Self-force in a gauge appropriate to separable wave equations

Details Self-force in a gauge appropriate to separable wave equations Self-force in a gauge appropriate to separable wave equations

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..aprs11004f&link_type=abstract

American Physical Society, APS April Meeting, April 22-26, 2006, abstract #S11.004

Physics

Scientific paper

Gravitational waves from the inspiral of a stellar-size black hole to a supermassive black hole can be accurately approximated by a point particle moving in a Kerr background. The talk presents progress on computing the self-force in a gauge that is constructed from the gauge-invariant Weyl tensor. The gauge and the renormalization method are chosen to compute a perturbed metric and renormalized self-force from the Teukolsky equation. The method is related to earlier work by Cohen, Kegeles, Lousto, Detweiler, and Whiting, and to the MiSaTaQuWa renormalization.

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