Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope
An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced-Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by \(\nu_\mu\) (\(\bar{\nu}_{\mu}\)) charged...
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creator | ANTARES Collaboration Albert, A André, M Anton, G Ardid, M Aubert, J J Aublin, J Basa, S Belhorma, B Bertin, V Biagi, S Bissinger, M Boumaaza, J Brunner, J Capone, A Carr, J Celli, S Chabab, M Chau, T N Chiarusi, T Circella, M Colomer-Molla, M Coniglione, R Coyle, P Creusot, A de Wasseige, G Deschamps, A Distefano, C I Di Palma Donzaud, C Dornic, D Eberl, T N El Khayati Enzenhöfer, A Fermani, P Ferrara, G Gay, P Glotin, H Gozzini, R R Gracia Ruiz Graf, K Guidi, C Heijboer, A J Hello, Y Hernández-Rey, J J Hößl, J Huang, F de Jong, M Jongen, M Kadler, M Katz, U Khan-Chowdhury, N R Kreykenbohm, I Kulikovskiy, V R Le Breton Lefèvre, D Leonora, E Lincetto, M Lopez-Coto, D Loucatos, S Maggi, G Manczak, J Margiotta, A Marinelli, A Mele, R Melis, K Migliozzi, P Moussa, A Muller, R Nauta, L Navas, S Nielsen, C Nuñez-Castiñeyra, A Păvălaş, G E Pellegrino, C Perrin-Terrin, M Piattelli, P Poirè, C Popa, V Randazzo, N Reck, S Sanguineti, M Sapienza, P Schüssler, F Spurio, M Stolarczyk, Th Strandberg, B Taiuti, M Tayalati, Y Thakore, T Tingay, S J Trovato, A Vallage, B V Van Elewyck Versari, F Viola, S Vivolo, D Wilms, J Zaborov, D Zornoza, J D |
description | An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced-Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by \(\nu_\mu\) (\(\bar{\nu}_{\mu}\)) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-flavour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within \(\pm\)500~s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic radiated energy are set for each GW event analysed. |
doi_str_mv | 10.48550/arxiv.2003.04022 |
format | Article |
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In addition to the search for long tracks induced by \(\nu_\mu\) (\(\bar{\nu}_{\mu}\)) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-flavour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within \(\pm\)500~s around the time of six GW events yields no neutrino counterparts. 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U</creatorcontrib><creatorcontrib>Khan-Chowdhury, N R</creatorcontrib><creatorcontrib>Kreykenbohm, I</creatorcontrib><creatorcontrib>Kulikovskiy, V</creatorcontrib><creatorcontrib>R Le Breton</creatorcontrib><creatorcontrib>Lefèvre, D</creatorcontrib><creatorcontrib>Leonora, E</creatorcontrib><creatorcontrib>Lincetto, M</creatorcontrib><creatorcontrib>Lopez-Coto, D</creatorcontrib><creatorcontrib>Loucatos, S</creatorcontrib><creatorcontrib>Maggi, G</creatorcontrib><creatorcontrib>Manczak, J</creatorcontrib><creatorcontrib>Margiotta, A</creatorcontrib><creatorcontrib>Marinelli, A</creatorcontrib><creatorcontrib>Mele, R</creatorcontrib><creatorcontrib>Melis, K</creatorcontrib><creatorcontrib>Migliozzi, P</creatorcontrib><creatorcontrib>Moussa, A</creatorcontrib><creatorcontrib>Muller, R</creatorcontrib><creatorcontrib>Nauta, L</creatorcontrib><creatorcontrib>Navas, S</creatorcontrib><creatorcontrib>Nielsen, C</creatorcontrib><creatorcontrib>Nuñez-Castiñeyra, A</creatorcontrib><creatorcontrib>Păvălaş, G E</creatorcontrib><creatorcontrib>Pellegrino, C</creatorcontrib><creatorcontrib>Perrin-Terrin, M</creatorcontrib><creatorcontrib>Piattelli, P</creatorcontrib><creatorcontrib>Poirè, C</creatorcontrib><creatorcontrib>Popa, V</creatorcontrib><creatorcontrib>Randazzo, N</creatorcontrib><creatorcontrib>Reck, S</creatorcontrib><creatorcontrib>Sanguineti, M</creatorcontrib><creatorcontrib>Sapienza, P</creatorcontrib><creatorcontrib>Schüssler, F</creatorcontrib><creatorcontrib>Spurio, M</creatorcontrib><creatorcontrib>Stolarczyk, Th</creatorcontrib><creatorcontrib>Strandberg, B</creatorcontrib><creatorcontrib>Taiuti, M</creatorcontrib><creatorcontrib>Tayalati, Y</creatorcontrib><creatorcontrib>Thakore, T</creatorcontrib><creatorcontrib>Tingay, S J</creatorcontrib><creatorcontrib>Trovato, A</creatorcontrib><creatorcontrib>Vallage, B</creatorcontrib><creatorcontrib>V Van Elewyck</creatorcontrib><creatorcontrib>Versari, F</creatorcontrib><creatorcontrib>Viola, S</creatorcontrib><creatorcontrib>Vivolo, D</creatorcontrib><creatorcontrib>Wilms, J</creatorcontrib><creatorcontrib>Zaborov, D</creatorcontrib><creatorcontrib>Zornoza, J D</creatorcontrib><title>Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope</title><title>arXiv.org</title><description>An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced-Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by \(\nu_\mu\) (\(\bar{\nu}_{\mu}\)) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-flavour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within \(\pm\)500~s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic radiated energy are set for each GW event analysed.</description><subject>Emission analysis</subject><subject>Flavors</subject><subject>Fluence</subject><subject>Gravitation</subject><subject>Gravitational waves</subject><subject>Neutrinos</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Experiment</subject><subject>Searching</subject><subject>Time dependent 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20210206</creationdate><title>Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope</title><author>ANTARES Collaboration ; Albert, A ; André, M ; Anton, G ; Ardid, M ; Aubert, J J ; Aublin, J ; Basa, S ; Belhorma, B ; Bertin, V ; Biagi, S ; Bissinger, M ; Boumaaza, J ; Brunner, J ; Capone, A ; Carr, J ; Celli, S ; Chabab, M ; Chau, T N ; Chiarusi, T ; Circella, M ; Colomer-Molla, M ; Coniglione, R ; Coyle, P ; Creusot, A ; de Wasseige, G ; Deschamps, A ; Distefano, C ; I Di Palma ; Donzaud, C ; Dornic, D ; Eberl, T ; N El Khayati ; Enzenhöfer, A ; Fermani, P ; Ferrara, G ; Gay, P ; Glotin, H ; Gozzini, R ; R Gracia Ruiz ; Graf, K ; Guidi, C ; Heijboer, A J ; Hello, Y ; Hernández-Rey, J J ; Hößl, J ; Huang, F ; de Jong, M ; Jongen, M ; Kadler, M ; Katz, U ; Khan-Chowdhury, N R ; Kreykenbohm, I ; Kulikovskiy, V ; R Le Breton ; Lefèvre, D ; Leonora, E ; Lincetto, M ; Lopez-Coto, D ; Loucatos, S ; Maggi, G ; Manczak, J ; Margiotta, A ; Marinelli, A ; Mele, R ; Melis, K ; Migliozzi, P ; Moussa, A ; Muller, R ; Nauta, L ; Navas, S ; Nielsen, C ; Nuñez-Castiñeyra, A ; Păvălaş, G E ; Pellegrino, C ; Perrin-Terrin, M ; Piattelli, P ; Poirè, C ; Popa, V ; Randazzo, N ; Reck, S ; Sanguineti, M ; Sapienza, P ; Schüssler, F ; Spurio, M ; Stolarczyk, Th ; Strandberg, B ; Taiuti, M ; Tayalati, Y ; Thakore, T ; Tingay, S J ; Trovato, A ; Vallage, B ; V Van Elewyck ; Versari, F ; Viola, S ; Vivolo, D ; Wilms, J ; Zaborov, D ; Zornoza, J D</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a521-7c641f448e87718453e78987e75f8a104ec5638c83236493886cbe2651971ffd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Emission analysis</topic><topic>Flavors</topic><topic>Fluence</topic><topic>Gravitation</topic><topic>Gravitational waves</topic><topic>Neutrinos</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - High Energy Physics - Experiment</topic><topic>Searching</topic><topic>Time dependent analysis</topic><toplevel>online_resources</toplevel><creatorcontrib>ANTARES Collaboration</creatorcontrib><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>André, M</creatorcontrib><creatorcontrib>Anton, G</creatorcontrib><creatorcontrib>Ardid, M</creatorcontrib><creatorcontrib>Aubert, J J</creatorcontrib><creatorcontrib>Aublin, J</creatorcontrib><creatorcontrib>Basa, S</creatorcontrib><creatorcontrib>Belhorma, B</creatorcontrib><creatorcontrib>Bertin, V</creatorcontrib><creatorcontrib>Biagi, S</creatorcontrib><creatorcontrib>Bissinger, M</creatorcontrib><creatorcontrib>Boumaaza, J</creatorcontrib><creatorcontrib>Brunner, J</creatorcontrib><creatorcontrib>Capone, A</creatorcontrib><creatorcontrib>Carr, J</creatorcontrib><creatorcontrib>Celli, S</creatorcontrib><creatorcontrib>Chabab, M</creatorcontrib><creatorcontrib>Chau, T N</creatorcontrib><creatorcontrib>Chiarusi, T</creatorcontrib><creatorcontrib>Circella, M</creatorcontrib><creatorcontrib>Colomer-Molla, M</creatorcontrib><creatorcontrib>Coniglione, R</creatorcontrib><creatorcontrib>Coyle, P</creatorcontrib><creatorcontrib>Creusot, A</creatorcontrib><creatorcontrib>de Wasseige, G</creatorcontrib><creatorcontrib>Deschamps, A</creatorcontrib><creatorcontrib>Distefano, C</creatorcontrib><creatorcontrib>I Di Palma</creatorcontrib><creatorcontrib>Donzaud, C</creatorcontrib><creatorcontrib>Dornic, 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D</creatorcontrib><creatorcontrib>Zornoza, J D</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ANTARES Collaboration</au><au>Albert, A</au><au>André, M</au><au>Anton, G</au><au>Ardid, M</au><au>Aubert, J J</au><au>Aublin, J</au><au>Basa, S</au><au>Belhorma, B</au><au>Bertin, V</au><au>Biagi, S</au><au>Bissinger, M</au><au>Boumaaza, J</au><au>Brunner, J</au><au>Capone, A</au><au>Carr, J</au><au>Celli, S</au><au>Chabab, M</au><au>Chau, T N</au><au>Chiarusi, T</au><au>Circella, M</au><au>Colomer-Molla, M</au><au>Coniglione, R</au><au>Coyle, P</au><au>Creusot, A</au><au>de Wasseige, G</au><au>Deschamps, A</au><au>Distefano, C</au><au>I Di Palma</au><au>Donzaud, C</au><au>Dornic, D</au><au>Eberl, T</au><au>N El Khayati</au><au>Enzenhöfer, A</au><au>Fermani, P</au><au>Ferrara, G</au><au>Gay, P</au><au>Glotin, H</au><au>Gozzini, R</au><au>R Gracia Ruiz</au><au>Graf, K</au><au>Guidi, C</au><au>Heijboer, A J</au><au>Hello, Y</au><au>Hernández-Rey, J J</au><au>Hößl, J</au><au>Huang, F</au><au>de Jong, M</au><au>Jongen, M</au><au>Kadler, M</au><au>Katz, U</au><au>Khan-Chowdhury, N R</au><au>Kreykenbohm, I</au><au>Kulikovskiy, V</au><au>R Le Breton</au><au>Lefèvre, D</au><au>Leonora, E</au><au>Lincetto, M</au><au>Lopez-Coto, D</au><au>Loucatos, S</au><au>Maggi, G</au><au>Manczak, J</au><au>Margiotta, A</au><au>Marinelli, A</au><au>Mele, R</au><au>Melis, K</au><au>Migliozzi, P</au><au>Moussa, A</au><au>Muller, R</au><au>Nauta, L</au><au>Navas, S</au><au>Nielsen, C</au><au>Nuñez-Castiñeyra, A</au><au>Păvălaş, G E</au><au>Pellegrino, C</au><au>Perrin-Terrin, M</au><au>Piattelli, P</au><au>Poirè, C</au><au>Popa, V</au><au>Randazzo, N</au><au>Reck, S</au><au>Sanguineti, M</au><au>Sapienza, P</au><au>Schüssler, F</au><au>Spurio, M</au><au>Stolarczyk, Th</au><au>Strandberg, B</au><au>Taiuti, M</au><au>Tayalati, Y</au><au>Thakore, T</au><au>Tingay, S J</au><au>Trovato, A</au><au>Vallage, B</au><au>V Van Elewyck</au><au>Versari, F</au><au>Viola, S</au><au>Vivolo, D</au><au>Wilms, J</au><au>Zaborov, D</au><au>Zornoza, J D</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope</atitle><jtitle>arXiv.org</jtitle><date>2021-02-06</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>An offline search for a neutrino counterpart to gravitational-wave (GW) events detected during the second observation run (O2) of Advanced-LIGO and Advanced-Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by \(\nu_\mu\) (\(\bar{\nu}_{\mu}\)) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational-wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all-neutrino-flavour and all-sky time dependent analysis are presented. The search for prompt neutrino emission within \(\pm\)500~s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic radiated energy are set for each GW event analysed.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2003.04022</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2021-02 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_2003_04022 |
source | arXiv.org; Free E- Journals |
subjects | Emission analysis Flavors Fluence Gravitation Gravitational waves Neutrinos Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Experiment Searching Time dependent analysis |
title | Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope |
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