Electromagnetism in Curved Spacetime| Electromagnetism in Curved Spacetime |
In General > s.a. astrophysics;
black-hole and gravitational phenomenology.
* Remark: In flat spacetime, the Coulomb law
implies the Gauss law, but the latter is the one that generalizes to curved spacetime.
@ General references:
Cohen & Kegeles PRD(74);
Bini et al IJMPD(01)gq/00 [integral formulation];
Araujo Diniz et al ht/00;
Tsagas CQG(05)gq/04;
Sundkvist JMP(06) [covariant parametrization];
Mitskievich a0802 [classification of fields];
Notte-Cuello et al RPMP(08) [effective geometry];
Subramanian AN(10)-a0911 [early universe, rev];
Smolić CQG(14)-a1404 [spacetimes with symmetries];
Cabral & Lobo FP(16)-a1602 [and spacetime geometry];
Côté et al GRG(19)-a1905 [conformal invariance];
Mavrogiannis & Tsagas a2104
[in terms of potentials, with imperfect fluid, and cosmology].
@ Electric and magnetic fields: Ellis in(73);
Crater AJP(94)oct,
comment Vanzella et al AJP(96)aug;
Mabin et al TPT(17) [phenomenology].
@ Asymptotics: Goldberg & Kerr JMP(64) [multipoles];
Alexander & Bergmann FP(84);
Nolan AP(95) [NP];
Misner et al PRD(06) [numerical, beyond scri];
> s.a. spatial infinity [asymptotic symmetries].
@ Electric-magnetic duality: Deser et al PRD(97)ht/96 [black holes];
Cardoso et al PLB(96)ht [action for electric/magnetic currents].
@ Complex techniques: Kaiser JPA(04)gq/01 [Kerr-Newman fields];
Gsponer gq/04 [Lanczos-Newman electrodynamics].
> Related topics:
see Geometrization; green functions;
light [propagation]; polarization;
wave phenomena.
Specific Types of Spacetimes > s.a. FLRW models;
huygens' principle; null infinity.
@ Kerr black holes: Mukhopadhyay CQG(02)gq;
Fernandes & Lahiri EPJC(19)-a1803;
Grant & Flanagan CQG(20)-a1910 [conserved currents].
@ Other black holes: Harpaz FP(07) [electric field in Schwarzschild spacetime];
Valiente Kroon a0802 [near infinity];
> s.a. black-hole phenomenology; fields in
schwarzschild space; generalized reissner-nordström spacetimes.
@ de Sitter spacetime:
Otchik & Red'kov pr(86)-a1001 [waves];
Tsaregorodtsev & Medvedev G&C(98)gq [charged particle];
Cotăescu & Crucean PTP(10)-a0806;
Bini et al GRG(10) [exact solution];
Veko et al NPCS-a1410.
@ Other cosmological models: Hu & Shiokawa PRD(98)gq/97 [FLRW + stochastic];
Montani & Cherubini IJMPD(05) [isotropic universe];
Fleury et al PRD(15)-a1410 [homogeneous, anisotropic Bianchi I universe].
@ Other spacetimes: Tomaschitz JMP(93) [multiply connected];
Perez Bergliaffa & Hibberd PRD(00)gq [wormholes];
Sakai & Shibata ApJ(03)ap/02 [and pulsars];
Alvarez & Olive CMP(06)ht/03 [manifolds with boundary];
Nouri-Zonoz CQG(04) [NUT space];
Padmanabhan & Padmanabhan GRG(10)-a0910 [Rindler space, as model for weak gravitational field];
Kassandrov G&C(11)-a1105 [Kerr-Schild spacetimes];
Asenjo & Hojman CQG(17)-a1608 [when waves do not propagate along null geodesics].
@ In higher dimensions: Mitskievich a0707-MG11;
Dalmazi & Santos PRD(11)-a1105;
Delphenich a1812 [5D];
Henneaux & Troessaert PRD(19)-a1903.
@ Generalized backgrounds: Wise CQG(06) [on a chain complex];
Tarasov MPLA(06)-a0711 [on a fractal];
Harikumar EPL(10)-a1002 [on κ-Minkowski spacetime, and duality].
Coupling to Gravity > s.a. lorentzian geometry [analog];
gravitating matter; unified theories.
* Motivation: Improved
experimental tests of general relativity, including electromagnetic fields
around black holes, and alternatives theories.
* Idea: The Maxwell equations
in terms of (E, B) and (D, H) do not require
a metric or connection, but the constitutive relationships between those two pairs
do; The coupling to gravity may be non-minimal, and in particular it may require
non-metricity and/or torsion.
@ General references: Bergmann et al PR(50) [with Einstein's general relativity];
Barut et al HPA(94) [and spacetime models];
& Toupin & Schoenberg; Senovilla gq/03-proc [conserved tensor];
Rosquist CQG(06)gq/04 [Compton scale effects];
Hehl & Obukhov GRG(08) [and the equivalence principle];
Füzfa PRD(16)-a1504
+ news IBT(16)jan [artificial gravitational fields];
Vollick PRD(16)-a1612 [from modified Palatini action].
@ 3D: Barnich et al CQG(15)-a1503 [asymptotically flat];
Pérez et al JHEP(16)-a1512 [AdS spacetime, asymptotic structure].
@ Special situations: Shatskiy JETP(01)gq/02 [field of a ring current around a Kerr black hole];
Gürlebeck et al PRD(11) [layers of electric and magnetic monopoles and dipoles];
Vancea a1708 [field line solutions];
> s.a. gravitational waves; solutions of general relativity.
@ Non-minimal: Prasanna & Mohanty CQG(03) [constraints];
Balakin & Lemos CQG(05)gq;
Annulli et al PRD(19)-a1901 [non-perturbative astrophysical effects].
@ With non-metricity and torsion: Vandyck JPA(96);
Hehl & Obukhov LNP(01)gq/00.
@ In quantum spacetime: Lewandowski et al PRD(17)-a1709 [emergence of rainbow metric];
> s.a. non-commutative spacetime;
photons in quantum gravity.
Phenomenology and Related Topics > s.a. electricity;
modified electrodynamics [pre-metric]; self-dual fields.
@ General references: Cabral & Lobo EPJP(17)-a1603 [astrophysical applications];
Bunney & Gradoni a1912 [doppler and gravitational redshifts].
@ Gravitomagnetic effects: Nouri-Zonoz PRD(99)gq [Faraday rotation];
Kopeikin & Mashhoon PRD(02)gq/01.
@ Optical geometry: Sonego & Abramowicz JMP(98);
Abramowicz & Sonego 04;
Bittencourt et al CQG(16)-a1510 [importance and flexibility];
> s.a. optics; self-force.
@ Negative refraction:
Lakhtakia et al PLA(05).
main page
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