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NEUTRINO ANALYSIS OF THE 2010 SEPTEMBER CRAB NEBULA FLARE AND TIME-INTEGRATED CONSTRAINTS ON NEUTRINO EMISSION FROM THE CRAB USING ICECUBE

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dc.contributor.authorAbbasi, R.
dc.contributor.authorAbdou, Y.
dc.contributor.authorAbu-Zayyad, T.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J. A.
dc.contributor.authorAhlers, M.
dc.contributor.authorAltmann, D.
dc.contributor.authorAndeen, K.
dc.contributor.authorAuffenberg, J.
dc.contributor.authorBai, X.
dc.contributor.authorBaker, M.
dc.contributor.authorBarwick, S. W.
dc.contributor.authorBay, R.
dc.contributor.authorAlba, J. L. Bazo
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dc.contributor.authorBenZvi, S.
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dc.contributor.authorBerghaus, P.
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dc.contributor.authorEhrlich, R.
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dc.contributor.otherUniversity of Wisconsin System
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dc.contributor.otherUniversity of California Berkeley
dc.contributor.otherHelmholtz Association
dc.contributor.otherDeutsches Elektronen-Synchrotron (DESY)
dc.contributor.otherUnited States Department of Energy (DOE)
dc.contributor.otherLawrence Berkeley National Laboratory
dc.contributor.otherUniversity System of Ohio
dc.contributor.otherOhio State University
dc.contributor.otherUniversite Libre de Bruxelles
dc.contributor.otherRuhr University Bochum
dc.contributor.otherUniversity of Wurzburg
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dc.contributor.otherUniversity of Kansas
dc.contributor.otherOskar Klein Centre
dc.contributor.otherStockholm University
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dc.contributor.otherUppsala University
dc.contributor.otherPennsylvania Commonwealth System of Higher Education (PCSHE)
dc.contributor.otherPennsylvania State University
dc.contributor.otherPennsylvania State University - University Park
dc.contributor.otherDortmund University of Technology
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dc.contributor.otherEcole Polytechnique Federale de Lausanne
dc.contributor.otherMax Planck Society
dc.contributor.otherUniversity System of Georgia
dc.contributor.otherGeorgia Institute of Technology
dc.contributor.otherClark Atlanta University
dc.contributor.otherSouthern University System
dc.contributor.otherSouthern University & A&M College
dc.contributor.otherUniversity of Alberta
dc.contributor.otherJohannes Gutenberg University of Mainz
dc.contributor.otherUniversity of Mons
dc.contributor.otherChiba University
dc.contributor.otherUniversity of Alaska System
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dc.contributor.otherUniversity West Indies Mona Jamaica
dc.contributor.otherUniversity of the West Indies Open Campus
dc.contributor.otherUniversity of Alabama Tuscaloosa
dc.contributor.otherUniversita degli Studi di Bari Aldo Moro
dc.contributor.otherNational Aeronautics & Space Administration (NASA)
dc.contributor.otherNASA Goddard Space Flight Center
dc.date.accessioned2019-06-25T13:44:48Z
dc.date.available2019-06-25T13:44:48Z
dc.date.issued2011-12-28
dc.description.abstractWe present the results of a search for high-energy muon neutrinos with the IceCube detector in coincidence with the Crab Nebula flare reported on 2010 September by various experiments. Due to the unusual flaring state of the otherwise steady source we performed a prompt analysis of the 79-string configuration data to search for neutrinos that might be emitted along with the observed. gamma-rays. We performed two different and complementary data selections of neutrino events in the time window of 10 days around the flare. One event selection is optimized for discovery of E-upsilon(2). neutrino spectrum typical of first-order Fermi acceleration. A similar event selection has also been applied to the 40-string data to derive the time-integrated limits to the neutrino emission from the Crab. The other event selection was optimized for discovery of neutrino spectra with softer spectral index and TeV energy cutoffs as observed for various Galactic sources in. gamma-rays. The 90% confidence level (CL) best upper limits on the Crab flux during the 10 day flare are 4.73 x 10(-11) cm(-2) s(-1) TeV-1 for an E-upsilon(2). neutrino spectrum and 2.50 x 10(-10) cm(-2) s(-1) TeV-1 for a softer neutrino spectra of E-upsilon(-2.7), as indicated by Fermi measurements during the flare. In this paper, we also illustrate the impact of the time-integrated limit on the Crab neutrino steady emission. The limit obtained using 375.5 days of the 40-string configuration is compared to existing models of neutrino production from the Crab and its impact on astrophysical parameters is discussed. The most optimistic predictions of some models are already rejected by the IceCube neutrino telescope with more than 90% CL.en_US
dc.format.mimetypeapplication/pdf
dc.identifier.citationAbbasi, R., et al. (2012): Neutrino Analysis of the 2010 September Crab Nebula Flare and Time-integrated Constraints on Neutrino Emission from the Crab Using IceCube. The Astrophysical Journal, 745(1). DOI: http://dx.doi.org/10.1088/0004-637X/745/1/45
dc.identifier.doi10.1088/0004-637X/745/1/45
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dc.identifier.urihttp://ir.ua.edu/handle/123456789/5835
dc.languageEnglish
dc.language.isoen_US
dc.publisherIOP Publishing
dc.subjectgamma rays: general
dc.subjectISM: supernova remnants
dc.subjectneutrinos
dc.subjectpulsars: individual (Crab Pulsar)
dc.subjectHIGH-ENERGY NEUTRINOS
dc.subjectGAMMA-RAY FLARES
dc.subjectPULSAR
dc.subjectSYSTEM
dc.subjectAstronomy & Astrophysics
dc.titleNEUTRINO ANALYSIS OF THE 2010 SEPTEMBER CRAB NEBULA FLARE AND TIME-INTEGRATED CONSTRAINTS ON NEUTRINO EMISSION FROM THE CRAB USING ICECUBEen_US
dc.typetext
dc.typeArticle

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