High-order post-Newtonian expansion of the redshift invariant for eccentric-orbit nonspinning extreme-mass-ratio inspirals-Reference-Cited by-同舟云学术

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High-order post-Newtonian expansion of the redshift invariant for eccentric-orbit nonspinning extreme-mass-ratio inspirals

Published:2022-08-02 Issue:4 Volume:106 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Munna Christopher^ORCID,Evans Charles R.^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.106.044004/fulltext

Reference70 articles.

1. Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit nonspinning extreme-mass-ratio inspirals to the 19th order

2. Determination of new coefficients in the angular momentum and energy fluxes at infinity to 9PN order for eccentric Schwarzschild extreme-mass-ratio inspirals using mode-by-mode fitting

3. Eccentric-orbit extreme-mass-ratio-inspiral radiation: Analytic forms of leading-logarithm and subleading-logarithm flux terms at high PN orders

4. Eccentric-orbit extreme-mass-ratio-inspiral radiation. II. 1PN correction to leading-logarithm and subleading-logarithm flux sequences and the entire perturbative 4PN flux

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

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Defining eccentricity for gravitational wave astronomy;Physical Review D;2023-11-03

2. High-order post-Newtonian expansion of the generalized redshift invariant for eccentric-orbit, equatorial extreme-mass-ratio inspirals with a spinning primary;Physical Review D;2023-10-10

3. Tidal heating and torquing of the primary black hole in eccentric-orbit, nonspinning, extreme-mass-ratio inspirals to 22PN order;Physical Review D;2023-08-21

4. Post-Newtonian expansion of the spin-precession invariant for eccentric-orbit nonspinning extreme-mass-ratio inspirals to 9PN and e16;Physical Review D;2022-08-25

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