The search for neutrinos from gamma-ray bursts with AMANDA

被引：0
|
作者：
Kuehn, K. [1 ]
机构：
[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
来源：
PROCEEDINGS OF THE 29TH INTERNATIONAL COSMIC RAY CONFERENCE, VOL 5: OG 2.5, 2.6 & 2.7 | 2005年
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Antarctic Muon and Neutrino Detector Array (AMANDA), located at the South Pole, has been searching the heavens for astrophysical neutrino sources (both discrete and diffuse) since 1997. The AMANDA telescope detects Cerenkov radiation caused by high-energy neutrinos traveling through the nearby ice; here we describe AMANDA's technique to search for neutrinos from gamma-ray bursts, both concurrent with the photon emission and prior to it (during the "precursor" phase). We present preliminary results from several years (1997-2003) of observations, and we also briefly discuss the current status and future potential of an expanded search for GRBs.
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页码：131 / 134
页数：4
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