New class of high-energy transients from crashes of supernova ejecta with massive circumstellar material shells

被引：129

作者：

Murase, Kohta ^{[1
,2
]}

Thompson, Todd A. ^{[1
,3
]}

Lacki, Brian C. ^{[1
,3
]}

Beacom, John F. ^{[1
,2
,3
]}

机构：

[1] Ohio State Univ, CCAPP, Columbus, OH 43210 USA

[2] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA

[3] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA

来源：

PHYSICAL REVIEW D | 2011年 / 84卷 / 04期

基金：

美国国家科学基金会;

关键词：

GAMMA-RAY EMISSION; CORE-COLLAPSE SUPERNOVAE; VERY-HIGH-ENERGY; COSMIC-RAYS; SHOCK BREAKOUT; LUMINOUS SUPERNOVA; PAIR-INSTABILITY; IIN SUPERNOVA; ACCELERATION; NEUTRINOS;

D O I：

10.1103/PhysRevD.84.043003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A new class of core-collapse supernovae (SNe) has been discovered in recent years by optical/infrared surveys; these SNe suggest the presence of one or more extremely dense (similar to 10(5-11) cm(-3)) shells of circumstellar material (CSM) on 10(2-4) AU scales. We consider the collisions of the SN ejecta with these massive CSM shells as potential cosmic-ray (CR) accelerators. If similar to 10% of the SN energy goes into CRs, multi-TeV neutrinos and/or GeV-TeV gamma rays almost simultaneous with the optical/infrared light curves are detectable for SNe at less than or similar to 20-30 Mpc. A new type of coordinated multimessenger search for such transients of duration similar to 1-10 months is required; these may give important clues to the physical origin of such SNe and to CR acceleration mechanisms.

引用

页数：7

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