Pulsar timing array signals induced by black hole binaries in relativistic eccentric orbits
Pulsar timing array signals induced by black hole binaries in relativistic eccentric orbits
About this item
Full title
Author / Creator
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
Individual supermassive black hole binaries in non-circular orbits are possible nanohertz gravitational wave sources for the rapidly maturing Pulsar Timing Array experiments. We develop an accurate and efficient approach to compute Pulsar Timing Array signals due to gravitational waves from inspiraling supermassive black hole binaries in relativist...
Alternative Titles
Full title
Pulsar timing array signals induced by black hole binaries in relativistic eccentric orbits
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2353321223
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2353321223
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.2002.03285
