What is the source of the PTA GW signal?

The most conservative interpretation of the nHz stochastic gravitational wave background (SGWB) discovered by NANOGrav and other Pulsar Timing Array (PTA) Collaborations is astrophysical, namely that it originates from supermassive black hole (SMBH) binaries. However, alternative cosmological models...

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Detalles Bibliográficos
Autores principales: Ellis, John, Fairbairn, Malcolm, Franciolini, Gabriele, Hütsi, Gert, Iovino, Antonio, Lewicki, Marek, Raidal, Martti, Urrutia, Juan, Vaskonen, Ville, Veermäe, Hardi
Lenguaje:eng
Publicado: 2023
Materias:
hep-th
Particle Physics - Theory
astro-ph.CO
Astrophysics and Astronomy
Acceso en línea:http://cds.cern.ch/record/2867719

Internet

http://cds.cern.ch/record/2867719

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