COSMOLOGY WITH 100-TEV GAMMA-RAY TELESCOPES

被引:43
作者
HALZEN, F
PROTHEROE, RJ
STANEV, T
VANKOV, HP
机构
[1] UNIV ADELAIDE, DEPT PHYS & MATH PHYS, ADELAIDE, SA 5001, AUSTRALIA
[2] UNIV DELAWARE, BARTOL RES INST, NEWARK, DE 19716 USA
关键词
D O I
10.1103/PhysRevD.41.342
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that the secondary photons which are by-products of the energy loss of extragalactic cosmic rays interacting with the cosmic background have a characteristic energy of 10-100 TeV. For a model where the extragalactic cosmic rays are uniformly distributed in space and in time over the past 109 yr the flux of 100-TeV photons is 10-5 of the cosmic-ray flux. Such fluxes are attractively close to the resolution of the new generation of -ray telescopes and their detection can provide important cosmological information. © 1990 The American Physical Society.
引用
收藏
页码:342 / 346
页数:5
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