Local flux of low-energy antiprotons from evaporating primordial black holes

被引:86
作者
Maki, K
Mitsui, T
Orito, S
机构
[1] Department of Physics, School of Science, University of Tokyo, Tokyo
关键词
D O I
10.1103/PhysRevLett.76.3474
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We investigate low-energy cosmic-ray antiprotons (<(p)over bar 's>) arising from the fragmentation of quarks and gluons emitted from evaporating primordial black holes (PBHs). To calculate the local interstellar flux of these <(p)over bar 's>, their propagation in the Galaxy is described by a 3D Monte Carlo simulation based on the diffusion model. This flux is used with recent observations to derive new upper limits on (i) the local PBH explosion rate R < 1.7 x 10(-2) pc(-3) yr(-1), (ii) the fraction of the Universe's mass going into PBHs with particular mass, and (iii) the average density of PBHs in the Universe.
引用
收藏
页码:3474 / 3477
页数:4
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