Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos

Agnes, P.; Albergo, S.; Albuquerque, I. F. M.; Alexander, T.; Alici, A.; Alton, A. K.; Amaudruz, P.; Arcelli, S.; Ave, M.; Avetissov, I. Ch; Avetisov, I, R.; Azzolini, O.; Back, H. O.; Balmforth, Z.; Barbarian, V; Olmedo, A. Barrado; Barrillon, P.; Basco, A.; Batignani, G.; Bondar, A.; Bonivento, W. M.; Borisova, E.; Bottino, B.; Boulay, M. G.; Buccino, G.; Bussino, S.; Busto, J.; Buzulutskov, A.; Cadeddu, M.; Cadoni, M.; Caminata, A.; Canci, N.; Cappello, G.; Caravati, M.; Cardenas-Montes, M.; Carlini, M.; Carnesecchi, F.; Castello, P.; Catalanotti, S.; Cataudella, V; Cavalcante, P.; Cavuoti, S.; Cebrian, S.; Ruiz, J. M. Cela; Celano, B.; Chashin, S.; Chepurnov, A.; Chyhyrynets, E.; Cicalo, C.; Cifarelli, L.; Cintas, D.; Coccetti, F.; Cocco, V; Colocci, M.; Vilda, E. Conde; Consiglio, L.; Copello, S.; Corning, J.; Covone, G.; Czudak, P.; D'Auria, S.; Rolo, M. D. Da Rocha; Dadoun, O.; Daniel, M.; Davini, S.; De Candia, A.; De Cecco, S.; De Falco, A.; De Filippis, G.; De Gruttola, D.; De Guido, G.; De Rosa, G.; Della Valle, M.; Dellacasa, G.; De Pasquale, S.; Derbin, V, A.; Devoto, A.; Di Noto, L.; Dionisi, C.; Di Stefano, P.; Dolganov, G.; Dordei, F.; Doria, L.; Downing, M.; Erjavec, T.; Diaz, M. Fernandez; Fiorillo, G.; Franceschi, A.; Franco, D.; Frolov, E.; Funicello, N.; Gabriele, F.; Galbiati, C.; Garbini, M.; Abia, P. Garcia; Gendotti, A.; Ghiano, C.; Giampaolo, R. A.; Giganti, C.; Giorgi, M. A.; Giovanetti, G. K.; Casanueva, V. Goicoechea; Gola, A.; Diaz, R. Graciani; Grigoriev, G. Y.; Grobov, A.; Gromov, M.; Guan, M.; Guerzoni, M.; Gulino, M.; Guo, C.; Hackett, B. R.; Hallin, A.; Haranczyk, M.; Hill, S.; Horikawa, S.; Hubaut, F.; Hugues, T.; Hungerford, V, E.; Ianni, An; Ippolito, V; James, C. C.; Jillings, C.; Kachru, P.; Kemp, A. A.; Kendziora, C. L.; Keppel, G.; Khomyakov, V, A.; Kim, S.; Kish, A.; Kochanek, I; Kondo, K.; Korga, G.; Kubankin, A.; Kugathasan, R.; Kuss, M.; Kuzniak, M.; La Commara, M.; Lai, M.; Langrock, S.; Leyton, M.; Li, X.; Lidey, L.; Lissia, M.; Longo, G.; Machulin, I. N.; Mapelli, L.; Marasciulli, A.; Margotti, A.; Mari, S. M.; Maricic, J.; Martinez, M.; Rojas, A. D. Martinez; Martoff, C. J.; Masoni, A.; Mazzi, A.; McDonald, A. B.; Mclaughlin, J.; Messina, A.; Meyers, P. D.; Miletic, T.; Milincic, R.; Moggi, A.; Moharana, A.; Moioli, S.; Monroe, J.; Morisi, S.; Morrocchi, M.; Mozhevitina, E. N.; Mroz, T.; Muratova, V. N.; Muscas, C.; Musenich, L.; Musico, P.; Nania, R.; Napolitano, T.; Agasson, A. Navrer; Nessi, M.; Nikulin, I; Nowak, J.; Oleinik, A.; Oleynikov, V; Pagani, L.; Pallavicini, M.; Pandola, L.; Pantic, E.; Paoloni, E.; Paternoster, G.; Pegoraro, P. A.; Pelczar, K.; Pellegrini, L. A.; Pellegrino, C.; Perotti, F.; Pesudo, V; Picciau, E.; Pietropaolo, F.; Pira, C.; Pocar, A.; Poehlmann, D. M.; Pordes, S.; Poudel, S. S.; Pralavorio, P.; Price, D.; Raffaelli, F.; Ragusa, F.; Ramirez, A.; Razeti, M.; Razeto, A.; Renshaw, A. L.; Rescia, S.; Rescigno, M.; Resnati, F.; Retiere, F.; Rignanese, L. P.; Ripoli, C.; Rivetti, A.; Rode, J.; Romero, L.; Rossi, M.; Rubbia, A.; Salatino, P.; Samoylov, O.; Garcia, E. Sanchez; Sandford, E.; Sanfilippo, S.; Santone, D.; Santorelli, R.; Savarese, C.; Scapparone, E.; Schlitzer, B.; Scioli, G.; Semenov, D. A.; Shaw, B.; Shchagin, A.; Sheshukov, A.; Simeone, M.; Skensved, P.; Skorokhvatov, M. D.; Smirnov, O.; Smith, B.; Sokolov, A.; Steri, A.; Stracka, S.; Strickland, V; Stringer, M.; Sulis, S.; Suvorov, Y.; Szelc, A. M.; Tartaglia, R.; Testera, G.; Thorpe, T. N.; Tonazzo, A.; Torres-Lara, S.; Tricomi, A.; Unzhakov, V, E.; Usai, G.; John, T. Vallivilayil; Viant, T.; Viel, S.; Vishneva, A.; Vogelaar, R. B.; Wada, M.; Wang, H.; Wang, Y.; Westerdale, S.; Wheadon, R. J.; Williams, L.; Wojcik, Ma M.; Wojcik, Ma; Xiao, X.; Yang, C.; Ye, Z.; Zani, A.; Zichichi, A.; Zuzel, G.; Zykova, M. P.

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Author(s): Show less -	Agnes, P. ^[1] ; Albergo, S. ^{[2, 3]} ; Albuquerque, I. F. M. ^[4] ; Alexander, T. ^[5] ; Alici, A. ^{[6, 7]} ; Alton, A. K. ^[8] ; Amaudruz, P. ^[9] ; Arcelli, S. ^{[6, 7]} ; Ave, M. ^[4] ; Avetissov, I. Ch ^[10] ; Avetisov, I, R. ; Azzolini, O. ^[11] ; Back, H. O. ^[5] ; Balmforth, Z. ^[12] ; Barbarian, V ^[13] ; Olmedo, A. Barrado ^[14] ; Barrillon, P. ^[15] ; Basco, A. ^[16] ; Batignani, G. ^{[17, 18]} ; Bondar, A. ^{[19, 20]} ; Bonivento, W. M. ^[21] ; Borisova, E. ^{[19, 20]} ; Bottino, B. ^{[22, 23]} ; Boulay, M. G. ^[24] ; Buccino, G. ^[25] ; Bussino, S. ^{[26, 27]} ; Busto, J. ^[15] ; Buzulutskov, A. ^{[19, 20]} ; Cadeddu, M. ^{[21, 28]} ; Cadoni, M. ^{[21, 28]} ; Caminata, A. ^[22] ; Canci, N. ^[29] ; Cappello, G. ^{[2, 3]} ; Caravati, M. ^[21] ; Cardenas-Montes, M. ^[14] ; Carlini, M. ^[30] ; Carnesecchi, F. ^{[6, 7, 31]} ; Castello, P. ^{[21, 32]} ; Catalanotti, S. ^{[16, 33]} ; Cataudella, V ^{[16, 33]} ; Cavalcante, P. ^[29] ; Cavuoti, S. ^{[16, 33, 34]} ; Cebrian, S. ^[35] ; Ruiz, J. M. Cela ^[14] ; Celano, B. ^[16] ; Chashin, S. ^[13] ; Chepurnov, A. ^[13] ; Chyhyrynets, E. ^[11] ; Cicalo, C. ^[21] ; Cifarelli, L. ^{[6, 7]} ; Cintas, D. ^[35] ; Coccetti, F. ^[31] ; Cocco, V ^[21] ; Colocci, M. ^{[6, 7]} ; Vilda, E. Conde ^[14] ; Consiglio, L. ^[29] ; Copello, S. ^{[22, 23]} ; Corning, J. ^[36] ; Covone, G. ^{[16, 33]} ; Czudak, P. ^[37] ; D'Auria, S. ^[38] ; Rolo, M. D. Da Rocha ^[39] ; Dadoun, O. ^[40] ; Daniel, M. ^[14] ; Davini, S. ^[22] ; De Candia, A. ^{[16, 33]} ; De Cecco, S. ^{[41, 42]} ; De Falco, A. ^{[21, 28]} ; De Filippis, G. ^{[16, 33]} ; De Gruttola, D. ^{[43, 44]} ; De Guido, G. ^[45] ; De Rosa, G. ^{[16, 33]} ; Della Valle, M. ^{[16, 34]} ; Dellacasa, G. ^[39] ; De Pasquale, S. ^{[43, 44]} ; Derbin, V, A. ; Devoto, A. ^{[21, 28]} ; Di Noto, L. ^[22] ; Dionisi, C. ^{[41, 42]} ; Di Stefano, P. ^[36] ; Dolganov, G. ^[46] ; Dordei, F. ^[21] ; Doria, L. ^[47] ; Downing, M. ^{[48, 49]} ; Erjavec, T. ^[50] ; Diaz, M. Fernandez ^[14] ; Fiorillo, G. ^{[16, 33]} ; Franceschi, A. ^[51] ; Franco, D. ^[52] ; Frolov, E. ^{[19, 20]} ; Funicello, N. ^{[43, 44]} ; Gabriele, F. ^[29] ; Galbiati, C. ^{[30, 53, 29]} ; Garbini, M. ^{[6, 31]} ; Abia, P. Garcia ^[14] ; Gendotti, A. ^[54] ; Ghiano, C. ^[29] ; Giampaolo, R. A. ^{[39, 55]} ; Giganti, C. ^[40] ; Giorgi, M. A. ^{[17, 18]} ; Giovanetti, G. K. ^[56] ; Casanueva, V. Goicoechea ^[57] ; Gola, A. ^{[58, 59]} ; Diaz, R. Graciani ^[60] ; Grigoriev, G. Y. ^[46] ; Grobov, A. ^{[46, 61]} ; Gromov, M. ^{[62, 13]} ; Guan, M. ^[63] ; Guerzoni, M. ^[6] ; Gulino, M. ^{[64, 65]} ; Guo, C. ^[63] ; Hackett, B. R. ^[5] ; Hallin, A. ^[66] ; Haranczyk, M. ^[37] ; Hill, S. ^[12] ; Horikawa, S. ^{[30, 29]} ; Hubaut, F. ^[15] ; Hugues, T. ^[67] ; Hungerford, V, E. ; Ianni, An ^{[53, 29]} ; Ippolito, V ^[41] ; James, C. C. ^[68] ; Jillings, C. ^{[69, 70]} ; Kachru, P. ^{[30, 29]} ; Kemp, A. A. ^[36] ; Kendziora, C. L. ^[68] ; Keppel, G. ^[11] ; Khomyakov, V, A. ; Kim, S. ^[71] ; Kish, A. ^[57] ; Kochanek, I ^[29] ; Kondo, K. ^[29] ; Korga, G. ^[12] ; Kubankin, A. ^[72] ; Kugathasan, R. ^{[39, 55]} ; Kuss, M. ^[17] ; Kuzniak, M. ^[67] ; La Commara, M. ^{[16, 73]} ; Lai, M. ^{[21, 28, 52]} ; Langrock, S. ^[69] ; Leyton, M. ^[16] ; Li, X. ^[53] ; Lidey, L. ^[5] ; Lissia, M. ^[21] ; Longo, G. ^{[16, 33]} ; Machulin, I. N. ^{[46, 61]} ; Mapelli, L. ^[53] ; Marasciulli, A. ^[18] ; Margotti, A. ^[6] ; Mari, S. M. ^{[26, 27]} ; Maricic, J. ^[57] ; Martinez, M. ^{[35, 74]} ; Rojas, A. D. Martinez ^{[39, 55]} ; Martoff, C. J. ^[71] ; Masoni, A. ^[21] ; Mazzi, A. ^{[58, 59]} ; McDonald, A. B. ^[36] ; Mclaughlin, J. ^{[9, 12]} ; Messina, A. ^{[41, 42]} ; Meyers, P. D. ^[53] ; Miletic, T. ^[57] ; Milincic, R. ^[57] ; Moggi, A. ^[17] ; Moharana, A. ^{[30, 29]} ; Moioli, S. ^[45] ; Monroe, J. ^[12] ; Morisi, S. ^{[16, 33]} ; Morrocchi, M. ^{[17, 18]} ; Mozhevitina, E. N. ^[75] ; Mroz, T. ^[37] ; Muratova, V. N. ^[76] ; Muscas, C. ^{[21, 32]} ; Musenich, L. ^{[22, 23]} ; Musico, P. ^[22] ; Nania, R. ^[6] ; Napolitano, T. ^[51] ; Agasson, A. Navrer ^[40] ; Nessi, M. ^[25] ; Nikulin, I ^[72] ; Nowak, J. ^[77] ; Oleinik, A. ^[72] ; Oleynikov, V ^{[19, 20]} ; Pagani, L. ^[50] ; Pallavicini, M. ^{[22, 23]} ; Pandola, L. ^[64] ; Pantic, E. ^[50] ; Paoloni, E. ^{[17, 18]} ; Paternoster, G. ^{[58, 59]} ; Pegoraro, P. A. ^{[21, 32]} ; Pelczar, K. ^[37] ; Pellegrini, L. A. ^[45] ; Pellegrino, C. ^{[6, 31]} ; Perotti, F. ^{[38, 78]} ; Pesudo, V ^[14] ; Picciau, E. ^{[21, 28]} ; Pietropaolo, F. ^[25] ; Pira, C. ^[11] ; Pocar, A. ^{[48, 49]} ; Poehlmann, D. M. ^[50] ; Pordes, S. ^[68] ; Poudel, S. S. ^[79] ; Pralavorio, P. ^[15] ; Price, D. ^[80] ; Raffaelli, F. ^[17] ; Ragusa, F. ^{[81, 38]} ; Ramirez, A. ^[79] ; Razeti, M. ^[21] ; Razeto, A. ^[29] ; Renshaw, A. L. ^[79] ; Rescia, S. ^[82] ; Rescigno, M. ^[41] ; Resnati, F. ^[25] ; Retiere, F. ^[9] ; Rignanese, L. P. ^{[6, 7]} ; Ripoli, C. ^{[43, 44]} ; Rivetti, A. ^[39] ; Rode, J. ^{[52, 40]} ; Romero, L. ^[14] ; Rossi, M. ^{[22, 23]} ; Rubbia, A. ^[54] ; Salatino, P. ^{[16, 83]} ; Samoylov, O. ^[62] ; Garcia, E. Sanchez ^[14] ; Sandford, E. ^[80] ; Sanfilippo, S. ^{[26, 27]} ; Santone, D. ^[12] ; Santorelli, R. ^[14] ; Savarese, C. ^[53] ; Scapparone, E. ^[6] ; Schlitzer, B. ^[50] ; Scioli, G. ^{[6, 7]} ; Semenov, D. A. ^[76] ; Shaw, B. ^[9] ; Shchagin, A. ^[72] ; Sheshukov, A. ^[62] ; Simeone, M. ^{[16, 83]} ; Skensved, P. ^[36] ; Skorokhvatov, M. D. ^{[46, 61]} ; Smirnov, O. ^[62] ; Smith, B. ^[9] ; Sokolov, A. ^{[19, 20]} ; Steri, A. ^[21] ; Stracka, S. ^[17] ; Strickland, V ^[24] ; Stringer, M. ^[36] ; Sulis, S. ^{[21, 32]} ; Suvorov, Y. ^{[46, 16, 33]} ; Szelc, A. M. ^[80] ; Tartaglia, R. ^[29] ; Testera, G. ^[22] ; Thorpe, T. N. ^{[30, 29]} ; Tonazzo, A. ^[52] ; Torres-Lara, S. ^[79] ; Tricomi, A. ^{[2, 3]} ; Unzhakov, V, E. ; Usai, G. ^{[21, 28]} ; John, T. Vallivilayil ^{[30, 29]} ; Viant, T. ^[54] ; Viel, S. ^[24] ; Vishneva, A. ^[62] ; Vogelaar, R. B. ^[84] ; Wada, M. ^[67] ; Wang, H. ^[85] ; Wang, Y. ^[85] ; Westerdale, S. ^[21] ; Wheadon, R. J. ^[39] ; Williams, L. ^[86] ; Wojcik, Ma M. ^[37] ; Wojcik, Ma ^[87] ; Xiao, X. ^[85] ; Yang, C. ^[63] ; Ye, Z. ^[79] ; Zani, A. ^[25] ; Zichichi, A. ^{[6, 7]} ; Zuzel, G. ^[37] ; Zykova, M. P. ^[75] Total Authors: 276
Affiliation: Show less -	^[1] Univ Houston, Dept Phys, Houston, TX 77204 - USA ^[2] Univ Catania, I-95124 Catania - Italy ^[3] INFN Catania, I-95121 Catania - Italy ^[4] Univ Sao Paulo, Inst Fis, BR-05508090 Sao Paulo, SP - Brazil ^[5] Pacific Northwest Natl Lab, Richland, WA 99352 - USA ^[6] INFN Bologna, I-40126 Bologna - Italy ^[7] Univ Bologna, Phys Dept, I-40126 Bologna - Italy ^[8] Augustana Univ, Phys Dept, Sioux Falls, SD 57197 - USA ^[9] TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3 - Canada ^[10] Mendeleev Univ Chem Technol, Moscow 125047 - Russia ^[11] Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Legnaro - Italy ^[12] Royal Holloway Univ London, Dept Phys, Egham TW20 0EX, Surrey - England ^[13] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119234 - Russia ^[14] CIEMAT, Ctr Invest Energet Medioambientales & Tecnol, Madrid 28040 - Spain ^[15] Aix Marseille Univ, Ctr Phys Particules Marseille, CNRS, IN2P3, CPPM, Marseille - France ^[16] INFN Napoli, I-80126 Naples - Italy ^[17] INFN Pisa, I-56127 Pisa - Italy ^[18] Univ Pisa, Phys Dept, I-56127 Pisa - Italy ^[19] Novosibirsk State Univ, Novosibirsk 630090 - Russia ^[20] Budker Inst Nucl Phys, Novosibirsk 630090 - Russia ^[21] INFN Cagliari, I-09042 Cagliari - Italy ^[22] INFN Genova, I-16146 Genoa - Italy ^[23] Univ Genoa, Phys Dept, I-16146 Genoa - Italy ^[24] Carleton Univ, Dept Phys, Ottawa, ON K1S 5B6 - Canada ^[25] European Org Nucl Res, CERN, CH-1211 Geneva 23 - Switzerland ^[26] INFN Roma Tre, I-00146 Rome - Italy ^[27] Univ Roma Tre, Math & Phys Dept, I-00146 Rome - Italy ^[28] Univ Cagliari, Phys Dept, I-09042 Cagliari - Italy ^[29] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67100 Assergi, AQ - Italy ^[30] Gran Sasso Sci Inst, I-67100 Laquila - Italy ^[31] Museo Fis & Ctr Studi & Ric Enrico Fermi, I-00184 Rome - Italy ^[32] Univ Cagliari, Dept Elect & Elect Engn, I-09123 Cagliari - Italy ^[33] Univ Federico II Napoli, Phys Dept, I-80126 Naples - Italy ^[34] Ist Nazl Fis Nucl, Osservatorio Astron Capodimonte, I-80131 Naples - Italy ^[35] Univ Zaragoza, Ctr Astroparticulas & Fis Altas Energias, Zaragoza 50009 - Spain ^[36] Queens Univ, Dept Phys Engn Phys & Astron, Kingston, ON K7L 3N6 - Canada ^[37] Jagiellonian Univ, M Smoluchowski Inst Phys, PL-30348 Krakow - Poland ^[38] INFN Milano, I-20133 Milan - Italy ^[39] INFN Torino, I-10125 Turin - Italy ^[40] Sorbonne Univ, Univ Paris Diderot, LPNHE, CNRS IN2P3, F-75252 Paris - France ^[41] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome - Italy ^[42] Sapienza Univ Roma, Phys Dept, I-00185 Rome - Italy ^[43] INFN Salerno, I-84084 Salerno - Italy ^[44] Univ Salerno, Phys Dept, I-84084 Salerno - Italy ^[45] Politecn Milan, Chem Mat & Chem Engn Dept G Natta, I-20133 Milan - Italy ^[46] Kurchatov Inst, Natl Res Ctr, Moscow 123182 - Russia ^[47] Johannes Gutenberg Univ Mainz, Inst Kernphys, D-55099 Mainz - Germany ^[48] Univ Massachusetts, Amherst Ctr Fundamental Interact, Amherst, MA 01003 - USA ^[49] Univ Massachusetts, Phys Dept, Amherst, MA 01003 - USA ^[50] Univ Calif Davis, Dept Phys, Davis, CA 95616 - USA ^[51] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati - Italy ^[52] Univ Paris, CNRS, APC, Astroparticule & Cosmol, F-75013 Paris - France ^[53] Princeton Univ, Phys Dept, Princeton, NJ 08544 - USA ^[54] Swiss Fed Inst Technol, Inst Particle Phys, CH-8093 Zurich - Switzerland ^[55] Politecn Torino, Dept Elect & Commun, I-10129 Turin - Italy ^[56] Williams Coll, Phys Dept, Williamstown, MA 01267 - USA ^[57] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 - USA ^[58] Fdn Bruno Kessler, I-38123 Povo - Italy ^[59] Trento Inst Fundamental Phys & Applicat, I-38123 Povo - Italy ^[60] Univ Barcelona, E-08028 Barcelona, Catalonia - Spain ^[61] Natl Res Nucl Univ, MEPhI, Moscow 115409 - Russia ^[62] Joint Inst Nucl Res, Dubna 141980 - Russia ^[63] Inst High Energy Phys, Beijing 100049 - Peoples R China ^[64] Ist Nazl Fis Nucl, Lab Nazl Sud, I-95123 Catania - Italy ^[65] Univ Enna Kore, Engn & Architecture Fac, I-94100 Enna - Italy ^[66] Univ Alberta, Dept Phys, Edmonton, AB T6G 2R3 - Canada ^[67] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, AstroCeNT, PL-00614 Warsaw - Poland ^[68] Fermilab Natl Accelerator Lab, Batavia, IL 60510 - USA ^[69] Laurentian Univ, Dept Phys & Astron, Sudbury, ON P3E 2C6 - Canada ^[70] SNOLAB, Lively, ON P3Y 1N2 - Canada ^[71] Temple Univ, Phys Dept, Philadelphia, PA 19122 - USA ^[72] Belgorod Natl Res Univ, Radiat Phys Lab, Belgorod 308007 - Russia ^[73] Univ Federico II Napoli, Pharm Dept, I-80131 Naples - Italy ^[74] Univ Zaragoza, Fdn ARAID, Zaragoza 50009 - Spain ^[75] Khomyakov, A., V, Avetisov, R., I, Mendeleev Univ Chem Technol, Moscow 125047 - Russia ^[76] Derbin, A., V, V, St Petersburg Nucl Phys Inst, Gatchina 188350 - Russia ^[77] Univ Lancaster, Phys Dept, Lancaster LA1 4YB - England ^[78] Politecn Milan, Civil & Environm Engn Dept, I-20133 Milan - Italy ^[79] Hungerford, E., V, Univ Houston, Dept Phys, Houston, TX 77204 - USA ^[80] Univ Manchester, Dept Phys & Astron, Manchester M13 9PL, Lancs - England ^[81] Univ Milan, Phys Dept, I-20133 Milan - Italy ^[82] Brookhaven Natl Lab, Upton, NY 11973 - USA ^[83] Univ Federico II Napoli, Chem Mat Ind Prod Engn Dept, I-80126 Naples - Italy ^[84] Virginia Tech, Blacksburg, VA 24061 - USA ^[85] Univ Calif Los Angeles, Phys & Astron Dept, Los Angeles, CA 90095 - USA ^[86] Ft Lewis Coll, Dept Phys & Engn, Durango, CO 81301 - USA ^[87] Lodz Univ Technol, Inst Appl Radiat Chem, PL-93590 Lodz - Poland Total Affiliations: 87
Document type:	Journal article
Source:	Journal of Cosmology and Astroparticle Physics; n. 3 MAR 2021.
Web of Science Citations:	2
Abstract
Future liquid-argon DarkSide-20k and Argo detectors, designed for direct dark matter search, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutrino-nucleus scattering. This interaction channel is flavor-insensitive with a high-cross section, enabling for a high-statistics neutrino detection with target masses of similar to 50 t and similar to 360 t for DarkSide-20k and Argo respectively. Thanks to the low-energy threshold of similar to 0.5 keV(nr) achievable by exploiting the ionization channel, DarkSide-20k and Argo have the potential to discover supernova bursts throughout our galaxy and up to the Small Magellanic Cloud, respectively, assuming a 11-M-circle dot progenitor star. We report also on the sensitivity to the neutronization burst, whose electron neutrino flux is suppressed by oscillations when detected via charged current and elastic scattering. Finally, the accuracies in the reconstruction of the average and total neutrino energy in the different phases of the supernova burst, as well as its time profile, are also discussed, taking into account the expected background and the detector response. (AU)

FAPESP's process:	17/26238-4 - Direct dark matter detection within the Darkside program
Grantee:	Maximo David Ave Pernas
Support Opportunities:	Research Grants - Young Investigators Grants

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