoe, R., Di Vacri, M. L., Dolinski, M. J., Echevers, J., Elbeltagi, M., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Ferrara, S., Feyzbakhsh, S., Gallina, G., Gautam, P., Giacomini, G., Gingras, C., Goeldi, D., Gorham, A., Gornea, R., Gratta, G., Hansen, E. V., Hardy, C. A., Harouaka, K., Heffner, M., Hoppe, E. W., House, A., Hughes, M., Iverson, A., Jamil, A., Jewell, M., Karelin, A., Kaufman, L. J., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leach, K. G., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lindsay, R., MacLellan, R., Martel-Dion, P., Massacret, N., McElroy, T., Peregrina, M. Medina, Mong, B., Moore, D. C., Murray, K., Nattress, J., Natzke, C. R., Newby, R. J., Nolet, F., Nusair, O., Ondze, J. C. Nzobadila, Odgers, K., Odian, A., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Raguzin, E., Ramonnye, G. J., Rasiwala, H., Rescia, S., Retière, F., Richard, C., Richman, M., Ringuette, J., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Saldanha, R., Sangiorgio, S., Soma, A. K., Spadoni, F., Stekhanov, V., Stiegler, T., Tarka, M., Thibado, S., Tidball, A., Todd, J., Totev, T., Triambak, S., Tsang, R., Vachon, F., Veeraraghavan, V., Viel, S., Vivo-Vilches, C., Walent, M., Wichoski, U., Worcester, M., Wu, S. X., Xia, Q., Yan, W., Yang, L., and Zeldovich, O.
Subjects: Physics - Instrumentation and Detectors
Abstract: Silicon photomultipliers are regarded as a very promising technology for next-generation, cutting-edge detectors for low-background experiments in particle physics. This work presents systematic reflectivity studies of Silicon Photomultipliers (SiPM) and other samples in liquid xenon at vacuum ultraviolet (VUV) wavelengths. A dedicated setup at the University of M\"unster has been used that allows to acquire angle-resolved reflection measurements of various samples immersed in liquid xenon with 0.45{\deg} angular resolution. Four samples are investigated in this work: one Hamamatsu VUV4 SiPM, one FBK VUV-HD SiPM, one FBK wafer sample and one Large-Area Avalanche Photodiode (LA-APD) from EXO-200. The reflectivity is determined to be 25-36% at an angle of incidence of 20{\deg} for the four samples and increases to up to 65% at 70{\deg} for the LA-APD and the FBK samples. The Hamamatsu VUV4 SiPM shows a decline with increasing angle of incidence. The reflectivity results will be incorporated in upcoming light response simulations of the nEXO detector., Comment: 18 pages, 11 figures
Published: 2021
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15. Search for Majoron-emitting modes of Xe136 double beta decay with the complete EXO-200 dataset

Author: Al Kharusi, S, Anton, G, Badhrees, I, Barbeau, PS, Beck, D, Belov, V, Bhatta, T, Breidenbach, M, Brunner, T, Cao, GF, Cen, WR, Chambers, C, Cleveland, B, Coon, M, Craycraft, A, Daniels, T, Darroch, L, Daugherty, SJ, Davis, J, Delaquis, S, Der Mesrobian-Kabakian, A, DeVoe, R, Dilling, J, Dolgolenko, A, Dolinski, MJ, Echevers, J, Fairbank, W, Fairbank, D, Farine, J, Feyzbakhsh, S, Fierlinger, P, Fudenberg, D, Gautam, P, Gornea, R, Gratta, G, Hall, C, Hansen, EV, Hoessl, J, Hufschmidt, P, Hughes, M, Iverson, A, Jamil, A, Jessiman, C, Jewell, MJ, Johnson, A, Karelin, A, Kaufman, LJ, Koffas, T, Krücken, R, Kuchenkov, A, Kumar, KS, Lan, Y, Larson, A, Lenardo, BG, Leonard, DS, Li, GS, Li, S, Li, Z, Licciardi, C, Lin, YH, MacLellan, R, McElroy, T, Michel, T, Mong, B, Moore, DC, Murray, K, Njoya, O, Nusair, O, Odian, A, Ostrovskiy, I, Perna, A, Piepke, A, Pocar, A, Retière, F, Robinson, AL, Rowson, PC, Ruddell, D, Runge, J, Schmidt, S, Sinclair, D, Skarpaas, K, Soma, AK, Stekhanov, V, Tarka, M, Thibado, S, Todd, J, Tolba, T, Totev, TI, Tsang, R, Veenstra, B, Veeraraghavan, V, Vogel, P, Vuilleumier, J-L, Wagenpfeil, M, Watkins, J, Weber, M, Wen, LJ, Wichoski, U, Wrede, G, and Wu, SX
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences
Abstract: A search for Majoron-emitting modes of the neutrinoless double beta decay of Xe136 is performed with the full EXO-200 dataset. This dataset consists of a total Xe136 exposure of 234.1 kg·yr, and includes data with detector upgrades that have improved the energy threshold relative to previous searches. A lower limit of T1/2Xe136>4.3×1024 yr at 90% C.L. on the half-life of the spectral index n=1 Majoron decay was obtained, a factor of 3.6 more stringent than the previous limit from EXO-200 and a factor of 1.6 more stringent than the previous best limit from KamLAND-Zen. This limit corresponds to a constraint on the Majoron-neutrino coupling constant of |geeM|
Published: 2021

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

Author: Stiegler, T., Sangiorgio, S., Brodsky, J. P., Heffner, M., Kharusi, S. Al, Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Bolotnikov, A., Breur, P. A., Brown, E., Brunner, T., Caden, E., Cao, G. F., Cao, L., Chambers, C., Chana, B., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Craycraft, A., Dalmasson, J., Daniels, T., Darroch, L., Croix, A. De St., Der Mesrobian-Kabakian, A., Deslandes, K., DeVoe, R., Di Vacri, M. L., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Echevers, J., Edaltafar, F., Elbeltagi, M., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Ferrara, S., Feyzbakhsh, S., Gallina, G., Gautam, P., Giacomini, G., Goeldi, D., Gornea, R., Gratta, G., Hansen, E. V., Hoppe, E. W., Hößl, J., House, A., Hughes, M., Iverson, A., Jamil, A., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leach, K. G., Lenardo, B. G., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lv, P., MacLellan, R., Massacret, N., McElroy, T., Medina-Peregrina, M., Michel, T., Mong, B., Moore, D. C., Murray, K., Nakarmi, P., Natzke, C. R., Newby, R. J., Ni, K., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Odian, A., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Radeka, V., Raguzin, E., Rescia, S., Retière, F., Richman, M., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Saldanha, R., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Sun, X. L., Tarka, M., Thibado, S., Tidball, A., Todd, J., Totev, T. I., Tsang, R., Tsang, T., Vachon, F., Veeraraghavan, V., Viel, S., Visser, G., Vivo-Vilches, C., Vuilleumier, J. -L., Wagenpfeil, M., Wager, T., Walent, M., Wang, Q., Wei, W., Wen, L. J., Wichoski, U., Worcester, M., Wu, S. X., Wu, W. H., Wu, X., Xia, Q., Yang, H., Yang, L., Zeldovich, O., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors
Abstract: nEXO is a proposed tonne-scale neutrinoless double beta decay ($0\nu\beta\beta$) experiment using liquid ${}^{136}Xe$ (LXe) in a Time Projection Chamber (TPC) to read out ionization and scintillation signals. Between the field cage and the LXe vessel, a layer of LXe ("skin" LXe) is present, where no ionization signal is collected. Only scintillation photons are detected, owing to the lack of optical barrier around the field cage. In this work, we show that the light originating in the skin LXe region can be used to improve background discrimination by 5% over previous published estimates. This improvement comes from two elements. First, a fraction of the $\gamma$-ray background is removed by identifying light from interactions with an energy deposition in the skin LXe. Second, background from ${}^{222}Rn$ dissolved in the skin LXe can be efficiently rejected by tagging the $\alpha$ decay in the ${}^{214}Bi-{}^{214}Po$ chain in the skin LXe., Comment: 11 pages, 12 figures
Published: 2020
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17. Search for $hep$ solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory

Author: Aharmim, B., Ahmed, S. N., Anthony, A. E., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Blucher, E., Bonventre, R., Boudjemline, K., Boulay, M. G., Cai, B., Callaghan, E. J., Caravaca, J., Chan, Y. D., Chauhan, D., Chen, M., Cleveland, B. T., Cox, G. A., Dai, X., Deng, H., Descamps, F. B., Detwiler, J. A., Doe, P. J., Doucas, G., Drouin, P. -L., Dunford, M., Elliott, S. R., Evans, H. C., Ewan, G. T., Farine, J., Fergani, H., Fleurot, F., Ford, R. J., Formaggio, J. A., Gagnon, N., Gilje, K., Goon, J. TM., Graham, K., Guillian, E., Habib, S., Hahn, R. L., Hallin, A. L., Hallman, E. D., Harvey, P. J., Hazama, R., Heintzelman, W. J., Heise, J., Helmer, R. L., Hime, A., Howard, C., Huang, M., Jagam, P., Jamieson, B., Jelley, N. A., Jerkins, M., Keeter, K. J., Klein, J. R., Kormos, L. L., Kos, M., Kraus, C., Krauss, C. B., Krüger, A., Kutter, T., Kyba, C. C. M., Labe, K., Land, B. J., Lange, R., LaTorre, A., Law, J., Lawson, I. T., Lesko, K. T., Leslie, J. R., Levine, I., Loach, J. C., MacLellan, R., Majerus, S., Mak, H. B., Maneira, J., Martin, R. D., Mastbaum, A., McCauley, N., McDonald, A. B., McGee, S. R., Miller, M. L., Monreal, B., Monroe, J., Nickel, B. G., Noble, A. J., O'Keeffe, H. M., Oblath, N. S., Okada, C. E., Ollerhead, R. W., Gann, G. D. Orebi, Oser, S. M., Ott, R. A., Peeters, S. J. M., Poon, A. W. P., Prior, G., Reitzner, S. D., Rielage, K., Robertson, B. C., Robertson, R. G. H., Schwendener, M. H., Secrest, J. A., Seibert, S. R., Simard, O., Sinclair, D., Skensved, P., Sonley, T. J., Stonehill, L. C., Tešić, G., Tolich, N., Tsui, T., Van Berg, R., VanDevender, B. A., Virtue, C. J., Wall, B. L., Waller, D., Tseung, H. Wan Chan, Wark, D. L., Wendland, J., West, N., Wilkerson, J. F., Wilson, J. R., Winchester, T., Wright, A., Yeh, M., Zhang, F., and Zuber, K.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: A search has been performed for neutrinos from two sources, the $hep$ reaction in the solar $pp$ fusion chain and the $\nu_e$ component of the diffuse supernova neutrino background (DSNB), using the full dataset of the Sudbury Neutrino Observatory with a total exposure of 2.47 kton-years after fiducialization. The $hep$ search is performed using both a single-bin counting analysis and a likelihood fit. We find a best-fit flux that is compatible with solar model predictions while remaining consistent with zero flux, and set a one-sided upper limit of $\Phi_{hep} < 30\times10^{3}~\mathrm{cm}^{-2}~\mathrm{s}^{-1}$ [90% credible interval (CI)]. No events are observed in the DSNB search region, and we set an improved upper bound on the $\nu_e$ component of the DSNB flux of $\Phi^\mathrm{DSNB}_{\nu_e} < 19~\textrm{cm}^{-2}~\textrm{s}^{-1}$ (90% CI) in the energy range $22.9 < E_\nu < 36.9$~MeV., Comment: 11 pages, 6 figures
Published: 2020
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18. Measurement of the Spectral Shape of the beta-decay of 137Xe to the Ground State of 137Cs in EXO-200 and Comparison with Theory

Author: Kharusi, S. Al, Anton, G., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Daniels, T., Darroch, L., Daugherty, S. J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Echevers, J., Fairbank Jr., W., Fairbank, D., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fudenberg, D., Gautam, P., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Karelin, A., Kaufman, L. J., Koffas, T., Kostensalo, J., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Li, G. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., McElroy, T., Michel, T., Mong, B., Moore, D. C., Murray, K., Nakarmi, P., Njoya, O., Nusair, O., Odian, A., Ostrovskiy, I., Piepke, A., Pocar, A., Retière, F., Robinson, A. L., Rowson, P. C., Ruddell, D., Runge, J., Schmidt, S., Sinclair, D., Skarpaas, K., Soma, A. K., Stekhanov, V., Suhonen, J., Tarka, M., Thibado, S., Todd, J., Tolba, T., Totev, T. I., Tsang, R., Veenstra, B., Veeraraghavan, V., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Watkins, J., Weber, M., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Xia, Q., Yahne, D. R., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., and Ziegler, T.
Subjects: Nuclear Experiment, Nuclear Theory
Abstract: We report on a comparison between the theoretically predicted and experimentally measured spectra of the first-forbidden non-unique $\beta$-decay transition $^{137}\textrm{Xe}(7/2^-)\to\,^{137}\textrm{Cs}(7/2^+)$. The experimental data were acquired by the EXO-200 experiment during a deployment of an AmBe neutron source. The ultra-low background environment of EXO-200, together with dedicated source deployment and analysis procedures, allowed for collection of a pure sample of the decays, with an estimated signal-to-background ratio of more than 99-to-1 in the energy range from 1075 to 4175 keV. In addition to providing a rare and accurate measurement of the first-forbidden non-unique $\beta$-decay shape, this work constitutes a novel test of the calculated electron spectral shapes in the context of the reactor antineutrino anomaly and spectral bump., Comment: Version as accepted by PRL
Published: 2020
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19. Reflectance of Silicon Photomultipliers at Vacuum Ultraviolet Wavelengths

Author: Lv, P., Cao, G. F., Wen, L. J., Kharusi, S. Al, Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breur, P. A., Brodsky, J. P., Brown, E., Brunner, T., Mamahit, S. Byrne, Caden, E., Cao, L., Chambers, C., Chana, B., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Craycraft, A., Dalmasson, J., Daniels, T., Darroch, L., Croix, A. De St., Der Mesrobian-Kabakian, A., Deslandes, K., DeVoe, R., Di Vacri, M. L., Dilling, J., Ding, Y. Y., Dolinski, M. J., Doria, L., Dragone, A., Echevers, J., Edaltafar, F., Elbeltagi, M., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Ferrara, S., Feyzbakhsh, S., Fucarino, A., Gallina, G., Gautam, P., Giacomini, G., Goeldi, D., Gornea, R., Gratta, G., Hansen, E. V., Heffner, M., Hoppe, E. W., Hößl, J., House, A., Hughes, M., Iverson, A., Jamil, A., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leach, K. G., Lenardo, B. G., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., MacLellan, R., Massacret, N., McElroy, T., Medina-Peregrina, M., Michel, T., Mong, B., Moore, D. C., Murray, K., Nakarmi, P., Natzke, C. R., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Odian, A., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Radeka, V., Raguzin, E., Rescia, S., Retière, F., Richman, M., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Runge, J., Saldanha, R., Sangiorgio, S., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Tarka, M., Todd, J., Totev, T. I., Tsang, R., Tsang, T., Vachon, F., Veeraraghavan, V., Viel, S., Visser, G., Vivo-Vilches, C., Vuilleumier, J. -L., Wagenpfeil, M., Wager, T., Walent, M., Wang, Q., Watkins, J., Wei, W., Wichoski, U., Wu, S. X., Wu, W. H., Wu, X., Xia, Q., Yang, H., Yang, L., Zeldovich, O., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: Characterization of the vacuum ultraviolet (VUV) reflectance of silicon photomultipliers (SiPMs) is important for large-scale SiPM-based photodetector systems. We report the angular dependence of the specular reflectance in a vacuum of SiPMs manufactured by Fondazionc Bruno Kessler (FBK) and Hamamatsu Photonics K.K. (HPK) over wavelengths ranging from 120 nm to 280 nm. Refractive index and extinction coefficient of the thin silicon-dioxide film deposited on the surface of the FBK SiPMs are derived from reflectance data of a FBK silicon wafer with the same deposited oxide film as SiPMs. The diffuse reflectance of SiPMs is also measured at 193 nm. We use the VUV spectral dependence of the optical constants to predict the reflectance of the FBK silicon wafer and FBK SiPMs in liquid xenon.
Published: 2019
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20. An integrated online radioassay data storage and analytics tool for nEXO

Author: Tsang, R.H.M., Piepke, A., Al Kharusi, S., Angelico, E., Arnquist, I.J., Atencio, A., Badhrees, I., Bane, J., Belov, V., Bernard, E.P., Bhat, A., Bhatta, T., Bolotnikov, A., Breur, P.A., Brodsky, J.P., Brown, E., Brunner, T., Caden, E., Cao, G.F., Cao, L.Q., Cesmecioglu, D., Chambers, C., Chambers, E., Chana, B., Charlebois, S.A., Chernyak, D., Chiu, M., Cleveland, B., Cohen, J.R., Collister, R., Cvitan, M., Dalmasson, J., Darroch, L., Deslandes, K., DeVoe, R., di Vacri, M.L., Ding, Y.Y., Dolinski, M.J., Echevers, J., Eckert, B., Elbeltagi, M., Elmansali, R., Fabris, L., Fairbank, W., Farine, J., Fu, Y.S., Gallacher, D., Gallina, G., Gautam, P., Giacomini, G., Gillis, W., Gingras, C., Goeldi, D., Gornea, R., Gratta, G., Guan, Y.D., Hardy, C.A., Hedges, S., Heffner, M., Hein, E., Holt, J., Hoppe, E.W., House, A., Hunt, W., Iverson, A., Jamil, A., Jiang, X.S., Karelin, A., Kaufman, L.J., Kotov, I., Krücken, R., Kuchenkov, A., Kumar, K.S., Larson, A., Leach, K.G., Lenardo, B.G., Leonard, D.S., Li, G., Li, S., Li, Z., Licciardi, C., Lindsay, R., MacLellan, R., Mahtab, M., Majidi, S., Malbrunot, C., Martel-Dion, P., Masbou, J., Massacret, N., McMichael, K., Mong, B., Moore, D.C., Murray, K., Nattress, J., Natzke, C.R., Ngwadla, X.E., Ni, K., Nolan, A., Nowicki, S.C., Nzobadila Ondze, J.C., Orrell, J.L., Ortega, G.S., Overman, C.T., Peltz-Smalley, H., Perna, A., Pinto Franco, T., Pocar, A., Pratte, J.-F., Radeka, V., Raguzin, E., Rasiwala, H., Ray, D., Rebeiro, B.M., Rescia, S., Retière, F., Richardson, G., Ringuette, J., Riot, V., Rowson, P.C., Roy, N., Rudolph, L., Saldanha, R., Sangiorgio, S., Schwartz, S., Soderstrom, J., Soma, A.K., Spadoni, F., Stekhanov, V., Sun, X.L., Teimoori Barakoohi, E., Thibado, S., Tidball, A., Totev, T., Triambak, S., Tsang, T., Tyuka, O.A., Underwood, R., van Bruggen, E., Veeraraghavan, V., Vidal, M., Viel, S., Walent, M., Wamba, K., Wang, Q.D., Wang, W., Wang, Y.G., Watts, M., Wei, W., Wen, L.J., Wichoski, U., Wilde, S., Worcester, M., Wu, S., Wu, X.M., Yang, H., Yang, L., Yvaine, M., Zeldovich, O., Zhao, J., and Ziegler, T.
Published: 2023
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21. Measurements of electron transport in liquid and gas Xenon using a laser-driven photocathode

Author: Njoya, O., Tsang, T., Tarka, M., Fairbank, W., Kumar, K. S., Rao, T., Wager, T., Kharusi, S. Al, Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Brodsky, J. P., Brown, E., Brunner, T., Caden, E., Cao, G. F., Cao, L., Cen, W. R., Chambers, C., Chana, B., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Craycraft, A., Dalmasson, J., Daniels, T., Darroch, L., Daugherty, S. J., Croix, A. De St., Der Mesrobian-Kabakian, A., DeVoe, R., Di Vacri, M. L., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Echevers, J., Elbeltagi, M., Fabris, L., Fairbank, D., Farine, J., Ferrara, S., Feyzbakhsh, S., Fontaine, R., Fucarino, A., Gallina, G., Gautam, P., Giacomini, G., Goeldi, D., Gornea, R., Gratta, G., Hansen, E. V., Heffner, M., Hoppe, E. W., Hossl, J., House, A., Hughes, M., Iverson, A., Jamil, A., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Kodroff, D., Koffas, T., Krucken, R., Kuchenkov, A., Lan, Y., Larson, A., Leach, K. G., Lenardo, B. G., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lin, Y. H., Lv, P., MacLellan, R., McElroy, T., Medina-Peregrina, M., Michel, T., Mong, B., Moore, D. C., Murray, K., Nakarmi, P., Natzke, C. R., Newby, R. J., Ning, Z., Nolet, F., Nusair, O., Odgers, K., Odian, A., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Radeka, V., Raguzin, E., Rescia, S., Retiere, F., Richman, M., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Runge, J., Saldanha, R., Sangiorgio, S., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Todd, J., Tolba, T., Totev, T. I., Tsang, R., Vachon, F., Veeraraghavan, V., Viel, S., Visser, G., Vivo-Vilches, C., Vuilleumier, J. -L., Wagenpfeil, M., Walent, M., Wang, Q., Ward, M., Watkins, J., Weber, M., Wei, W., Wen, L. J., Wichoski, U., Wu, S. X., Wu, W. H., Wu, X., Xia, Q., Yang, H., Yang, L., Yen, Y. -R., Zeldovich, O., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract: Measurements of electron drift properties in liquid and gaseous xenon are reported. The electrons are generated by the photoelectric effect in a semi-transparent gold photocathode driven in transmission mode with a pulsed ultraviolet laser. The charges drift and diffuse in a small chamber at various electric fields and a fixed drift distance of 2.0 cm. At an electric field of 0.5 kV/cm, the measured drift velocities and corresponding temperature coefficients respectively are $1.97 \pm 0.04$ mm/$\mu$s and $(-0.69\pm0.05)$\%/K for liquid xenon, and $1.42 \pm 0.03$ mm/$\mu$s and $(+0.11\pm0.01)$\%/K for gaseous xenon at 1.5 bar. In addition, we measure longitudinal diffusion coefficients of $25.7 \pm 4.6$ cm$^2$/s and $149 \pm 23$ cm$^2$/s, for liquid and gas, respectively. The quantum efficiency of the gold photocathode is studied at the photon energy of 4.73 eV in liquid and gaseous xenon, and vacuum. These charge transport properties and the behavior of photocathodes in a xenon environment are important in designing and calibrating future large scale noble liquid detectors.
Published: 2019
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22. Reflectivity and PDE of VUV4 Hamamatsu SiPMs in Liquid Xenon

Author: Nakarmi, P., Ostrovskiy, I., Soma, A. K., Retiere, F., Kharusi, S. Al, Alfaris, M., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Blatchford, J., Breur, P. A., Brodsky, J. P., Brown, E., Brunner, T., Mamahit, S. Byrne, Caden, E., Cao, G. F., Cao, L., Chambers, C., Chana, B., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Craycraft, A., Dalmasson, J., Daniels, T., Darroch, L., Croix, A. De St., Der Mesrobian-Kabakian, A., DeVoe, R., Di Vacri, M. L., Dilling, J., Ding, Y. Y., Dolinski, M. J., Doria, L., Dragone, A., Echevers, J., Edaltafar, F., Elbeltagi, M., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Ferrara, S., Feyzbakhsh, S., Fontaine, R., Fucarino, A., Gallina, G., Gautam, P., Giacomini, G., Goeldi, D., Gornea, R., Gratta, G., Hansen, E. V., Heffner, M., Hoppe, E. W., Hößle, J., House, A., Hughes, M., Iverson, A., Jamil, A., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leach, K. G., Lenardo, B. G., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lv, P., MacLellan, R., Massacret, N., McElroy, T., Medina-Peregrina, M., Michel, T., Mong, B., Moore, D. C., Murray, K., Natzke, C. R., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Odian, A., Oriunno, M., Orrell, l J. L., Ortega, G. S., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Radeka, V., Raguzin, E., Rescia, S., Richman, M., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Runge, J., Saldanha, R., Sangiorgio, S., VIII, K. Skarpaas, St-Hilaire, G., Stekhanov, r V., Stiegler, T., Sun, X. L., Tarka, M., Todd, J., Totev, T. I., Tsang, R., Tsang, T., Vachon, F., Veeraraghavan, V., Viel, S., Visser, G., Vivo-Vilches, C., Vuilleumier, J. -L., Wagenpfeil, M., Wager, T., Walent, M., Wang, Q., Ward, M., Watkins, J., Weber, M., Wei, W., Wen, L. J., Wichoski, U., Wu, S. X., Wu, W. H., Wu, X., Xia, Q., Yang, H., Yang, L., Zeldovich, O., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: Understanding reflective properties of materials and photodetection efficiency (PDE) of photodetectors is important for optimizing energy resolution and sensitivity of the next generation neutrinoless double beta decay, direct detection dark matter, and neutrino oscillation experiments that will use noble liquid gases, such as nEXO, DARWIN, DarkSide-20k, and DUNE. Little information is currently available about reflectivity and PDE in liquid noble gases, because such measurements are difficult to conduct in a cryogenic environment and at short enough wavelengths. Here we report a measurement of specular reflectivity and relative PDE of Hamamatsu VUV4 silicon photomultipliers (SiPMs) with 50 micrometer micro-cells conducted with xenon scintillation light (~175 nm) in liquid xenon. The specular reflectivity at 15 deg. incidence of three samples of VUV4 SiPMs is found to be 30.4+/-1.4%, 28.6+/-1.3%, and 28.0+/-1.3%, respectively. The PDE at normal incidence differs by +/-8% (standard deviation) among the three devices. The angular dependence of the reflectivity and PDE was also measured for one of the SiPMs. Both the reflectivity and PDE decrease as the angle of incidence increases. This is the first measurement of an angular dependence of PDE and reflectivity of a SiPM in liquid xenon., Comment: 21 pages, 15 figures, 6 tables. As accepted by JINST
Published: 2019
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23. Cosmogenic Neutron Production at the Sudbury Neutrino Observatory

Author: Aharmim, B., Ahmed, S. N., Anthony, A. E., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Bonventre, R., Boudjemline, K., Boulay, M. G., Cai, B., Callaghan, E. J., Caravaca, J., Chan, Y. D., Chauhan, D., Chen, M., Cleveland, B. T., Cox, G. A., Curley, R., Dai, X., Deng, H., Descamps, F. B., Detwiler, J. A., Doe, P. J., Doucas, G., Drouin, P. -L., Dunford, M., Elliott, S. R., Evans, H. C., Ewan, G. T., Farine, J., Fergani, H., Fleurot, F., Ford, R. J., Formaggio, J. A., Gagnon, N., Gilje, K., Goon, J. TM., Graham, K., Guillian, E., Habib, S., Hahn, R. L., Hallin, A. L., Hallman, E. D., Harvey, P. J., Hazama, R., Heintzelman, W. J., Heise, J., Helmer, R. L., Hime, A., Howard, C., Huang, M., Jagam, P., Jamieson, B., Jelley, N. A., Jerkins, M., Kéfélian, C., Keeter, K. J., Klein, J. R., Kormos, L. L., Kos, M., Kr\u, A., Kraus, C., Krauss, C. B., Kutter, T., Kyba, C. C. M., Land, B. J., Lange, R., Law, J., Lawson, I. T., Lesko, K. T., Leslie, J. R., Levine, I., Loach, J. C., MacLellan, R., Majerus, S., Mak, H. B., Maneira, J., Martin, R. D., Mastbaum, A., McCauley, N., McDonald, A. B., McGee, S. R., Miller, M. L., Monreal, B., Monroe, J., Nickel, B. G., Noble, A. J., O'Keeffe, H. M., Oblath, N. S., Okada, C. E., Ollerhead, R. W., Gann, G. D. Orebi, Oser, S. M., Ott, R. A., Peeters, S. J. M., Poon, A. W. P., Prior, G., Reitzner, S. D., Rielage, K., Robertson, B. C., Robertson, R. G. H., Schwendener, M. H., Secrest, J. A., Seibert, S. R., Simard, O., Sinclair, D., Skensved, P., Sonley, T. J., Stonehill, L. C., Teš, G., Tolich, N., Tsui, T., Van Berg, R., VanDevender, B. A., Virtue, C. J., Wall, B. L., Waller, D., Tseung, H. Wan Chan, Wark, D. L., Wendland, J., West, N., Wilkerson, J. F., Wilson, J. R., Winchester, T., Wright, A., Yeh, M., Zhang, F., and Zuber, K.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: Neutrons produced in nuclear interactions initiated by cosmic-ray muons present an irreducible background to many rare-event searches, even in detectors located deep underground. Models for the production of these neutrons have been tested against previous experimental data, but the extrapolation to deeper sites is not well understood. Here we report results from an analysis of cosmogenically produced neutrons at the Sudbury Neutrino Observatory. A specific set of observables are presented, which can be used to benchmark the validity of GEANT4 physics models. In addition, the cosmogenic neutron yield, in units of $10^{-4}\;\text{cm}^{2}/\left(\text{g}\cdot\mu\right)$, is measured to be $7.28 \pm 0.09\;\text{stat.} ^{+1.59}_{-1.12}\;\text{syst.}$ in pure heavy water and $7.30 \pm 0.07\;\text{stat.} ^{+1.40}_{-1.02}\;\text{syst.}$ in NaCl-loaded heavy water. These results provide unique insights into this potential background source for experiments at SNOLAB.
Published: 2019
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24. Measurement of the scintillation and ionization response of liquid xenon at MeV energies in the EXO-200 experiment

Author: Collaboration, EXO-200, Anton, G., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Daniels, T., Darroch, L., Daugherty, S. J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Echevers, J., Fairbank Jr., W., Fairbank, D., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fudenberg, D., Gautam, P., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Karelin, A., Kaufman, L. J., Koffas, T., Krucken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Li, G. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., McElroy, T., Michel, T., Mong, B., Moore, D. C., Murray, K., Neilson, R., Njoya, O., Nusair, O., Odian, A., Ostrovskiy, I., Piepke, A., Pocar, A., Retiere, F., Robinson, A. L., Rowson, P. C., Runge, J., Schmidt, S., Sinclair, D., Soma, A. K., Stekhanov, V., Tarka, M., Todd, J., Tolba, T., Tosi, D., Totev, T. I., Veenstra, B., Veeraraghavan, V., Vuilleumier, J. -L., Wagenpfeil, M., Watkins, J., Weber, M., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Xia, Q., Yahne, D. R., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., and Ziegle, T.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: Liquid xenon (LXe) is employed in a number of current and future detectors for rare event searches. We use the EXO-200 experimental data to measure the absolute scintillation and ionization yields generated by $\gamma$ interactions from $^{228}$Th (2615~keV), $^{226}$Ra (1764~keV) and $^{60}$Co (1332~keV and 1173~keV) calibration sources, over a range of electric fields. The $W$-value that defines the recombination-independent energy scale is measured to be $11.5~\pm~0.5$~(syst.)~$\pm~0.1$~(stat.) eV. These data are also used to measure the recombination fluctuations in the number of electrons and photons produced by the calibration sources at the MeV-scale, which deviate from extrapolations of lower-energy data. Additionally, a semi-empirical model for the energy resolution of the detector is developed, which is used to constrain the recombination efficiency, i.e., the fraction of recombined electrons that result in the emission of a detectable photon. Detailed measurements of the absolute charge and light yields for MeV-scale electron recoils are important for predicting the performance of future neutrinoless double beta decay detectors.
Published: 2019
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25. Simulation of charge readout with segmented tiles in nEXO

Author: Li, Z., Cen, W. R., Robinson, A., Moore, D. C., Wen, L. J., Odian, A., Kharusi, S. Al, Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Brodsky, J. P., Brown, E., Brunner, T., Caden, E., Cao, G. F., Cao, L., Chambers, C., Chana, B., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Craycraft, A., Dalmasson, J., Daniels, T., Darroch, L., Daugherty, S. J., Croix, A. De St., Der Mesrobian-Kabakian, A., DeVoe, R., Di Vacri, M. L., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Echevers, J., Elbeltagi, M., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Ferrara, S., Feyzbakhsh, S., Fontaine, R., Fucarino, A., Gallina, G., Gautam, P., Giacomini, G., Goeldi, D., Gornea, R., Gratta, G., Hansen, E. V., Heffner, M., Hoppe, E. W., Hößl, J., House, A., Hughes, M., Iverson, A., Jamil, A., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Kodroff, D., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leach, K. G., Lenardo, B. G., Leonard, D. S., Li, G., Li, S., Licciardi, C., Lin, Y. H., Lv, P., MacLellan, R., McElroy, T., Medina-Peregrina, M., Michel, T., Mong, B., Murray, K., Nakarmi, P., Natzke, C. R., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Radeka, V., Raguzin, E., Rescia, S., Retière, F., Richman, M., Rossignol, T., Rowson, P. C., Roy, N., Runge, J., Saldanha, R., Sangiorgio, S., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Tarka, M., Todd, J., Tolba, T., Totev, T. I., Tsang, R., Tsang, T., Vachon, F., Veeraraghavan, V., Viel, S., Visser, G., Vivo-Vilches, C., Vuilleumier, J. -L., Wagenpfeil, M., Walent, M., Wang, Q., Ward, M., Watkins, J., Weber, M., Wei, W., Wichoski, U., Wu, S. X., Wu, W. H., Wu, X., Xia, Q., Yang, H., Yang, L., Yen, Y. -R., Zeldovich, O., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract: nEXO is a proposed experiment to search for the neutrino-less double beta decay ($0\nu\beta\beta$) of $^{136}$Xe in a tonne-scale liquid xenon time projection chamber (TPC). The nEXO TPC will be equipped with charge collection tiles to form the anode. In this work, the charge reconstruction performance of this anode design is studied with a dedicated simulation package. A multi-variate method and a deep neural network are developed to distinguish simulated $0\nu\beta\beta$ signals from backgrounds arising from trace levels of natural radioactivity in the detector materials. These simulations indicate that the nEXO TPC with charge-collection tiles shows promising capability to discriminate the $0\nu\beta\beta$ signal from backgrounds. The estimated half-life sensitivity for $0\nu\beta\beta$ decay is improved by $\sim$20$~(32)\%$ with the multi-variate~(deep neural network) methods considered here, relative to the sensitivity estimated in the nEXO pre-conceptual design report.
Published: 2019
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26. Search for Neutrinoless Double-Beta Decay with the Complete EXO-200 Dataset

Author: Anton, G., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Daniels, T., Danilov, M., Darroch, L., Daugherty, S. J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Echevers, J., Fairbank Jr., W., Fairbank, D., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fudenberg, D., Gautam, P., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Johnson, A., Karelin, A., Kaufman, L. J., Koffas, T., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Li, G. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., McElroy, T., Michel, T., Mong, B., Moore, D. C., Murray, K., Njoya, O., Nusair, O., Odian, A., Ostrovskiy, I., Piepke, A., Pocar, A., Retière, F., Robinson, A. L., Rowson, P. C., Ruddell, D., Runge, J., Schmidt, S., Sinclair, D., Soma, A. K., Stekhanov, V., Tarka, M., Todd, J., Tolba, T., Totev, T. I., Veenstra, B., Veeraraghavan, V., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Watkins, J., Weber, M., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Xia, Q., Yahne, D. R., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., and Ziegler, T.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: A search for neutrinoless double-beta decay ($0\nu\beta\beta$) in $^{136}$Xe is performed with the full EXO-200 dataset using a deep neural network to discriminate between $0\nu\beta\beta$ and background events. Relative to previous analyses, the signal detection efficiency has been raised from 80.8% to 96.4$\pm$3.0% and the energy resolution of the detector at the Q-value of $^{136}$Xe $0\nu\beta\beta$ has been improved from $\sigma/E=1.23\%$ to $1.15\pm0.02\%$ with the upgraded detector. Accounting for the new data, the median 90% confidence level $0\nu\beta\beta$ half-life sensitivity for this analysis is $5.0 \cdot 10^{25}$ yr with a total $^{136}$Xe exposure of 234.1 kg$\cdot$yr. No statistically significant evidence for $0\nu\beta\beta$ is observed, leading to a lower limit on the $0\nu\beta\beta$ half-life of $3.5\cdot10^{25}$ yr at the 90% confidence level., Comment: v1, 7 pages, 5 figures; v2, fix references; v3, update to accepted version
Published: 2019
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27. Measurement of neutron production in atmospheric neutrino interactions at the Sudbury Neutrino Observatory

Author: SNO Collaboration, Aharmim, B., Ahmed, S. N., Anthony, A. E., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Bonventre, R., Boudjemline, K., Boulay, M. G., Cai, B., Callaghan, E. J., Caravaca, J., Chan, Y. D., Chauhan, D., Chen, M., Cleveland, B. T., Cox, G. A., Dai, X., Deng, H., Descamps, F. B., Detwiler, J. A., Doe, P. J., Doucas, G., Drouin, P. -L., Dunford, M., Elliott, S. R., Evans, H. C., Ewan, G. T., Farine, J., Fergani, H., Fleurot, F., Ford, R. J., Formaggio, J. A., Gagnon, N., Gilje, K., Goon, J. TM., Graham, K., Guillian, E., Habib, S., Hahn, R. L., Hallin, A. L., Hallman, E. D., Harvey, P. J., Hazama, R., Heintzelman, W. J., Heise, J., Helmer, R. L., Hime, A., Howard, C., Huang, M., Jagam, P., Jamieson, B., Jelley, N. A., Jerkins, M., Keeter, K. J., Klein, J. R., Kormos, L. L., Kos, M., Kruger, A., Kraus, C., Krauss, C. B., Kutter, T., Kyba, C. C. M., Land, B. J., Lange, R., Law, J., Lawson, I. T., Lesko, K. T., Leslie, J. R., Levine, I., Loach, J. C., MacLellan, R., Majerus, S., Mak, H. B., Maneira, J., Martin, R. D., Mastbaum, A., McCauley, N., McDonald, A. B., McGee, S. R., Miller, M. L., Monreal, B., Monroe, J., Nickel, B. G., Noble, A. J., O'Keeffe, H. M., Oblath, N. S., Okada, C. E., Ollerhead, R. W., Gann, G. D. Orebi, Oser, S. M., Ott, R. A., Peeters, S. J. M., Poon, A. W. P., Prior, G., Reitzner, S. D., Rielage, K., Robertson, B. C., Robertson, R. G. H., Schwendener, M. H., Secrest, J. A., Seibert, S. R., Simard, O., Sinclair, D., Singh, J., Skensved, P., Smiley, M., Sonley, T. J., Stonehill, L. C., Tesic, G., Tolich, N., Tsui, T., Van Berg, R., VanDevender, B. A., Virtue, C. J., Wall, B. L., Waller, D., Tseung, H. Wan Chan, Wark, D. L., Wendland, J., West, N., Wilkerson, J. F., Wilson, J. R., Winchester, T., Wright, A., Yeh, M., Zhang, F., and Zuber, K.
Subjects: High Energy Physics - Experiment
Abstract: Neutron production in GeV-scale neutrino interactions is a poorly studied process. We have measured the neutron multiplicities in atmospheric neutrino interactions in the Sudbury Neutrino Observatory experiment and compared them to the prediction of a Monte Carlo simulation using GENIE and a minimally modified version of GEANT4. We analyzed 837 days of exposure corresponding to Phase I, using pure heavy water, and Phase II, using a mixture of Cl in heavy water. Neutrons produced in atmospheric neutrino interactions were identified with an efficiency of $15.3\%$ and $44.3\%$, for Phase I and II respectively. The neutron production is measured as a function of the visible energy of the neutrino interaction and, for charged current quasi-elastic interaction candidates, also as a function of the neutrino energy. This study is also performed classifying the complete sample into two pairs of event categories: charged current quasi-elastic and non charged current quasi-elastic, and $\nu_{\mu}$ and $\nu_e$. Results show good overall agreement between data and Monte Carlo for both phases, with some small tension with a statistical significance below $2\sigma$ for some intermediate energies.
Published: 2019
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28. Characterization of the Hamamatsu VUV4 MPPCs for nEXO

Author: Gallina, G., Giampa, P., Retiere, F., Kroeger, J., Zhang, G., Ward, M., Margetak, P., Lic, G., Tsang, T., Doria, L., Kharusi, S. Al, Alfaris, M., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Blatchford, J., Brodsky, J. P., Brown, E., Brunner, T., Cao, G. F., Cao, L., Cen, W. R., Chambers, C., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Craycraft, A., Dalmasson, J., Daniels, T., Darroch, L., Daugherty, S. J., Croix, A. De St., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Echevers, J., Elbeltagi, M., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Feyzbakhsh, S., Fontaine, R., Gautam, P., Giacomini, G., Gornea, R., Gratta, G., Hansen, E. V., Heffner, M., Hoppe, E. W., Hoßl, J., House, A., Hughes, M., Ito, Y., Iverson, A., Jamil, A., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Kodroff, D., Koffas, T., Krucken, R., Kuchenkov, A., Kumar, K. S., Lana, Y., Larson, A., Lenardo, B. G., Leonarda, D. S., Lik, S., Li, Z., Licciardi, C., Linw, Y. H., Lv, P., MacLellan, R., McElroy, T., Medina-Peregrina, M., Michel, T., Mong, B., Moore, D. C., Murray, K., Nakarmi, P., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Odian, A., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepkez, A., Pocar, A., Pratte, J. -F., Qiu, D., Radeka, V., Raguzin, E., Rescia, S., Richman, M., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Saldanha, R., Sangiorgio, S., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Tarka, M., Todd, J., Tolba, T., Totev, T. I., Tsang, R., Vachon, F., Veeraraghavan, V., Visser, G., Vuilleumier, J. -L., Wagenpfeil, M., Walent, M., Wang, Q., Watkins, J., Weber, M., Wei, W., Wen, L. J., Wichoski, U., Wu, S. X., Wu, W. H., Wu, X., Xia, Q., Yang, H., Yang, L., Yen, Y. -R., Zeldovich, O., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors
Abstract: In this paper we report on the characterization of the Hamamatsu VUV4 (S/N: S13370-6152) Vacuum Ultra-Violet (VUV) sensitive Silicon Photo-Multipliers (SiPMs) as part of the development of a solution for the detection of liquid xenon scintillation light for the nEXO experiment. Various SiPM features, such as: dark noise, gain, correlated avalanches, direct crosstalk and Photon Detection Efficiency (PDE) were measured in a dedicated setup at TRIUMF. SiPMs were characterized in the range $163 \text{ } \text{K} \leq \text{T}\leq 233 \text{ } \text{K}$. At an over voltage of $3.1\pm0.2$ V and at $\text{T}=163 \text{ }\text{K}$ we report a number of Correlated Avalanches (CAs) per pulse in the $1 \upmu\text{s}$ interval following the trigger pulse of $0.161\pm0.005$. At the same settings the Dark-Noise (DN) rate is $0.137\pm0.002 \text{ Hz/mm}^{2}$. Both the number of CAs and the DN rate are within nEXO specifications. The PDE of the Hamamatsu VUV4 was measured for two different devices at $\text{T}=233 \text{ }\text{K}$ for a mean wavelength of $189\pm7\text{ nm}$. At $3.6\pm0.2$ V and $3.5\pm0.2$ V of over voltage we report a PDE of $13.4\pm2.6\text{ }\%$ and $11\pm2\%$, corresponding to a saturation PDE of $14.8\pm2.8\text{ }\%$ and $12.2\pm2.3\%$, respectively. Both values are well below the $24\text{ }\%$ saturation PDE advertised by Hamamatsu. More generally, the second device tested at $3.5\pm0.2$ V of over voltage is below the nEXO PDE requirement. The first one instead yields a PDE that is marginally close to meeting the nEXO specifications. This suggests that with modest improvements the Hamamatsu VUV4 MPPCs could be considered as an alternative to the FBK-LF SiPMs for the final design of the nEXO detector.
Published: 2019
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29. GEANT4 models of HPGe detectors for radioassay

Author: Tsang, R. H. M., Piepke, A., Auty, D. J., Cleveland, B., Delaquis, S., Didberidze, T., MacLellan, R., Meng, Y., Nusair, O., and Tolba, T.
Subjects: Physics - Instrumentation and Detectors
Abstract: Radiation transport models of two high purity germanium detectors, GeII and GeIII, located at the University of Alabama have been created in GEANT4 \cite{geant4}. These detectors have been used extensively for radioassay measurements of materials used in various low background experiments. The two models have been validated against actual data under several scenarios typically seen in radioassay measurements. The systematic uncertainties of the models for GeII and GeIII are estimated to be $\sim$12\% and $\sim$9\% respectively., Comment: 24 pages
Published: 2019
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30. Search for hep solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory

Author: Aharmim, B, Ahmed, SN, Anthony, AE, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Blucher, E, Bonventre, R, Boudjemline, K, Boulay, MG, Cai, B, Callaghan, EJ, Caravaca, J, Chan, YD, Chauhan, D, Chen, M, Cleveland, BT, Cox, GA, Dai, X, Deng, H, Descamps, FB, Detwiler, JA, Doe, PJ, Doucas, G, Drouin, PL, Dunford, M, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Gagnon, N, Gilje, K, Goon, JTM, Graham, K, Guillian, E, Habib, S, Hahn, RL, Hallin, AL, Hallman, ED, Harvey, PJ, Hazama, R, Heintzelman, WJ, Heise, J, Helmer, RL, Hime, A, Howard, C, Huang, M, Jagam, P, Jamieson, B, Jelley, NA, Jerkins, M, Keeter, KJ, Klein, JR, Kormos, LL, Kos, M, Kraus, C, Krauss, CB, Krüger, A, Kutter, T, Kyba, CCM, Labe, K, Land, BJ, Lange, R, Latorre, A, Law, J, Lawson, IT, Lesko, KT, Leslie, JR, Levine, I, Loach, JC, Maclellan, R, Majerus, S, Mak, HB, Maneira, J, Martin, RD, Mastbaum, A, McCauley, N, McDonald, AB, McGee, SR, Miller, ML, Monreal, B, Monroe, J, Nickel, BG, Noble, AJ, O'Keeffe, HM, Oblath, NS, Okada, CE, Ollerhead, RW, Orebi Gann, GD, Oser, SM, Ott, RA, Peeters, SJM, and Poon, AWP
Subjects: hep-ex, nucl-ex
Abstract: A search has been performed for neutrinos from two sources, the hep reaction in the solar pp fusion chain and the νe component of the diffuse supernova neutrino background (DSNB), using the full dataset of the Sudbury Neutrino Observatory with a total exposure of 2.47 kton-years after fiducialization. The hep search is performed using both a single-bin counting analysis and a likelihood fit. We find a best-fit flux that is compatible with solar model predictions while remaining consistent with zero flux, and set a one-sided upper limit of φhep
Published: 2020

31. Constraints on Neutrino Lifetime from the Sudbury Neutrino Observatory

Author: SNO Collaboration, Aharmim, B., Ahmed, S. N., Anthony, A. E., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Bonventre, R., Boudjemline, K., Boulay, M. G., Cai, B., Callaghan, E. J., Caravaca, J., Chan, Y. D., Chauhan, D., Chen, M., Cleveland, B. T., Cox, G. A., Dai, X., Deng, H., Descamps, F. B., Detwiler, J. A., Doe, P. J., Doucas, G., Drouin, P. -L., Dunford, M., Elliott, S. R., Evans, H. C., Ewan, G. T., Farine, J., Fergani, H., Fleurot, F., Ford, R. J., Formaggio, J. A., Gagnon, N., Gilje, K., Goon, J. TM., Graham, K., Guillian, E., Habib, S., Hahn, R. L., Hallin, A. L., Hallman, E. D., Harvey, P. J., Hazama, R., Heintzelman, W. J., Heise, J., Helmer, R. L., Hime, A., Howard, C., Huang, M., Jagam, P., Jamieson, B., Jelley, N. A., Jerkins, M., Kéfélian, C., Keeter, K. J., Klein, J. R., Kormos, L. L., Kos, M., Krüger, A., Kraus, C., Krauss, C. B., Kutter, T., Kyba, C. C. M., Land, B. J., Lange, R., Law, J., Lawson, I. T., Lesko, K. T., Leslie, J. R., Levine, I., Loach, J. C., MacLellan, R., Majerus, S., Mak, H. B., Maneira, J., Martin, R. D., Mastbaum, A., McCauley, N., McDonald, A. B., McGee, S. R., Miller, M. L., Monreal, B., Monroe, J., Nickel, B. G., Noble, A. J., O'Keeffe, H. M., Oblath, N. S., Okada, C. E., Ollerhead, R. W., Gann, G. D. Orebi, Oser, S. M., Ott, R. A., Peeters, S. J. M., Poon, A. W. P., Prior, G., Reitzner, S. D., Rielage, K., Robertson, B. C., Robertson, R. G. H., Schwendener, M. H., Secrest, J. A., Seibert, S. R., Simard, O., Sinclair, D., Skensved, P., Sonley, T. J., Stonehill, L. C., Tešić, G., Tolich, N., Tsui, T., Van Berg, R., VanDevender, B. A., Virtue, C. J., Wall, B. L., Waller, D., Tseung, H. Wan Chan, Wark, D. L., Wendland, J., West, N., Wilkerson, J. F., Wilson, J. R., Winchester, T., Wright, A., Yeh, M., Zhang, F., and Zuber, K.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: The long baseline between the Earth and the Sun makes solar neutrinos an excellent test beam for exploring possible neutrino decay. The signature of such decay would be an energy-dependent distortion of the traditional survival probability which can be fit for using well-developed and high precision analysis methods. Here a model including neutrino decay is fit to all three phases of $^8$B solar neutrino data taken by the Sudbury Neutrino Observatory. This fit constrains the lifetime of neutrino mass state $\nu_2$ to be ${>8.08\times10^{-5}}$ s/eV at $90\%$ confidence. An analysis combining this SNO result with those from other solar neutrino experiments results in a combined limit for the lifetime of mass state $\nu_2$ of ${>1.04\times10^{-3}}$ s/eV at $99\%$ confidence.
Published: 2018
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32. Cosmogenic neutron production at the Sudbury Neutrino Observatory

Author: Aharmim, B, Ahmed, SN, Anthony, AE, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Bonventre, R, Boudjemline, K, Boulay, MG, Cai, B, Callaghan, EJ, Caravaca, J, Chan, YD, Chauhan, D, Chen, M, Cleveland, BT, Cox, GA, Curley, R, Dai, X, Deng, H, Descamps, FB, Detwiler, JA, Doe, PJ, Doucas, G, Drouin, PL, Dunford, M, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Gagnon, N, Gilje, K, Goon, JTM, Graham, K, Guillian, E, Habib, S, Hahn, RL, Hallin, AL, Hallman, ED, Harvey, PJ, Hazama, R, Heintzelman, WJ, Heise, J, Helmer, RL, Hime, A, Howard, C, Huang, M, Jagam, P, Jamieson, B, Jelley, NA, Jerkins, M, Kéfélian, C, Keeter, KJ, Klein, JR, Kormos, LL, Kos, M, Krüger, A, Kraus, C, Krauss, CB, Kutter, T, Kyba, CCM, Land, BJ, Lange, R, Law, J, Lawson, IT, Lesko, KT, Leslie, JR, Levine, I, Loach, JC, MacLellan, R, Majerus, S, Mak, HB, Maneira, J, Martin, RD, Mastbaum, A, McCauley, N, McDonald, AB, McGee, SR, Miller, ML, Monreal, B, Monroe, J, Nickel, BG, Noble, AJ, O'Keeffe, HM, Oblath, NS, Okada, CE, Ollerhead, RW, Orebi Gann, GD, Oser, SM, Ott, RA, Peeters, SJM, Poon, AWP, and Prior, G
Subjects: hep-ex, nucl-ex
Abstract: Neutrons produced in nuclear interactions initiated by cosmic-ray muons present an irreducible background to many rare-event searches, even in detectors located deep underground. Models for the production of these neutrons have been tested against previous experimental data, but the extrapolation to deeper sites is not well understood. Here we report results from an analysis of cosmogenically produced neutrons at the Sudbury Neutrino Observatory. A specific set of observables are presented, which can be used to benchmark the validity of geant4 physics models. In addition, the cosmogenic neutron yield, in units of 10-4 cm2/(g·μ), is measured to be 7.28±0.09(stat)-1.12+1.59(syst) in pure heavy water and 7.30±0.07(stat)-1.02+1.40(syst) in NaCl-loaded heavy water. These results provide unique insights into this potential background source for experiments at SNOLAB.
Published: 2019

33. Tests of Lorentz invariance at the Sudbury Neutrino Observatory

Author: SNO Collaboration, Aharmim, B., Ahmed, S. N., Anthony, A. E., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Blucher, E., Bonventre, R., Boudjemline, K., Boulay, M. G., Cai, B., Callaghan, E. J., Caravaca, J., Chan, Y. D., Chauhan, D., Chen, M., Cleveland, B. T., Cox, G. A., Dai, X., Deng, H., Descamps, F. B., Detwiler, J. A., Doe, P. J., Doucas, G., Drouin, P. -L., Dunford, M., Elliott, S. R., Evans, H. C., Ewan, G. T., Farine, J., Fergani, H., Fleurot, F., Ford, R. J., Formaggio, J. A., Gagnon, N., Gilje, K., Goon, J. TM., Graham, K., Guillian, E., Habib, S., Hahn, R. L., Hallin, A. L., Hallman, E. D., Harvey, P. J., Hazama, R., Heintzelman, W. J., Heise, J., Helmer, R. L., Hime, A., Howard, C., Huang, M., Jagam, P., Jamieson, B., Jelley, N. A., Jerkins, M., Kefelian, C., Keeter, K. J., Klein, J. R., Kormos, L. L., Kos, M., Kruger, A., Kraus, C., Krauss, C. B., Kutter, T., Kyba, C. C. M., Labe, K., Land, B. J., Lange, R., LaTorre, A., Law, J., Lawson, I. T., Lesko, K. T., Leslie, J. R., Levine, I., Loach, J. C., MacLellan, R., Majerus, S., Mak, H. B., Maneira, J., Martin, R. D., Mastbaum, A., McCauley, N., McDonald, A. B., McGee, S. R., Miller, M. L., Monreal, B., Monroe, J., Nickel, B. G., Noble, A. J., O'Keeffe, H. M., Oblath, N. S., Okada, C. E., Ollerhead, R. W., Gann, G. D. Orebi, Oser, S. M., Ott, R. A., Peeters, S. J. M., Poon, A. W. P., Prior, G., Reitzner, S. D., Rielage, K., Robertson, B. C., Robertson, R. G. H., Schwendener, M. H., Secrest, J. A., Seibert, S. R., Simard, O., Sinclair, D., Skensved, P., Sonley, T. J., Stonehill, L. C., Tesic, G., Tolich, N., Tsui, T., Van Berg, R., VanDevender, B. A., Virtue, C. J., Wall, B. L., Waller, D., Tseung, H. Wan Chan, Wark, D. L., Wendland, J., West, N., Wilkerson, J. F., Winchester, T., Wilson, J. R., Wright, A., Yeh, M., Zhang, F., and Zuber, K.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: Experimental tests of Lorentz symmetry in systems of all types are critical for ensuring that the basic assumptions of physics are well-founded. Data from all phases of the Sudbury Neutrino Observatory, a kiloton-scale heavy water Cherenkov detector, are analyzed for possible violations of Lorentz symmetry in the neutrino sector. Such violations would appear as one of eight possible signal types in the detector: six seasonal variations in the solar electron neutrino survival probability differing in energy and time dependence, and two shape changes to the oscillated solar neutrino energy spectrum. No evidence for such signals is observed, and limits on the size of such effects are established in the framework of the Standard Model Extension, including 40 limits on perviously unconstrained operators and improved limits on 15 additional operators. This makes limits on all minimal, Dirac-type Lorentz violating operators in the neutrino sector available for the first time.
Published: 2018
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34. The DUNE Far Detector Interim Design Report, Volume 3: Dual-Phase Module

Author: DUNE Collaboration, Abi, B., Acciarri, R., Acero, M. A., Adamowski, M., Adams, C., Adams, D., Adamson, P., Adinolfi, M., Ahmad, Z., Albright, C. H., Soplin, L. Aliaga, Alion, T., Monsalve, S. Alonso, Alrashed, M., Alt, C., Anderson, J., Anderson, K., Andreopoulos, C., Andrews, M. P., Andrews, R. A., Ankowski, A., Anthony, J., Antonello, M., Antonova, M., Antusch, S., Fernandez, A. Aranda, Ariga, A., Ariga, T., Sierra, D. Aristizabal, Diaz, E. Arrieta, Asaadi, J., Ascencio, M., Asner, D., Athar, M. S., Auger, M., Aurisano, A., Aushev, V., Autiero, D., Azfar, F., Back, A., Back, H., Back, J., Backhouse, C., Baesso, P., Bagby, L., Bai, X., Baird, M., Balantekin, B., Balasubramanian, S., Baller, B., Ballett, P., Balleyguier, L., Bambah, B., Band, H., Bansal, M., Bansal, S., Barenboim, G., Barker, G. J., Barnes, C., Barr, G., Monarca, J. Barranco, Barros, N., Barrow, J., Bashyal, A., Basque, V., Bass, M., Bay, F., Bays, K., Bazo, J. L., Beacom, J. F., Bechetoille, E., Behera, B. R., Bellantoni, L., Bellettini, G., Bellini, V., Beltramello, O., Belver, D., Benekos, N., Benetti, P. A., Bercellie, A., Berman, E., Bernardini, P., Berner, R., Berns, H. G., Bernstein, R. H., Bertolucci, S., Betancourt, M., Bhatnagar, V., Bhattacharjee, M., Bhuyan, B., Biagi, S., Bian, J., Biery, K., Bilki, B., Bishai, M., Bitadze, A., Blackburn, T., Blake, A., Siffert, B. Blanco, Blaszczyk, F., Blaufuss, E., Blazey, G. C., Blennow, M., Blucher, E., Bocean, V., Boffelli, F., Boissevain, J., Bolognesi, S., Bolton, T., Bonesini, M., Boone, T., Booth, A., Booth, C., Bordoni, S., Borkum, A., Boschi, T., Bour, P., Bourguille, B., Boyd, S. B., Boyden, D., Bracinik, J., Brailsford, D., Brandt, A., Bremer, J., Brice, S. J., Bromberg, C., Brooijmans, G., Brooke, J., Brown, G., Buchanan, N., Budd, H., de Holanda, P. C., Cai, T., Caiulo, D., Calafiura, P., Calatayud, A., Calcutt, J., Callahan, C., Calligarich, E., Calvo, E., Camilleri, L., Caminata, A., Campanelli, M., Cancelo, G., Cankocak, K., Cantini, C., Caratelli, D., Carlus, B., Carneiro, M., Terrazas, I. Caro, Carroll, T. J., Carvallo, M. P., Cascella, M., Castromonte, C., Catano-Mur, E., Cavalli-Sforza, M., Cavanna, F., Cazzato, E., Centro, S., Cerati, G., Cervelli, A., Villanueva, A. Cervera, Cervi, T., Chalifour, M., Chappuis, A., Chatterjee, A., Chattopadhyay, S., Chaves, J., Chen, H., Chen, M. -C., Chen, S., Cherdack, D., Chi, C. -Y., Childress, S., Cho, K., Choubey, S., Choudhary, B. C., Christensen, A., Christian, D., Christodoulou, G., Christofferson, C. -A., Church, E., Clarke, P., Coan, T. E., Cocco, A., Collin, G. H., Conley, E., Conrad, J. M., Convery, M., Corey, R., Corwin, L., Cotte, P., Cremonesi, L., Crespo-Anadón, J. I., Prats, J. Creus, Cristaldo, E., Crivelli, P., Cronin-Hennessy, D., Crowley, C., Cuesta, C., Curioni, A., Cussans, D., Dabrowski, M., Dale, D., Da Motta, H., Davenne, T., Davenport, E., Davies, G. S., Davies, J., Davini, S., Dawson, J., De, K., Decowski, M. P., Neto, P. Dedin, Astiz, I. de Icaza, Delbart, A., Delepine, D., Delgado, M., Dell, A., Neto, J. de Mello, DeMuth, D., Deng, Z., Dennis, S., Densham, C., De Bonis, I., De Gouvêa, A., De Jong, P., De Lurgio, P., De Rijck, S., De Roeck, A., de Vries, J. J., Dharmapalan, R., Dhingra, N., Diamantopoulou, M., Diaz, F., Díaz, J. S., Bautista, G. Diaz, Ding, P., Distefano, C., Diwan, M., Di Domizio, S., Di Giulio, L., Di Luise, S., Djurcic, Z., Doizon, F., Dokania, N., Dolinski, M. J., Dong, R., Anjos, J. dos, Douglas, D., Drake, G., Duchesneau, D., Duffy, K., Dung, B., Dutta, D., Duvernois, M., Duyang, H., Dvornikov, O., Dwyer, D. A., Dye, S., Dyshkant, A. S., Dytman, S., Eads, M., Eberly, B., Edmunds, D., Eisch, J., Elagin, A., Elliott, S., Ellsworth, W., Elnimr, M., Emery, S., Eno, S., Ereditato, A., Escobar, C. O., Sanchez, L. Escudero, Evans, J. J., Ezeribe, A., Fahey, K., Falcone, A., Falk, L., Farbin, A., Farnese, C., Farzan, Y., Fasoli, M., Fava, A., Felix, J., Fernandez-Martinez, E., Menendez, P. Fernandez, Ferraro, F., Feyzi, F., Fields, L., Filkins, A., Filthaut, F., Finch, A., Fischer, O., Fitton, M., Fitzpatrick, R., Flanagan, W., Fleming, B. T., Flight, R., Forest, T., Fowler, J., Fox, W., Franc, J., Francis, K., Franchini, P., Franco, D., Freeman, J., Freestone, J., Fried, J., Friedland, A., Fuess, S., Furic, I., Furmanski, A., Gago, A. M., Gallagher, H., Gallego-Ros, A., Galymov, V., Gamberini, E., Gambetta, S., Gamble, T., Gandhi, R., Gandrajula, R., Gao, S., Garcia-Gamez, D., Gardiner, S., Gastler, D., Gehrlein, J., Gelli, B., Gendotti, A., Ghorbani-Moghaddam, Z., Ghosh, A., Gibin, D., Gil-Botella, I., Girerd, C., Giri, A. K., Glavin, S., Goeldi, D., Gogota, O., Gold, M., Gollapinni, S., Gollwitzer, K., Gomes, R. A., Gomez, L., Bermeo, L. V. Gomez, Cadenas, J. J. Gomez, Gong, H., Gonnella, F., Gonzalez-Cuevas, J. A., Goodman, M., Goodwin, O., Gorbunov, D., Goswami, S., Goudzovski, E., Grace, C., Graf, N., Graham, M., Gramellini, E., Gran, R., Grant, A., Grant, C., Grant, N., Greco, V., Green, S., Greenlee, H., Greenler, L., Greenwood, M., Greer, J., Griffith, W. C., Groh, M., Grudzinski, J., Grzelak, K., Guanghua, G., Guardincerri, E., Guarino, V., Guedes, G. P., Guenette, R., Guglielmi, A., Guo, B., Gupta, S., Gupta, V., Guthikonda, K. K., Gutierrez, R., Guzowski, P., Guzzo, M. M., Habig, A., Hackenburg, R. W., Hackenburg, A., Hackett, B., Hadavand, H., Haenni, R., Hahn, A., Haigh, J., Haines, T., Haiston, J., Hamernik, T., Hamilton, P., Han, J., Handler, T., Hans, S., Harris, D. A., Hartnell, J., Hasegawa, T., Hatcher, R., Hatzikoutelis, A., Hays, S., Hazen, E., Headley, M., Heavey, A., Heegerv, K., Heise, J., Hennessy, K., Henry, S., Hernandez, A., Hernandez-Garcia, J., Herner, K., Hewes, V, Hignight, J., Higuera, A., Hill, T., Hillier, S., Himmel, A., Hohl, C., Holin, A., Hoppe, E., Horikawa, S., Horton-Smith, G., Hostert, M., Hourlier, A., Howard, B., Howell, R., Huang, J., Hugon, J., Hurh, P., Hylen, J., Illingworth, R., Insler, J., Introzzi, G., Ioannisian, A., Izmaylov, A., Jaffe, D. E., James, C., James, E., Jang, C. -H., Jediny, F., Jeong, Y. S., Jhingan, A., Ji, W., Jipa, A., Jiménez, S., Johnson, C., Johnson, M., Johnson, R., Johnstone, J., Jones, B., Jones, S., Joshi, J., Jostlein, H., Jung, C. K., Junk, T., Kaboth, A., Kadenko, I., Kamiya, F., Kamyshkov, Y., Karagiorgi, G., Karasavvas, D., Karyotakis, Y., Kasai, S., Kasetti, S., Kaur, K., Kayser, B., Kazaryan, N., Kearns, E., Keener, P., Kemp, E., Kendziora, C., Ketchum, W., Kettell, S. H., Khabibullin, M., Khotjantsev, A., Kim, D., Kirby, B., Kirby, M., Klein, J., Ko, Y. -J., Kobilarcik, T., Kocaman, B., Koerner, L. W., Kohn, S., Koizumi, G., Koller, P., Kopylov, A., Kordosky, M., Kormos, L., Kosc, T., Kose, U., Kostelecký, V. A., Kothekar, K., Kramer, M., Krennrich, F., Kreslo, I., Kriesel, K., Kropp, W., Kudenko, Y., Kudryavtsev, V. A., Kulagin, S., Kumar, J., Kumar, L., Kumar, A., Kumbhare, S., Kuruppu, C., Kus, V., Kutter, T., LaZur, R., Lande, K., Lane, C., Lang, K., Langford, T., Lanni, F., Lasorak, P., Last, D., Lastoria, C., Laundrie, A., Lazanu, I., Le, T., Learned, J., Lebrun, P., Lee, D., Miotto, G. Lehmann, de Oliveira, M. A. Leigui, Li, Q., Li, S., Li, S. W., Li, X., Li, Y., Li, Z., Liao, H. -Y., Lin, S. -K., Lin, C-J. S., Linehan, R., Linhart, V., Link, J., Liptak, Z., Lissauer, D., Littenberg, L., Littlejohn, B., Liu, J., Liu, T., LoMonaco, L., LoSecco, J. M., Lockwitz, S., Lockyer, N., Loew, T., Lokajicek, M., Long, K., Loo, K., Lopez, J. P., Lorca, D., Lord, T., Losada, M., Louis, W. C., Luethi, M., Luk, K. -B., Lundin, T., Luo, X., Lurkin, N., Lux, T., Luzio, V. P., Lykken, J., Maalampi, J., MacLellan, R., Machado, A. A., Machado, P., Macias, C. T., Macier, J., Madigan, P., Magill, S., Mahler, G., Mahn, K., Malek, M., Maloney, J. A., Mammoliti, F., Mandal, S. K., Mandrioli, G., Manenti, L., Manly, S., Mann, A., Marchionni, A., Marciano, W., Marcocci, S., Marfatia, D., Mariani, C., Maricic, J., Marinho, F., Marino, A. D., Marshak, M., Marshall, C., Marshall, J., Marteau, J., Martin-Albo, J., Martinez, D., Martinez, N., Martinez, H., Mason, K., Mastbaum, A., Masud, M., Mathez, H., Matsuno, S., Matthews, J., Mauger, C., Mauri, N., Mavrokoridis, K., Mazza, R., Mazzacane, A., Mazzucato, E., McCauley, N., McCluskey, E., McConkey, N., McDonald, K., McFarland, K. S., McGivern, C., McGowan, A., McGrew, C., McKeown, R., McNab, A., McNulty, D., McTaggart, R., Meddage, V., Mefodiev, A., Mehta, P., Mei, D., Mena, O., Menary, S., Mendez, H., Mendez, D. P., Menegolli, A., Meng, G., Messier, M., Metcalf, W., Mewes, M., Meyer, H., Miao, T., Migenda, J., Milincic, R., Miller, J., Miller, W., Mills, J., Milne, C., Mineev, O., Miranda, O., Mishra, C. S., Mishra, S. R., Mislivec, A., Mitrica, B., Mladenov, D., Mocioiu, I., Moffat, K., Moggi, N., Mohanta, R., Mokhov, N., Molina, J., Bueno, L. Molina, Montanari, A., Montanari, C., Montanari, D., Zetina, L. Montano, Moon, J., Mooney, M., Moore, C., Moreno, D., Morgan, B., Moroni, G. F., Morris, C., Morse, W., Mossey, C., Moura, C. A., Mousseau, J., Mualem, L., Muether, M., Mufson, S., Muheim, F., Muramatsu, H., Murphy, S., Musser, J., Nachtman, J., Nalbandyan, M., Nandakumar, R., Naples, D., Narita, S., Navarro, G., Navarro, J., Navas-Nicolás, D., Nayak, N., Nebot-Guinot, M., Needham, M., Negishi, K., Nelson, J., Nessi, M., Newbold, D., Newcomer, M., Nichol, R., Nicholls, T. C., Niner, E., Norman, A., Norris, B., Norris, J., Novella, P., Nowak, E., Nowak, J., Nunes, M. S., O'Keeffe, H., Oberling, M., Del Campo, A. Olivares, Olivier, A., Onel, Y., Onishchuk, Y., Ovsjannikova, T., Ozturk, S., Pagani, L., Pakvasa, S., Palamara, O., Paley, J., Pallavicini, M., Palomares, C., Palomino, J., Pantic, E., Paolo, A., Paolone, V., Papadimitriou, V., Papaleo, R., Paramesvaran, S., Park, J., Parke, S., Parsa, Z., Pascoli, S., Pasternak, J., Pater, J., Patrizii, L., Patterson, R. B., Patton, S. J., Patzak, T., Paudel, A., Paulos, B., Paulucci, L., Pavlovic, Z., Pawloski, G., Payam, P., Payne, D., Pec, V., Peeters, S. J. M., Pennacchio, E., Penzo, A., Perdue, G. N., Peres, O. l. G., Periale, L., Petridis, K., Petrillo, G., Petti, R., Picchi, P., Pickering, L., Pietropaolo, F., Pillow, J., Plonski, P., Plunkett, R., Poling, R., Pons, X., Poonthottathil, N., Popovic, M., Pordes, R., Pordes, S., Potekhin, M., Potenza, R., Potukuchi, B., Poudel, S., Pozimski, J., Pozzato, M., Prakasj, T., Preece, R., Prokofiev, O., Pruthi, N., Przewlocki, P., Psihas, F., PugnËre, D., Pushka, D., Qi, K., Qian, X., Raaf, J. L., Raboanary, R., Radeka, V., Rademacker, J., Radescu, V., Radics, B., Radovic, A., Rafique, A., Rajaoalisoa, M., Rakhno, I., Rakotondramanana, H. T., Rakotondravohitra, L., Ramachers, Y. A., Rameika, R. A., Delgado, M. A. Ramirez, Ramsey, J., Ramson, B. J., Rappoldi, A., Raselli, G. L., Ratoff, P., Ravat, S., Ravinez, O., Razafinime, H., Rebel, B., Redondo, D., Regenfus, C., Reggiani-Guzzo, M., Rehak, T., Reichenbacher, J., Reitzner, D., Reno, M. H., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Riesselmann, K., Rigaut, Y. -A., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Alonso, M. J. Rodriguez, Roe, B., Roeth, A. J., Roser, R. M., Ross-Lonergan, M., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Rucinski, R., Russell, B., Russell, J., Ruterbories, D., Vagins, M. R., Saakyan, R., Sahu, N., Sala, P., Salukvadze, G., Samios, N., Sanchez, F., Sanchez, M. C., Sandoval, C., Sands, B., Sankar, S. U., Santana, S., Santos, L. M., Santucci, G., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Scaramelli, A., Scarpelli, A., Schaffer, T., Schellman, H., Schlabach, P., Schloesser, C. M., Schmitz, D. 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P., Zennamo, J., Zhang, C., Zhao, M., Zhou, Y. -L., Zhu, G., Zimmerman, E. D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., and Zwaska, R.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: The DUNE IDR describes the proposed physics program and technical designs of the DUNE far detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable the DUNE experiment to make the ground-breaking discoveries that will help to answer fundamental physics questions. Volume 3 describes the dual-phase module's subsystems, the technical coordination required for its design, construction, installation, and integration, and its organizational structure., Comment: 280 pages, 109 figures. arXiv admin note: text overlap with arXiv:1807.10327
Published: 2018

35. The DUNE Far Detector Interim Design Report Volume 1: Physics, Technology and Strategies

Author: DUNE Collaboration, Abi, B., Acciarri, R., Acero, M. A., Adamowski, M., Adams, C., Adams, D., Adamson, P., Adinolfi, M., Ahmad, Z., Albright, C. H., Soplin, L. Aliaga, Alion, T., Monsalve, S. Alonso, Alrashed, M., Alt, C., Anderson, J., Anderson, K., Andreopoulos, C., Andrews, M. P., Andrews, R. A., Ankowski, A., Anthony, J., Antonello, M., Antonova, M., Antusch, S., Fernandez, A. Aranda, Ariga, A., Ariga, T., Sierra, D. Aristizabal, Diaz, E. Arrieta, Asaadi, J., Ascencio, M., Asner, D., Athar, M. S., Auger, M., Aurisano, A., Aushev, V., Autiero, D., Azfar, F., Back, A., Back, H., Back, J., Backhouse, C., Baesso, P., Bagby, L., Bai, X., Baird, M., Balantekin, B., Balasubramanian, S., Baller, B., Ballett, P., Balleyguier, L., Bambah, B., Band, H., Bansal, M., Bansal, S., Barenboim, G., Barker, G. J., Barnes, C., Barr, G., Monarca, J. Barranco, Barros, N., Barrow, J., Bashyal, A., Basque, V., Bass, M., Bay, F., Bays, K., Bazo, J. L., Beacom, J. F., Bechetoille, E., Behera, B. R., Bellantoni, L., Bellettini, G., Bellini, V., Beltramello, O., Belver, D., Benekos, N., Benetti, P. A., Bercellie, A., Berman, E., Bernardini, P., Berner, R., Berns, H. G., Bernstein, R. H., Bertolucci, S., Betancourt, M., Bhatnagar, V., Bhattacharjee, M., Bhuyan, B., Biagi, S., Bian, J., Biery, K., Bilki, B., Bishai, M., Bitadze, A., Blackburn, T., Blake, A., Siffert, B. Blanco, Blaszczyk, F., Blaufuss, E., Blazey, G. C., Blennow, M., Blucher, E., Bocean, V., Boffelli, F., Boissevain, J., Bolognesi, S., Bolton, T., Bonesini, M., Boone, T., Booth, A., Booth, C., Bordoni, S., Borkum, A., Boschi, T., Bour, P., Bourguille, B., Boyd, S. B., Boyden, D., Bracinik, J., Brailsford, D., Brandt, A., Bremer, J., Brice, S. J., Bromberg, C., Brooijmans, G., Brooke, J., Brown, G., Buchanan, N., Budd, H., de Holanda, P. C., Cai, T., Caiulo, D., Calafiura, P., Calatayud, A., Calcutt, J., Callahan, C., Calligarich, E., Calvo, E., Camilleri, L., Caminata, A., Campanelli, M., Cancelo, G., Cankocak, K., Cantini, C., Caratelli, D., Carlus, B., Carneiro, M., Terrazas, I. Caro, Carroll, T. J., Carvallo, M. P., Cascella, M., Castromonte, C., Catano-Mur, E., Cavalli-Sforza, M., Cavanna, F., Cazzato, E., Centro, S., Cerati, G., Cervelli, A., Villanueva, A. Cervera, Cervi, T., Chalifour, M., Chappuis, A., Chatterjee, A., Chattopadhyay, S., Chaves, J., Chen, H., Chen, M. -C., Chen, S., Cherdack, D., Chi, C. -Y., Childress, S., Cho, K., Choubey, S., Choudhary, B. C., Christensen, A., Christian, D., Christodoulou, G., Christofferson, C. -A., Church, E., Clarke, P., Coan, T. E., Cocco, A., Collin, G. H., Conley, E., Conrad, J. M., Convery, M., Corey, R., Corwin, L., Cotte, P., Cremonesi, L., Crespo-Anadón, J. I., Prats, J. 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S., Dytman, S., Eads, M., Eberly, B., Edmunds, D., Eisch, J., Elagin, A., Elliott, S., Ellsworth, W., Elnimr, M., Emery, S., Eno, S., Ereditato, A., Escobar, C. O., Sanchez, L. Escudero, Evans, J. J., Ezeribe, A., Fahey, K., Falcone, A., Falk, L., Farbin, A., Farnese, C., Farzan, Y., Fasoli, M., Fava, A., Felix, J., Fernandez-Martinez, E., Menendez, P. Fernandez, Ferraro, F., Feyzi, F., Fields, L., Filkins, A., Filthaut, F., Finch, A., Fischer, O., Fitton, M., Fitzpatrick, R., Flanagan, W., Fleming, B. T., Flight, R., Forest, T., Fowler, J., Fox, W., Franc, J., Francis, K., Franchini, P., Franco, D., Freeman, J., Freestone, J., Fried, J., Friedland, A., Fuess, S., Furic, I., Furmanski, A., Gago, A. M., Gallagher, H., Gallego-Ros, A., Galymov, V., Gamberini, E., Gambetta, S., Gamble, T., Gandhi, R., Gandrajula, R., Gao, S., Garcia-Gamez, D., Gardiner, S., Gastler, D., Gehrlein, J., Gelli, B., Gendotti, A., Ghorbani-Moghaddam, Z., Ghosh, A., Gibin, D., Gil-Botella, I., Girerd, C., Giri, A. K., Glavin, S., Goeldi, D., Gogota, O., Gold, M., Gollapinni, S., Gollwitzer, K., Gomes, R. A., Gomez, L., Bermeo, L. V. Gomez, Cadenas, J. J. Gomez, Gong, H., Gonnella, F., Gonzalez-Cuevas, J. A., Goodman, M., Goodwin, O., Gorbunov, D., Goswami, S., Goudzovski, E., Grace, C., Graf, N., Graham, M., Gramellini, E., Gran, R., Grant, A., Grant, C., Grant, N., Greco, V., Green, S., Greenlee, H., Greenler, L., Greenwood, M., Greer, J., Griffith, W. C., Groh, M., Grudzinski, J., Grzelak, K., Guanghua, G., Guardincerri, E., Guarino, V., Guedes, G. P., Guenette, R., Guglielmi, A., Guo, B., Gupta, S., Gupta, V., Guthikonda, K. K., Gutierrez, R., Guzowski, P., Guzzo, M. M., Habig, A., Hackenburg, R. W., Hackenburg, A., Hackett, B., Hadavand, H., Haenni, R., Hahn, A., Haigh, J., Haines, T., Haiston, J., Hamernik, T., Hamilton, P., Han, J., Handler, T., Hans, S., Harris, D. A., Hartnell, J., Hasegawa, T., Hatcher, R., Hatzikoutelis, A., Hays, S., Hazen, E., Headley, M., Heavey, A., Heegerv, K., Heise, J., Hennessy, K., Henry, S., Hernandez, A., Hernandez-Garcia, J., Herner, K., Hewes, V, Hignight, J., Higuera, A., Hill, T., Hillier, S., Himmel, A., Hohl, C., Holin, A., Hoppe, E., Horikawa, S., Horton-Smith, G., Hostert, M., Hourlier, A., Howard, B., Howell, R., Huang, J., Hugon, J., Hurh, P., Hylen, J., Illingworth, R., Insler, J., Introzzi, G., Ioannisian, A., Izmaylov, A., Jaffe, D. E., James, C., James, E., Jang, C. -H., Jediny, F., Jeong, Y. S., Jhingan, A., Ji, W., Jipa, A., Jiménez, S., Johnson, C., Johnson, M., Johnson, R., Johnstone, J., Jones, B., Jones, S., Joshi, J., Jostlein, H., Jung, C. K., Junk, T., Kaboth, A., Kadenko, I., Kamiya, F., Kamyshkov, Y., Karagiorgi, G., Karasavvas, D., Karyotakis, Y., Kasai, S., Kasetti, S., Kaur, K., Kayser, B., Kazaryan, N., Kearns, E., Keener, P., Kemp, E., Kendziora, C., Ketchum, W., Kettell, S. H., Khabibullin, M., Khotjantsev, A., Kim, D., Kirby, B., Kirby, M., Klein, J., Ko, Y. -J., Kobilarcik, T., Kocaman, B., Koerner, L. W., Kohn, S., Koizumi, G., Koller, P., Kopylov, A., Kordosky, M., Kormos, L., Kosc, T., Kose, U., Kostelecký, V. A., Kothekar, K., Kramer, M., Krennrich, F., Kreslo, I., Kriesel, K., Kropp, W., Kudenko, Y., Kudryavtsev, V. A., Kulagin, S., Kumar, J., Kumar, L., Kumar, A., Kumbhare, S., Kuruppu, C., Kus, V., Kutter, T., LaZur, R., Lande, K., Lane, C., Lang, K., Langford, T., Lanni, F., Lasorak, P., Last, D., Lastoria, C., Laundrie, A., Lazanu, I., Le, T., Learned, J., Lebrun, P., Lee, D., Miotto, G. Lehmann, de Oliveira, M. A. Leigui, Li, Q., Li, S., Li, S. W., Li, X., Li, Y., Li, Z., Liao, H. -Y., Lin, S. -K., Lin, C-J. S., Linehan, R., Linhart, V., Link, J., Liptak, Z., Lissauer, D., Littenberg, L., Littlejohn, B., Liu, J., Liu, T., LoMonaco, L., LoSecco, J. M., Lockwitz, S., Lockyer, N., Loew, T., Lokajicek, M., Long, K., Loo, K., Lopez, J. P., Lorca, D., Lord, T., Losada, M., Louis, W. C., Luethi, M., Luk, K. -B., Lundin, T., Luo, X., Lurkin, N., Lux, T., Luzio, V. P., Lykken, J., Maalampi, J., MacLellan, R., Machado, A. A., Machado, P., Macias, C. T., Macier, J., Madigan, P., Magill, S., Mahler, G., Mahn, K., Malek, M., Maloney, J. A., Mammoliti, F., Mandal, S. K., Mandrioli, G., Manenti, L., Manly, S., Mann, A., Marchionni, A., Marciano, W., Marcocci, S., Marfatia, D., Mariani, C., Maricic, J., Marinho, F., Marino, A. D., Marshak, M., Marshall, C., Marshall, J., Marteau, J., Martin-Albo, J., Martinez, D., Martinez, N., Martinez, H., Mason, K., Mastbaum, A., Masud, M., Mathez, H., Matsuno, S., Matthews, J., Mauger, C., Mauri, N., Mavrokoridis, K., Mazza, R., Mazzacane, A., Mazzucato, E., McCauley, N., McCluskey, E., McConkey, N., McDonald, K., McFarland, K. S., McGivern, C., McGowan, A., McGrew, C., McKeown, R., McNab, A., McNulty, D., McTaggart, R., Meddage, V., Mefodiev, A., Mehta, P., Mei, D., Mena, O., Menary, S., Mendez, H., Mendez, D. P., Menegolli, A., Meng, G., Messier, M., Metcalf, W., Mewes, M., Meyer, H., Miao, T., Migenda, J., Milincic, R., Miller, J., Miller, W., Mills, J., Milne, C., Mineev, O., Miranda, O., Mishra, C. S., Mishra, S. R., Mislivec, A., Mitrica, B., Mladenov, D., Mocioiu, I., Moffat, K., Moggi, N., Mohanta, R., Mokhov, N., Molina, J., Bueno, L. Molina, Montanari, A., Montanari, C., Montanari, D., Zetina, L. Montano, Moon, J., Mooney, M., Moore, C., Moreno, D., Morgan, B., Moroni, G. F., Morris, C., Morse, W., Mossey, C., Moura, C. A., Mousseau, J., Mualem, L., Muether, M., Mufson, S., Muheim, F., Muramatsu, H., Murphy, S., Musser, J., Nachtman, J., Nalbandyan, M., Nandakumar, R., Naples, D., Narita, S., Navarro, G., Navarro, J., Navas-Nicolás, D., Nayak, N., Nebot-Guinot, M., Needham, M., Negishi, K., Nelson, J., Nessi, M., Newbold, D., Newcomer, M., Nichol, R., Nicholls, T. C., Niner, E., Norman, A., Norris, B., Norris, J., Novella, P., Nowak, E., Nowak, J., Nunes, M. S., O'Keeffe, H., Oberling, M., Del Campo, A. Olivares, Olivier, A., Onel, Y., Onishchuk, Y., Ovsjannikova, T., Ozturk, S., Pagani, L., Pakvasa, S., Palamara, O., Paley, J., Pallavicini, M., Palomares, C., Palomino, J., Pantic, E., Paolo, A., Paolone, V., Papadimitriou, V., Papaleo, R., Paramesvaran, S., Park, J., Parke, S., Parsa, Z., Pascoli, S., Pasternak, J., Pater, J., Patrizii, L., Patterson, R. B., Patton, S. J., Patzak, T., Paudel, A., Paulos, B., Paulucci, L., Pavlovic, Z., Pawloski, G., Payam, P., Payne, D., Pec, V., Peeters, S. J. M., Pennacchio, E., Penzo, A., Perdue, G. N., Peres, O. l. G., Periale, L., Petridis, K., Petrillo, G., Petti, R., Picchi, P., Pickering, L., Pietropaolo, F., Pillow, J., Plonski, P., Plunkett, R., Poling, R., Pons, X., Poonthottathil, N., Popovic, M., Pordes, R., Pordes, S., Potekhin, M., Potenza, R., Potukuchi, B., Poudel, S., Pozimski, J., Pozzato, M., Prakasj, T., Preece, R., Prokofiev, O., Pruthi, N., Przewlocki, P., Psihas, F., PugnËre, D., Pushka, D., Qi, K., Qian, X., Raaf, J. L., Raboanary, R., Radeka, V., Rademacker, J., Radescu, V., Radics, B., Radovic, A., Rafique, A., Rajaoalisoa, M., Rakhno, I., Rakotondramanana, H. T., Rakotondravohitra, L., Ramachers, Y. A., Rameika, R. A., Delgado, M. A. Ramirez, Ramsey, J., Ramson, B. J., Rappoldi, A., Raselli, G. L., Ratoff, P., Ravat, S., Ravinez, O., Razafinime, H., Rebel, B., Redondo, D., Regenfus, C., Reggiani-Guzzo, M., Rehak, T., Reichenbacher, J., Reitzner, D., Reno, M. H., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Riesselmann, K., Rigaut, Y. -A., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Alonso, M. J. Rodriguez, Roe, B., Roeth, A. J., Roser, R. M., Ross-Lonergan, M., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Rucinski, R., Russell, B., Russell, J., Ruterbories, D., Vagins, M. R., Saakyan, R., Sahu, N., Sala, P., Salukvadze, G., Samios, N., Sanchez, F., Sanchez, M. C., Sandoval, C., Sands, B., Sankar, S. U., Santana, S., Santos, L. M., Santucci, G., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Scaramelli, A., Scarpelli, A., Schaffer, T., Schellman, H., Schlabach, P., Schloesser, C. M., Schmitz, D. 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P., Zennamo, J., Zhang, C., Zhao, M., Zhou, Y. -L., Zhu, G., Zimmerman, E. D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., and Zwaska, R.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: The DUNE IDR describes the proposed physics program and technical designs of the DUNE Far Detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable the DUNE experiment to make the ground-breaking discoveries that will help to answer fundamental physics questions. Volume 1 contains an executive summary that describes the general aims of this document. The remainder of this first volume provides a more detailed description of the DUNE physics program that drives the choice of detector technologies. It also includes concise outlines of two overarching systems that have not yet evolved to consortium structures: computing and calibration. Volumes 2 and 3 of this IDR describe, for the single-phase and dual-phase technologies, respectively, each detector module's subsystems, the technical coordination required for its design, construction, installation, and integration, and its organizational structure., Comment: 83 pages, 11 figures
Published: 2018

36. The DUNE Far Detector Interim Design Report, Volume 2: Single-Phase Module

Author: DUNE Collaboration, Abi, B., Acciarri, R., Acero, M. A., Adamowski, M., Adams, C., Adams, D., Adamson, P., Adinolfi, M., Ahmad, Z., Albright, C. H., Soplin, L. Aliaga, Alion, T., Monsalve, S. Alonso, Alrashed, M., Alt, C., Anderson, J., Anderson, K., Andreopoulos, C., Andrews, M. P., Andrews, R. A., Ankowski, A., Anthony, J., Antonello, M., Antonova, M., Antusch, S., Fernandez, A. Aranda, Ariga, A., Ariga, T., Sierra, D. Aristizabal, Diaz, E. Arrieta, Asaadi, J., Ascencio, M., Asner, D., Athar, M. S., Auger, M., Aurisano, A., Aushev, V., Autiero, D., Azfar, F., Back, A., Back, H., Back, J., Backhouse, C., Baesso, P., Bagby, L., Bai, X., Baird, M., Balantekin, B., Balasubramanian, S., Baller, B., Ballett, P., Balleyguier, L., Bambah, B., Band, H., Bansal, M., Bansal, S., Barenboim, G., Barker, G. J., Barnes, C., Barr, G., Monarca, J. Barranco, Barros, N., Barrow, J., Bashyal, A., Basque, V., Bass, M., Bay, F., Bays, K., Bazo, J. L., Beacom, J. F., Bechetoille, E., Behera, B. R., Bellantoni, L., Bellettini, G., Bellini, V., Beltramello, O., Belver, D., Benekos, N., Benetti, P. A., Bercellie, A., Berman, E., Bernardini, P., Berner, R., Berns, H. G., Bernstein, R. H., Bertolucci, S., Betancourt, M., Bhatnagar, V., Bhattacharjee, M., Bhuyan, B., Biagi, S., Bian, J., Biery, K., Bilki, B., Bishai, M., Bitadze, A., Blackburn, T., Blake, A., Siffert, B. Blanco, Blaszczyk, F., Blaufuss, E., Blazey, G. C., Blennow, M., Blucher, E., Bocean, V., Boffelli, F., Boissevain, J., Bolognesi, S., Bolton, T., Bonesini, M., Boone, T., Booth, A., Booth, C., Bordoni, S., Borkum, A., Boschi, T., Bour, P., Bourguille, B., Boyd, S. B., Boyden, D., Bracinik, J., Brailsford, D., Brandt, A., Bremer, J., Brice, S. J., Bromberg, C., Brooijmans, G., Brooke, J., Brown, G., Buchanan, N., Budd, H., de Holanda, P. C., Cai, T., Caiulo, D., Calafiura, P., Calatayud, A., Calcutt, J., Callahan, C., Calligarich, E., Calvo, E., Camilleri, L., Caminata, A., Campanelli, M., Cancelo, G., Cankocak, K., Cantini, C., Caratelli, D., Carlus, B., Carneiro, M., Terrazas, I. Caro, Carroll, T. J., Carvallo, M. P., Cascella, M., Castromonte, C., Catano-Mur, E., Cavalli-Sforza, M., Cavanna, F., Cazzato, E., Centro, S., Cerati, G., Cervelli, A., Villanueva, A. Cervera, Cervi, T., Chalifour, M., Chappuis, A., Chatterjee, A., Chattopadhyay, S., Chaves, J., Chen, H., Chen, M. -C., Chen, S., Cherdack, D., Chi, C. -Y., Childress, S., Cho, K., Choubey, S., Choudhary, B. C., Christensen, A., Christian, D., Christodoulou, G., Christofferson, C. -A., Church, E., Clarke, P., Coan, T. E., Cocco, A., Collin, G. H., Conley, E., Conrad, J. M., Convery, M., Corey, R., Corwin, L., Cotte, P., Cremonesi, L., Crespo-Anadón, J. I., Prats, J. 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W., Li, X., Li, Y., Li, Z., Liao, H. -Y., Lin, S. -K., Lin, C-J. S., Linehan, R., Linhart, V., Link, J., Liptak, Z., Lissauer, D., Littenberg, L., Littlejohn, B., Liu, J., Liu, T., LoMonaco, L., LoSecco, J. M., Lockwitz, S., Lockyer, N., Loew, T., Lokajicek, M., Long, K., Loo, K., Lopez, J. P., Lorca, D., Lord, T., Losada, M., Louis, W. C., Luethi, M., Luk, K. -B., Lundin, T., Luo, X., Lurkin, N., Lux, T., Luzio, V. P., Lykken, J., Maalampi, J., MacLellan, R., Machado, A. A., Machado, P., Macias, C. T., Macier, J., Madigan, P., Magill, S., Mahler, G., Mahn, K., Malek, M., Maloney, J. A., Mammoliti, F., Mandal, S. K., Mandrioli, G., Manenti, L., Manly, S., Mann, A., Marchionni, A., Marciano, W., Marcocci, S., Marfatia, D., Mariani, C., Maricic, J., Marinho, F., Marino, A. 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L., Ratoff, P., Ravat, S., Ravinez, O., Razafinime, H., Rebel, B., Redondo, D., Regenfus, C., Reggiani-Guzzo, M., Rehak, T., Reichenbacher, J., Reitzner, D., Reno, M. H., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Riesselmann, K., Rigaut, Y. -A., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Alonso, M. J. Rodriguez, Roe, B., Roeth, A. J., Roser, R. M., Ross-Lonergan, M., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Rucinski, R., Russell, B., Russell, J., Ruterbories, D., Vagins, M. R., Saakyan, R., Sahu, N., Sala, P., Salukvadze, G., Samios, N., Sanchez, F., Sanchez, M. C., Sandoval, C., Sands, B., Sankar, S. U., Santana, S., Santos, L. M., Santucci, G., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Scaramelli, A., Scarpelli, A., Schaffer, T., Schellman, H., Schlabach, P., Schloesser, C. M., Schmitz, D. W., Schneps, J., Scholberg, K., Schukraft, A., Segreto, E., Sehrawat, S., Sensenig, J., Seong, I., Sepulveda-Quiroz, J. A., Sergi, A., Sergiampietri, F., Sessumes, D., Sexton, K., Sexton-Kennedy, L., Sgalaberna, D., Shaevitz, M. H., Shafaq, S., Shahi, J. S., Shahsavarani, S., Shanahan, P., Sharma, H. R., Sharma, R., Sharma, R. K., Shaw, T., Shin, S., Shoemaker, I., Shooltz, D., Shrock, R., Simos, N., Sinclair, J., Sinev, G., Singh, V., Singh, J., Singh, I., Sipos, R., Sippach, F. W., Sirri, G., Siyeon, K., Smargianaki, D., Smith, A., Smith, E., Smith, P., Smolik, J., Smy, M., Snider, E. L., Snopok, P., Sobczyk, J., Sobel, H., Soderberg, M., Salinas, C. J. Solano, Söldner-Rembold, S., Solomey, N., Sondheim, W., Sorel, M., Soto-Oton, J. A., Sousa, A., Soustruznik, K., Spagliardi, F., Spanu, M., Spitz, J., Spooner, N. J. C., Staley, R., Stancari, M., Stanco, L., Stefanik, A., Steiner, H. M., Stewart, J., Stock, J., Stocker, F., Stoica, S., Stone, J., Strait, J., Strait, M., Strauss, T., Striganov, S., Stuart, A., Sullivan, G., Sultana, M., Sun, Y., Surdo, A., Susic, V., Suter, L., Sutera, C. M., Svoboda, R., Szczerbinska, B., Szelc, A. M., Tagg, N., Talaga, R., Tanaka, H., Oregui, B. Tapia, Tariq, S., Tatar, E., Tayloe, R., Tenti, M., Terao, K., Ternes, C. A., Terranova, F., Testera, G., Thea, A., Thompson, L. F., Thompson, J., Thorn, C., Timilsina, A., Timm, S. C., Todd, J., Tonazzo, A., Tope, T., Torbunov, D., Torti, M., Tórtola, M., Tortorici, F., Toups, M., Touramanis, C., Trevor, J., Tripathi, M., Tromeur, W., Tropin, I., Trzaska, W. H., Tsai, Y. -T., Tsang, K. V., Tsaris, A., Tufanli, S., Tull, C., Turner, J., Tzanov, M., Tziaferi, E., Uchida, Y., Urheim, J., Usher, T., Valdiviesso, G. A., Valencia, E., Valerio, L., Vallari, Z., Valle, J. W. F., Van Berg, R., Van de Water, R., Varanini, F., Varner, G., Vasel, J., Vasseur, G., Vaziri, K., Velev, G., Ventura, S., Verdugo, A., Vermeulen, M., Vernon, E., Verzocchi, M., Viant, T., Vignoli, C., Vihonen, S., Vilela, C., Viren, B., Vokac, P., Vrba, T., Wachala, T., Wahl, D., Wallbank, M., Wang, H., Wang, J., Wang, T. -C., Wang, B., Wang, Y., Wang, Z., Warburton, K., Warner, D., Wascko, M. O., Waters, D., Watson, A., Weber, A., Weber, M., Wei, H., Wei, W., Weinstein, A., Wenman, D., Wetstein, M., While, M., White, A., Whitehead, L. H., Whittington, D., Wierman, K., Wilking, M., Wilkinson, C., Willhite, J., Williams, Z., Wilson, R. J., Wilson, P., Wittich, P., Wolcott, J., Wongjirad, T., Wood, K., Wood, L., Worcester, E., Worcester, M., Wu, S., Wu, W., Xu, W., Yanagisawa, C., Yang, S., Yang, T., Yang, G., Ye, J., Yeh, M., Yershov, N., Yonehara, K., Yoshimura, L., Yu, B., Yu, J., Zalesak, J., Zambelli, L., Zamorano, B., Zani, A., Zaremba, K., Zazueta, L., Zeller, G. P., Zennamo, J., Zhang, C., Zhao, M., Zhou, Y. -L., Zhu, G., Zimmerman, E. D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., and Zwaska, R.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: The DUNE IDR describes the proposed physics program and technical designs of the DUNE far detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable the DUNE experiment to make the ground-breaking discoveries that will help to answer fundamental physics questions. Volume 2 describes the single-phase module's subsystems, the technical coordination required for its design, construction, installation, and integration, and its organizational structure., Comment: 324 pages, 130 figures. arXiv admin note: text overlap with arXiv:1807.10340
Published: 2018

37. Study of Silicon Photomultiplier Performance in External Electric Fields

Author: Sun, X. L., Tolba, T., Cao, G. F., Lv, P., Wen, L. J., Odian, A., Vachon, F., Alamre, A., Albert, J. B., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Bourque, F., Brodsky, J. P., Brown, E., Brunner, T., Burenkov, A., Cao, L., Cen, W. R., Chambers, C., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Côté, M., Craycraft, A., Cree, W., Dalmasson, J., Daniels, T., Darroch, L., Daugherty, S. J., Daughhetee, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Echevers, J., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fontaine, R., Fudenberg, D., Gallina, G., Giacomini, G., Gornea, R., Gratta, G., Hansen, E. V., Harris, D., Heffner, M., Hoppe, E. W., Hößl, J., House, A., Hufschmidt, P., Hughes, M., Ito, Y., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Kodroff, D., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., Michel, T., Moe, M., Mong, B., Moore, D. C., Murray, K., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Qiu, D., Radeka, V., Raguzin, E., Rao, T., Rescia, S., Retière, F., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Saldanha, R., Sangiorgio, S., Schmidt, S., Schneider, J., Sinclair, D., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Tarka, M., Todd, J., Totev, T. I., Tsang, R., Tsang, T., Veenstra, B., Veeraraghavan, V., Visser, G., Vuilleumier, J. -L., Wagenpfeil, M., Wang, Q., Watkins, J., Weber, M., Wei, W., Wichoski, U., Wrede, G., Wu, S. X., Wu, W. H., Xia, Q., Yang, L., Yen, Y. -R., Zeldovich, O., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors
Abstract: We report on the performance of silicon photomultiplier (SiPM) light sensors operating in electric field strength up to 30 kV/cm and at a temperature of 149K, relative to their performance in the absence of an external electric field. The SiPM devices used in this study show stable gain, photon detection efficiency, and rates of correlated pulses, when exposed to external fields, within the estimated uncertainties. No observable physical damage to the bulk or surface of the devices was caused by the exposure., Comment: 16 pages, 12 figures, 2 tables and two conferences (INPC2016 and TIPP2017)
Published: 2018
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38. Imaging individual barium atoms in solid xenon for barium tagging in nEXO

Author: Chambers, C., Walton, T., Fairbank, D., Craycraft, A., Yahne, D. R., Todd, J., Iverson, A., Fairbank, W., Alamare, A., Albert, J. B., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Bourque, F., Brodsky, J. P., Brown, E., Brunner, T., Burenkov, A., Cao, G. F., Cao, L., Cen, W. R., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Cree, W., Côté, M., Dalmasson, J., Daniels, T., Darroch, L., Daugherty, S. J., Daughhetee, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Echevers, J., Fabris, L., Farine, J., Feyzbakhsh, S., Fontaine, R., Fudenberg, D., Giacomini, G., Gornea, R., Gratta, G., Hansen, E. V., Heffner, M., Hoppe, E. W., Hößl, J., House, A., Hufschmidt, P., Hughes, M., Ito, Y., Jamil, A., Jessiman, C., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Kodroff, D., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lin, Y. H., Lv, P., MacLellan, R., Michel, T., Mong, B., Moore, D. C., Murray, K., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Odian, A., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Qiu, D., Radeka, V., Raguzin, E., Rao, T., Rescia, S., Retière, F., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Saldanha, R., Sangiorgio, S., Schmidt, S., Schneider, J., Schubert, A., Sinclair, D., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Tarka, M., Tolba, T., Tsang, T. I. Totev. R., Tsang, T., Vachon, F., Veenstra, B., Veeraraghavan, V., Visser, G., Vuilleumier, J. -L., Wagenpfeil, M., Wang, Q., Watkins, J., Weber, M., Wei, W., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Wu, W. H., Xia, Q., Yang, L., Yen, Y. -R., Zeldovich, O., Zhang, X., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract: The search for neutrinoless double beta decay probes the fundamental properties of neutrinos, including whether or not the neutrino and antineutrino are distinct. Double beta detectors are large and expensive, so background reduction is essential for extracting the highest sensitivity. The identification, or 'tagging', of the $^{136}$Ba daughter atom from double beta decay of $^{136}$Xe provides a technique for eliminating backgrounds in the nEXO neutrinoless double beta decay experiment. The tagging scheme studied in this work utilizes a cryogenic probe to trap the barium atom in solid xenon, where the barium atom is tagged via fluorescence imaging in the solid xenon matrix. Here we demonstrate imaging and counting of individual atoms of barium in solid xenon by scanning a focused laser across a solid xenon matrix deposited on a sapphire window. When the laser sits on an individual atom, the fluorescence persists for $\sim$30~s before dropping abruptly to the background level, a clear confirmation of one-atom imaging. No barium fluorescence persists following evaporation of a barium deposit to a limit of $\leq$0.16\%. This is the first time that single atoms have been imaged in solid noble element. It establishes the basic principle of a barium tagging technique for nEXO.
Published: 2018

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

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

Author: nEXO Collaboration, Kharusi, S. Al, Alamre, A., Albert, J. B., Alfaris, M., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., Bourque, F., Brodsky, J. P., Brown, E., Brunner, T., Burenkov, A., Cao, G. F., Cao, L., Cen, W. R., Chambers, C., Charlebois, S. A., Chiu, M., Cleveland, B., Conley, R., Coon, M., Côté, M., Craycraft, A., Cree, W., Dalmasson, J., Daniels, T., Danovitch, D., Darroch, L., Daugherty, S. J., Daughhetee, J., DeVoe, R., Delaquis, S., Der Mesrobian-Kabakian, A., Di Vacri, M. L., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Echevers, J., Fabris, L., Fairbank, D., Fairbank, W., Farine, J., Ferrara, S., Feyzbakhsh, S., Fierlinger, P., Fontaine, R., Fudenberg, D., Gallina, G., Giacomini, G., Gornea, R., Gratta, G., Haller, G., Hansen, E. V., Harris, D., Hasi, J., Heffner, M., Hoppe, E. W., Hößl, J., House, A., Hufschmidt, P., Hughes, M., Ito, Y., Iverson, A., Jamil, A., Jessiman, C., Jewell, M. J., Jiang, X. S., Karelin, A., Kaufman, L. J., Kenney, C., Killick, R., Kodroff, D., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Larson, A., Lenardo, B. G., Leonard, D. S., Lewis, C. M., Li, G., Li, S., Li, Z., Licciardi, C., Lin, Y. H., Lv, P., MacLellan, R., McFarlane, K., Michel, T., Mong, B., Moore, D. C., Murray, K., Newby, R. J., Nguyen, T., Ning, Z., Njoya, O., Nolet, F., Nusair, O., Odgers, K., Odian, A., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Patel, M., Peña-Perez, A., Piepke, A., Pocar, A., Pratte, J. -F., Qiu, D., Radeka, V., Raguzin, E., Rao, T., Rescia, S., Retière, F., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Runge, J., Saldanha, R., Sangiorgio, S., Schmidt, S., Schneider, J., Schubert, A., Segal, J., Skarpaas~VIII, K., Soma, A. K., Spitaels, K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Tarka, M., Todd, J., Tolba, T., Totev, T. I., Tsang, R., Tsang, T., Vachon, F., Veenstra, B., Veeraraghavan, V., Visser, G., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Wang, Q., Ward, M., Watkins, J., Weber, M., Wei, W., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Wu, W. H., Xia, Q., Yang, L., Yen, Y. -R., Zeldovich, O., Zhang, X., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract: The projected performance and detector configuration of nEXO are described in this pre-Conceptual Design Report (pCDR). nEXO is a tonne-scale neutrinoless double beta ($0\nu\beta\beta$) decay search in $^{136}$Xe, based on the ultra-low background liquid xenon technology validated by EXO-200. With $\simeq$ 5000 kg of xenon enriched to 90% in the isotope 136, nEXO has a projected half-life sensitivity of approximately $10^{28}$ years. This represents an improvement in sensitivity of about two orders of magnitude with respect to current results. Based on the experience gained from EXO-200 and the effectiveness of xenon purification techniques, we expect the background to be dominated by external sources of radiation. The sensitivity increase is, therefore, entirely derived from the increase of active mass in a monolithic and homogeneous detector, along with some technical advances perfected in the course of a dedicated R&D program. Hence the risk which is inherent to the construction of a large, ultra-low background detector is reduced, as the intrinsic radioactive contamination requirements are generally not beyond those demonstrated with the present generation $0\nu\beta\beta$ decay experiments. Indeed, most of the required materials have been already assayed or reasonable estimates of their properties are at hand. The details described herein represent the base design of the detector configuration as of early 2018. Where potential design improvements are possible, alternatives are discussed. This design for nEXO presents a compelling path towards a next generation search for $0\nu\beta\beta$, with a substantial possibility to discover physics beyond the Standard Model., Comment: 182 pages, minor revisions
Published: 2018

41. Deep Neural Networks for Energy and Position Reconstruction in EXO-200

Author: Delaquis, S., Jewell, M. J., Ostrovskiy, I., Weber, M., Ziegler, T., Dalmasson, J., Kaufman, L. J., Richards, T., Albert, J. B., Anton, G., Badhrees, I., Barbeau, P. S., Bayerlein, R., Beck, D., Belov, V., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Cree, W., Daniels, T., Danilov, M., Daugherty, S. J., Daughhetee, J., Davis, J., Der Mesrobian-Kabakian, A., DeVoe, R., Dilling, J., Dolgolenko, A., Dolinski, M. J., Fairbank Jr., W., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fudenberg, D., Gornea, R., Gratta, G., Hall, C., Hansen, E. V., Harris, D., Hoessl, J., Hufschmidt, P., Hughes, M., Iverson, A., Jamil, A., Johnson, A., Karelin, A., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Leonard, D. S., Li, G. S., Li, S., Licciardi, C., Lin, Y. H., MacLellan, R., Michel, T., Mong, B., Moore, D., Murray, K., Njoya, O., Odian, A., Piepke, A., Pocar, A., Retière, F., Robinson, A. L., Rowson, P. C., Schmidt, S., Schubert, A., Sinclair, D., Soma, A. K., Stekhanov, V., Tarka, M., Todd, J., Tolba, T., Veeraraghavan, V., Vuilleumier, J. -L., Wagenpfeil, M., Waite, A., Watkins, J., Wen, L. J., Wichoski, U., Wrede, G., Xia, Q., Yang, L., Yen, Y. -R., and Zeldovich, O. Ya.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment, Nuclear Experiment
Abstract: We apply deep neural networks (DNN) to data from the EXO-200 experiment. In the studied cases, the DNN is able to reconstruct the relevant parameters - total energy and position - directly from raw digitized waveforms, with minimal exceptions. For the first time, the developed algorithms are evaluated on real detector calibration data. The accuracy of reconstruction either reaches or exceeds what was achieved by the conventional approaches developed by EXO-200 over the course of the experiment. Most existing DNN approaches to event reconstruction and classification in particle physics are trained on Monte Carlo simulated events. Such algorithms are inherently limited by the accuracy of the simulation. We describe a unique approach that, in an experiment such as EXO-200, allows to successfully perform certain reconstruction and analysis tasks by training the network on waveforms from experimental data, either reducing or eliminating the reliance on the Monte Carlo., Comment: Accepted version. 33 pages, 28 figures
Published: 2018
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42. Measurement of neutron production in atmospheric neutrino interactions at the Sudbury Neutrino Observatory

Author: Aharmim, B, Ahmed, SN, Anthony, AE, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Bonventre, R, Boudjemline, K, Boulay, MG, Cai, B, Callaghan, EJ, Caravaca, J, Chan, YD, Chauhan, D, Chen, M, Cleveland, BT, Cox, GA, Dai, X, Deng, H, Descamps, FB, Detwiler, JA, Doe, PJ, Doucas, G, Drouin, P-L, Dunford, M, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Gagnon, N, Gilje, K, Goon, JTM, Graham, K, Guillian, E, Habib, S, Hahn, RL, Hallin, AL, Hallman, ED, Harvey, PJ, Hazama, R, Heintzelman, WJ, Heise, J, Helmer, RL, Hime, A, Howard, C, Huang, M, Jagam, P, Jamieson, B, Jelley, NA, Jerkins, M, Keeter, KJ, Klein, JR, Kormos, LL, Kos, M, Kruger, A, Kraus, C, Krauss, CB, Kutter, T, Kyba, CCM, Land, BJ, Lange, R, Law, J, Lawson, IT, Lesko, KT, Leslie, JR, Levine, I, Loach, JC, MacLellan, R, Majerus, S, Mak, HB, Maneira, J, Martin, RD, Mastbaum, A, McCauley, N, McDonald, AB, McGee, SR, Miller, ML, Monreal, B, Monroe, J, Nickel, BG, Noble, AJ, O'Keeffe, HM, Oblath, NS, Okada, CE, Ollerhead, RW, Gann, GD Orebi, Oser, SM, Ott, RA, Peeters, SJM, Poon, AWP, Prior, G, Reitzner, SD, and Rielage, K
Subjects: hep-ex
Abstract: Neutron production in GeV-scale neutrino interactions is a poorly studiedprocess. We have measured the neutron multiplicities in atmospheric neutrinointeractions in the Sudbury Neutrino Observatory experiment and compared themto the prediction of a Monte Carlo simulation using GENIE and a minimallymodified version of GEANT4. We analyzed 837 days of exposure corresponding toPhase I, using pure heavy water, and Phase II, using a mixture of Cl in heavywater. Neutrons produced in atmospheric neutrino interactions were identifiedwith an efficiency of $15.3\%$ and $44.3\%$, for Phase I and II respectively.The neutron production is measured as a function of the visible energy of theneutrino interaction and, for charged current quasi-elastic interactioncandidates, also as a function of the neutrino energy. This study is alsoperformed classifying the complete sample into two pairs of event categories:charged current quasi-elastic and non charged current quasi-elastic, and$\nu_{\mu}$ and $\nu_e$. Results show good overall agreement between data andMonte Carlo for both phases, with some small tension with a statisticalsignificance below $2\sigma$ for some intermediate energies.
Published: 2019

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

Author: Chambers, C, Walton, T, Fairbank, D, Craycraft, A, Yahne, DR, Todd, J, Iverson, A, Fairbank, W, Alamare, A, Albert, JB, Anton, G, Arnquist, IJ, Badhrees, I, Barbeau, PS, Beck, D, Belov, V, Bhatta, T, Bourque, F, Brodsky, JP, Brown, E, Brunner, T, Burenkov, A, Cao, GF, Cao, L, Cen, WR, Charlebois, SA, Chiu, M, Cleveland, B, Coon, M, Cree, W, Côté, M, Dalmasson, J, Daniels, T, Darroch, L, Daugherty, SJ, Daughhetee, J, Delaquis, S, Mesrobian-Kabakian, A Der, DeVoe, R, Dilling, J, Ding, YY, Dolinski, MJ, Dragone, A, Echevers, J, Fabris, L, Farine, J, Feyzbakhsh, S, Fontaine, R, Fudenberg, D, Giacomini, G, Gornea, R, Gratta, G, Hansen, EV, Heffner, M, Hoppe, EW, Hößl, J, House, A, Hufschmidt, P, Hughes, M, Ito, Y, Jamil, A, Jessiman, C, Jewell, MJ, Jiang, XS, Karelin, A, Kaufman, LJ, Kodroff, D, Koffas, T, Kravitz, S, Krücken, R, Kuchenkov, A, Kumar, KS, Lan, Y, Larson, A, Leonard, DS, Li, G, Li, S, Li, Z, Licciardi, C, Lin, YH, Lv, P, MacLellan, R, Michel, T, Mong, B, Moore, DC, Murray, K, Newby, RJ, Ning, Z, Njoya, O, Nolet, F, Nusair, O, Odgers, K, Odian, A, Oriunno, M, Orrell, JL, Ortega, GS, Ostrovskiy, I, Overman, CT, Parent, S, and Piepke, A
Subjects: physics.ins-det, nucl-ex, Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, nEXO Collaboration, General Science & Technology
Abstract: The search for neutrinoless double beta decay probes the fundamentalproperties of neutrinos, including whether or not the neutrino and antineutrinoare distinct. Double beta detectors are large and expensive, so backgroundreduction is essential for extracting the highest sensitivity. Theidentification, or 'tagging', of the $^{136}$Ba daughter atom from double betadecay of $^{136}$Xe provides a technique for eliminating backgrounds in thenEXO neutrinoless double beta decay experiment. The tagging scheme studied inthis work utilizes a cryogenic probe to trap the barium atom in solid xenon,where the barium atom is tagged via fluorescence imaging in the solid xenonmatrix. Here we demonstrate imaging and counting of individual atoms of bariumin solid xenon by scanning a focused laser across a solid xenon matrixdeposited on a sapphire window. When the laser sits on an individual atom, thefluorescence persists for $\sim$30~s before dropping abruptly to the backgroundlevel, a clear confirmation of one-atom imaging. No barium fluorescencepersists following evaporation of a barium deposit to a limit of $\leq$0.16\%.This is the first time that single atoms have been imaged in solid nobleelement. It establishes the basic principle of a barium tagging technique fornEXO.
Published: 2019

44. Constraints on neutrino lifetime from the Sudbury Neutrino Observatory

Author: Aharmim, B, Ahmed, SN, Anthony, AE, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Bonventre, R, Boudjemline, K, Boulay, MG, Cai, B, Callaghan, EJ, Caravaca, J, Chan, YD, Chauhan, D, Chen, M, Cleveland, BT, Cox, GA, Dai, X, Deng, H, Descamps, FB, Detwiler, JA, Doe, PJ, Doucas, G, Drouin, P-L, Dunford, M, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Gagnon, N, Gilje, K, Goon, J TM, Graham, K, Guillian, E, Habib, S, Hahn, RL, Hallin, AL, Hallman, ED, Harvey, PJ, Hazama, R, Heintzelman, WJ, Heise, J, Helmer, RL, Hime, A, Howard, C, Huang, M, Jagam, P, Jamieson, B, Jelley, NA, Jerkins, M, Kéfélian, C, Keeter, KJ, Klein, JR, Kormos, LL, Kos, M, Krüger, A, Kraus, C, Krauss, CB, Kutter, T, Kyba, CCM, Land, BJ, Lange, R, Law, J, Lawson, IT, Lesko, KT, Leslie, JR, Levine, I, Loach, JC, MacLellan, R, Majerus, S, Mak, HB, Maneira, J, Martin, RD, Mastbaum, A, McCauley, N, McDonald, AB, McGee, SR, Miller, ML, Monreal, B, Monroe, J, Nickel, BG, Noble, AJ, O’Keeffe, HM, Oblath, NS, Okada, CE, Ollerhead, RW, Gann, GD Orebi, Oser, SM, Ott, RA, Peeters, SJM, Poon, AWP, Prior, G, and Reitzner, SD
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, hep-ex, nucl-ex
Abstract: The long baseline between Earth and the Sun makes solar neutrinos an excellent test beam for exploring possible neutrino decay. The signature of such decay would be an energy-dependent distortion of the traditional survival probability which can be fit for using well-developed and high-precision analysis methods. Here a model including neutrino decay is fit to all three phases of B8 solar neutrino data taken by the Sudbury Neutrino Observatory (SNO). This fit constrains the lifetime of neutrino mass state ν2 to be >8.08×10-5 s/eV at 90% confidence. An analysis combining this SNO result with those from other solar neutrino experiments results in a combined limit for the lifetime of mass state ν2 of >1.92×10-3 s/eV at 90% confidence.
Published: 2019

45. Tests of Lorentz invariance at the Sudbury Neutrino Observatory

Author: Aharmim, B, Ahmed, SN, Anthony, AE, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Blucher, E, Bonventre, R, Boudjemline, K, Boulay, MG, Cai, B, Callaghan, EJ, Caravaca, J, Chan, YD, Chauhan, D, Chen, M, Cleveland, BT, Cox, GA, Dai, X, Deng, H, Descamps, FB, Detwiler, JA, Doe, PJ, Doucas, G, Drouin, P-L, Dunford, M, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Gagnon, N, Gilje, K, Goon, J TM, Graham, K, Guillian, E, Habib, S, Hahn, RL, Hallin, AL, Hallman, ED, Harvey, PJ, Hazama, R, Heintzelman, WJ, Heise, J, Helmer, RL, Hime, A, Howard, C, Huang, M, Jagam, P, Jamieson, B, Jelley, NA, Jerkins, M, Kéfélian, C, Keeter, KJ, Klein, JR, Kormos, LL, Kos, M, Krüger, A, Kraus, C, Krauss, CB, Kutter, T, Kyba, CCM, Labe, K, Land, BJ, Lange, R, LaTorre, A, Law, J, Lawson, IT, Lesko, KT, Leslie, JR, Levine, I, Loach, JC, MacLellan, R, Majerus, S, Mak, HB, Maneira, J, Martin, RD, Mastbaum, A, McCauley, N, McDonald, AB, McGee, SR, Miller, ML, Monreal, B, Monroe, J, Nickel, BG, Noble, AJ, O’Keeffe, HM, Oblath, NS, Okada, CE, Ollerhead, RW, Gann, GD Orebi, Oser, SM, Ott, RA, and Peeters, SJM
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, hep-ex, nucl-ex
Abstract: Experimental tests of Lorentz symmetry in systems of all types are critical for ensuring that the basic assumptions of physics are well founded. Data from all phases of the Sudbury Neutrino Observatory, a kiloton-scale heavy water Cherenkov detector, are analyzed for possible violations of Lorentz symmetry in the neutrino sector. Such violations would appear as one of eight possible signal types in the detector: six seasonal variations in the solar electron neutrino survival probability differing in energy and time dependence and two shape changes to the oscillated solar neutrino energy spectrum. No evidence for such signals is observed, and limits on the size of such effects are established in the framework of the standard model extension, including 38 limits on previously unconstrained operators and improved limits on 16 additional operators. This makes limits on all minimal, Dirac-type Lorentz violating operators in the neutrino sector available for the first time.
Published: 2018

46. Search for nucleon decays with EXO-200

Author: Albert, J. B., Anton, G., Badhrees, I., Barbeau, P. S., Bayerlein, R., Beck, D., Belov, V., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Cree, W., Daniels, T., Danilov, M., Daugherty, S. J., Daughhetee, J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Didberidze, T., Dilling, J., Dolgolenko, A., Dolinski, M. J., Fairbank Jr., W., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fudenberg, D., Gornea, R., Graham, K., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Homiller, S., Hufschmidt, P., Hughes, M., Jamil, A., Jewell, M. J., Johnson, A., Johnston, S., Karelin, A., Kaufman, L. J., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Leonard, D. S., Li, G. S., Li, S., Licciardi, C., Lin, Y. H., MacLellan, R., Michel, T., Mong, B., Moore, D., Murray, K., Nelson, R., Njoya, O., Odian, A., Ostrovskiy, I., Piepke, A., Pocar, A., Retière, F., Robinson, A. L., Rowson, P. C., Schmidt, S., Schubert, A., Sinclair, D., Soma, A. K., Stekhanov, V., Tarka, M., Tolba, T., Tsang, R., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Waite, A., Walton, T., Weber, M., Wen, L. J., Wichoski, U., Wrede, G., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., Zettlemoyer, J., and Ziegler, T.
Subjects: High Energy Physics - Experiment, Nuclear Experiment, Physics - Instrumentation and Detectors
Abstract: A search for instability of nucleons bound in $^{136}$Xe nuclei is reported with 223 kg$\cdot$yr exposure of $^{136}$Xe in the EXO-200 experiment. Lifetime limits of 3.3$\times 10^{23}$ and 1.9$\times 10^{23}$ yrs are established for nucleon decay to $^{133}$Sb and $^{133}$Te, respectively. These are the most stringent to date, exceeding the prior decay limits by a factor of 9 and 7, respectively.
Published: 2017
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47. Sensitivity and discovery potential of the proposed nEXO experiment to neutrinoless double beta decay

Author: nEXO Collaboration, Albert, J. B., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bourque, F., Brodsky, J. P., Brown, E., Brunner, T., Burenkov, A., Cao, G. F., Cao, L., Cen, W. R., Chambers, C., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Côté, M., Craycraft, A., Cree, W., Dalmasson, J., Daniels, T., Daugherty, S. J., Daughhetee, J., DeVoe, R., Delaquis, S., Der Mesrobian-Kabakian, A., Didberidze, T., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Fabris, L., Fairbank, W., Farine, J., Feyzbakhsh, S., Fontaine, R., Fudenberg, D., Giacomini, G., Gornea, R., Graham, K., Gratta, G., Hansen, E. V., Harris, D., Hasan, M., Heffner, M., Hoppe, E. W., Hößl, J., House, A., Hufschmidt, P., Hughes, M., Ito, Y., Iverson, A., Jamil, A., Jewell, M. J., Jiang, X. S., Johnson, T. N., Johnston, S., Karelin, A., Kaufman, L. J., Killick, R., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Leonard, D. S., Li, G., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., Michel, T., Mong, B., Moore, D. C., Murray, K., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Odgers, K., Odian, A., Oriunno, M., Orrell, J. L., Ortega, G. S., Ostrovskiy, I., Overman, C. T., Parent, S., Piepke, A., Pocar, A., Pratte, J. -F., Qiu, D., Radeka, V., Raguzin, E., Rao, T., Rescia, S., Retière, F., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Saldanha, R., Sangiorgio, S., Schmidt, S., Schneider, J., Schubert, A., Sinclair, D., VIII, K. Skarpaas, Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Tarka, M., Todd, J., Tolba, T., Tsang, R., Tsang, T., Vachon, F., Veeraraghavan, V., Visser, G., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Wang, Q., Weber, M., Wei, W., Wen, L. J., Wichoski, U., Wrede, G., Wu, S. X., Wu, W. H., Yang, L., Yen, Y. -R., Zeldovich, O., Zettlemoyer, J., Zhang, X., Zhao, J., Zhou, Y., and Ziegler, T.
Subjects: Nuclear Experiment, Physics - Instrumentation and Detectors
Abstract: The next-generation Enriched Xenon Observatory (nEXO) is a proposed experiment to search for neutrinoless double beta ($0\nu\beta\beta$) decay in $^{136}$Xe with a target half-life sensitivity of approximately $10^{28}$ years using $5\times10^3$ kg of isotopically enriched liquid-xenon in a time projection chamber. This improvement of two orders of magnitude in sensitivity over current limits is obtained by a significant increase of the $^{136}$Xe mass, the monolithic and homogeneous configuration of the active medium, and the multi-parameter measurements of the interactions enabled by the time projection chamber. The detector concept and anticipated performance are presented based upon demonstrated realizable background rates., Comment: v2 as published
Published: 2017
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48. Characterization of an Ionization Readout Tile for nEXO

Author: nEXO Collaboration, Jewell, M., Schubert, A., Cen, W. R., Dalmasson, J., DeVoe, R., Fabris, L., Gratta, G., Jamil, A., Li, G., Odian, A., Patel, M., Pocar, A., Qiu, D., Wang, Q., Wen, L. J., Albert, J. B., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P., Beck, D., Belov, V., Bourque, F., Brodsky, J. P., Brown, E., Brunner, T., Burenkov, A., Cao, G. F., Cao, L., Chambers, C., Charlebois, S. A., Chiu, M., Cleveland, B., Coon, M., Craycraft, A., Cree, W., Côté, M., Daniels, T., Daugherty, S. J., Daughhetee, J., Delaquis, S., Der Mesrobian-Kabakian, A., Didberidze, T., Dilling, J., Ding, Y. Y., Dolinski, M. J., Dragone, A., Fairbank, W., Farine, J., Feyzbakhsh, S., Fontaine, R., Fudenberg, D., Giacomini, G., Gornea, R., Hansen, E. V., Harris, D., Hasan, M., Heffner, M., Hoppe, E. W., House, A., Hufschmidt, P., Hughes, M., Hößl, J., Ito, Y., Iverson, A., Jiang, X. S., Johnston, S., Karelin, A., Kaufman, L. J., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Leonard, D. S., Li, S., Li, Z., Licciardi, C., Lin, Y. H., MacLellan, R., Michel, T., Mong, B., Moore, D., Murray, K., Newby, R. J., Ning, Z., Njoya, O., Nolet, F., Odgers, K., Oriunno, M., Orrell, J. L., Ostrovskiy, I., Overman, C. T., Ortega, G. S., Parent, S., Piepke, A., Pratte, J. -F., Radeka, V., Raguzin, E., Rao, T., Rescia, S., Retiere, F., Robinson, A., Rossignol, T., Rowson, P. C., Roy, N., Saldanha, R., Sangiorgio, S., Schmidt, S., Schneider, J., Sinclair, D., Skarpaas, K., Soma, A. K., St-Hilaire, G., Stekhanov, V., Stiegler, T., Sun, X. L., Tarka, M., Todd, J., Tolba, T., Tsang, R., Tsang, T., Vachon, F., Veeraraghavan, V., Visser, G., Vuilleumier, J. -L., Wagenpfeil, M., Weber, M., Wei, W., Wichoski, U., Wrede, G., Wu, S. X., Wu, W. H., Xuan, Z., Yang, L., Yayun, D., Yen, Y. -R., Zeldovich, O., Zhang, X., Zhao, J., Zhe, N., Zhou, Y., and Ziegler, T.
Subjects: Physics - Instrumentation and Detectors
Abstract: A new design for the anode of a time projection chamber, consisting of a charge-detecting "tile", is investigated for use in large scale liquid xenon detectors. The tile is produced by depositing 60 orthogonal metal charge-collecting strips, 3~mm wide, on a 10~\si{\cm} $\times$ 10~\si{\cm} fused-silica wafer. These charge tiles may be employed by large detectors, such as the proposed tonne-scale nEXO experiment to search for neutrinoless double-beta decay. Modular by design, an array of tiles can cover a sizable area. The width of each strip is small compared to the size of the tile, so a Frisch grid is not required. A grid-less, tiled anode design is beneficial for an experiment such as nEXO, where a wire tensioning support structure and Frisch grid might contribute radioactive backgrounds and would have to be designed to accommodate cycling to cryogenic temperatures. The segmented anode also reduces some degeneracies in signal reconstruction that arise in large-area crossed-wire time projection chambers. A prototype tile was tested in a cell containing liquid xenon. Very good agreement is achieved between the measured ionization spectrum of a $^{207}$Bi source and simulations that include the microphysics of recombination in xenon and a detailed modeling of the electrostatic field of the detector. An energy resolution $\sigma/E$=5.5\% is observed at 570~\si{keV}, comparable to the best intrinsic ionization-only resolution reported in literature for liquid xenon at 936~V/\si{cm}., Comment: 18 pages, 13 figures, as published
Published: 2017
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49. Search for Neutrinoless Double-Beta Decay with the Upgraded EXO-200 Detector

Author: Albert, J. B., Anton, G., Badhrees, I., Barbeau, P. S., Bayerlein, R., Beck, D., Belov, V., Breidenbach, M., Brunner, T., Cao, G. F., Cen, W. R., Chambers, C., Cleveland, B., Coon, M., Craycraft, A., Cree, W., Daniels, T., Danilov, M., Daugherty, S. J., Daughhetee, J., Davis, J., Delaquis, S., Der Mesrobian-Kabakian, A., DeVoe, R., Didberidze, T., Dilling, J., Dolgolenko, A., Dolinski, M. J., Fairbank Jr., W., Farine, J., Feyzbakhsh, S., Fierlinger, P., Fudenberg, D., Gornea, R., Graham, K., Gratta, G., Hall, C., Hansen, E. V., Hoessl, J., Hufschmidt, P., Hughes, M., Jamil, A., Jewell, M. J., Johnson, A., Johnston, S., Karelin, A., Kaufman, L. J., Koffas, T., Kravitz, S., Krücken, R., Kuchenkov, A., Kumar, K. S., Lan, Y., Leonard, D. S., Li, G. S., Li, S., Licciardi, C., Lin, Y. H., MacLellan, R., Michel, T., Mong, B., Moore, D., Murray, K., Nelson, R., Njoya, O., Odian, A., Ostrovskiy, I., Piepke, A., Pocar, A., Retière, F., Rowson, P. C., Russell, J. J., Schmidt, S., Schubert, A., Sinclair, D., Stekhanov, V., Tarka, M., Tolba, T., Tsang, R., Vogel, P., Vuilleumier, J. -L., Wagenpfeil, M., Waite, A., Walton, T., Weber, M., Wen, L. J., Wichoski, U., Wrede, G., Yang, L., Yen, Y. -R., Zeldovich, O. Ya., Zettlemoyer, J., and Ziegler, T.
Subjects: High Energy Physics - Experiment, Nuclear Experiment
Abstract: Results from a search for neutrinoless double-beta decay $0\nu\beta\beta$ of $^{136}$Xe are presented using the first year of data taken with the upgraded EXO-200 detector. Relative to previous searches by EXO-200, the energy resolution of the detector has been improved to $\sigma/E$=1.23%, the electric field in the drift region has been raised by 50%, and a system to suppress radon in the volume between the cryostat and lead shielding has been implemented. In addition, analysis techniques that improve topological discrimination between $0\nu\beta\beta$ and background events have been developed. Incorporating these hardware and analysis improvements, the median 90% confidence level $0\nu\beta\beta$ half-life sensitivity after combining with the full data set acquired before the upgrade has increased 2-fold to $3.7 \times 10^{25}$ yr. No statistically significant evidence for $0\nu\beta\beta$ is observed, leading to a lower limit on the $0\nu\beta\beta$ half-life of $1.8\times10^{25}$ yr at the 90% confidence level., Comment: 6 pages, 4 figures, final version submitted to PRL
Published: 2017
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50. The Single-Phase ProtoDUNE Technical Design Report

Author: Abi, B., Acciarri, R., Acero, M. A., Adamowski, M., Adams, C., Adams, D. L., Adamson, P., Adinolfi, M., Ahmad, Z., Albright, C. H., Alion, T., Anderson, J., Anderson, K., Andreopoulos, C., Andrews, M. P., Andrews, R. A., Anjos, J. dos, Ankowski, A., Anthony, J., Antonello, M., Fernandez, A. Aranda, Ariga, A., Ariga, T., Diaz, E. Arrieta, Asaadi, J., Ascencio, M., Asner, D. M., Athar, M. S., Auger, M., Aurisano, A., Aushev, V., Autiero, D., Azfar, F., Back, J. J., Back, H. O., Backhouse, C., Bai, X., Baird, M., Balantekin, A. B., Balasubramanian, S., Baller, B., Ballett, P., Bambah, B., Band, H., Bansal, M., Bansal, S., Barker, G. J., Barr, G., Monarca, J. Barranco, Barros, N., Bashyal, A., Bass, M., Bay, F., Bazo, J. L., Beacom, J. F., Behera, B. R., Bellettini, G., Bellini, V., Beltramello, O., Benekos, N., Benetti, P. A., Bercellie, A., Berman, E., Berns, H., Bernstein, R., Bertolucci, S., Bhatnagar, V., Bhuyan, B., Bian, J., Biery, K., Bishai, M., Bitadze, A., Blackburn, T., Blake, A., Blaszczyk, F. d. M., Blaufuss, E., Blazey, G. C., Blennow, M., Blucher, E., Bocean, V., Boffelli, F., Boissevain, J., Bolognesi, S., Bolton, T., Bonesini, M., Boone, T., Booth, C., Bordoni, S., Bour, P., Bourguille, B., Boyd, S. B., Boyden, D., Brailsford, D., Brandt, A., Bremer, J., Brice, S. J., Bromberg, C., Brooijmans, G., Brown, G., Brunetti, G., Buchanan, N., Budd, H., Calafiura, P., Calatayud, A., Calligarich, E., Calvo, E., Camilleri, L., Campanelli, M., Cantini, C., Carls, B., Cascella, M., Catano-Mur, E., Cavaili-Sforza, M., Cavanna, F., Centro, S., Villanueva, A. Cervera, Cervi, T., Chalifour, M., Chappuis, A., Chatterjee, A., Chattopadhyay, S., Chaussard, L., Chembra, S., Chen, H., Chen, M., Cherdack, D., Chi, C., Childress, S., Choubey, S., Choudhary, B. C., Christodoulou, G., Christofferson, C., Church, E., Coan, T. E., Cocco, A., Cole, P., Collin, G., Conrad, J. M., Convery, M., Corey, R., Corwin, L., Crespo-Anadón, J. I., Prats, J. Creus, Crivelli, P., Cronin-Hennessy, D., Crowley, C., Curioni, A., Cussans, D., da Motta, H., Dale, D., Davenne, T., Davies, G. S., Davies, J., Dawson, J., De, K., De Bonis, I., De Gouvea, A., de Holanda, P. C., De Jong, P., De Lurgio, P., de Vries, J. J., Decowski, M. P., Dedin-Neto, P., Delbart, A., Delepine, D., Delgado, M., Demuth, D., Dennis, S., Densham, C., Dharmapalan, R., Dhingra, N., Diamantopoulou, M., Diaz, J. S., Bautista, G. Diaz, Ding, P., Diwan, M., Djurcic, Z., Dolinski, M. J., Drake, G., Duchesneau, D., Dutta, D., Duvernois, M., Duyang, H., Dwyer, D. A., Dye, S., Dyshkant, A. S., Dytman, S., Eads, M., Eberly, B., Edmunds, D., Elliott, S., Ellsworth, W. M., Elnimr, M., Emery, S., Eno, S., Ereditato, A., Escobar, C. O., Sanchez, L. Escudero, Evans, J. J., Fahey, K., Falcone, A., Falk, L., Farbin, A., Farnese, C., Farzan, Y., Fasoli, M., Fava, A., Felix, J., Menendez, P. Fernandez, Fernandez-Martinez, E., Fields, L., Filthaut, F., Finch, A., Fitton, M., Fleming, B. T., Forest, T., Fowler, J., Fox, W., Freeman, J., Freestone, J., Friant, D., Fried, J., Friedland, A., Fuess, S., Fujikawa, B., Gago, A., Gallagher, H., Galvin, S., Galymov, S., Gamble, T., Gandhi, R., Gao, S., Garcia-Gamez, D., Gardiner, S., Gastler, D., Gendotti, A., Gibin, D., Gil-Botella, I., Gill, R., Giri, A. K., Goeldi, D., Gold, M., Gollapinni, S., Gomes, R. A., Cadenas, J. J. Gomez, Goodman, M. C., Gorbunov, D., Goswami, S., Graf, N., Graham, M., Gramelini, E., Gran, R., Grant, C., Grant, N., Greco, V., Greenlee, H., Greenler, L., Groh, M., Grzelak, K., Guardincerri, E., Guarino, V., Guedes, G. P., Guenette, R., Guglielmi, A., Guthikonda, K. K., Guzzo, M. M., Habig, A. T., Hackenburg, A., Hackenburg, R. W., Hadavand, H., Haenni, R., Hahn, A., Haigh, M. 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K., Warner, D., Wascko, M., Waters, D., Weber, A., Weber, M., Wei, W., Weinstein, A., Wenman, D., Wetstein, M., White, A., Whitehead, L. H., Whittington, D., Wilking, M. J., Willhite, J., Wilson, P., Wilson, R. J., Wittich, P., Wolcott, J., Wong, H. H., Wongjirad, T., Wood, K., Wood, L. S., Worcester, E., Worcester, M., Wu, S., Xu, W., Yanagisawa, C., Yang, S., Yang, T., Ye, J., Yeh, M., Yershov, N., Yonehara, K., Yu, B., Yu, J., Zalesak, J., Zambelli, L., Zamorano, B., Zang, L., Zani, A., Zaremba, K., Zeller, G. P., Zhang, C., Zhou, Y., Zimmerman, E. D., Zito, M., Zuklin, J., Zutshi, V., and Zwaska, R.
Subjects: Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract: ProtoDUNE-SP is the single-phase DUNE Far Detector prototype that is under construction and will be operated at the CERN Neutrino Platform (NP) starting in 2018. ProtoDUNE-SP, a crucial part of the DUNE effort towards the construction of the first DUNE 10-kt fiducial mass far detector module (17 kt total LAr mass), is a significant experiment in its own right. With a total liquid argon (LAr) mass of 0.77 kt, it represents the largest monolithic single-phase LArTPC detector to be built to date. It's technical design is given in this report., Comment: 165 pages, fix references, author list and minor numbers
Published: 2017

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