Transparency of the Sun to gamma rays due to axionlike particles

被引:26
作者
Fairbairn, Malcolm [1 ]
Rashba, Timur
Troitsky, Sergey
机构
[1] Stockholm Univ, S-10691 Stockholm, Sweden
[2] Perimeter Inst, Waterloo, ON N2L 2Y5, Canada
[3] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst Phys, D-80805 Munich, Germany
[4] Pushkov Inst IZMIRAN, Troitsk 142190, Russia
[5] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia
关键词
D O I
10.1103/PhysRevLett.98.201801
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It is shown that the Sun can become partially transparent to high energy photons in the presence of a pseudoscalar. In particular, if the axion interpretation of the PVLAS result were true, then up to 2% of GeV energy gamma rays might pass through the Sun, while an even stronger effect is expected for some axion parameters. We discuss the possibilities of observing this effect. Present data are limited to the observation of the solar occultation of 3C 279 by the Energetic Gamma-Ray Experiment Telescope in 1991; 98% C.L. detection of a nonzero flux of gamma rays passing through the Sun is not yet conclusive. Since the same occultation happens every October, future experiments, e.g., the Gamma-Ray Large Area Space Telescope, are expected to have better sensitivity.
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页数:4
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