Matter Dynamics in Gravitation  

Particles and Fields, Couplings > s.a. canonical general relativity; matter phenomenology; solutions of general relativity with matter.
* Idea: Study of the ways in which matter fields can be coupled to gravity, and their consequences.
@ General references: Ahluwalia GRG(97)gq [flavor oscillation clocks and redshifts]; Smoller gq/02; Ehlers et al AJP(06)gq/05, Mitra gq/06 [pressure contribution to gravity source]; Ellis et al GRG(07) [causality and speed of sound]; Faraoni a0710 [anomalous coupling of Ricci curvature to matter].
@ Particles: Banchet CQG(07) [dipolar particles]; Rosquist a0802-in [effect on electromagnetic fields]; > s.a. particle effects.
@ Laws of motion, precession: Dixon PTRS(74); Thorne & Hartle PRD(85); Basalyga & Gorbatsievich gq/99 [atoms]; > s.a. orbits of gravitating objects [including two-body problem].
@ With Maxwell fields: Solanki et al PRD(04) [torsion, bounds]; Grøn & Nass a0806 [particle as perpetuum mobile]; > s.a. born-infeld.
@ Einstein-Yang-Mills: Vignolo & Cianci JMP(04) [tetrad-affine]; Llibre & Valls JPA(05) [first integrals]; Balakin & Zayats gq/06-G&C [non-minimal]; > s.a. first-order actions for general relativity.
@ Other examples: Finster et al MPLA(99)gq [Einstein-Dirac-Maxwell]; Bekaert et al PLB(00) [2-form fields]; Mohanty et al PRD(02) [fermions, and CPT violation]; Feng et al GRG(04) [supersymmetric elementary particles]; Banks et al JHEP(06)ht [gauge theories].
@ Kinetic theory, Einstein-Vlasov: Andreasson LRR(05)gq [properties of solutions]; > s.a. stochastic processes.
> Other: see formulations of electromagnetism; dirac fields; electricity; gravity; light; scalar fields; self-force; types of field theories.

Extended Media > s.a. force; gravitomagnetism; phenomenology; solutions of general relativity with matter; tests of general relativity.
@ General references: Ferrari & Ibáñez PLA(89) [colliding clouds of null particles]; Montani et al NCB(00)gq; Unzicker gq/00 [continuum mechanics]; Carter in(83)gq/01 [and gravitational radiation]; Aguirregabiria & Bel GRG(01)gq [arbitrary mass and size]; Montani et al CQG(03)gq [macroscopic, polarization]; Kiefer & Weber AdP(05); Alberghi et al CQG(06) [thick shell]; Ferrarese & Bini 07.
@ Shells: Schmidt GRG(84)gq/01 [tension]; Barrabès & Israel PRD(91) [null]; Cherubini et al PLB(02) [charged]; Guerrero et al PRD(02)gq; Scardigli gq/02-PhD; Kijowski et al IJGMP(05) [Lagrangian and Hamiltonian], gq/05 [general solution], PRD(06) [variational principle]; Khosravi et al CQG(06) [thick]; > s.a. metric matching, models in canonical general relativity.
@ Disks, plates: Klein & Richter PRL(99)gq [dust]; Petroff & Meinel PRD(01)gq [rigid dust disk]; Teixeira gq/05, Jones et al AJP(08)-a0708 [infinite plane].
@ Binding energy: Bizon et al CQG(90); Hsu gq/98.
> Fields and systems: see cosmic strings; fluids; membrane.
> Topics: see angular momentum; energy-momentum tensor; gravitational energy; radiation; rotation.

Single Objects > s.a. ADM formalism; black holes; chaotic motion; collapse; cosmology [with isolated bodies]; Gravastar; neutron stars.
* Idea: Study of the dynamics of isolated gravitating bodies, including black holes, and their properties such as conserved quantities; Effective dynamics of extended objects also provides useful approximations for gravitational wave production.
@ Rotating objects: Hartle & Sharp PRL(65) [equilibrium]; Hartle et al ApJ(72) [stability of rotating stars]; Xanthopoulos JMP(81); Manko PRL(90); Mars & Senovilla MPLA(98)gq; Bradley et al CQG(00)gq [pfluid ball]; Zhang et al MPLA(01); Tartaglia gq/02, comment Iorio GRG(04)gq/03 [weak field]; Stergioulas LRR(03) [rev]; Abramowicz et al gq/03, Martín-Martín et al gq/04-in [solution]; Karpov G&C(04); Lynden-Bell PRD(04)gq [charged sphere]; Nolan & Vera gq/05-in [cosmological backgrounds]; Bonnor GRG(05) [negligible mass]; Anderson gq/05 [approximate eom]; Cabezas et al GRG(07) [constant mass density]; Vogt & Letelier PRD(07) [thick disk].
@ Kerr interior metrics: Cohen JMP(67) [slow rotation]; Burghardt SBLS(07)-a0711, SBLS(07)-a0711 [differentially rotating fluid].
@ Static objects: Wald PRD(72) [electromagnetic field]; Radford gq/06 [spherical symmetry]; González & Letelier PRD(04), Vogt & Letelier PRD(05)gq [thick disk]; Karageorgis & Stalker a0707 [bounds on 2m/r]; Ponce de León a0711 [non-Schwarzschild star exteriors]; Bimonte et al PRD(08)-a0801 [magnetic stresses and energy].
@ Extended objects: Arnowitt et al AP(65) [minimum size]; Capovilla & Guven PRD(97)mp/98, PRD(98)mp [with edges]; Vaidya GRG(99), GRG(99) [star + radiation]; Füzfa et al GRG(02)gq/01 [ = constant sphere]; Gibbons FP(02)ht [maximal tension = c4/4G]; Zsigrai CQG(03)gq [ellipsoids]; Mahomed NCB(03) [charged spheres]; Anandan et al IJMPD(03)gq-GRF, PRD(03) [action]; Capovilla et al CQG(04) [Hamiltonian]; Racine & Flanagan PRD(05)gq/04 [arbitrary shape, PN-1]; Goldberger & Rothstein PRD(06)ht/04 [effective field theory]; Boonserm et al PRD(05)gq [perfect fluid spheres]; Blanchet et al PRD(05) [PN expansion of field]; Porto PRD(06)gq/05 [spin effects]; Choquet-Bruhat & Friedrich CQG(06) [isolated bodies, initial-value problem]; Böhmer & Harko CQG(06) [bounds on physical parameters], GRG(07)gq [lower bound for the mass-radius ratio]; Galloway & O'Murchadha a0802 [sizes]; > s.a. Elasticity.
@ Moving bodies: Harte PRD(06)gq/05 [in flat space]; Hennig et al gq/07 [inelastic collisions and radiated energy]; Bialynicki-Birula & Bialynicka-Birula PRA(08)-a0804 [electromagnetic radiation].
@ Other theories: Arminjon RJP(03)gq/02 [scalar gravity]; Frolov gq/07-in [Poincaré gauge theory, rotating object].

N-Body Problems, Astrophysics and Cosmology > s.a. astrophysics; gas; newtonian gravity and tests; relativistic cosmology.
* Dufour effect: Density gradients prevent gravitating clouds in thermodynamic equilibrium from being isothermal.
@ Many bodies: Kandrup PRP(80) [fluctuations in mean field theory]; Liu gq/02 [v distribution in gravitational field]; Stabenau & Jain PRD(06)ap [in modified gravity]; Valageas PRE(06)ap [1D, relaxation]; > s.a. chaos in gravitation; classical systems.
@ Self-gravitating: Seidov & Skvirsky ap/00; Laliena NPB(04)ap/02 [phase structure], NPB(03)ap [thermodynamic limit]; Chavanis ap/02-in [Fermi gas]; > s.a. Scalar Theory.
@ Clustering: Atrio-Barandela (92); Del Popolo A&A(96)ap/01, ap/01-in [statistics]; Rothman & Anninos PRD(97)gq/96 [inhomogeneity measure]; Scoccimarro ap/00; Bottaccio et al cm/01/EPL [simulations]; Padmanabhan ap/02-in, Khagol(02)ap/03 [cosmological]; Matarrese et al JCAP(03) [with quintessence scalar field]; Valageas a0711 [expansion schemes]; Sylos Labini a0806-in.
@ Tidal heating: Booth & Creighton PRD(00)gq [quasilocal calculation].
@ Bodies in galaxies: Fragile & Mathews ApJ(00)ap/99 [stars around Milky Way center].
@ Description of galaxies: Matos & Guzmán CQG(01)gq [two scalars + dust = galaxy]; Roberts GRG(04)ap/02 [metric]; Hartnett IJTP(05)gq/04 [Carmeli metric and rotation curves]; Vogt & Letelier PRD(05)gq/04 [AGN with disk], MNRAS(05)gq, ap/05; Matos et al GRG(05)ap/04 [halos]; Cooperstock & Tieu ap/05, comment Cross ap/06, Garfinkle CQG(06); Zingg et al ap/06 [re rotating dust solutions]; Cooperstock & Tieu IJMPA(07)ap/06; Pedraza et al a0806-MNRAS [Kalnajs family]; > s.a. perturbations of FRW models.
@ Dark matter in expanding universe: Padmanabhan in(00)ap/99.
@ Techniques: Scoccimarro ap/00-in [ito Feynman diagrams]; Aarseth 03 [numerical simulations].
> Related topics: see geometry and topology of the universe; gravitational thermodynamics.

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