GeV Neutrinos from Collisional Heating in GRBs: Detection Prospects with IceCube-DeepCore

被引：0
|
作者：
Bartos, Imre [1 ]
机构：
[1] Columbia Univ, Dept Phys, New York, NY 10027 USA
来源：
6TH INTERNATIONAL WORKSHOP ON VERY LARGE VOLUME NEUTRINO TELESCOPES (VLVVT 13) | 2014年 / 1630卷
关键词：
Gamma-ray bursts; high-energy neutrinos; IceCube; DeepCore; collisional heating; GAMMA-RAY BURSTS; FIREBALLS; DYNAMICS;
D O I：
10.1063/1.4902778
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The observed gamma-ray burst (GRB) emission may be due to jet reheating via nuclear collisions. The role of this collisional heating can be probed through the observation of 10-100 GeV neutrinos, which are generated in nuclear collisions along with gamma rays. Neutrino and gamma-ray luminosities are closely related, which further aids observations. If the main mechanism behind the production of GRBs is collisional heating then IceCube-DeepCore could detect the GeV-neutrino emission of GRBs with a few years of observation.
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收藏
页码：86 / 88
页数：3
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