Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore
The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by the thermonuclear runaway, recent GeV gamma-r...
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| creator | Adams, J Alves, A A Ashida, Y Axani, S N Balagopal, A Baricevic, M Barwick, S W J Becker Tjus Bellenghi, C Bernardini, E Blot, S Bontempo, F Bourbeau, E Coppin, P Countryman, S Cowen, D F Desai, A de Wasseige, G DeYoung, T Diaz, A Dujmovic, H Erpenbeck, H Fan, K L Fiedlschuster, S Fox, D Franckowiak, A Garcia, A Gerhardt, L Glaser, C Glüsenkamp, T Grant, D Günther, C Hallgren, A Hardin, J Hatch, P Henningsen, F Hussain, R Iovine, N Ishihara, A Kardum, L Karg, T Katz, U Kochocki, A Koirala, R Kolanoski, H Köpke, L Krupczak, E Kurahashi, N Lazar, J P K Leonard DeHolton L Lu Lucarelli, F Ma, W Y Madsen, J Mancina, S Maruyama, R Mayhew, F McElroy, T Medina, A Meier, M Merckx, Y Moore, R W Moulai, M Naab, R Naumann, U Niederhausen, H Pollmann, A Obertacke Oeyen, B Paudel, E N Paul, L C Pérez de los Heros Rack-Helleis, J Resconi, E Safa, I Schaufel, M Seckel, D Sharma, A Shimizu, N Snihur, R Soedingrekso, J Spiczak, G M Spiering, C Stanev, T Stein, R Taboada, I Ter-Antonyan, S Tilav, S Tosi, D Twagirayezu, J P Valtonen-Mattila, N Vandenbroucke, J J van Santen Veitch-Michaelis, J Weigel, P Whitehorn, N Wiebusch, C H Willey, N Yanez, J P S Yu Yuan, T |
| description | The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by the thermonuclear runaway, recent GeV gamma-ray observations have supported the notion that a significant portion of the luminosity could come from radiative shocks. More recently, observations of novae have lent evidence that these shocks are acceleration sites for hadrons for at least some types of novae. In this scenario, a flux of neutrinos may accompany the observed gamma rays. As the gamma rays from most novae have only been observed up to a few GeV, novae have previously not been considered as targets for neutrino telescopes, which are most sensitive at and above TeV energies. Here, we present the first search for neutrinos from novae with energies between a few GeV and 10 TeV using IceCube-DeepCore, a densely instrumented region of the IceCube Neutrino Observatory with a reduced energy threshold. We search both for a correlation between gamma-ray and neutrino emission as well as between optical and neutrino emission from novae. We find no evidence for neutrino emission from the novae considered in this analysis and set upper limits for all gamma-ray detected novae. |
| doi_str_mv | 10.48550/arxiv.2212.06810 |
| format | Article |
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Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by the thermonuclear runaway, recent GeV gamma-ray observations have supported the notion that a significant portion of the luminosity could come from radiative shocks. More recently, observations of novae have lent evidence that these shocks are acceleration sites for hadrons for at least some types of novae. In this scenario, a flux of neutrinos may accompany the observed gamma rays. As the gamma rays from most novae have only been observed up to a few GeV, novae have previously not been considered as targets for neutrino telescopes, which are most sensitive at and above TeV energies. Here, we present the first search for neutrinos from novae with energies between a few GeV and 10 TeV using IceCube-DeepCore, a densely instrumented region of the IceCube Neutrino Observatory with a reduced energy threshold. We search both for a correlation between gamma-ray and neutrino emission as well as between optical and neutrino emission from novae. We find no evidence for neutrino emission from the novae considered in this analysis and set upper limits for all gamma-ray detected novae.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2212.06810</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Binary stars ; Dwarf novae ; Emission analysis ; Gamma rays ; Hadrons ; Luminosity ; Neutrinos ; Novae ; Physics - High Energy Astrophysical Phenomena ; Searching ; Telescopes ; White dwarf stars</subject><ispartof>arXiv.org, 2024-07</ispartof><rights>2024. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.3847/1538-4357/acdc1b$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.2212.06810$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Adams, J</creatorcontrib><creatorcontrib>Alves, A A</creatorcontrib><creatorcontrib>Ashida, Y</creatorcontrib><creatorcontrib>Axani, S N</creatorcontrib><creatorcontrib>Balagopal, A</creatorcontrib><creatorcontrib>Baricevic, M</creatorcontrib><creatorcontrib>Barwick, S W</creatorcontrib><creatorcontrib>J Becker Tjus</creatorcontrib><creatorcontrib>Bellenghi, C</creatorcontrib><creatorcontrib>Bernardini, E</creatorcontrib><creatorcontrib>Blot, S</creatorcontrib><creatorcontrib>Bontempo, F</creatorcontrib><creatorcontrib>Bourbeau, E</creatorcontrib><creatorcontrib>Coppin, P</creatorcontrib><creatorcontrib>Countryman, S</creatorcontrib><creatorcontrib>Cowen, D F</creatorcontrib><creatorcontrib>Desai, A</creatorcontrib><creatorcontrib>de Wasseige, G</creatorcontrib><creatorcontrib>DeYoung, T</creatorcontrib><creatorcontrib>Diaz, A</creatorcontrib><creatorcontrib>Dujmovic, H</creatorcontrib><creatorcontrib>Erpenbeck, H</creatorcontrib><creatorcontrib>Fan, K L</creatorcontrib><creatorcontrib>Fiedlschuster, S</creatorcontrib><creatorcontrib>Fox, D</creatorcontrib><creatorcontrib>Franckowiak, A</creatorcontrib><creatorcontrib>Garcia, A</creatorcontrib><creatorcontrib>Gerhardt, 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Lu</creatorcontrib><creatorcontrib>Lucarelli, F</creatorcontrib><creatorcontrib>Ma, W Y</creatorcontrib><creatorcontrib>Madsen, J</creatorcontrib><creatorcontrib>Mancina, S</creatorcontrib><creatorcontrib>Maruyama, R</creatorcontrib><creatorcontrib>Mayhew, F</creatorcontrib><creatorcontrib>McElroy, T</creatorcontrib><creatorcontrib>Medina, A</creatorcontrib><creatorcontrib>Meier, M</creatorcontrib><creatorcontrib>Merckx, Y</creatorcontrib><creatorcontrib>Moore, R W</creatorcontrib><creatorcontrib>Moulai, M</creatorcontrib><creatorcontrib>Naab, R</creatorcontrib><creatorcontrib>Naumann, U</creatorcontrib><creatorcontrib>Niederhausen, H</creatorcontrib><creatorcontrib>Pollmann, A Obertacke</creatorcontrib><creatorcontrib>Oeyen, B</creatorcontrib><creatorcontrib>Paudel, E N</creatorcontrib><creatorcontrib>Paul, L</creatorcontrib><creatorcontrib>C Pérez de los Heros</creatorcontrib><creatorcontrib>Rack-Helleis, J</creatorcontrib><creatorcontrib>Resconi, E</creatorcontrib><creatorcontrib>Safa, I</creatorcontrib><creatorcontrib>Schaufel, M</creatorcontrib><creatorcontrib>Seckel, D</creatorcontrib><creatorcontrib>Sharma, A</creatorcontrib><creatorcontrib>Shimizu, N</creatorcontrib><creatorcontrib>Snihur, R</creatorcontrib><creatorcontrib>Soedingrekso, J</creatorcontrib><creatorcontrib>Spiczak, G M</creatorcontrib><creatorcontrib>Spiering, C</creatorcontrib><creatorcontrib>Stanev, T</creatorcontrib><creatorcontrib>Stein, R</creatorcontrib><creatorcontrib>Taboada, I</creatorcontrib><creatorcontrib>Ter-Antonyan, S</creatorcontrib><creatorcontrib>Tilav, S</creatorcontrib><creatorcontrib>Tosi, D</creatorcontrib><creatorcontrib>Twagirayezu, J P</creatorcontrib><creatorcontrib>Valtonen-Mattila, N</creatorcontrib><creatorcontrib>Vandenbroucke, J</creatorcontrib><creatorcontrib>J van Santen</creatorcontrib><creatorcontrib>Veitch-Michaelis, J</creatorcontrib><creatorcontrib>Weigel, P</creatorcontrib><creatorcontrib>Whitehorn, N</creatorcontrib><creatorcontrib>Wiebusch, C H</creatorcontrib><creatorcontrib>Willey, N</creatorcontrib><creatorcontrib>Yanez, J P</creatorcontrib><creatorcontrib>S Yu</creatorcontrib><creatorcontrib>Yuan, T</creatorcontrib><title>Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore</title><title>arXiv.org</title><description>The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by the thermonuclear runaway, recent GeV gamma-ray observations have supported the notion that a significant portion of the luminosity could come from radiative shocks. More recently, observations of novae have lent evidence that these shocks are acceleration sites for hadrons for at least some types of novae. In this scenario, a flux of neutrinos may accompany the observed gamma rays. As the gamma rays from most novae have only been observed up to a few GeV, novae have previously not been considered as targets for neutrino telescopes, which are most sensitive at and above TeV energies. Here, we present the first search for neutrinos from novae with energies between a few GeV and 10 TeV using IceCube-DeepCore, a densely instrumented region of the IceCube Neutrino Observatory with a reduced energy threshold. We search both for a correlation between gamma-ray and neutrino emission as well as between optical and neutrino emission from novae. We find no evidence for neutrino emission from the novae considered in this analysis and set upper limits for all gamma-ray detected novae.</description><subject>Binary stars</subject><subject>Dwarf novae</subject><subject>Emission analysis</subject><subject>Gamma rays</subject><subject>Hadrons</subject><subject>Luminosity</subject><subject>Neutrinos</subject><subject>Novae</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Searching</subject><subject>Telescopes</subject><subject>White dwarf stars</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkE1Lw0AURQdBsNT-AFcOuE5882YmH0uJVQulLgxuwyR5oSkmE2eSqv_e2Lq6m8PlnsvYjYBQJVrDvXHf7TFEFBhClAi4YAuUUgSJQrxiK-8PAIBRjFrLBVu_kXHVnjfWcT-VQU7vfEfT6Nre8nXXet_anjfOdnxnj4b4Vzvu-aaibCopeCQaMuvoml025sPT6j-XLH9a59lLsH193mQP28CkGgJlagVSRUllJCLVVCuZKqFjiZCAiOK6oVqAURVWs0mFAnQJVEdaiFJLlEt2e649ORaDazvjfoo_1-LkOhN3Z2Jw9nMiPxYHO7l-3lRgrOcHZKqV_AW9alSZ</recordid><startdate>20240726</startdate><enddate>20240726</enddate><creator>Adams, J</creator><creator>Alves, A A</creator><creator>Ashida, Y</creator><creator>Axani, S N</creator><creator>Balagopal, A</creator><creator>Baricevic, M</creator><creator>Barwick, S W</creator><creator>J Becker 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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>20240726</creationdate><title>Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore</title><author>Adams, J ; Alves, A A ; Ashida, Y ; Axani, S N ; Balagopal, A ; Baricevic, M ; Barwick, S W ; J Becker Tjus ; Bellenghi, C ; Bernardini, E ; Blot, S ; Bontempo, F ; Bourbeau, E ; Coppin, P ; Countryman, S ; Cowen, D F ; Desai, A ; de Wasseige, G ; DeYoung, T ; Diaz, A ; Dujmovic, H ; Erpenbeck, H ; Fan, K L ; Fiedlschuster, S ; Fox, D ; Franckowiak, A ; Garcia, A ; Gerhardt, L ; Glaser, C ; Glüsenkamp, T ; Grant, D ; Günther, C ; Hallgren, A ; Hardin, J ; Hatch, P ; Henningsen, F ; Hussain, R ; Iovine, N ; Ishihara, A ; Kardum, L ; Karg, T ; Katz, U ; Kochocki, A ; Koirala, R ; Kolanoski, H ; Köpke, L ; Krupczak, E ; Kurahashi, N ; Lazar, J P ; K Leonard DeHolton ; L Lu ; Lucarelli, F ; Ma, W Y ; Madsen, J ; Mancina, S ; Maruyama, R ; Mayhew, F ; McElroy, T ; Medina, A ; Meier, M ; Merckx, Y ; Moore, R W ; Moulai, M ; Naab, R ; Naumann, U ; Niederhausen, H ; Pollmann, A Obertacke ; Oeyen, B ; Paudel, E N ; Paul, L ; C Pérez de los Heros ; Rack-Helleis, J ; Resconi, E ; Safa, I ; Schaufel, M ; Seckel, D ; Sharma, A ; Shimizu, N ; Snihur, R ; Soedingrekso, J ; Spiczak, G M ; Spiering, C ; Stanev, T ; Stein, R ; Taboada, I ; Ter-Antonyan, S ; Tilav, S ; Tosi, D ; Twagirayezu, J P ; Valtonen-Mattila, N ; Vandenbroucke, J ; J van Santen ; Veitch-Michaelis, J ; Weigel, P ; Whitehorn, N ; Wiebusch, C H ; Willey, N ; Yanez, J P ; S Yu ; Yuan, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a950-4ad403468ca322eded439415732080167dfed10a4c2c550c2105b0ed6511b5323</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Binary stars</topic><topic>Dwarf novae</topic><topic>Emission analysis</topic><topic>Gamma rays</topic><topic>Hadrons</topic><topic>Luminosity</topic><topic>Neutrinos</topic><topic>Novae</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Searching</topic><topic>Telescopes</topic><topic>White dwarf stars</topic><toplevel>online_resources</toplevel><creatorcontrib>Adams, J</creatorcontrib><creatorcontrib>Alves, A A</creatorcontrib><creatorcontrib>Ashida, Y</creatorcontrib><creatorcontrib>Axani, S N</creatorcontrib><creatorcontrib>Balagopal, A</creatorcontrib><creatorcontrib>Baricevic, M</creatorcontrib><creatorcontrib>Barwick, S W</creatorcontrib><creatorcontrib>J Becker Tjus</creatorcontrib><creatorcontrib>Bellenghi, C</creatorcontrib><creatorcontrib>Bernardini, E</creatorcontrib><creatorcontrib>Blot, S</creatorcontrib><creatorcontrib>Bontempo, F</creatorcontrib><creatorcontrib>Bourbeau, E</creatorcontrib><creatorcontrib>Coppin, P</creatorcontrib><creatorcontrib>Countryman, S</creatorcontrib><creatorcontrib>Cowen, D F</creatorcontrib><creatorcontrib>Desai, A</creatorcontrib><creatorcontrib>de Wasseige, G</creatorcontrib><creatorcontrib>DeYoung, T</creatorcontrib><creatorcontrib>Diaz, A</creatorcontrib><creatorcontrib>Dujmovic, H</creatorcontrib><creatorcontrib>Erpenbeck, H</creatorcontrib><creatorcontrib>Fan, K L</creatorcontrib><creatorcontrib>Fiedlschuster, S</creatorcontrib><creatorcontrib>Fox, D</creatorcontrib><creatorcontrib>Franckowiak, A</creatorcontrib><creatorcontrib>Garcia, A</creatorcontrib><creatorcontrib>Gerhardt, L</creatorcontrib><creatorcontrib>Glaser, C</creatorcontrib><creatorcontrib>Glüsenkamp, T</creatorcontrib><creatorcontrib>Grant, D</creatorcontrib><creatorcontrib>Günther, C</creatorcontrib><creatorcontrib>Hallgren, A</creatorcontrib><creatorcontrib>Hardin, J</creatorcontrib><creatorcontrib>Hatch, P</creatorcontrib><creatorcontrib>Henningsen, F</creatorcontrib><creatorcontrib>Hussain, R</creatorcontrib><creatorcontrib>Iovine, N</creatorcontrib><creatorcontrib>Ishihara, A</creatorcontrib><creatorcontrib>Kardum, L</creatorcontrib><creatorcontrib>Karg, T</creatorcontrib><creatorcontrib>Katz, U</creatorcontrib><creatorcontrib>Kochocki, A</creatorcontrib><creatorcontrib>Koirala, R</creatorcontrib><creatorcontrib>Kolanoski, H</creatorcontrib><creatorcontrib>Köpke, L</creatorcontrib><creatorcontrib>Krupczak, E</creatorcontrib><creatorcontrib>Kurahashi, N</creatorcontrib><creatorcontrib>Lazar, J P</creatorcontrib><creatorcontrib>K Leonard DeHolton</creatorcontrib><creatorcontrib>L Lu</creatorcontrib><creatorcontrib>Lucarelli, F</creatorcontrib><creatorcontrib>Ma, W Y</creatorcontrib><creatorcontrib>Madsen, J</creatorcontrib><creatorcontrib>Mancina, S</creatorcontrib><creatorcontrib>Maruyama, R</creatorcontrib><creatorcontrib>Mayhew, F</creatorcontrib><creatorcontrib>McElroy, T</creatorcontrib><creatorcontrib>Medina, A</creatorcontrib><creatorcontrib>Meier, M</creatorcontrib><creatorcontrib>Merckx, Y</creatorcontrib><creatorcontrib>Moore, R W</creatorcontrib><creatorcontrib>Moulai, M</creatorcontrib><creatorcontrib>Naab, R</creatorcontrib><creatorcontrib>Naumann, U</creatorcontrib><creatorcontrib>Niederhausen, H</creatorcontrib><creatorcontrib>Pollmann, A Obertacke</creatorcontrib><creatorcontrib>Oeyen, B</creatorcontrib><creatorcontrib>Paudel, E N</creatorcontrib><creatorcontrib>Paul, L</creatorcontrib><creatorcontrib>C Pérez de los Heros</creatorcontrib><creatorcontrib>Rack-Helleis, J</creatorcontrib><creatorcontrib>Resconi, E</creatorcontrib><creatorcontrib>Safa, I</creatorcontrib><creatorcontrib>Schaufel, M</creatorcontrib><creatorcontrib>Seckel, D</creatorcontrib><creatorcontrib>Sharma, A</creatorcontrib><creatorcontrib>Shimizu, N</creatorcontrib><creatorcontrib>Snihur, R</creatorcontrib><creatorcontrib>Soedingrekso, J</creatorcontrib><creatorcontrib>Spiczak, G M</creatorcontrib><creatorcontrib>Spiering, C</creatorcontrib><creatorcontrib>Stanev, T</creatorcontrib><creatorcontrib>Stein, R</creatorcontrib><creatorcontrib>Taboada, I</creatorcontrib><creatorcontrib>Ter-Antonyan, S</creatorcontrib><creatorcontrib>Tilav, S</creatorcontrib><creatorcontrib>Tosi, D</creatorcontrib><creatorcontrib>Twagirayezu, J P</creatorcontrib><creatorcontrib>Valtonen-Mattila, N</creatorcontrib><creatorcontrib>Vandenbroucke, J</creatorcontrib><creatorcontrib>J van Santen</creatorcontrib><creatorcontrib>Veitch-Michaelis, J</creatorcontrib><creatorcontrib>Weigel, P</creatorcontrib><creatorcontrib>Whitehorn, N</creatorcontrib><creatorcontrib>Wiebusch, C H</creatorcontrib><creatorcontrib>Willey, N</creatorcontrib><creatorcontrib>Yanez, J P</creatorcontrib><creatorcontrib>S Yu</creatorcontrib><creatorcontrib>Yuan, T</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</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>Adams, J</au><au>Alves, A A</au><au>Ashida, Y</au><au>Axani, S N</au><au>Balagopal, A</au><au>Baricevic, M</au><au>Barwick, S W</au><au>J Becker Tjus</au><au>Bellenghi, C</au><au>Bernardini, E</au><au>Blot, S</au><au>Bontempo, F</au><au>Bourbeau, E</au><au>Coppin, P</au><au>Countryman, S</au><au>Cowen, D F</au><au>Desai, A</au><au>de Wasseige, G</au><au>DeYoung, T</au><au>Diaz, A</au><au>Dujmovic, H</au><au>Erpenbeck, H</au><au>Fan, K L</au><au>Fiedlschuster, S</au><au>Fox, D</au><au>Franckowiak, A</au><au>Garcia, A</au><au>Gerhardt, L</au><au>Glaser, C</au><au>Glüsenkamp, T</au><au>Grant, D</au><au>Günther, C</au><au>Hallgren, A</au><au>Hardin, J</au><au>Hatch, P</au><au>Henningsen, F</au><au>Hussain, R</au><au>Iovine, N</au><au>Ishihara, A</au><au>Kardum, L</au><au>Karg, T</au><au>Katz, U</au><au>Kochocki, A</au><au>Koirala, R</au><au>Kolanoski, H</au><au>Köpke, L</au><au>Krupczak, E</au><au>Kurahashi, N</au><au>Lazar, J P</au><au>K Leonard DeHolton</au><au>L Lu</au><au>Lucarelli, F</au><au>Ma, W Y</au><au>Madsen, J</au><au>Mancina, S</au><au>Maruyama, R</au><au>Mayhew, F</au><au>McElroy, T</au><au>Medina, A</au><au>Meier, M</au><au>Merckx, Y</au><au>Moore, R W</au><au>Moulai, M</au><au>Naab, R</au><au>Naumann, U</au><au>Niederhausen, H</au><au>Pollmann, A Obertacke</au><au>Oeyen, B</au><au>Paudel, E N</au><au>Paul, L</au><au>C Pérez de los Heros</au><au>Rack-Helleis, J</au><au>Resconi, E</au><au>Safa, I</au><au>Schaufel, M</au><au>Seckel, D</au><au>Sharma, A</au><au>Shimizu, N</au><au>Snihur, R</au><au>Soedingrekso, J</au><au>Spiczak, G M</au><au>Spiering, C</au><au>Stanev, T</au><au>Stein, R</au><au>Taboada, I</au><au>Ter-Antonyan, S</au><au>Tilav, S</au><au>Tosi, D</au><au>Twagirayezu, J P</au><au>Valtonen-Mattila, N</au><au>Vandenbroucke, J</au><au>J van Santen</au><au>Veitch-Michaelis, J</au><au>Weigel, P</au><au>Whitehorn, N</au><au>Wiebusch, C H</au><au>Willey, N</au><au>Yanez, J P</au><au>S Yu</au><au>Yuan, T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore</atitle><jtitle>arXiv.org</jtitle><date>2024-07-26</date><risdate>2024</risdate><eissn>2331-8422</eissn><abstract>The understanding of novae, the thermonuclear eruptions on the surfaces of white dwarf stars in binaries, has recently undergone a major paradigm shift. Though the bolometric luminosity of novae was long thought to arise directly from photons supplied by the thermonuclear runaway, recent GeV gamma-ray observations have supported the notion that a significant portion of the luminosity could come from radiative shocks. More recently, observations of novae have lent evidence that these shocks are acceleration sites for hadrons for at least some types of novae. In this scenario, a flux of neutrinos may accompany the observed gamma rays. As the gamma rays from most novae have only been observed up to a few GeV, novae have previously not been considered as targets for neutrino telescopes, which are most sensitive at and above TeV energies. Here, we present the first search for neutrinos from novae with energies between a few GeV and 10 TeV using IceCube-DeepCore, a densely instrumented region of the IceCube Neutrino Observatory with a reduced energy threshold. We search both for a correlation between gamma-ray and neutrino emission as well as between optical and neutrino emission from novae. We find no evidence for neutrino emission from the novae considered in this analysis and set upper limits for all gamma-ray detected novae.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2212.06810</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2024-07 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_2212_06810 |
| source | arXiv.org; Free E- Journals |
| subjects | Binary stars Dwarf novae Emission analysis Gamma rays Hadrons Luminosity Neutrinos Novae Physics - High Energy Astrophysical Phenomena Searching Telescopes White dwarf stars |
| title | Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-01T11%3A04%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Search%20for%20sub-TeV%20Neutrino%20Emission%20from%20Novae%20with%20IceCube-DeepCore&rft.jtitle=arXiv.org&rft.au=Adams,%20J&rft.date=2024-07-26&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2212.06810&rft_dat=%3Cproquest_arxiv%3E2754223954%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2754223954&rft_id=info:pmid/&rfr_iscdi=true |