Astrophysical neutrino telescopes

被引：33

作者：

McDonald, AB ^{[1
]}

Spiering, C

Schönert, S

Kearns, ET

Kajita, T

机构：

[1] Queens Univ, SNO Inst, Kingston, ON K7L 3N6, Canada

[2] DESY Zeuthen, D-15738 Zeuthen, Germany

[3] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[4] Boston Univ, Dept Phys, Boston, MA 02215 USA

[5] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan

来源：

REVIEW OF SCIENTIFIC INSTRUMENTS | 2004年 / 75卷 / 02期

关键词：

D O I：

10.1063/1.1642740

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

This review describes telescopes designed to study neutrinos from astrophysical sources. These sources include the sun and supernovae emitting neutrino energies up to tens of MeV, atmospheric neutrino sources caused by cosmic ray interactions, and other sources generating neutrino energies ranging up to 1x10(20) eV. Measurements with these telescopes also provide information on neutrino properties, including clear evidence for neutrino flavor change. Telescopes in operation in the past and present are described, along with plans for future instruments to expand this rapidly growing field of particle astrophysics. (C) 2004 American Institute of Physics.

引用

页码：293 / 316

页数：24

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