TeV neutrinos from core collapse supernovae and hypernovae -: art. no. 181101

被引：112

作者：

Razzaque, S

Mészáros, P

Waxman, E

机构：

[1] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[2] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

[3] Inst Adv Study, Princeton, NJ 08540 USA

[4] Hungarian Acad Sci, Budapest, Hungary

[5] Weizmann Inst Sci, Fac Phys, IL-76100 Rehovot, Israel

来源：

PHYSICAL REVIEW LETTERS | 2004年 / 93卷 / 18期

关键词：

D O I：

10.1103/PhysRevLett.93.181101

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A fraction of core-collapse supernovae of type Ib/c are associated with gamma-ray bursts, which are thought to produce highly relativistic jets. Recently, it has been hypothesized that a larger fraction of core-collapse supernovae produce slower jets, which may contribute to the disruption and ejection of the supernova envelope, and explain the unusually energetic hypernovae. We explore the TeV neutrino signatures expected from such slower jets, and calculate the expected detection rates with upcoming Gigaton Cherenkov experiments. We conclude that individual jetted supernovae may be detectable from nearby galaxies.

引用

页码：181101 / 1

页数：4

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