Stochastic gravitational wave background from stellar origin binary black holes in LISA

We use the latest constraints on the population of stellar origin binary black holes (SOBBH) from LIGO/Virgo/KAGRA (LVK) observations, to estimate the stochastic gravitational wave background (SGWB) they generate in the frequency band of LISA.In order to account for the faint and distant binaries, w...

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Detalles Bibliográficos
Autores principales: Babak, Stanislav, Caprini, Chiara, Figueroa, Daniel G., Karnesis, Nikolaos, Marcoccia, Paolo, Nardini, Germano, Pieroni, Mauro, Ricciardone, Angelo, Sesana, Alberto, Torrado, Jesús
Lenguaje:eng
Publicado: 2023
Materias:
gr-qc
General Relativity and Cosmology
astro-ph.CO
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2023/08/034
http://cds.cern.ch/record/2856417

Internet

https://dx.doi.org/10.1088/1475-7516/2023/08/034
http://cds.cern.ch/record/2856417

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