|  Gravitomagnetism | 
In General
  > s.a. duality; formulations of canonical general relativity;
  newtonian gravity; stress-energy pseudotensor.
  * Idea: Originally,
    a prerelativistic theory of gravity proposed in 1893 by Oliver Heaviside,
    based on an analogy between Maxwell's theory of electromagnetism and gravity;
    It is a flat-space, linear theory with no self-interaction, but the retardation
    of the field due to the speed of light is taken into account; In the current view,
    it is a special-relativistic theory that arises in the slow-motion, weak-field
    approximation of general relativity.
  * Field equations: The analogs of
    Maxwell's equations are (H = constant introduced by Heaviside, such that
    (G/H)1/2 = c)
∇ · g = −4πG ρ , ∇ × g = −∂h/∂t , ∇ · h = 0 , ∇ × h = −4πH ρ v + (H/G) ∂g/∂t .
  @ Reviews:
    Jantzen et al in(96)gq/01;
    Bini & Jantzen gq/00-proc [references],
    NCB(00) [rev];
    Ruggiero & Tartaglia NCB(02)gq;
    Mashhoon in(07)gq/03 [and Larmor theorem];
    Schäfer GRG(04)gq-in [rev];
    Iorio ed-06;
    Bakopoulos a1610-MS;
    news cosmos(19)sep [effects].
  @ General references: Heaviside Electr(1893);
    in Heaviside 1894;
    Thirring ZP(18);
    Bedford & Krumm AJP(85)sep;
    Wheeler IJMPA(88) [conceptual];
    Thorne in(88);
    Harris AJP(91)may [slow motion, weak field  equations]; & Schutz;
    Maartens & Bassett CQG(98)gq/97 [general formalism];
    Clark & Tucker CQG(00)gq [perturbative];
    Pascual-Sánchez NCB(00)gq [harmonic gauge];
    Mashhoon gq/00-proc;
    Tartaglia & Ruggiero EJP(04)gq/03 [vs electromagnetism];
    Wu CTP(05)gq [in gauge theory of gravity];
    Maartens GRG(08) [non-linear];
    Malekolkalami & Farhoudi MPLA(09)gq/06;
    Li a1012 [beyond linear order];
    Costa & Natário GRG(14)-a1207 [analogies with electromagnetism];
    Nouri-Zonoz & Parvizi GRG(16)-a1406 [Papapetrou field];
    Costa et al a1603
      [intrinsic/extrinsic gravitomagnetism and curvature scalar invariants];
    > s.a. riemann tensor [differential-geometric].
  @ Quantum theory: Santos & Khanna IJMPA(16)-a1605 [at finite temperature].
Effects, Phenomenology > s.a. maxwell fields in curved spacetime.
  * Idea: Gravitomagnetic fields arise from
    moving matter, like magnetic fields from moving charges, or from distributions of gravitomagnetic
    monopoles, if they exist (this requires torsion); They do not arise in scalar gravity.
  * Clock effect: A deviation
    from Kepler's third law for  a particle in orbit around a (slowly) spinning body,
    such as a typical planet or star, in the weak-field and slow-motion approximation
    of general relativity; i.e., a change in the period of revolution of clocks;
    > s.a. Wikipedia page.
  * Other examples: Precession of
    planetary orbits (not a good test); Precession of gyroscopes; These effects arise
    in a post-Newtonian, special relativistic treatment of gravitation.
  @ General references: Nordtvedt gq/02 [from special relativity + equivalence principle];
    Shen gq/03 [and quantum mechanics];
    Mashhoon CQG(08)-a0802 [time-varying fields].
  @ Observation: Ahmedov & Rakhmatov FP(03)gq [in electromagnetic systems];
    Kopeikin IJMPD(06)gq/05 [based on PPN expansion];
    Ciufolini a0704 [lunar laser ranging and satellites];
    Ruggiero & Tartaglia EPJP(19)-a1810 [satellite-based tests].
  @ Clock effect:
    Mashhoon et al AdP(99)gq/98,
    LNP(01)gq/99,
    PLA(01)gq;
    Bonnor & Steadman CQG(99);
    Semerák CQG(99) [extremely accelerated observers];
    Tartaglia GRG(00)gq;
    Lichtenegger et al ASR(00),
    ASR-gq/01;
    Bini et al CQG(01)gq/00;
    Bini & Jantzen gq/01-in;
    Iorio CQG(01)gq/00,
    et al CQG(02)gq/01,
    Tartaglia & Ruggiero gq/01 [neutron interferometry];
    Lichtenegger et al AdP(06)gq/02-conf;
    Faruque PLA(04) [spinning particle in Kerr];
    Iorio & Lichtenegger CQG(05) [Earth space-based];
    Hackmann & Lämmerzahl PRD(14)-a1406 [generalized];
    Faruque et al a1502 [in quantum mechanics];
    > s.a. tests of general relativity.
  @ On quantum systems: Camacho IJMPD(01)gq/00 [spin-1/2 systems];
    Adler & Chen PRD(10)-a0912 [spin-0 particle in electromagnetic + weak gravitational field].
  @ Extrinsic gravitomagnetism: Kopeikin & Fomalont GRG(07)gq/05,
    Kopeikin IJMPD(06) [and light deflection].
  @ Other effects: Pascual-Sánchez gq/99-in;
    de Matos & Tajmar IJP(01)gq/00 [gravitomagnetic Barnett effect];
    Tartaglia & Ruggiero gq/01 [rotating mass and light];
    Flanders & Japaridze IJTP(02)gq/01 [interaction between moving objects];
    Mashhoon IJMPD(05)ap [critical speed];
    Mitskievich & López Benítez a0707-MGXI [Zeeman-type];
    Bini et al CQG(08)-a0803 [gravitational induction];
    Chicone & Mashhoon PRD(11)-a1005 [and astrophysical jets],
    PLA(11) [gravitomagnetic accelerators];
    Ruggiero IJMPD(15)-a1502 [effects of massive rings],
    ASS(16)-a1507 [gravitomagnetic fields of rotating rings];
    Cashen et al PRD(17)-a1610 [gravitomagnetic dynamical friction];
    Crişan et al Univ(21)-a2103 [knot solutions].
  > And tests of general relativity:
    see gravitational phenomenology;  tests
    with orbits [frame dragging, geodetic precession] and with light.
  > Other effects:
    see gases [ultracold boson gases]; Tajmar Effect;
    Thomas Precession.
Related Topics
  > s.a. theta sectors [torsion-induced].
  @ Tidal tensor approach: 
    Costa & Herdeiro IAU(09)-a0912 [limitations of electromagnetic analogy];
    Voicu JNMP(12)-a1111 [geometric version].
  @ Specific spacetimes: Bini et al CQG(03)gq [Kerr-Newman-Taub-NUT],
    PRD(03)gq [Kerr-Taub-NUT];
    Kerr et al CQG(03)gq [with cosmological constant];
    > s.a. modified kerr solutions [Kerr-de Sitter].
  @ In teleparallel gravity: Spaniol & de Andrade IJMPD(10)-a0802;
    Ming et al IJMPD(17)-a1712 [alternative approach].
  @ In other theories:
    Nayeri & Reynolds ht/01 [brane effects];
    Camacho GRG(02)gq;
    Barros & Romero IJMPA(05) [Brans-Dicke];
    Iorio & Ruggiero JCAP(09)-a0810 [f(R) theories];
    Bailey PRD(10)-a1005 [Lorentz-violating];
    Exirifard JCAP(13)-a1111 [tensor-vector-scalar theory];
    Tasseten & Tekin PRD(16)-a1506 [massive gravity];
    Madriz & Montes a1703 [scalar-tensor gauge theory of gravity];
    Exirifard IJMPD(19)-a1906 [Scalar-Vector-Tensor theory, MOG];
    > s.a. non-local gravity.
  @ Related topics: Lynden-Bell & Nouri-Zonoz RMP(98)gq/96 [monopoles];
    Shapiro PRL(96)
    + pn(96)nov [and LIGO];
    Maartens et al CQG(02)gq/01 [and holonomy];
    Ghose a0905 [and relativistic particles];
    Malekolkalami & Farhoudi IJTP(14)-a1311 [and non-commutative geometry].
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