Gravitational
Radiation Reaction and Self-Force| Gravitational
Radiation Reaction and Self-Force |
In General > s.a. orbits
of gravitating bodies; Post-Newtonian Formalism; radiation
reaction in general.
* Results: A point
particle perturbs the spacetime metric, and affects its own motion;
In the zero mass limit it moves along a geodesic, but to first order in m it
accelerates, and there are two effects, a time-dependent inertial mass and
a deviation from geodesic motion (like geodesic motion for a modified metric);
The infinite self-field can be unambiguously decomposed into a singular piece
that
exerts no force, and a smooth remainder that is responsible
for the acceleration.
* Approaches: Barack/Burko/Ori's mode-sum regularization prescription
(MSRP).
@ General references: DeWitt & Brehme AP(60);
Kennefick gq/97 [history];
Quinn & Wald PRD(97)gq/96 [axiomatic];
Blanchet & Faye JMP(01)gq/00;
Quinn PRD(00)gq [and
scalar field]; Detweiler PRL(01)gq/00;
Barack & Ori PRD(01)gq [gauge-independent];
Poisson LRR(04)gq/03 [review
from scratch], CQG(04), gq/04-GR17;
Detweiler CQG(05)gq [rev];
Messaritaki gq/07 [singular
field].
@ Approaches: Barack & Ori PRD(00)gq/99,
Burko gq/99-in
[MSRP];
Detweiler & Whiting PRD(03)gq/02 [decomposition];
Ori & Rosenthal PRD(03)gq/02, JMP(04)gq/03 [extended
object approach];
Anderson et al PRD(05)gq/04 [quasi-local
terms];
Anderson & Wiseman CQG(05)gq [matched
expansion]; Pound et al PRD(05)gq [limitations
of adiabatic approximation]; Rosenthal PRD(06)gq [second-order];
Gal'tsov et al gq/07-in
[local method].
@ Related topics: Quinn & Wald PRD(99)gq [energy
conservation];
Whiting & Detweiler IJMPD(03)
[and equivalence principle].
In Specific Spacetimes
@ Schwarzschild: Burko CQG(00)gq/99 [static
particle], PRL(00)gq [in
orbit]; Wiseman PRD(00)gq;
Barack & Burko PRD(00)gq [plunging];
Nakano & Sasaki PTP(01)gq/00,
et al PTP(01)gq;
Barack PRD(00)gq, PRD(01)gq [mode
sum regularization], et al PRL(02)gq/01;
Mino et al PTP(02)gq/01;
Barack & Ori PRD(02)gq [regularization
parameters]; Barack & Loustó PRD(02)gq;
Burko PRD(03);
Detweiler et al PRD(03)gq/02;
Sago et al PRD(03)gq/02,
Nakano et al PRD(03)
[gauge problem]; Messaritaki gq/03-PhD;
Anderson & Hu PRD(04)gq/03 [part
+ scalar field];
Hikida et al PTP(04)gq/03 [scalar
charged particle]; Detweiler & Poisson PRD(04)gq/03 [
=
0, 1 multipoles]; Rosenthal PRD(04), PRD(04)gq [massive
field approach]; Hikida et al PTP(05)gq/04, CQG(05)gq/04 [regularization];
Anderson et al PRD(06)gq/05 [radial];
Haas & Poisson PRD(06)gq [particle
with scalar charge]; Barack & Sago gq/07 [circular
orbit]; Detweiler a0804 [circular
orbit].
@ Kerr: Kennefick & Ori PRD(96)gq/95,
Kennefick PRD(98)gq [circular
orbits]; Barack & Ori PRL(03);
Sago et al PTP(05)gq [evolution
of E, L, Q]; Barack et al a0709 [m-mode regularization].
@ Other spacetimes: Burko et al PRD(01)gq/00 [spherical
shell]; Burko & Liu PRD(01)gq [axisymmetric
black hole]; Burko et al PRD(02),
Haas & Poisson CQG(05)gq/04 [cosmological
spacetimes]; Shankar & Whiting PRD(07)-a0707 [charge
near spherical conducting star]; Khusnutdinov & Bakhmatov a0707 [wormhole].
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Send feedback and suggestions to bombelli at olemiss.edu – Modified
11 jun 2008