Unveiling the gravitational universe at $\mu$-Hz frequencies

We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to $\mu$-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the co...

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Detalles Bibliográficos
Autores principales: Sesana, Alberto, Korsakova, Natalia, Sedda, Manuel Arca, Baibhav, Vishal, Barausse, Enrico, Barke, Simon, Berti, Emanuele, Bonetti, Matteo, Capelo, Pedro R., Caprini, Chiara, Garcia-Bellido, Juan, Haiman, Zoltan, Jani, Karan, Jennrich, Oliver, Johansson, Peter H., Khan, Fazeel Mahmood, Korol, Valeriya, Lamberts, Astrid, Lupi, Alessandro, Mangiagli, Alberto, Mayer, Lucio, Nardini, Germano, Pacucci, Fabio, Petiteau, Antoine, Raccanelli, Alvise, Rajendran, Surjeet, Regan, John, Shao, Lijing, Spallicci, Alessandro, Tamanini, Nicola, Volonteri, Marta, Warburton, Niels, Wong, Kaze, Zumalacarregui, Miguel
Lenguaje:eng
Publicado: 2019
Materias:
gr-qc
General Relativity and Cosmology
astro-ph.HE
Astrophysics and Astronomy
astro-ph.IM
Acceso en línea:https://dx.doi.org/10.1007/s10686-021-09709-9
http://cds.cern.ch/record/2790828

Internet

https://dx.doi.org/10.1007/s10686-021-09709-9
http://cds.cern.ch/record/2790828

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