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Formation and Evolution of Primordial Black Hole Binaries in the Early Universe
The abundance of primordial black holes (PBHs) in the mass range 0.1–103 M⊙ can potentially be tested by gravitational wave observations due to the large merger rate of PBH binaries formed in the early universe. To put the estimates of the latter on a firmer footing, we first derive analytical PBH m...
| Autores principales: | , , , |
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| Lenguaje: | eng |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2019/02/018 http://cds.cern.ch/record/2650543 |