SEARCH FOR PROMPT NEUTRINO EMISSION FROM GAMMA-RAY BURSTS WITH ICECUBE
Journal Article
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· Astrophysical Journal Letters
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- School of Chemistry and Physics, University of Adelaide, Adelaide, SA 5005 Australia (Australia)
- DESY, D-15735 Zeuthen (Germany)
- Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch (New Zealand)
- Université Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels (Belgium)
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin, Madison, WI 53706 (United States)
- Oskar Klein Centre and Department of Physics, Stockholm University, SE-10691 Stockholm (Sweden)
- Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, D-91058 Erlangen (Germany)
- Department of Physics, Pennsylvania State University, University Park, PA 16802 (United States)
- Physikalisches Institut, RWTH Aachen University, D-52056 Aachen (Germany)
- Physics Department, South Dakota School of Mines and Technology, Rapid City, SD 57701 (United States)
- Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States)
- Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099 Mainz (Germany)
- Department of Physics, University of California, Berkeley, CA 94720 (United States)
- Department of Physics and Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210 (United States)
- Fakultät für Physik and Astronomie, Ruhr-Universität Bochum, D-44780 Bochum (Germany)
- Department of Physics, University of Wuppertal, D-42119 Wuppertal (Germany)
We present constraints derived from a search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs). A single low-significance neutrino, compatible with the atmospheric neutrino background, was found in coincidence with one of the 506 observed bursts. Although GRBs have been proposed as candidate sources for ultra-high-energy cosmic rays, our limits on the neutrino flux disfavor much of the parameter space for the latest models. We also find that no more than ∼1% of the recently observed astrophysical neutrino flux consists of prompt emission from GRBs that are potentially observable by existing satellites.
- OSTI ID:
- 22518972
- Journal Information:
- Astrophysical Journal Letters, Vol. 805, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 2041-8205
- Country of Publication:
- United States
- Language:
- English
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