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arXiv 2203.00740physics.ins-dethep-ex
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中微子低能物理学LArTPCs

Low-Energy Physics in Neutrino LArTPCs

D. Caratelli, W. Foreman, A. Friedland, S. Gardiner, I. Gil-Botella, G. Karagiorgi, M. Kirby, G. Lehmann Miotto, B. R. Littlejohn, M. Mooney, J. Reichenbacher, … 展开作者

D. Caratelli, W. Foreman, A. Friedland, S. Gardiner, I. Gil-Botella, G. Karagiorgi, M. Kirby, G. Lehmann Miotto, B. R. Littlejohn, M. Mooney, J. Reichenbacher, A. Sousa, K. Scholberg, J. Yu, T. Yang, S. Andringa, J. Asaadi, T. J. C. Bezerra, F. Capozzi, F. Cavanna, E. Church, A. Himmel, T. Junk, J. Klein, I. Lepetic, S. Li, P. Sala, H. Schellman, M. Sorel, J. Wang, M. H. L. S. Wang, W. Wu, J. Zennamo, M. A. Acero, M. R. Adames, H. Amar, D. A. Andrade, C. Andreopoulos, A. M. Ankowski, M. A. Arroyave, V. Aushev, M. A. Ayala-Torres, P. Baldi, C. Backhouse, A. B. Balantekin, W. A. Barkhouse, P. Barham Alzas, J. L. Barrow, J. B. R. Battat, M. C. Q. Bazetto, J. F. Beacom, B. Behera, G. Bellettini, J. Berger, A. T. Bezerra, J. Bian, B. Bilki, B. Bles, T. Bolton, L. Bomben, M. Bonesini, C. Bonilla-Diaz, F. Boran, A. N. Borkum, N. Bostan, D. Brailsford, A. Branca, G. Brunetti, T. Cai, A. Chappell, N. Charitonidis, P. H. P. Cintra, E. Conley, T. E. Coan, P. Cova, L. M. Cremaldi, J. I. Crespo-Anadon, C. Cuesta, R. Dallavalle, G. S. Davies, S. De, P. Dedin Neto, M. Delgado, N. Delmonte, P. B. Denton, A. De Roeck, R. Dharmapalan, Z. Djurcic, F. Dolek, S. Doran, R. Dorrill, K. E. Duffy, B. Dutta, O. Dvornikov, S. Edayath, J. J. Evans, A. C. Ezeribe, A. Falcone, M. Fani, J. Felix, Y. Feng, L. Fields, P. Filip, G. Fiorillo, D. Franco, D. Garcia-Gamez, A. Giri, O. Gogota, S. Gollapinni, M. Goodman, E. Gramellini, R. Gran, P. Granger, C. Grant, S. E. Greenberg, M. Groh, R. Guenette, D. Guffanti, D. A. Harris, A. Hatzikoutelis, K. M. Heeger, M. Hernandez Morquecho, K. Herner, J. Ho, P C. Holanda, N. Ilic, C. M. Jackson, W. Jang, H. -Th. Janka, J. H. Jo, F. R. Joaquim, R. S. Jones, N. Jovancevic, Y. -J. Jwa, D. Kalra, D. M. Kaplan, I. Katsioulas, E. Kearns, K. J. Kelly, E. Kemp, W. Ketchum, A. Kish, L. W. Koerner, T. Kosc, K. Kothekar, I. Kreslo, S. Kubota, V. A. Kudryavtsev, P. Kumar, T. Kutter, J. Kvasnicka, I. Lazanu, T. LeCompte, Y. Li, Y. Liu, M. Lokajicek, W. C. Louis, K. B. Luk, X. Luo, P. A. N. Machado, I. M. Machulin, K. Mahn, M. Man, R. C. Mandujano, J. Maneira, A. Marchionni, D. Marfatia, F. Marinho, C. Mariani, C. M. Marshall, F. Martinez Lopez, D. A. Martinez Caicedo, A. Mastbaum, M. Matheny, N. McConkey, P. Mehta, O. E. B. Messer, A. Minotti, O. G. Miranda, P. Mishra, I. Mocioiu, A. Mogan, R. Mohanta, T. Mohayai, C. Montanari, L. M. Montano Zetina, A. F. Moor, D. Moretti, C. A. Moura, L. M. Mualem, J. Nachtman, S. Narita, A. Navrer-Agasson, M. Nebot-Guinot, J. Nikolov, J. A. Nowak, J. P. Ochoa-Ricoux, E. O'Connor, Y. Onel, Y. Onishchuk, G. D. Orebi Gann, V. Pandey, E. G. Parozzi, S. Parveen, M. Parvu, R. B. Patterson, L. Paulucci, V. Pec, S. J. M. Peeters, F. Pompa, N. Poonthottathil, S. S. Poudel, F. Psihas, A. Rafique, B. J. Ramson, J. S. Real, A. Rikalo, M. Ross-Lonergan, B. Russell, S. Sacerdoti, N. Sahu, D. A. Sanders, D. Santoro, M. V. Santos, C. R. Senise, P. N. Shanahan, H. R Sharma, R. K. Sharma, W. Shi, S. Shin, J. Singh, J. Singh, L. Singh, P. Singh, V. Singh, M. Soderberg, S. Soldner-Rembold, J. Soto-Oton, K. Spurgeon, A. F. Steklain, F. Stocker, T. Stokes, J. Strait, M. Strait, T. Strauss, L. Suter, R. Svoboda, A. M. Szelc, M. Szydagis, E. Tarpara, E. Tatar, F. Terranova, G. Testera, N. Chithirasree, N. Todorovic, A. Tonazzo, M. Torti, F. Tortorici, M. Toups, D. Q. Tran, M. Travar, Y. -D. Tsai, Y. -T. Tsai, S. Z. Tu, J. Urheim, H. Utaegbulam, S. Valder, G. A. Valdiviesso, R. Valentim, S. Vergani, B. Viren, A. Vranicar, B. Wang, D. Waters, P. Weatherly, M. Weber, H. Wei, S. Westerdale, L. H. Whitehead, D. Whittington, A. Wilkinson, R. J. Wilson, M. Worcester, K. Wresilo, B. Yaeggy, G. Yang, J. Zalesak, B. Zamorano, J. Zuklin

摘要:

在本白皮书中,我们概述了与液态氩时间投影室(LArTPC)探测器中低能(小于100 MeV)特征的探测和重建相关的一些科学机遇和挑战。主要结论总结如下。1)LArTPC具有独特的灵敏度,通过检测事件的功能,在几十兆电子伏的范围内和以下的一系列物理和天体物理学的签名。2)低能特征信号是GeV量级加速器中微子相互作用末态的重要组成部分,它们的重建可以提高LArTPC实验的振荡物理灵敏度。3)来自加速器和自然源的BSM信号也在低能量范围内生成不同的签名,并且这些签名的重建可以增加基于LArTPC的搜索中可访问的BSM场景的广度。4)中微子相互作用的截面和其他核物理过程中的氩有关的子百兆电子伏LArTPC签名知之甚少。需要改进的理论和实验测量。π介子静止衰变源和带电粒子和中子试验束是通过实验提高这种认识的理想设施。5)在低能量范围内有具体的校准需要,以及控制和了解放射性和宇宙成因背景的具体需要。6)应探索未来LArTPC技术的新想法,以提高低能耗能力。这些措施包括新的电荷增强和读出系统,增强光子探测,低放射性氩,氙掺杂。7)低能量特征,无论是稳态还是超新星爆发或更大GeV级事件拓扑的一部分,都具有特定的触发,DAQ和重建要求,必须在传统GeV级数据收集和分析途径的范围之外解决。

英文摘要:

In this white paper, we outline some of the scientific opportunities and challenges related to detection and reconstruction of low-energy (less than 100 MeV) signatures in liquid argon time-projection chamber (LArTPC) detectors. Key takeaways are summarized as follows. 1) LArTPCs have unique sensitivity to a range of physics and astrophysics signatures via detection of event features at and below the few tens of MeV range. 2) Low-energy signatures are an integral part of GeV-scale accelerator neutrino interaction final states, and their reconstruction can enhance the oscillation physics sensitivities of LArTPC experiments. 3) BSM signals from accelerator and natural sources also generate diverse signatures in the low-energy range, and reconstruction of these signatures can increase the breadth of BSM scenarios accessible in LArTPC-based searches. 4) Neutrino interaction cross sections and other nuclear physics processes in argon relevant to sub-hundred-MeV LArTPC signatures are poorly understood. Improved theory and experimental measurements are needed. Pion decay-at-rest sources and charged particle and neutron test beams are ideal facilities for experimentally improving this understanding. 5) There are specific calibration needs in the low-energy range, as well as specific needs for control and understanding of radiological and cosmogenic backgrounds. 6) Novel ideas for future LArTPC technology that enhance low-energy capabilities should be explored. These include novel charge enhancement and readout systems, enhanced photon detection, low radioactivity argon, and xenon doping. 7) Low-energy signatures, whether steady-state or part of a supernova burst or larger GeV-scale event topology, have specific triggering, DAQ and reconstruction requirements that must be addressed outside the scope of conventional GeV-scale data collection and analysis pathways.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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