Physics
Scientific paper
Apr 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aps..apre10005p&link_type=abstract
American Physical Society, 2008 APS April Meeting and HEDP/HEDLA Meeting, April 11-15, 2008, abstract #E10.005
Physics
Scientific paper
Gravitational radiation from the inspiral of a stellar mass sized black hole into a supermassive rotating black hole is an important candidate for detection with the proposed Laser Interferometer Space Antenna. A complete and self-consistent description of the motion of the particle requires knowledge of the gravitational self-force. We report progress on computing the self-force from a method based on regularizing solutions to the Teukolsky equation. In this talk, we focus on describing the general procedure for computing the self-force in the Kerr spacetime.
Friedman John
Keidl Tobias
Kim Dong Hoon
Messaritaki Eirini
Price Larry
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