Approximate waveforms for extreme-mass-ratio inspirals in modified gravity spacetimes
Extreme mass-ratio inspirals, in which a stellar-mass compact object spirals into a supermassive black hole, are prime candidates for detection with space-borne milliHertz gravitational wave detectors, similar to the Laser Interferometer Space Antenna. The gravitational waves generated during such i...
Main Authors: | Yunes, Nicolas, Gair, Jonathan R. |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | en_US |
Published: |
American Physical Society (APS)
2012
|
Online Access: | http://hdl.handle.net/1721.1/68660 |
Similar Items
-
New Kludge scheme for the construction of approximate waveforms for extreme-mass-ratio inspirals
by: Sopuerta, Carlos F., et al.
Published: (2012) -
Effect of massive perturbers on extreme mass-ratio inspiral waveforms
by: Yunes, Nicolas, et al.
Published: (2011) -
Research Update on Extreme-Mass-Ratio Inspirals
by: Amaro-Seoane, Pau, et al.
Published: (2017) -
Accuracy of the post-Newtonian approximation. II. Optimal asymptotic expansion of the energy flux for quasicircular, extreme mass-ratio inspirals into a Kerr black hole
by: Zhang, Zhongyang, et al.
Published: (2011) -
Modeling Extreme Mass Ratio Inspirals within the Effective-One-Body Approach
by: Yunes, Nicolas, et al.
Published: (2011)