Test the mergers of the primordial black holes by high frequency gravitational-wave detector
Abstract The black hole could have a primordial origin if its mass is less than $$1M_\odot $$ 1 M ⊙ . The mergers of these black hole binaries generate stochastic gravitational-wave background (SGWB). We investigate the SGWB in high frequency band $$10^{8}$$ 10 8 – $$10^{10}\,\mathrm {Hz}$$ 10 10 Hz...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2017-09-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-017-5216-8 |