Searching for energetic cosmic axions in a laboratory experiment

被引：0
|
作者：
M. Fairbairn
S. Gninenko
N. Krasnikov
V. Matveev
T. Rashba
A. Rubbia
S. Troitsky
机构：
[1] CERN,
[2] Institute for Nuclear Research of RAS,undefined
[3] Max-Planck-Institut für Physik (Werner-Heisenberg-Institut),undefined
[4] Pushkov Institute (IZMIRAN),undefined
[5] Institut für Teilchenphysik,undefined
[6] ETHZ,undefined
来源：
The European Physical Journal C | 2007年 / 52卷
关键词：
Spectral Energy Distribution; Time Projection Chamber; Crab Pulsar; Astrophysical Source; Stellar Interior;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Astrophysical sources of energetic gamma rays provide the right conditions for maximal mixing between (pseudo)scalar (axion-like) particles and photons if their coupling is strong enough. This is independent of whether or not the axion interaction is standard at all energies or becomes suppressed in the extreme conditions of the stellar interior. The flux of such particles through the Earth could be observed using a metre long, Tesla strength superconducting solenoid. The rate of events in CAST caused by axions from the Crab pulsar is also estimated.
引用
收藏
页码：899 / 904
页数：5
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