Session J11: Theoretical Gravity
1:30 PM–3:18 PM, Sunday, May 3, 2009
Room: Plaza Court 1
Sponsoring Unit:
GGR
Chair: John Friedman, University of Wisconsin-Milwaukee
Abstract ID: BAPS.2009.APR.J11.7
Abstract: J11.00007 : Finding Fields and Self-Force in a Gauge Appropriate to Separable Wave Equations
2:42 PM–2:54 PM
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Abstract 
Authors:
Tobias Keidl
(University of Wisconsin--Washington County)
John Friedman
(University of Wisconsin--Milwaukee)
Dong-Hoon Kim
(Caltech)
Larry Price
(University of Wisconsin--Milwaukee)
Abhay Shah
(University of Wisconsin--Milwaukee)
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. A procedure for finding the renormalized self-force from the Tuekolsky equation \footnote{Teukolsky, S. A., Astrophys. J., \textbf{185}, 635-647, (1973)} has been outlined in the separate paper \footnote{T.~S.~Keidl, J.~L.~Friedman, A.~G.~Wiseman, Phys. Rev. D, in press; gr-qc0611072}. This talk focuses on analytic work developed in this formalism and incorporating the $l=0$ and $l=1$ parts of the self-force. The self-force is calculated from either the renormalized spin $+2$ or the spin $-2$ Weyl scalar ($\psi_0$ or $\psi_4$). The self-force is can then be calculated algebraically from either renormalized Weyl scalar.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2009.APR.J11.7