Published August 20, 2009 | Version v1
Journal article

SEARCH FOR HIGH-ENERGY MUON NEUTRINOS FROM THE 'NAKED-EYE' GRB 080319B WITH THE IceCube NEUTRINO TELESCOPE

  • 1. Department of Physics, University of Wisconsin, Madison, WI 53706 (United States)
  • 2. Department of Subatomic and Radiation Physics, University of Gent, B-9000 Gent (Belgium)
  • 3. Department of Physics, University of Wisconsin, River Falls, WI 54022 (United States)
  • 4. Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch (New Zealand)
  • 5. Department of Physics, University of Oxford, 1 Keble Road, Oxford OX1 3NP (United Kingdom)
  • 6. Department of Physics, University of Wuppertal, D-42119 Wuppertal (Germany)
  • 7. Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, DE 19716 (United States)
  • 8. Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States)
  • 9. Department of Physics, University of California, Berkeley, CA 94720 (United States)
  • 10. DESY, D-15735 Zeuthen (Germany)
  • 11. Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States)
  • 12. Department of Physics and Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210 (United States)
  • 13. Universite Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels (Belgium)
  • 14. Department of Physics, TU Dortmund University, D-44221 Dortmund (Germany)

Description

We report on a search with the IceCube detector for high-energy muon neutrinos from GRB 080319B, one of the brightest gamma-ray bursts (GRBs) ever observed. The fireball model predicts that a mean of 0.1 events should be detected by IceCube for a bulk Lorentz boost of the jet of 300. In both the direct on-time window of 66 s and an extended window of about 300 s around the GRB, no excess was found above background. The 90% CL upper limit on the number of track-like events from the GRB is 2.7, corresponding to a muon neutrino fluence limit of 9.5 x 10-3 erg cm-2 in the energy range between 120 TeV and 2.2 PeV, which contains 90% of the expected events.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/701/2/1721

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
701
Journal Issue
2
Journal Page Range
p. 1721-1731
ISSN
0004-637X
CODEN
ASJOAB

INIS

Optional Information

Collaborations
IceCube Collaboration