The KM3NeT potential for the next core-collapse supernova observation with neutrinos
The KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophysics and oscillation research, respectively. Instrumenting a large volume of sea water with $\sim$ 6,200 optical modules...
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Format: | Other/Unknown Material |
Language: | English |
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2021
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Online Access: | https://oskar-bordeaux.fr/handle/20.500.12278/38349 |
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ftoskarbordeaux:oai:oskar-bordeaux.fr:20.500.12278/38349 |
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Open Polar |
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OSKAR Bordeaux (Open Science Knowledge ARchive) |
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ftoskarbordeaux |
language |
English |
topic |
KM3NeT: sensitivity neutrino: detector neutrino: burst neutrino: flux supernova: collapse photomultiplier background water oscillation stability signature accretion Cherenkov spectral horizon optical galaxy cloud tube Physique [physics]/Astrophysique [astro-ph] |
spellingShingle |
KM3NeT: sensitivity neutrino: detector neutrino: burst neutrino: flux supernova: collapse photomultiplier background water oscillation stability signature accretion Cherenkov spectral horizon optical galaxy cloud tube Physique [physics]/Astrophysique [astro-ph] AIELLO, S. ALBERT, A. GARRE, S. Alves ALY, Z. AMBROSONE, A. AMELI, F. ANDRE, M. ANDROULAKIS, G. ANGHINOLFI, M. ANGUITA, M. ANTON, G. ARDID, M. ARDID, S. AUBLIN, J. BAGATELAS, C. BARET, B. BASEGMEZ DU PREE, S. BENDAHMAN, M. BENFENATI, F. BERBEE, E. VAN DEN BERG, A.M. BERTIN, V. BIAGI, S. BISSINGER, M. BOETTCHER, M. CABO, M. Bou BOUMAAZA, J. BOUTA, M. BOUWHUIS, M. BOZZA, C. BRÂNZA¸S, H. BRUIJN, R. BRUNNER, J. BUIS, E. BUOMPANE, R. BUSTO, J. CAIFFI, B. CALVO, D. CAPONE, A. CARRETERO, V. CASTALDI, P. CELLI, S. CHABAB, M. CHAU, N. CHEN, A. CHERUBINI, S. CHIARELLA, V. CHIARUSI, T. CIRCELLA, M. COCIMANO, R. COELHO, J.A.B. COLEIRO, A. COLOMER MOLLA, M. CONIGLIONE, R. COYLE, P. CREUSOT, A. CUTTONE, G. DALLIER, R. DE MARTINO, B. DE PALMA, M. DI MARINO, M. DI PALMA, I. DIAZ, A.F. DIEGO-TORTOSA, D. DISTEFANO, C. DOMI, A. DONZAUD, C. DORNIC, D. DÖRR, M. DROUHIN, D. EBERL, T. EDDYAMOUI, A. VAN EEDEN, T. VAN EIJK, D. BOJADDAINI, I. El ELSAESSER, D. ENZENHÖFER, A. ESPINOSA, V. FERMANI, P. FERRARA, G. FILIPOVIC, M.D. FILIPPINI, F. FUSCO, L.A. GABELLA, O. GAL, T. SOTO, A. Garcia GARUFI, F. GATELET, Y. GEISSELBRECHT, N. GIALANELLA, L. GIORGIO, E. GOZZINI, S.R. GRACIA, R. GRAF, K. GRASSO, D. GRELLA, G. GUDERIAN, D. GUIDI, C. HAEFNER, J. HAMDAOUI, H. VAN HAREN, H. HEIJBOER, A. HEKALO, A. HENNIG, L. HERNANDEZ-REY, J.J. HOFESTÄDT, J. HUANG, F. IBNSALIH, W. Idrissi ILLUMINATI, G. JAMES, C.W. DE JONG, M. DE JONG, P. JUNG, B.J. KADLER, M. KALACZYNSKI, P. KALEKIN, O. KATZ, U.F. KHAN CHOWDHURY, N.R. KISTAURI, G. VAN DER KNAAP, F. KOOIJMAN, P. KOUCHNER, A. KRETER, M. KULIKOVSKIY, V. LAHMANN, R. LAMOUREUX, M. LAROSA, G. LE BRETON, R. LE STUM, S. LEONARDI, O. LEONE, F. LEONORA, E. LESSING, N. LEVI, G. LINCETTO, M. LINDSEY CLARK, M. LIPREAU, T. LONGHITANO, F. LOPEZ-COTO, D. MADERER, L. MANCZAK, J. MANNHEIM, K. MARGIOTTA, A. MARINELLI, A. MARKOU, C. MARTIN, L. MARTINEZ-MORA, J.A. MARTINI, A. MARZAIOLI, F. MASTROIANNI, S. MAZZOU, S. MELIS, K.W. MIELE, G. MIGLIOZZI, P. MIGNECO, E. MIJAKOWSKI, P. MIRANDA, L.S. MOLLO, C.M. MORGANTI, M. MOSER, M. MOUSSA, A. MULLER, R. MUSUMECI, M. NAUTA, L. NAVAS, S. NICOLAU, C.A. FEARRAIGH, B.O. O'SULLIVAN, M. ORGANOKOV, M. ORLANDO, A. GONZALEZ, J. Palacios PAPALASHVILI, G. PAPALEO, R. PASSARO, G. PASTORE, C. P˘AUN, A.M. PAVALAS, G.E. PELLEGRINO, C. PERRIN-TERRIN, M. PESTEL, V. PIATTELLI, P. PIETERSE, C. PIKOUNIS, K. PISANTI, O. POIRÈ, C. POPA, V. PRADIER, T. PÜHLHOFER, G. PULVIRENTI, S. RABYANG, O. RAFFAELLI, F. RANDAZZO, N. RAZZAQUE, S. REAL, D. RECK, S. RICCOBENE, G. RIVOIRE, S. ROMANOV, A. ROVELLI, A. SALESA GREUS, F. SAMTLEBEN, D.F.E. SANCHEZ LOSA, A. SANGUINETI, M. SANTANGELO, A. SANTONOCITO, D. SAPIENZA, P. SCHNABEL, J. SCHNEIDER, M.F. SCHUMANN, J. SCHUTTE, H.M. SENECA, J. SGURA, I. SHANIDZE, R. SHARMA, A. SIMEONE, F. SINOPOULOU, A. SPISSO, B. SPURIO, M. STAVROPOULOS, D. STELLACCI, S.M. TAIUTI, M. TAYALATI, Y. TENLLADO, E. THAKORE, T. THIERSEN, H. TINGAY, S. TSOURAPIS, V. TZAMARIUDAKI, E. TZANETATOS, D. UNBEHAUN, T. VAN ELEWYCK, V. VANNOYE, G. VASILEIADIS, G. VERSARI, F. VIOLA, S. VIVOLO, D. DE WASSEIGE, G. WILMS, J. WOJACZYNSKI, R. DE WOLF, E. ZAVATARELLI, S. ZEGARELLI, A. ZITO, D. ZORNOZA, J.D. ZUÑIGA, J. ZYWUCKA, N. The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
topic_facet |
KM3NeT: sensitivity neutrino: detector neutrino: burst neutrino: flux supernova: collapse photomultiplier background water oscillation stability signature accretion Cherenkov spectral horizon optical galaxy cloud tube Physique [physics]/Astrophysique [astro-ph] |
description |
The KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophysics and oscillation research, respectively. Instrumenting a large volume of sea water with $\sim$ 6,200 optical modules comprising a total of $\sim$ 200,000 photomultiplier tubes, KM3NeT will achieve sensitivity to $\sim$ 10 MeV neutrinos from Galactic and near-Galactic core-collapse supernovae through the observation of coincident hits in photomultipliers above the background. In this paper, the sensitivity of KM3NeT to a supernova explosion is estimated from detailed analyses of background data from the first KM3NeT detection units and simulations of the neutrino signal. The KM3NeT observational horizon (for a $5\,\sigma$ discovery) covers essentially the Milky-Way and for the most optimistic model, extends to the Small Magellanic Cloud ($\sim$ 60 kpc). Detailed studies of the time profile of the neutrino signal allow assessment of the KM3NeT capability to determine the arrival time of the neutrino burst with a few milliseconds precision for sources up to 5$-$8 kpc away, and detecting the peculiar signature of the \textit{standing accretion shock instability} if the core-collapse supernova explosion happens closer than 3$-$5 pc, depending on the progenitor mass. KM3NeT's capability to measure the neutrino flux spectral parameters is also presented. |
format |
Other/Unknown Material |
author |
AIELLO, S. ALBERT, A. GARRE, S. Alves ALY, Z. AMBROSONE, A. AMELI, F. ANDRE, M. ANDROULAKIS, G. ANGHINOLFI, M. ANGUITA, M. ANTON, G. ARDID, M. ARDID, S. AUBLIN, J. BAGATELAS, C. BARET, B. BASEGMEZ DU PREE, S. BENDAHMAN, M. BENFENATI, F. BERBEE, E. VAN DEN BERG, A.M. BERTIN, V. BIAGI, S. BISSINGER, M. BOETTCHER, M. CABO, M. Bou BOUMAAZA, J. BOUTA, M. BOUWHUIS, M. BOZZA, C. BRÂNZA¸S, H. BRUIJN, R. BRUNNER, J. BUIS, E. BUOMPANE, R. BUSTO, J. CAIFFI, B. CALVO, D. CAPONE, A. CARRETERO, V. CASTALDI, P. CELLI, S. CHABAB, M. CHAU, N. CHEN, A. CHERUBINI, S. CHIARELLA, V. CHIARUSI, T. CIRCELLA, M. COCIMANO, R. COELHO, J.A.B. COLEIRO, A. COLOMER MOLLA, M. CONIGLIONE, R. COYLE, P. CREUSOT, A. CUTTONE, G. DALLIER, R. DE MARTINO, B. DE PALMA, M. DI MARINO, M. DI PALMA, I. DIAZ, A.F. DIEGO-TORTOSA, D. DISTEFANO, C. DOMI, A. DONZAUD, C. DORNIC, D. DÖRR, M. DROUHIN, D. EBERL, T. EDDYAMOUI, A. VAN EEDEN, T. VAN EIJK, D. BOJADDAINI, I. El ELSAESSER, D. ENZENHÖFER, A. ESPINOSA, V. FERMANI, P. FERRARA, G. FILIPOVIC, M.D. FILIPPINI, F. FUSCO, L.A. GABELLA, O. GAL, T. SOTO, A. Garcia GARUFI, F. GATELET, Y. GEISSELBRECHT, N. GIALANELLA, L. GIORGIO, E. GOZZINI, S.R. GRACIA, R. GRAF, K. GRASSO, D. GRELLA, G. GUDERIAN, D. GUIDI, C. HAEFNER, J. HAMDAOUI, H. VAN HAREN, H. HEIJBOER, A. HEKALO, A. HENNIG, L. HERNANDEZ-REY, J.J. HOFESTÄDT, J. HUANG, F. IBNSALIH, W. Idrissi ILLUMINATI, G. JAMES, C.W. DE JONG, M. DE JONG, P. JUNG, B.J. KADLER, M. KALACZYNSKI, P. KALEKIN, O. KATZ, U.F. KHAN CHOWDHURY, N.R. KISTAURI, G. VAN DER KNAAP, F. KOOIJMAN, P. KOUCHNER, A. KRETER, M. KULIKOVSKIY, V. LAHMANN, R. LAMOUREUX, M. LAROSA, G. LE BRETON, R. LE STUM, S. LEONARDI, O. LEONE, F. LEONORA, E. LESSING, N. LEVI, G. LINCETTO, M. LINDSEY CLARK, M. LIPREAU, T. LONGHITANO, F. LOPEZ-COTO, D. MADERER, L. MANCZAK, J. MANNHEIM, K. MARGIOTTA, A. MARINELLI, A. MARKOU, C. MARTIN, L. MARTINEZ-MORA, J.A. MARTINI, A. MARZAIOLI, F. MASTROIANNI, S. MAZZOU, S. MELIS, K.W. MIELE, G. MIGLIOZZI, P. MIGNECO, E. MIJAKOWSKI, P. MIRANDA, L.S. MOLLO, C.M. MORGANTI, M. MOSER, M. MOUSSA, A. MULLER, R. MUSUMECI, M. NAUTA, L. NAVAS, S. NICOLAU, C.A. FEARRAIGH, B.O. O'SULLIVAN, M. ORGANOKOV, M. ORLANDO, A. GONZALEZ, J. Palacios PAPALASHVILI, G. PAPALEO, R. PASSARO, G. PASTORE, C. P˘AUN, A.M. PAVALAS, G.E. PELLEGRINO, C. PERRIN-TERRIN, M. PESTEL, V. PIATTELLI, P. PIETERSE, C. PIKOUNIS, K. PISANTI, O. POIRÈ, C. POPA, V. PRADIER, T. PÜHLHOFER, G. PULVIRENTI, S. RABYANG, O. RAFFAELLI, F. RANDAZZO, N. RAZZAQUE, S. REAL, D. RECK, S. RICCOBENE, G. RIVOIRE, S. ROMANOV, A. ROVELLI, A. SALESA GREUS, F. SAMTLEBEN, D.F.E. SANCHEZ LOSA, A. SANGUINETI, M. SANTANGELO, A. SANTONOCITO, D. SAPIENZA, P. SCHNABEL, J. SCHNEIDER, M.F. SCHUMANN, J. SCHUTTE, H.M. SENECA, J. SGURA, I. SHANIDZE, R. SHARMA, A. SIMEONE, F. SINOPOULOU, A. SPISSO, B. SPURIO, M. STAVROPOULOS, D. STELLACCI, S.M. TAIUTI, M. TAYALATI, Y. TENLLADO, E. THAKORE, T. THIERSEN, H. TINGAY, S. TSOURAPIS, V. TZAMARIUDAKI, E. TZANETATOS, D. UNBEHAUN, T. VAN ELEWYCK, V. VANNOYE, G. VASILEIADIS, G. VERSARI, F. VIOLA, S. VIVOLO, D. DE WASSEIGE, G. WILMS, J. WOJACZYNSKI, R. DE WOLF, E. ZAVATARELLI, S. ZEGARELLI, A. ZITO, D. ZORNOZA, J.D. ZUÑIGA, J. ZYWUCKA, N. |
author_facet |
AIELLO, S. ALBERT, A. GARRE, S. Alves ALY, Z. AMBROSONE, A. AMELI, F. ANDRE, M. ANDROULAKIS, G. ANGHINOLFI, M. ANGUITA, M. ANTON, G. ARDID, M. ARDID, S. AUBLIN, J. BAGATELAS, C. BARET, B. BASEGMEZ DU PREE, S. BENDAHMAN, M. BENFENATI, F. BERBEE, E. VAN DEN BERG, A.M. BERTIN, V. BIAGI, S. BISSINGER, M. BOETTCHER, M. CABO, M. Bou BOUMAAZA, J. BOUTA, M. BOUWHUIS, M. BOZZA, C. BRÂNZA¸S, H. BRUIJN, R. BRUNNER, J. BUIS, E. BUOMPANE, R. BUSTO, J. CAIFFI, B. CALVO, D. CAPONE, A. CARRETERO, V. CASTALDI, P. CELLI, S. CHABAB, M. CHAU, N. CHEN, A. CHERUBINI, S. CHIARELLA, V. CHIARUSI, T. CIRCELLA, M. COCIMANO, R. COELHO, J.A.B. COLEIRO, A. COLOMER MOLLA, M. CONIGLIONE, R. COYLE, P. CREUSOT, A. CUTTONE, G. DALLIER, R. DE MARTINO, B. DE PALMA, M. DI MARINO, M. DI PALMA, I. DIAZ, A.F. DIEGO-TORTOSA, D. DISTEFANO, C. DOMI, A. DONZAUD, C. DORNIC, D. DÖRR, M. DROUHIN, D. EBERL, T. EDDYAMOUI, A. VAN EEDEN, T. VAN EIJK, D. BOJADDAINI, I. El ELSAESSER, D. ENZENHÖFER, A. ESPINOSA, V. FERMANI, P. FERRARA, G. FILIPOVIC, M.D. FILIPPINI, F. FUSCO, L.A. GABELLA, O. GAL, T. SOTO, A. Garcia GARUFI, F. GATELET, Y. GEISSELBRECHT, N. GIALANELLA, L. GIORGIO, E. GOZZINI, S.R. GRACIA, R. GRAF, K. GRASSO, D. GRELLA, G. GUDERIAN, D. GUIDI, C. HAEFNER, J. HAMDAOUI, H. VAN HAREN, H. HEIJBOER, A. HEKALO, A. HENNIG, L. HERNANDEZ-REY, J.J. HOFESTÄDT, J. HUANG, F. IBNSALIH, W. Idrissi ILLUMINATI, G. JAMES, C.W. DE JONG, M. DE JONG, P. JUNG, B.J. KADLER, M. KALACZYNSKI, P. KALEKIN, O. KATZ, U.F. KHAN CHOWDHURY, N.R. KISTAURI, G. VAN DER KNAAP, F. KOOIJMAN, P. KOUCHNER, A. KRETER, M. KULIKOVSKIY, V. LAHMANN, R. LAMOUREUX, M. LAROSA, G. LE BRETON, R. LE STUM, S. LEONARDI, O. LEONE, F. LEONORA, E. LESSING, N. LEVI, G. LINCETTO, M. LINDSEY CLARK, M. LIPREAU, T. LONGHITANO, F. LOPEZ-COTO, D. MADERER, L. MANCZAK, J. MANNHEIM, K. MARGIOTTA, A. MARINELLI, A. MARKOU, C. MARTIN, L. MARTINEZ-MORA, J.A. MARTINI, A. MARZAIOLI, F. MASTROIANNI, S. MAZZOU, S. MELIS, K.W. MIELE, G. MIGLIOZZI, P. MIGNECO, E. MIJAKOWSKI, P. MIRANDA, L.S. MOLLO, C.M. MORGANTI, M. MOSER, M. MOUSSA, A. MULLER, R. MUSUMECI, M. NAUTA, L. NAVAS, S. NICOLAU, C.A. FEARRAIGH, B.O. O'SULLIVAN, M. ORGANOKOV, M. ORLANDO, A. GONZALEZ, J. Palacios PAPALASHVILI, G. PAPALEO, R. PASSARO, G. PASTORE, C. P˘AUN, A.M. PAVALAS, G.E. PELLEGRINO, C. PERRIN-TERRIN, M. PESTEL, V. PIATTELLI, P. PIETERSE, C. PIKOUNIS, K. PISANTI, O. POIRÈ, C. POPA, V. PRADIER, T. PÜHLHOFER, G. PULVIRENTI, S. RABYANG, O. RAFFAELLI, F. RANDAZZO, N. RAZZAQUE, S. REAL, D. RECK, S. RICCOBENE, G. RIVOIRE, S. ROMANOV, A. ROVELLI, A. SALESA GREUS, F. SAMTLEBEN, D.F.E. SANCHEZ LOSA, A. SANGUINETI, M. SANTANGELO, A. SANTONOCITO, D. SAPIENZA, P. SCHNABEL, J. SCHNEIDER, M.F. SCHUMANN, J. SCHUTTE, H.M. SENECA, J. SGURA, I. SHANIDZE, R. SHARMA, A. SIMEONE, F. SINOPOULOU, A. SPISSO, B. SPURIO, M. STAVROPOULOS, D. STELLACCI, S.M. TAIUTI, M. TAYALATI, Y. TENLLADO, E. THAKORE, T. THIERSEN, H. TINGAY, S. TSOURAPIS, V. TZAMARIUDAKI, E. TZANETATOS, D. UNBEHAUN, T. VAN ELEWYCK, V. VANNOYE, G. VASILEIADIS, G. VERSARI, F. VIOLA, S. VIVOLO, D. DE WASSEIGE, G. WILMS, J. WOJACZYNSKI, R. DE WOLF, E. ZAVATARELLI, S. ZEGARELLI, A. ZITO, D. ZORNOZA, J.D. ZUÑIGA, J. ZYWUCKA, N. |
author_sort |
AIELLO, S. |
title |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_short |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_full |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_fullStr |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_full_unstemmed |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_sort |
km3net potential for the next core-collapse supernova observation with neutrinos |
publishDate |
2021 |
url |
https://oskar-bordeaux.fr/handle/20.500.12278/38349 |
long_lat |
ENVELOPE(-68.705,-68.705,-71.251,-71.251) |
geographic |
Milky Way |
geographic_facet |
Milky Way |
genre |
Orca |
genre_facet |
Orca |
op_relation |
https://oskar-bordeaux.fr/handle/20.500.12278/38349 2102.05977 |
_version_ |
1766161616988012544 |
spelling |
ftoskarbordeaux:oai:oskar-bordeaux.fr:20.500.12278/38349 2023-05-15T17:53:54+02:00 The KM3NeT potential for the next core-collapse supernova observation with neutrinos AIELLO, S. ALBERT, A. GARRE, S. Alves ALY, Z. AMBROSONE, A. AMELI, F. ANDRE, M. ANDROULAKIS, G. ANGHINOLFI, M. ANGUITA, M. ANTON, G. ARDID, M. ARDID, S. AUBLIN, J. BAGATELAS, C. BARET, B. BASEGMEZ DU PREE, S. BENDAHMAN, M. BENFENATI, F. BERBEE, E. VAN DEN BERG, A.M. BERTIN, V. BIAGI, S. BISSINGER, M. BOETTCHER, M. CABO, M. Bou BOUMAAZA, J. BOUTA, M. BOUWHUIS, M. BOZZA, C. BRÂNZA¸S, H. BRUIJN, R. BRUNNER, J. BUIS, E. BUOMPANE, R. BUSTO, J. CAIFFI, B. CALVO, D. CAPONE, A. CARRETERO, V. CASTALDI, P. CELLI, S. CHABAB, M. CHAU, N. CHEN, A. CHERUBINI, S. CHIARELLA, V. CHIARUSI, T. CIRCELLA, M. COCIMANO, R. COELHO, J.A.B. COLEIRO, A. COLOMER MOLLA, M. CONIGLIONE, R. COYLE, P. CREUSOT, A. CUTTONE, G. DALLIER, R. DE MARTINO, B. DE PALMA, M. DI MARINO, M. DI PALMA, I. DIAZ, A.F. DIEGO-TORTOSA, D. DISTEFANO, C. DOMI, A. DONZAUD, C. DORNIC, D. DÖRR, M. DROUHIN, D. EBERL, T. EDDYAMOUI, A. VAN EEDEN, T. VAN EIJK, D. BOJADDAINI, I. El ELSAESSER, D. ENZENHÖFER, A. ESPINOSA, V. FERMANI, P. FERRARA, G. FILIPOVIC, M.D. FILIPPINI, F. FUSCO, L.A. GABELLA, O. GAL, T. SOTO, A. Garcia GARUFI, F. GATELET, Y. GEISSELBRECHT, N. GIALANELLA, L. GIORGIO, E. GOZZINI, S.R. GRACIA, R. GRAF, K. GRASSO, D. GRELLA, G. GUDERIAN, D. GUIDI, C. HAEFNER, J. HAMDAOUI, H. VAN HAREN, H. HEIJBOER, A. HEKALO, A. HENNIG, L. HERNANDEZ-REY, J.J. HOFESTÄDT, J. HUANG, F. IBNSALIH, W. Idrissi ILLUMINATI, G. JAMES, C.W. DE JONG, M. DE JONG, P. JUNG, B.J. KADLER, M. KALACZYNSKI, P. KALEKIN, O. KATZ, U.F. KHAN CHOWDHURY, N.R. KISTAURI, G. VAN DER KNAAP, F. KOOIJMAN, P. KOUCHNER, A. KRETER, M. KULIKOVSKIY, V. LAHMANN, R. LAMOUREUX, M. LAROSA, G. LE BRETON, R. LE STUM, S. LEONARDI, O. LEONE, F. LEONORA, E. LESSING, N. LEVI, G. LINCETTO, M. LINDSEY CLARK, M. LIPREAU, T. LONGHITANO, F. LOPEZ-COTO, D. MADERER, L. MANCZAK, J. MANNHEIM, K. MARGIOTTA, A. MARINELLI, A. MARKOU, C. MARTIN, L. MARTINEZ-MORA, J.A. MARTINI, A. MARZAIOLI, F. MASTROIANNI, S. MAZZOU, S. MELIS, K.W. MIELE, G. MIGLIOZZI, P. MIGNECO, E. MIJAKOWSKI, P. MIRANDA, L.S. MOLLO, C.M. MORGANTI, M. MOSER, M. MOUSSA, A. MULLER, R. MUSUMECI, M. NAUTA, L. NAVAS, S. NICOLAU, C.A. FEARRAIGH, B.O. O'SULLIVAN, M. ORGANOKOV, M. ORLANDO, A. GONZALEZ, J. Palacios PAPALASHVILI, G. PAPALEO, R. PASSARO, G. PASTORE, C. P˘AUN, A.M. PAVALAS, G.E. PELLEGRINO, C. PERRIN-TERRIN, M. PESTEL, V. PIATTELLI, P. PIETERSE, C. PIKOUNIS, K. PISANTI, O. POIRÈ, C. POPA, V. PRADIER, T. PÜHLHOFER, G. PULVIRENTI, S. RABYANG, O. RAFFAELLI, F. RANDAZZO, N. RAZZAQUE, S. REAL, D. RECK, S. RICCOBENE, G. RIVOIRE, S. ROMANOV, A. ROVELLI, A. SALESA GREUS, F. SAMTLEBEN, D.F.E. SANCHEZ LOSA, A. SANGUINETI, M. SANTANGELO, A. SANTONOCITO, D. SAPIENZA, P. SCHNABEL, J. SCHNEIDER, M.F. SCHUMANN, J. SCHUTTE, H.M. SENECA, J. SGURA, I. SHANIDZE, R. SHARMA, A. SIMEONE, F. SINOPOULOU, A. SPISSO, B. SPURIO, M. STAVROPOULOS, D. STELLACCI, S.M. TAIUTI, M. TAYALATI, Y. TENLLADO, E. THAKORE, T. THIERSEN, H. TINGAY, S. TSOURAPIS, V. TZAMARIUDAKI, E. TZANETATOS, D. UNBEHAUN, T. VAN ELEWYCK, V. VANNOYE, G. VASILEIADIS, G. VERSARI, F. VIOLA, S. VIVOLO, D. DE WASSEIGE, G. WILMS, J. WOJACZYNSKI, R. DE WOLF, E. ZAVATARELLI, S. ZEGARELLI, A. ZITO, D. ZORNOZA, J.D. ZUÑIGA, J. ZYWUCKA, N. 2021-05-10T17:04:02Z https://oskar-bordeaux.fr/handle/20.500.12278/38349 en eng https://oskar-bordeaux.fr/handle/20.500.12278/38349 2102.05977 KM3NeT: sensitivity neutrino: detector neutrino: burst neutrino: flux supernova: collapse photomultiplier background water oscillation stability signature accretion Cherenkov spectral horizon optical galaxy cloud tube Physique [physics]/Astrophysique [astro-ph] Document de travail - Pré-publication 2021 ftoskarbordeaux 2021-05-11T22:31:03Z The KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophysics and oscillation research, respectively. Instrumenting a large volume of sea water with $\sim$ 6,200 optical modules comprising a total of $\sim$ 200,000 photomultiplier tubes, KM3NeT will achieve sensitivity to $\sim$ 10 MeV neutrinos from Galactic and near-Galactic core-collapse supernovae through the observation of coincident hits in photomultipliers above the background. In this paper, the sensitivity of KM3NeT to a supernova explosion is estimated from detailed analyses of background data from the first KM3NeT detection units and simulations of the neutrino signal. The KM3NeT observational horizon (for a $5\,\sigma$ discovery) covers essentially the Milky-Way and for the most optimistic model, extends to the Small Magellanic Cloud ($\sim$ 60 kpc). Detailed studies of the time profile of the neutrino signal allow assessment of the KM3NeT capability to determine the arrival time of the neutrino burst with a few milliseconds precision for sources up to 5$-$8 kpc away, and detecting the peculiar signature of the \textit{standing accretion shock instability} if the core-collapse supernova explosion happens closer than 3$-$5 pc, depending on the progenitor mass. KM3NeT's capability to measure the neutrino flux spectral parameters is also presented. Other/Unknown Material Orca OSKAR Bordeaux (Open Science Knowledge ARchive) Milky Way ENVELOPE(-68.705,-68.705,-71.251,-71.251) |