Gravitating N-Body Systems| Gravitating N-Body Systems |
N-Body Problems in General
> s.a. chaos in gravitation; classical
systems; gas [self-gravitating]; Scalar Theory.
@ Few-body systems: Will CQG(14)-a1404
[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 PRD(16)-a1511 [with second-order cosmological perturbations];
Barrera-Hinojosa & Li a1905 [GRAMSES].
@ 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];
Ghosh et a la 1904 [spiral galaxy halo];
> 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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