Gravitational Radiation Reaction and Self-Force| Gravitational Radiation Reaction and Self-Force |
In General > s.a. 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).
* Motivation:
2014, Calculating the gravitational self-force is the best approach
available to model the gravitational waves emitted by binary systems
with extreme-mass ratios.
@ Reviews: Poisson LRR(04)gq/03 [from scratch];
Detweiler CQG(05)gq;
Wald a0907-proc [intro];
Poisson et al LRR(11)-a1102;
Pound a1506-ch;
Barack & Pound RPP(19)-a1805 [for non-specialists].
@ 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;
Poisson CQG(04), gq/04-GR17;
Spallicci ch(10)-a1005-ln [and free fall, historical];
Bini & Damour PRD(12)-a1210 [general orbits, effective one-body formalism].
@ The singular field: Messaritaki PRD(07)gq;
Harte a1002-MG12 [effect on a body's multipole moments];
Heffernan a1403-PhD [local behavior].
@ The gauge issue: Barack & Ori PRD(01)gq [gauge-independent];
Gralla PRD(11)-a1104 [and averaging];
Cañizares & Sopuerta a1406 [new approach].
@ Approaches: Barack & Ori PRD(00)gq/99,
Burko AIP(00)gq/99 [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];
Gal'tsov et al in(06)gq/07 [local method];
Gralla & Wald CQG(08)-a0806,
a0907-proc [rigorous derivation];
Harte CQG(08)-a0807 [from generalized Killing fields];
Pound PRD(10)-a0907;
Wardell PhD(09)-a0910 [method of matched expansions];
Dolan & Barack PRD(11)-a1010 [m-mode regularization, and Schwarzschild spacetime];
Pound PRD(12)-a1206 [non-linear, field outside a small body];
Birnholtz et al PRD(13)-a1305;
Wardell et al PRD(14)-a1401 [via Green functions and worldline integration];
Birnholtz & Hadar PRD(15)-a1501 [in arbitrary dimensions];
Wardell in(15)-a1506 [computational strategies];
Oltean et al PRD(20)-a1907 [from quasilocal conservation laws].
@ Second-order: Rosenthal PRD(06)gq;
Gralla PRD(12)-a1203 [first-principles derivation];
Detweiler PRD(12);
Pound PRL(12)-a1201.
@ Numerical calculation: Vega et al PRD(09)-a0908 [(3+1) code],
CQG(11)-a1101;
Merlin & Shah PRD(15)-a1410 [from reconstructed metric perturbations].
@ Other situations / theories: Zimmerman & Poisson PRD(14)-a1406,
Zimmerman PRD(15)-a1505 [non-vacuum spacetimes];
Linz et al PRD(14)-a1406 [charged particles in electrovac spacetimes];
Zimmerman PRD(15)-a1507 [scalar-tensor gravity].
@ Related topics: Quinn & Wald PRD(99)gq [energy conservation];
Whiting & Detweiler IJMPD(03) [and the equivalence principle];
Linz et al PRD(14)-a1404 [on an accelerated particle];
Maia et al PRD(17)-a1705,
PRD(17)-a1705 [spinning bodies];
Chu et al PRD(20)-a1910 [tail-induced effects].
In Specific Spacetimes > s.a. black-hole binaries;
black-hole phenomenology; Geodetic Precession.
@ Schwarzschild, static particle: Burko CQG(00)gq/99;
Wiseman PRD(00)gq;
Rosenthal PRD(04)gq [massive field approach].
@ Schwarzschild, particle plunging radially: Barack PRD(00)gq;
Barack & Burko PRD(00)gq;
Barack & Loustó PRD(02)gq;
Anderson et al PRD(06)gq/05 [Hadamard-WKB expansion].
@ Schwarzschild, circular orbits: Burko PRL(00)gq;
Nakano et al PTP(01)gq;
Detweiler et al PRD(03)gq/02 [with scalar charge];
Detweiler & Poisson PRD(04)gq/03 [l = 0, 1 multipoles];
Hikida et al PTP(05)gq/04 [regularization];
Barack & Sago PRD(07)gq;
Detweiler PRD(08)-a0804;
Barack & Sago PRL(09)-a0902 [innermost circular orbit];
Blanchet et al PRD(10)-a0910;
Blanchet et al PRD(10)-a1002 [high-order post-Newtonian fit];
Shah et al PRD(11)-a1009 [conservative part of the self-force].
@ Schwarzschild, other situations: Nakano & Sasaki PTP(01)gq/00;
Barack 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];
Burko PRD(03);
Sago et al PRD(03)gq/02,
Nakano et al PRD(03) [gauge problem];
Messaritaki PhD(03)gq;
Anderson & Hu PRD(04)gq/03 [particle + scalar field];
Rosenthal PRD(04) [massive field approach];
Hikida et al CQG(05)gq/04 [regularization];
Sago et al PRD(08)-a0811 [comparing two approaches];
Damour PRD(09)-a0910 [effective one-body formalism];
Barack & Sago PRD(10)-a1002,
PRD(11)-a1101 [eccentric orbit];
Keidl et al PRD(10)-a1004 [in a radiation gauge];
Barack et al PRD(10) [precession effect];
Akcay PRD(11)-a1012,
Akcay et al PRD(12);
Vega et al PRD(13)-a1307 [eccentric orbits];
Vines & Flanagan PRD(15)-a1503 [motion under the conservative self-force];
Bini et al PRD(16)-a1601 [new analytical results];
Heffernan et al CQG(18)-a1712 [accelerated motion].
@ Schwarzschild, charged particle: Hikida et al PTP(04)gq/03,
Haas & Poisson PRD(06)gq [with scalar charge];
Cañizares & Sopuerta PRD(09)-a0903 [circular orbit];
Kim a1001;
Cañizares et al PRD(10)-a1006 [pseudospectral collocation methods];
Krtouš & Zelnikov PRD(20)-a1910 [static charge].
@ 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 PRD(07)-a0709,
Dolan et al PRD(11)-a1107 [m-mode regularization];
Barack CQG(09)-a0908 [extreme mass ratio];
Warburton & Barack PRD(10)-a1003,
PRD(11)-a1103;
Isoyama et al PRL(14)-a1404 [innermost stable circular equatorial orbit];
Warburton PRD(15)-a1408 [scalar charge];
Sago & Fujita PTEP(15)-a1505 [radiation reaction effect on orbital parameters];
van de Meent PRD(16)-a1606 [eccentric equatorial orbits];
van de Meent PRD(18)-a1711 [generic bound geodesics];
> s.a. particles in kerr spacetimes.
@ Other isolated objects: Burko et al PRD(01)gq/00 [spherical shell];
Burko & Liu PRD(01)gq [axisymmetric black hole];
Shankar & Whiting PRD(07)-a0707 [charge near spherical conducting star];
Drivas & Gralla CQG(11)-a1009 [dependence on central object];
Yen et al JCP(12)-a1210,
Wang et al ApJS(15)-a1509 [infinitesimally thin disk];
Castillo et al PRD(18)-a1804 [Reissner-Nordström black hole];
Mackewicz & Wald PRD(19)-a1909 [Kerr-Newman, spin self-force].
@ Wormholes: Khusnutdinov & Bakhmatov PRD(07)-a0707;
Bezerra & Khusnutdinov PRD(09)-a0901;
Khusnutdinov et al CQG(10).
@ Cosmological spacetimes: Burko et al PRD(02);
Haas & Poisson CQG(05)gq/04.
Applications
> s.a. dynamics of gravitating bodies; orbits
of gravitating objects [equations of motion]; Post-Newtonian Formalism.
@ References: Isoyama & Poisson CQG(12)-a1205 [as probe of internal structure of a massive body].
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