No tension between assembly models of super massive black hole binaries and pulsar observations

Pulsar timing arrays are presently the only means to search for the gravitational wave stochastic background from super massive black hole binary populations, considered to be within the grasp of current or near-future observations. The stringent upper limit from the Parkes Pulsar Timing Array has b...

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Detalles Bibliográficos
Autores principales: Middleton, Hannah, Chen, Siyuan, Del Pozzo, Walter, Sesana, Alberto, Vecchio, Alberto
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2018
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5805789/
https://www.ncbi.nlm.nih.gov/pubmed/29422487
http://dx.doi.org/10.1038/s41467-018-02916-7

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5805789/
https://www.ncbi.nlm.nih.gov/pubmed/29422487
http://dx.doi.org/10.1038/s41467-018-02916-7

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