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Gravitational wave energy emission and detection rates of Primordial Black Hole hyperbolic encounters
We describe in detail gravitational wave bursts from Primordial Black Hole (PBH) hyperbolic encounters. The bursts are one-time events, with the bulk of the released energy happening during the closest approach, which can be emitted in frequencies that could be within the range of both LIGO (10-1000...
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
2017
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| Acceso en línea: | https://dx.doi.org/10.1016/j.dark.2018.06.001 http://cds.cern.ch/record/2294544 |