| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9857884 | Nuclear Physics B - Proceedings Supplements | 2005 | 4 Pages |
Abstract
Gamma-ray bursts have been observed for more than three decades and, yet, much about their nature remains a mystery. Here we describe the results of the ongoing search for high-energy muon neutrinos from gamma-ray bursts with the Antarctic Muon and Neutrino Detector Array (AMANDA). Current results are consistent with no neutrino emission; thus preliminary upper limits are derived for the event rate, four-year combined flux, and single-year fluence. We also address plans for improving these limits in the future.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Kyler Kuehn, the AMANDA Collaboration the AMANDA Collaboration,