Gravitational waves from sub-lunar-mass primordial black-hole binaries: A new probe of extradimensions

被引:33
作者
Inoue, KT [1 ]
Tanaka, T
机构
[1] Natl Astron Observ, Div Theoret Astrophys, Tokyo 1818588, Japan
[2] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
关键词
D O I
10.1103/PhysRevLett.91.021101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In many brane world models, gravity is largely modified at the electroweak scale similar to1 TeV. In such models, primordial black holes (PBHs) with a lunar mass Msimilar to10(-7)M(circle dot) might have been produced when the temperature of the Universe was at similar to1 TeV. If a significant fraction of the dark halo of our galaxy consists of these lunar mass PBHs, a huge number of BH binaries will exist in our neighborhood. Third generation detectors such as EURO can detect gravitational waves from these binaries, and can also determine their chirp mass. With a new detector designed to be sensitive at high frequency bands greater than or similar to1 kHz, the existence of extradimensions could be confirmed.
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