Supernova Neutrino Detection

被引：237

作者：

Scholberg, Kate ^{[1
]}

机构：

[1] Duke Univ, Dept Phys, Durham, NC 27708 USA

来源：

ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE, VOL 62 | 2012年 / 62卷

关键词：

core collapse; neutrino properties; neutrino astrophysics; underground detectors; CROSS-SECTIONS; BETA-DECAY; REAL-TIME; BURST; PHYSICS; SEARCH; AR-40; OSCILLATION; TELESCOPE; FUTURE;

D O I：

10.1146/annurev-nucl-102711-095006

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：

A core-collapse supernova will produce an enormous burst of neutrinos of all flavors in the few-tens-of-MeV range. Measurement of the flavor, time, and energy structure of a nearby core-collapse neutrino burst will yield answers to many physics and astrophysics questions. The neutrinos left over from past cosmic supernovae are also observable, and their detection will improve knowledge of core-collapse rates and average neutrino emission. This review describes experimental techniques for detection of core-collapse neutrinos, as well as the sensitivities of current and future detectors.

引用

页码：81 / 103

页数：23

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