Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors

We consider stellar-origin black hole binaries, which are among the main astrophysical sources for next generation gravitational wave (GW) detectors such as the Einstein Telescope (ET) and Cosmic Explorer (CE). Using population models calibrated with the most recent LIGO/Virgo results from O3b run,...

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Detalles Bibliográficos
Autores principales: Pieroni, Mauro, Ricciardone, Angelo, Barausse, Enrico
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9606311/
https://www.ncbi.nlm.nih.gov/pubmed/36289256
http://dx.doi.org/10.1038/s41598-022-19540-7

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9606311/
https://www.ncbi.nlm.nih.gov/pubmed/36289256
http://dx.doi.org/10.1038/s41598-022-19540-7

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