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Cosmology with massive black hole binary mergers in the LISA era

In $\sim2034$ the Laser Interferometer Space Antenna (LISA) will detect the coalescence of massive black hole binaries (MBHBs) from $10^5$ to $10^7 {\, \rm M}_\odot$ up to $z\sim10$. The gravitational wave (GW) signal is expected to be accompanied by a powerful electromagnetic (EM) counterpart, from...

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Detalles Bibliográficos
Autores principales: Mangiagli, Alberto, Caprini, Chiara, Volonteri, Marta, Marsat, Sylvain, Vergani, Susanna, Tamanini, Nicola, Speri, Lorenzo
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:https://dx.doi.org/10.22323/1.414.0125
http://cds.cern.ch/record/2870197