Constraints on Minute-Scale Transient Astrophysical Neutrino Sources
| dc.contributor.author | Aartsen, M. G. | |
| dc.contributor.author | Ackermann, M. | |
| dc.contributor.author | Adams, J. | |
| dc.contributor.author | Aguilar, J. A. | |
| dc.contributor.author | Ahlers, M. | |
| dc.contributor.author | Ahrens, M. | |
| dc.contributor.author | Al Samarai, I. | |
| dc.contributor.author | Altmann, D. | |
| dc.contributor.author | Andeen, K. | |
| dc.contributor.author | Anderson, T. | |
| dc.contributor.author | Ansseau, I. | |
| dc.contributor.author | Anton, G. | |
| dc.contributor.author | Arguelles, C. | |
| dc.contributor.author | Auffenberg, J. | |
| dc.contributor.author | Axani, S. | |
| dc.contributor.author | Backes, P. | |
| dc.contributor.author | Bagherpour, H. | |
| dc.contributor.author | Bai, X. | |
| dc.contributor.author | Barbano, A. | |
| dc.contributor.author | Barron, J. P. | |
| dc.contributor.author | Barwick, S. W. | |
| dc.contributor.author | Baum, V. | |
| dc.contributor.author | Bay, R. | |
| dc.contributor.author | Beatty, J. J. | |
| dc.contributor.author | Tjus, J. Becker | |
| dc.contributor.author | Becker, K. -H. | |
| dc.contributor.author | BenZvi, S. | |
| dc.contributor.author | Berley, D. | |
| dc.contributor.author | Bernardini, E. | |
| dc.contributor.author | Besson, D. Z. | |
| dc.contributor.author | Binder, G. | |
| dc.contributor.author | Bindig, D. | |
| dc.contributor.author | Blaufuss, E. | |
| dc.contributor.author | Blot, S. | |
| dc.contributor.author | Bohm, C. | |
| dc.contributor.author | Boerner, M. | |
| dc.contributor.author | Bos, F. | |
| dc.contributor.author | Boeser, S. | |
| dc.contributor.author | Botner, O. | |
| dc.contributor.author | Bourbeau, E. | |
| dc.contributor.author | Bourbeau, J. | |
| dc.contributor.author | Bradascio, F. | |
| dc.contributor.author | Braun, J. | |
| dc.contributor.author | Brenzke, M. | |
| dc.contributor.author | Bretz, H. -P. | |
| dc.contributor.author | Bron, S. | |
| dc.contributor.author | Brostean-Kaiser, J. | |
| dc.contributor.author | Burgman, A. | |
| dc.contributor.author | Busse, R. S. | |
| dc.contributor.author | Carver, T. | |
| dc.contributor.author | Cheung, E. | |
| dc.contributor.author | Chirkin, D. | |
| dc.contributor.author | Christov, A. | |
| dc.contributor.author | Clark, K. | |
| dc.contributor.author | Classen, L. | |
| dc.contributor.author | Collin, G. H. | |
| dc.contributor.author | Conrad, J. M. | |
| dc.contributor.author | Coppin, P. | |
| dc.contributor.author | Correa, P. | |
| dc.contributor.author | Cowen, D. F. | |
| dc.contributor.author | Cross, R. | |
| dc.contributor.author | Dave, P. | |
| dc.contributor.author | Day, M. | |
| dc.contributor.author | de Andre, J. P. A. M. | |
| dc.contributor.author | De Clercq, C. | |
| dc.contributor.author | DeLaunay, J. J. | |
| dc.contributor.author | Dembinski, H. | |
| dc.contributor.author | Deoskar, K. | |
| dc.contributor.author | De Ridder, S. | |
| dc.contributor.author | Desiati, P. | |
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| dc.contributor.author | de Wasseige, G. | |
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| dc.contributor.author | Dunkman, M. | |
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| dc.contributor.author | Krings, K. | |
| dc.contributor.author | Kroll, M. | |
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| dc.contributor.author | Yoshida, S. | |
| dc.contributor.author | Yuan, T. | |
| dc.contributor.other | RWTH Aachen University | |
| dc.contributor.other | University of Adelaide | |
| dc.contributor.other | University of Alaska System | |
| dc.contributor.other | University of Alaska Anchorage | |
| dc.contributor.other | University of Texas System | |
| dc.contributor.other | University of Texas Arlington | |
| dc.contributor.other | Clark Atlanta University | |
| dc.contributor.other | University System of Georgia | |
| dc.contributor.other | Georgia Institute of Technology | |
| dc.contributor.other | Southern University System | |
| dc.contributor.other | Southern University & A&M College | |
| dc.contributor.other | University of California System | |
| dc.contributor.other | University of California Berkeley | |
| dc.contributor.other | United States Department of Energy (DOE) | |
| dc.contributor.other | Lawrence Berkeley National Laboratory | |
| dc.contributor.other | Humboldt University of Berlin | |
| dc.contributor.other | Ruhr University Bochum | |
| dc.contributor.other | University of Wurzburg | |
| dc.contributor.other | Universite Libre de Bruxelles | |
| dc.contributor.other | Vrije Universiteit Brussel | |
| dc.contributor.other | Massachusetts Institute of Technology (MIT) | |
| dc.contributor.other | Chiba University | |
| dc.contributor.other | University of Canterbury | |
| dc.contributor.other | University System of Maryland | |
| dc.contributor.other | University of Maryland College Park | |
| dc.contributor.other | University System of Ohio | |
| dc.contributor.other | Ohio State University | |
| dc.contributor.other | University of Copenhagen | |
| dc.contributor.other | Niels Bohr Institute | |
| dc.contributor.other | Dortmund University of Technology | |
| dc.contributor.other | Michigan State University | |
| dc.contributor.other | University of Alberta | |
| dc.contributor.other | University of Erlangen Nuremberg | |
| dc.contributor.other | University of Geneva | |
| dc.contributor.other | Ghent University | |
| dc.contributor.other | University of California Irvine | |
| dc.contributor.other | University of Kansas | |
| dc.contributor.other | University of Leicester | |
| dc.contributor.other | University of California Los Angeles | |
| dc.contributor.other | University of Wisconsin System | |
| dc.contributor.other | University of Wisconsin Madison | |
| dc.contributor.other | Johannes Gutenberg University of Mainz | |
| dc.contributor.other | Marquette University | |
| dc.contributor.other | Technical University of Munich | |
| dc.contributor.other | University of Munster | |
| dc.contributor.other | University of Delaware | |
| dc.contributor.other | Yale University | |
| dc.contributor.other | University of Oxford | |
| dc.contributor.other | Drexel University | |
| dc.contributor.other | South Dakota School Mines & Technology | |
| dc.contributor.other | University of Rochester | |
| dc.contributor.other | Oskar Klein Centre | |
| dc.contributor.other | Stockholm University | |
| dc.contributor.other | State University of New York (SUNY) System | |
| dc.contributor.other | State University of New York (SUNY) Stony Brook | |
| dc.contributor.other | Sungkyunkwan University (SKKU) | |
| dc.contributor.other | University of Alabama Tuscaloosa | |
| dc.contributor.other | Pennsylvania Commonwealth System of Higher Education (PCSHE) | |
| dc.contributor.other | Pennsylvania State University | |
| dc.contributor.other | Pennsylvania State University - University Park | |
| dc.contributor.other | Uppsala University | |
| dc.contributor.other | University of Wuppertal | |
| dc.contributor.other | Helmholtz Association | |
| dc.contributor.other | Deutsches Elektronen-Synchrotron (DESY) | |
| dc.contributor.other | University of Tokyo | |
| dc.date.accessioned | 2019-07-03T12:57:49Z | |
| dc.date.available | 2019-07-03T12:57:49Z | |
| dc.date.copyright | 2019 | |
| dc.date.issued | 2019-02-06 | |
| dc.description.abstract | High-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.mimetype | application/pdf | |
| dc.identifier.citation | Aartsen, 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.doi | 10.1103/PhysRevLett.122.051102 | |
| dc.identifier.issn | 0031-9007 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-6779-1172 | |
| dc.identifier.orcid | https://orcid.org/0000-0003-0705-2770 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-6418-3008 | |
| dc.identifier.orcid | https://orcid.org/0000-0003-1830-9076 | |
| dc.identifier.orcid | https://orcid.org/0000-0003-2794-512X | |
| dc.identifier.orcid | https://orcid.org/0000-0001-8121-5860 | |
| dc.identifier.orcid | https://orcid.org/0000-0003-4873-3783 | |
| dc.identifier.orcid | https://orcid.org/0000-0003-2252-9514 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-7669-266X | |
| dc.identifier.orcid | https://orcid.org/0000-0002-1748-7367 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-6958-6033 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-6014-5928 | |
| dc.identifier.orcid | https://orcid.org/0000-0001-6325-7688 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-7063-4418 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-1983-8271 | |
| dc.identifier.orcid | https://orcid.org/0000-0002-3157-0407 | |
| dc.identifier.orcid | https://orcid.org/0000-0001-9278-5906 | |
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| dc.identifier.uri | http://ir.ua.edu/handle/123456789/5883 | |
| dc.language | English | |
| dc.language.iso | en_US | |
| dc.publisher | American Physical Society | |
| dc.rights.holder | American Physical Society | |
| dc.subject | GAMMA-RAY BURSTS | |
| dc.subject | HIGH-ENERGY NEUTRINOS | |
| dc.subject | Physics, Multidisciplinary | |
| dc.subject | Physics | |
| dc.title | Constraints on Minute-Scale Transient Astrophysical Neutrino Sources | en_US |
| dc.type | text | |
| dc.type | Article |
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