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Prospects for Future Binary Black Hole GW Studies in Light of PTA Measurements
NANOGrav and other Pulsar Timing Arrays (PTAs) have discovered a common-spectrum process in the nHz range that may be due to gravitational waves (GWs): if so, they are likely to have been generated by black hole (BH) binaries with total masses > 109 M⊙. Using the Extended Press-Schechter formalis...
| Autores principales: | , , , , , , |
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| Lenguaje: | eng |
| Publicado: |
2023
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1051/0004-6361/202346268 http://cds.cern.ch/record/2848099 |