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

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-st...

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Detalles Bibliográficos
Autores principales: 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, R.I., Azzolini, O., Back, H.O., Balmforth, Z., Barbarian, V., Barrado Olmedo, A., 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., Cárdenas-Montes, M., Carlini, M., Carnesecchi, F., Castello, P., Catalanotti, S., Cataudella, V., Cavalcante, P., Cavuoti, S., Cebrian, S., Cela Ruiz, J.M., Celano, B., Chashin, S., Chepurnov, A., Chyhyrynets, E., Cicalò, C., Cifarelli, L., Cintas, D., Coccetti, F., Cocco, V., Colocci, M., Conde Vilda, E., Consiglio, L., Copello, S., Corning, J., Covone, G., Czudak, P., D'Auria, S., Da Rocha Rolo, M., 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, A.V., Devoto, A., Di Noto, L., Dionisi, C., Di Stefano, P., Dolganov, G., Dordei, F., Doria, L., Downing, M., Erjavec, T., Fernandez Diaz, M., Fiorillo, G., Franceschi, A., Franco, D., Frolov, E., Funicello, N., Gabriele, F., Galbiati, C., Garbini, M., Garcia Abia, P., Gendotti, A., Ghiano, C., Giampaolo, R.A., Giganti, C., Giorgi, M.A., Giovanetti, G.K., Goicoechea Casanueva, V., Gola, A., Graciani Diaz, R., 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, E.V., Ianni, An., Ippolito, V., James, C.C., Jillings, C., Kachru, P., Kemp, A.A., Kendziora, C.L., Keppel, G., Khomyakov, A.V., Kim, S., Kish, A., Kochanek, I., Kondo, K., Korga, G., Kubankin, A., Kugathasan, R., Kuss, M., Kuźniak, 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., Martínez, M., Martinez Rojas, A.D., 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., Mróz, T., Muratova, V.N., Muscas, C., Musenich, L., Musico, P., Nania, R., Napolitano, T., Navrer Agasson, A., 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., Sánchez García, E., 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, E.V., Usai, G., Vallivilayil John, T., 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.
Lenguaje:eng
Publicado: 2020
Materias:
physics.ins-det
Detectors and Experimental Techniques
astro-ph.IM
Astrophysics and Astronomy
astro-ph.HE
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2021/03/043
http://cds.cern.ch/record/2744914
_version_ 1780968667354234880
author 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, R.I.
Azzolini, O.
Back, H.O.
Balmforth, Z.
Barbarian, V.
Barrado Olmedo, A.
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.
Cárdenas-Montes, M.
Carlini, M.
Carnesecchi, F.
Castello, P.
Catalanotti, S.
Cataudella, V.
Cavalcante, P.
Cavuoti, S.
Cebrian, S.
Cela Ruiz, J.M.
Celano, B.
Chashin, S.
Chepurnov, A.
Chyhyrynets, E.
Cicalò, C.
Cifarelli, L.
Cintas, D.
Coccetti, F.
Cocco, V.
Colocci, M.
Conde Vilda, E.
Consiglio, L.
Copello, S.
Corning, J.
Covone, G.
Czudak, P.
D'Auria, S.
Da Rocha Rolo, M.
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, A.V.
Devoto, A.
Di Noto, L.
Dionisi, C.
Di Stefano, P.
Dolganov, G.
Dordei, F.
Doria, L.
Downing, M.
Erjavec, T.
Fernandez Diaz, M.
Fiorillo, G.
Franceschi, A.
Franco, D.
Frolov, E.
Funicello, N.
Gabriele, F.
Galbiati, C.
Garbini, M.
Garcia Abia, P.
Gendotti, A.
Ghiano, C.
Giampaolo, R.A.
Giganti, C.
Giorgi, M.A.
Giovanetti, G.K.
Goicoechea Casanueva, V.
Gola, A.
Graciani Diaz, R.
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, E.V.
Ianni, An.
Ippolito, V.
James, C.C.
Jillings, C.
Kachru, P.
Kemp, A.A.
Kendziora, C.L.
Keppel, G.
Khomyakov, A.V.
Kim, S.
Kish, A.
Kochanek, I.
Kondo, K.
Korga, G.
Kubankin, A.
Kugathasan, R.
Kuss, M.
Kuźniak, 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.
Martínez, M.
Martinez Rojas, A.D.
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.
Mróz, T.
Muratova, V.N.
Muscas, C.
Musenich, L.
Musico, P.
Nania, R.
Napolitano, T.
Navrer Agasson, A.
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.
Sánchez García, E.
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, E.V.
Usai, G.
Vallivilayil John, T.
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.
author_facet 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, R.I.
Azzolini, O.
Back, H.O.
Balmforth, Z.
Barbarian, V.
Barrado Olmedo, A.
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.
Cárdenas-Montes, M.
Carlini, M.
Carnesecchi, F.
Castello, P.
Catalanotti, S.
Cataudella, V.
Cavalcante, P.
Cavuoti, S.
Cebrian, S.
Cela Ruiz, J.M.
Celano, B.
Chashin, S.
Chepurnov, A.
Chyhyrynets, E.
Cicalò, C.
Cifarelli, L.
Cintas, D.
Coccetti, F.
Cocco, V.
Colocci, M.
Conde Vilda, E.
Consiglio, L.
Copello, S.
Corning, J.
Covone, G.
Czudak, P.
D'Auria, S.
Da Rocha Rolo, M.
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, A.V.
Devoto, A.
Di Noto, L.
Dionisi, C.
Di Stefano, P.
Dolganov, G.
Dordei, F.
Doria, L.
Downing, M.
Erjavec, T.
Fernandez Diaz, M.
Fiorillo, G.
Franceschi, A.
Franco, D.
Frolov, E.
Funicello, N.
Gabriele, F.
Galbiati, C.
Garbini, M.
Garcia Abia, P.
Gendotti, A.
Ghiano, C.
Giampaolo, R.A.
Giganti, C.
Giorgi, M.A.
Giovanetti, G.K.
Goicoechea Casanueva, V.
Gola, A.
Graciani Diaz, R.
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, E.V.
Ianni, An.
Ippolito, V.
James, C.C.
Jillings, C.
Kachru, P.
Kemp, A.A.
Kendziora, C.L.
Keppel, G.
Khomyakov, A.V.
Kim, S.
Kish, A.
Kochanek, I.
Kondo, K.
Korga, G.
Kubankin, A.
Kugathasan, R.
Kuss, M.
Kuźniak, 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.
Martínez, M.
Martinez Rojas, A.D.
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.
Mróz, T.
Muratova, V.N.
Muscas, C.
Musenich, L.
Musico, P.
Nania, R.
Napolitano, T.
Navrer Agasson, A.
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.
Sánchez García, E.
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, E.V.
Usai, G.
Vallivilayil John, T.
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.
author_sort Agnes, P.
collection CERN
description 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 ∼50 t and ∼360 t for DarkSide-20k and Argo respectively. Thanks to the low-energy threshold of ∼0.5 keVnr 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☉ 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.
id cern-2744914
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2020
record_format invenio
spelling cern-27449142023-05-19T04:07:44Zdoi:10.1088/1475-7516/2021/03/043http://cds.cern.ch/record/2744914engAgnes, P.Albergo, S.Albuquerque, I.F.M.Alexander, T.Alici, A.Alton, A.K.Amaudruz, P.Arcelli, S.Ave, M.Avetissov, I.Ch.Avetisov, R.I.Azzolini, O.Back, H.O.Balmforth, Z.Barbarian, V.Barrado Olmedo, A.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.Cárdenas-Montes, M.Carlini, M.Carnesecchi, F.Castello, P.Catalanotti, S.Cataudella, V.Cavalcante, P.Cavuoti, S.Cebrian, S.Cela Ruiz, J.M.Celano, B.Chashin, S.Chepurnov, A.Chyhyrynets, E.Cicalò, C.Cifarelli, L.Cintas, D.Coccetti, F.Cocco, V.Colocci, M.Conde Vilda, E.Consiglio, L.Copello, S.Corning, J.Covone, G.Czudak, P.D'Auria, S.Da Rocha Rolo, M.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, A.V.Devoto, A.Di Noto, L.Dionisi, C.Di Stefano, P.Dolganov, G.Dordei, F.Doria, L.Downing, M.Erjavec, T.Fernandez Diaz, M.Fiorillo, G.Franceschi, A.Franco, D.Frolov, E.Funicello, N.Gabriele, F.Galbiati, C.Garbini, M.Garcia Abia, P.Gendotti, A.Ghiano, C.Giampaolo, R.A.Giganti, C.Giorgi, M.A.Giovanetti, G.K.Goicoechea Casanueva, V.Gola, A.Graciani Diaz, R.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, E.V.Ianni, An.Ippolito, V.James, C.C.Jillings, C.Kachru, P.Kemp, A.A.Kendziora, C.L.Keppel, G.Khomyakov, A.V.Kim, S.Kish, A.Kochanek, I.Kondo, K.Korga, G.Kubankin, A.Kugathasan, R.Kuss, M.Kuźniak, 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.Martínez, M.Martinez Rojas, A.D.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.Mróz, T.Muratova, V.N.Muscas, C.Musenich, L.Musico, P.Nania, R.Napolitano, T.Navrer Agasson, A.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.Sánchez García, E.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, E.V.Usai, G.Vallivilayil John, T.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.Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinosphysics.ins-detDetectors and Experimental Techniquesastro-ph.IMAstrophysics and Astronomyastro-ph.HEAstrophysics and AstronomyFuture 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 ∼50 t and ∼360 t for DarkSide-20k and Argo respectively. Thanks to the low-energy threshold of ∼0.5 keVnr 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☉ 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.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 $\sim$50~t and $\sim$360~t for DarkSide-20k and ARGO, respectively. Thanks to the low-energy threshold of $\sim$0.5~keV$_{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$_{\odot}$ 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.arXiv:2011.07819oai:cds.cern.ch:27449142020-11-16
spellingShingle physics.ins-det
Detectors and Experimental Techniques
astro-ph.IM
Astrophysics and Astronomy
astro-ph.HE
Astrophysics and Astronomy
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, R.I.
Azzolini, O.
Back, H.O.
Balmforth, Z.
Barbarian, V.
Barrado Olmedo, A.
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.
Cárdenas-Montes, M.
Carlini, M.
Carnesecchi, F.
Castello, P.
Catalanotti, S.
Cataudella, V.
Cavalcante, P.
Cavuoti, S.
Cebrian, S.
Cela Ruiz, J.M.
Celano, B.
Chashin, S.
Chepurnov, A.
Chyhyrynets, E.
Cicalò, C.
Cifarelli, L.
Cintas, D.
Coccetti, F.
Cocco, V.
Colocci, M.
Conde Vilda, E.
Consiglio, L.
Copello, S.
Corning, J.
Covone, G.
Czudak, P.
D'Auria, S.
Da Rocha Rolo, M.
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, A.V.
Devoto, A.
Di Noto, L.
Dionisi, C.
Di Stefano, P.
Dolganov, G.
Dordei, F.
Doria, L.
Downing, M.
Erjavec, T.
Fernandez Diaz, M.
Fiorillo, G.
Franceschi, A.
Franco, D.
Frolov, E.
Funicello, N.
Gabriele, F.
Galbiati, C.
Garbini, M.
Garcia Abia, P.
Gendotti, A.
Ghiano, C.
Giampaolo, R.A.
Giganti, C.
Giorgi, M.A.
Giovanetti, G.K.
Goicoechea Casanueva, V.
Gola, A.
Graciani Diaz, R.
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, E.V.
Ianni, An.
Ippolito, V.
James, C.C.
Jillings, C.
Kachru, P.
Kemp, A.A.
Kendziora, C.L.
Keppel, G.
Khomyakov, A.V.
Kim, S.
Kish, A.
Kochanek, I.
Kondo, K.
Korga, G.
Kubankin, A.
Kugathasan, R.
Kuss, M.
Kuźniak, 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.
Martínez, M.
Martinez Rojas, A.D.
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.
Mróz, T.
Muratova, V.N.
Muscas, C.
Musenich, L.
Musico, P.
Nania, R.
Napolitano, T.
Navrer Agasson, A.
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.
Sánchez García, E.
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, E.V.
Usai, G.
Vallivilayil John, T.
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.
Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
title Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
title_full Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
title_fullStr Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
title_full_unstemmed Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
title_short Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
title_sort sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
topic physics.ins-det
Detectors and Experimental Techniques
astro-ph.IM
Astrophysics and Astronomy
astro-ph.HE
Astrophysics and Astronomy
url https://dx.doi.org/10.1088/1475-7516/2021/03/043
http://cds.cern.ch/record/2744914
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AT grobova sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT gromovm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT guanm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT guerzonim sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT gulinom sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT guoc sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT hackettbr sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT hallina sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT haranczykm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT hills sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT horikawas sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT hubautf sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT huguest sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT hungerfordev sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT iannian sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT ippolitov sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT jamescc sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT jillingsc sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kachrup sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kempaa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kendzioracl sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT keppelg sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT khomyakovav sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kims sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kisha sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kochaneki sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kondok sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT korgag sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kubankina sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kugathasanr sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kussm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT kuzniakm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT lacommaram sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT laim sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT langrocks sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT leytonm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT lix sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT lideyl sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT lissiam sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT longog sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT machulinin sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT mapellil sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT marasciullia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT margottia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT marism sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT maricicj sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT martinezm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT martinezrojasad sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT martoffcj sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT masonia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT mazzia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT mcdonaldab sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT mclaughlinj sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT messinaa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT meyerspd sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT miletict sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT milincicr sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT moggia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT moharanaa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT moiolis sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT monroej sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT morisis sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT morrocchim sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT mozhevitinaen sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT mrozt sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT muratovavn sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT muscasc sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT musenichl sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT musicop sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT naniar sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT napolitanot sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT navreragassona sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT nessim sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT nikulini sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT nowakj sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT oleinika sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT oleynikovv sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT paganil sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pallavicinim sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pandolal sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pantice sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT paolonie sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT paternosterg sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pegoraropa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pelczark sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pellegrinila sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pellegrinoc sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT perottif sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pesudov sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT picciaue sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pietropaolof sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pirac sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pocara sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT poehlmanndm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pordess sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT poudelss sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT pralavoriop sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT priced sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT raffaellif sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT ragusaf sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT ramireza sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT razetim sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT razetoa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT renshawal sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT rescias sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT rescignom sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT resnatif sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT retieref sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT rignaneselp sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT ripolic sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT rivettia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT rodej sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT romerol sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT rossim sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT rubbiaa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT salatinop sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT samoylovo sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT sanchezgarciae sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT sandforde sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT sanfilippos sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT santoned sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT santorellir sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT savaresec sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT scapparonee sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT schlitzerb sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT sciolig sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT semenovda sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT shawb sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT shchagina sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT sheshukova sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT simeonem sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT skensvedp sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT skorokhvatovmd sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT smirnovo sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT smithb sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT sokolova sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT steria sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT strackas sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT stricklandv sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT stringerm sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT suliss sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT suvorovy sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT szelcam sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT tartagliar sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT testerag sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT thorpetn sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT tonazzoa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT torreslaras sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT tricomia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT unzhakovev sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT usaig sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT vallivilayiljohnt sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT viantt sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT viels sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT vishnevaa sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT vogelaarrb sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT wadam sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT wangh sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT wangy sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT westerdales sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT wheadonrj sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT williamsl sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT wojcikmam sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT wojcikma sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT xiaox sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT yangc sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT yez sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT zania sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT zichichia sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT zuzelg sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos
AT zykovamp sensitivityoffutureliquidargondarkmattersearchexperimentstocorecollapsesupernovaneutrinos

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