Projection effects on the observed angular spectrum of the astrophysical stochastic gravitational wave background

The detection and characterization of the stochastic gravitational wave background (SGWB) is one of the main goals of gravitational wave (GW) experiments. The observed SGWB will be the combination of GWs from cosmological (as predicted by many models describing the physics of the early universe) and...

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Detalles Bibliográficos
Autores principales: Bertacca, Daniele, Ricciardone, Angelo, Bellomo, Nicola, Jenkins, Alexander C., Matarrese, Sabino, Raccanelli, Alvise, Regimbau, Tania, Sakellariadou, Mairi
Lenguaje:eng
Publicado: 2019
Materias:
gr-qc
General Relativity and Cosmology
astro-ph.CO
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.101.103513
http://cds.cern.ch/record/2690978

Internet

https://dx.doi.org/10.1103/PhysRevD.101.103513
http://cds.cern.ch/record/2690978

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