High-order post-Newtonian expansion of the generalized redshift invariant for eccentric-orbit, equatorial extreme-mass-ratio inspirals with a spinning primary-Reference-Cited by-同舟云学术

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High-order post-Newtonian expansion of the generalized redshift invariant for eccentric-orbit, equatorial extreme-mass-ratio inspirals with a spinning primary

Published:2023-10-10 Issue:8 Volume:108 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Munna Christopher^ORCID

Funder

National Science Foundation

University of North Carolina at Chapel Hill

National Aeronautics and Space Administration

Massachusetts Institute of Technology

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.108.084012/fulltext

Reference88 articles.

1. Two-timescale analysis of extreme mass ratio inspirals in Kerr spacetime: Orbital motion

2. Relativistic corrections to the gravitational radiation of a binary system and the fine structure of the spectrum

3. Gravitational radiation from a particle in circular orbit around a black hole. I. Analytical results for the nonrotating case

4. Gravitational radiation from a particle in circular orbit around a black hole. II. Numerical results for the nonrotating case

5. Gravitational waves from a point particle in circular orbit around a black hole: Logarithmic terms in the post-Newtonian expansion

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