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Constraints on Minute-Scale Transient Astrophysical Neutrino Sources

dc.contributor.authorAartsen, M. G.
dc.contributor.authorAckermann, M.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J. A.
dc.contributor.authorAhlers, M.
dc.contributor.authorAhrens, M.
dc.contributor.authorAl Samarai, I.
dc.contributor.authorAltmann, D.
dc.contributor.authorAndeen, K.
dc.contributor.authorAnderson, T.
dc.contributor.authorAnsseau, I.
dc.contributor.authorAnton, G.
dc.contributor.authorArguelles, C.
dc.contributor.authorAuffenberg, J.
dc.contributor.authorAxani, S.
dc.contributor.authorBackes, P.
dc.contributor.authorBagherpour, H.
dc.contributor.authorBai, X.
dc.contributor.authorBarbano, A.
dc.contributor.authorBarron, J. P.
dc.contributor.authorBarwick, S. W.
dc.contributor.authorBaum, V.
dc.contributor.authorBay, R.
dc.contributor.authorBeatty, J. J.
dc.contributor.authorTjus, J. Becker
dc.contributor.authorBecker, K. -H.
dc.contributor.authorBenZvi, S.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBesson, D. Z.
dc.contributor.authorBinder, G.
dc.contributor.authorBindig, D.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBlot, S.
dc.contributor.authorBohm, C.
dc.contributor.authorBoerner, M.
dc.contributor.authorBos, F.
dc.contributor.authorBoeser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBourbeau, E.
dc.contributor.authorBourbeau, J.
dc.contributor.authorBradascio, F.
dc.contributor.authorBraun, J.
dc.contributor.authorBrenzke, M.
dc.contributor.authorBretz, H. -P.
dc.contributor.authorBron, S.
dc.contributor.authorBrostean-Kaiser, J.
dc.contributor.authorBurgman, A.
dc.contributor.authorBusse, R. S.
dc.contributor.authorCarver, T.
dc.contributor.authorCheung, E.
dc.contributor.authorChirkin, D.
dc.contributor.authorChristov, A.
dc.contributor.authorClark, K.
dc.contributor.authorClassen, L.
dc.contributor.authorCollin, G. H.
dc.contributor.authorConrad, J. M.
dc.contributor.authorCoppin, P.
dc.contributor.authorCorrea, P.
dc.contributor.authorCowen, D. F.
dc.contributor.authorCross, R.
dc.contributor.authorDave, P.
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dc.contributor.authorDe Clercq, C.
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dc.contributor.authorDembinski, H.
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dc.contributor.authorDesiati, P.
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dc.contributor.authorde Wasseige, G.
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dc.contributor.authordi Lorenzo, V.
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dc.contributor.authorFahey, S.
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dc.contributor.otherRWTH Aachen University
dc.contributor.otherUniversity of Adelaide
dc.contributor.otherUniversity of Alaska System
dc.contributor.otherUniversity of Alaska Anchorage
dc.contributor.otherUniversity of Texas System
dc.contributor.otherUniversity of Texas Arlington
dc.contributor.otherClark Atlanta University
dc.contributor.otherUniversity System of Georgia
dc.contributor.otherGeorgia Institute of Technology
dc.contributor.otherSouthern University System
dc.contributor.otherSouthern University & A&M College
dc.contributor.otherUniversity of California System
dc.contributor.otherUniversity of California Berkeley
dc.contributor.otherUnited States Department of Energy (DOE)
dc.contributor.otherLawrence Berkeley National Laboratory
dc.contributor.otherHumboldt University of Berlin
dc.contributor.otherRuhr University Bochum
dc.contributor.otherUniversity of Wurzburg
dc.contributor.otherUniversite Libre de Bruxelles
dc.contributor.otherVrije Universiteit Brussel
dc.contributor.otherMassachusetts Institute of Technology (MIT)
dc.contributor.otherChiba University
dc.contributor.otherUniversity of Canterbury
dc.contributor.otherUniversity System of Maryland
dc.contributor.otherUniversity of Maryland College Park
dc.contributor.otherUniversity System of Ohio
dc.contributor.otherOhio State University
dc.contributor.otherUniversity of Copenhagen
dc.contributor.otherNiels Bohr Institute
dc.contributor.otherDortmund University of Technology
dc.contributor.otherMichigan State University
dc.contributor.otherUniversity of Alberta
dc.contributor.otherUniversity of Erlangen Nuremberg
dc.contributor.otherUniversity of Geneva
dc.contributor.otherGhent University
dc.contributor.otherUniversity of California Irvine
dc.contributor.otherUniversity of Kansas
dc.contributor.otherUniversity of Leicester
dc.contributor.otherUniversity of California Los Angeles
dc.contributor.otherUniversity of Wisconsin System
dc.contributor.otherUniversity of Wisconsin Madison
dc.contributor.otherJohannes Gutenberg University of Mainz
dc.contributor.otherMarquette University
dc.contributor.otherTechnical University of Munich
dc.contributor.otherUniversity of Munster
dc.contributor.otherUniversity of Delaware
dc.contributor.otherYale University
dc.contributor.otherUniversity of Oxford
dc.contributor.otherDrexel University
dc.contributor.otherSouth Dakota School Mines & Technology
dc.contributor.otherUniversity of Rochester
dc.contributor.otherOskar Klein Centre
dc.contributor.otherStockholm University
dc.contributor.otherState University of New York (SUNY) System
dc.contributor.otherState University of New York (SUNY) Stony Brook
dc.contributor.otherSungkyunkwan University (SKKU)
dc.contributor.otherUniversity of Alabama Tuscaloosa
dc.contributor.otherPennsylvania Commonwealth System of Higher Education (PCSHE)
dc.contributor.otherPennsylvania State University
dc.contributor.otherPennsylvania State University - University Park
dc.contributor.otherUppsala University
dc.contributor.otherUniversity of Wuppertal
dc.contributor.otherHelmholtz Association
dc.contributor.otherDeutsches Elektronen-Synchrotron (DESY)
dc.contributor.otherUniversity of Tokyo
dc.date.accessioned2019-07-03T12:57:49Z
dc.date.available2019-07-03T12:57:49Z
dc.date.copyright2019
dc.date.issued2019-02-06
dc.description.abstractHigh-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets, and neutron star mergers. IceCube's optical and x-ray follow-up program searches for such transient sources by looking for two or more muon neutrino candidates in directional coincidence and arriving within 100 s. The measured rate of neutrino alerts is consistent with the expected rate of chance coincidences of atmospheric background events and no likely electromagnetic counterparts have been identified in Swift follow-up observations. Here, we calculate generic bounds on the neutrino flux of short-lived transient sources. Assuming an E-2.5 neutrino spectrum, we find that the neutrino flux of rare sources, like long gamma-ray bursts, is constrained to < 5% of the detected astrophysical flux and the energy released in neutrinos (100 GeV to 10 PeV) by a median bright GRB-like source is < 10(52.5) erg. For a harder E-2.13 neutrino spectrum up to 30% of the flux could be produced by GRBs and the allowed median source energy is < 10(52) erg. A hypothetical population of transient sources has to be more common than 10(-5) Mpc(-3) yr(-1) (5 x 10(-8) Mpc(-3) yr(-1) for the E-2.13 spectrum) to account for the complete astrophysical neutrino flux.en_US
dc.format.mimetypeapplication/pdf
dc.identifier.citationAartsen, M.G., et al. (2019): Constraints on Minute-Scale Transient Astrophysical Neutrino Sources. Physical Review Letters, 122(5). DOI: https://doi.org/10.1103/PhysRevLett.122.051102
dc.identifier.doi10.1103/PhysRevLett.122.051102
dc.identifier.issn0031-9007
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dc.identifier.urihttp://ir.ua.edu/handle/123456789/5883
dc.languageEnglish
dc.language.isoen_US
dc.publisherAmerican Physical Society
dc.rights.holderAmerican Physical Society
dc.subjectGAMMA-RAY BURSTS
dc.subjectHIGH-ENERGY NEUTRINOS
dc.subjectPhysics, Multidisciplinary
dc.subjectPhysics
dc.titleConstraints on Minute-Scale Transient Astrophysical Neutrino Sourcesen_US
dc.typetext
dc.typeArticle

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MSantander_Constraints on Minute-Scale Transient Astrophysical Neutrino Sources_Physics and Astronomy.pdf
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