Dolgov, A. D. (2012) Contemporary gravitational waves from primordial black holes. Il nuovo cimento C, 35 (1). pp. 47-54. ISSN 1826-9885
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Abstract
Stochastic background of gravitational waves (GW) generated by the interactions between primordial black holes (PBH) in the early universe and by PBH evaporation is considered. If PBHs dominated in the cosmological energy density prior to their evaporation, GWs from the earlier stages (e.g., inflation) would be noticeably diluted. On the other hand, at the PBH dominance period they could form dense clusters where PBH binary formation might be significant. These binaries would be efficient sources of the gravitational waves.
| Item Type: | Article |
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| Uncontrolled Keywords: | Gravitational waves ; Cosmology ; Other quarks (e.g., 4th generations) |
| Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
| Depositing User: | Marina Spanti |
| Date Deposited: | 14 Apr 2020 16:40 |
| Last Modified: | 14 Apr 2020 16:40 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/17646 |
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