Astrophysical high energy neutrinos

被引：0
|
作者：
Razzaque, Soebur [1 ]
机构：
[1] Penn State Univ, Dept Phys, Dept Astron & Astrophys, University Pk, PA 16802 USA
来源：
NNN06: NEXT GENERATION NUCLEON DECAY AND NEUTRINO DETECTORS 2006 | 2007年 / 944卷
关键词：
cosmic ray; neutrino; gamma-ray burst; supernova;
D O I：
暂无
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
Astrophysical candidate sources of ultrahigh-energy cosmic-rays are also expected to produce high-energy neutrinos in situ and around their acceleration sites by interacting with abundant soft photons or nucleons. Detection of these neutrinos then may identify the yet unknown sources of the cosmic rays. I discuss different models of high-energy neutrino signals from astrophysical objects such as gamma-ray bursts and hyper-novae, and how detection/non-detection of these astronomical messengers may constrain the source models. I also discuss the detectability of these neutrinos in upcoming neutrino telescopes and how flavor tagging may be used to learn about the astrophysics of the sources.
引用
收藏
页码：130 / 139
页数：10
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