Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts

被引：16
|
作者：
Granot, J
Guetta, D
机构：
[1] Inst Adv Study, Princeton, NJ 08540 USA
[2] Osserv Astrofis Arcetri, I-50125 Florence, Italy
来源：
PHYSICAL REVIEW LETTERS | 2003年 / 90卷 / 19期
关键词：
D O I：
10.1103/PhysRevLett.90.191102
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The supranova model for gamma-ray bursts (GRBs) has recently gained popularity. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). High energy protons from the PWB can interact with photons from the rich radiation field inside the PWB or collide with cold protons from the supernova remnant, producing pions which decay into similar to10-10(3) TeV neutrinos. The predicted neutrino flux from the PWBs that host the GRBs should be easily detectable by planned 1 km(2) detectors.
引用
收藏
页码：1 / 191102
页数：4
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