Gravitating Many-Body Systems  

N-Body Problems in General > s.a. chaos in gravitation; classical systems; gas [self-gravitating]; Scalar Theory.
@ Few-body systems: Will a1404-CQG [relativistic precession and conserved quantities in hierarchical triple systems].
@ Many-body systems in general: Kandrup PRP(80) [fluctuations in mean-field theory]; Seidov & Skvirsky ap/00; Liu gq/02 [v distribution in gravitational field]; Laliena NPB(04)ap/02 [phase structure], NPB(03)ap [thermodynamic limit]; Chavanis ap/02-conf [Fermi gas]; Chruściel et al CQG(10) [initial data]; Tashiro & Tatekawa JPSJ(10)-a1108 [Brownian dynamics, non-Maxwellian distribution]; Schmidt GRG(12) [new formulation]; Turyshev & Toth IJMPD(15)-a1304 [new perturbative method].
@ Relativistic vs Newtonian: Chu PRD(09)-a0812 [N-body problem, 2PN]; Ledvinka et al a1003-MG12 [post-Minkowskian Hamiltonian]; Will PRD(14)-a1312 [post-Newtonian effects]; Rampf et al CQG(14)-a1409 [relation between Newtonian simulations and general relativity].
@ Special situations and related topics: Valageas PRE(06)ap [1D, relaxation]; Beig & Schoen CQG(09) [static configurations, no-go result]; Andersson & Schmidt CQG(09)-a0905 [static]; Teles et al JSM(10)-a1004 [2D, unbounded]; Hartung & Steinhoff PRD(11), AdP(11)-a1104 [spin-orbit and spin-spin Hamiltonians].
@ Statistical mechanics: Padmanabhan PRP(90); Zaslavskii PLA(91); Hut ap/97-proc; El-Zant PRE(98)ap [simulations]; de Vega et al CSF(99)ap/98, & Sánchez PLB(00)ht/99, NPB(02)ap/01, NPB(02)ap/01; Morikawa G&C(00); Cipriani & Pettini ASS(03)ap/01 [chaos and statistical mechanics]; Katz FP(03)ap/02 [intro]; Laliena NPB(03)ap, NPB(05)ap/03; Fischer ap/03/A&A [thermal equilibrium]; He MNRAS(12)-a1103 [equilibrium statistical mechanics]; Beraldo e Silva et al PRD(14)-a1410 [mixing]; Peñarrubia MNRAS-a1506 [non-equilibrium, probabilistic theory].
@ Thermodynamical aspects: Velázquez & Guzmán ap/03 [thermodynamic limit]; Golovko JPA(05)-a1504 [quantum effects at T = 0]; Casetti & Nardini JSM(10)-a1003 [solvable model].
@ In modified-gravity theories: Stabenau & Jain PRD(06)ap; Winther et al MNRAS(15)-a1506.

Astrophysics and Cosmological Aspects > s.a. astrophysics; newtonian and tests; cosmological models.
* Dufour effect: Density gradients prevent gravitating clouds in thermodynamic equilibrium from being isothermal.
@ Clustering: Antonuccio-Delogu & Atrio-Barandela ApJ(92)doi; Del Popolo A&A(96)ap/01, ap/01-proc [statistics]; Rothman & Anninos PRD(97)gq/96 [inhomogeneity measure]; Scoccimarro ApJ(00)ap; Bottaccio et al EPL(02)cm/01 [simulations]; Padmanabhan LNP-ap/02, Khagol(02)ap/03 [cosmological]; Matarrese et al JCAP(03) [with quintessence scalar field]; Valageas A&A(08)-a0711 [expansion schemes]; Sylos Labini AIP(08)-a0806; Padmanabhan a0812-ln [in an expanding universe, rev].
@ N-body simulations: Aarseth 03, Aarseth et al 08; Christopherson et al a1511 [with second-order cosmological perturbations].
@ Tidal heating: Booth & Creighton PRD(00)gq [quasilocal calculation].
@ Bodies in galaxies: Fragile & Mathews ApJ(00)ap/99 [stars around the Milky Way center]; Bel a1005 [solar-system model].
@ Description of galaxies: Matos & Guzmán CQG(01)gq [two scalars + dust = galaxy]; Roberts GRG(04)ap/02 [metric]; 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 ASTP(07)ap/06 [re rotating dust solutions]; Cooperstock & Tieu IJMPA(07)ap/06; Pedraza et al MNRAS(08)-a0806 [Kalnajs family]; Rakić & Schwarz a0811-conf [Newtonian aspects]; Chanamé IAU(10)-a1005 [Schwarzschild models]; Zotos CSF(11)-a1204 [chaotic motion and external perturbations]; Dey et al GRG(15)-a1407 [in modified theories of gravity]; > s.a. galaxy distribution; perturbations of FLRW models.
@ Rotation curves: Hartnett IJTP(05)gq/04 [Carmeli metric]; Carrick & Cooperstock ASS(12)-a1101; Razbin et al IJMPD(14).
@ Dark matter in expanding universe: Padmanabhan in(00)ap/99; Carati et al EPL(08)-a0903 [and effect of distant matter].
@ Techniques: Scoccimarro ap/00-proc [in terms of Feynman diagrams]; Barnes MNRAS(12)-a1205 [softening / smoothing].
> Related topics: see geometry and topology of the universe; gravitational thermodynamics.


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