|  Tests of General Relativity – Light Deflection | 
In General
  >  s.a. lensing;
  phenomenology of gravity; Runge-Lenz Vector.
 s.a. lensing;
  phenomenology of gravity; Runge-Lenz Vector.
  * Prediction: For a light ray grazing
    the Sun, using the Schwarzschild metric δφ = 1.75".
  * Results: Consistent with γ
    = 1; 1989, Analysis of radio waves using VLBI in progress, estimate σ(γ)
    = 0.002; 2005, VLBA results determined γ with an accuracy of 0.0003 using
    the deflection of four compact radio sources by the solar gravitational field.
  * Remark: In general relativity, although
    particle paths depend on orientation of spin, there is no optical birefringence
    (> see polarization).
  @ Observations: Dyson et al PTRS(20),
    Dyson Nat(21)feb [May 29, 1919 eclipse];
    Fomalont & Sramek PRL(76),
    Lebach et al PRL(95) [radio waves by the Sun];
    news sn(17)jun [starlight deflection by distant star];
    Bruns CQG(18)
    and CQG+ [reenactment of Eddington's measurement with the August 2017 eclipse].
  @ Theory, in Schwarzschild spacetime: Lerner AJP(97)dec;
    Iyer & Petters GRG(07) [analytical perturbation framework];
    Pérez & Lamine EJP(18)-a1806 [historical];
    Poutanen A&A(20)-a1909 [accurate analytic formula].
  @ Theory, in general:
    Palatini MSAI(23)-a1608;
    Richter & Matzner ASS(81),
    PRD(82),
    PRD(82) [rotating star];
    Bruckman & Esteban AJP(93)aug;
    Dodelson & Wiegert ap/97 [by vector perturbations];
    Gerard & Pireaux gq/99;
    Díaz-Miguel PRD(04) [fall in uniform g field];
    Magnan a0712 [complete derivation];
    Bhadra a1007
      [source and observer not at infinity, weak-deflection limit];
    Mak et al AHEP(18)-a1805 [Laplace-Adomian decomposition method];
    Ono & Asada Univ-a1906 [finite-distance source and observer];
    Arakida a2006 [definition of deflection angle].
  @ Beyond linear order: Bodenner & Will AJP(03)aug [to second order];
    Brügmann PRD(05)gq [post-linear order];
    Hioe PLA(09) [exact expression];
    Linet & Teyssandier PRD(16)-a1511 [time transfer functions, unified description of Shapiro and lensing effects].
  @ And the equivalence principle: Ferraro AJP(03)feb-gq/02;
    Díaz-Miguel a0809.
  @ Related topics: 
    Mohanty & Prasanna ap/95 [no birefringence];
    Fomalont et al IAU(10)-a0912;
    Unnikrishnan & Gillies IJMPD(09) [classical, quantum, and exotic light];
    Li & Chang PRD(10) [quantum gravity effects];
    > s.a. history of relativistic physics [1919 eclipse expedition].
By Different Objects / In Other Theories of Gravity
  > s.a. brans-dicke phenomenology; cosmic-string
  phenomenology; torsion phenomenology.
  @ In Schwarzschild-de Sitter / Kottler spacetime:
    Islam PLA(83);
    Lake PRD(02);
    Rindler & Ishak PRD(07)-a0709 [non-vanishing effect];
    Gibbons et al CQG(08)-a0808;
    Miraghaei & Nouri-Zonoz GRG(10)-a0810 [Newtonian limit];
    Bhadra et al PRD(10)-a1007;
    Arakida & Kasai PRD(12)-a1110;
    Lebedev & Lake a1308,
    a1609;
    Hammad MPLA(13)-a1309;
    Butcher PRD(16)-a1602;
    Faraoni & Lapierre-Leonard PRD(17)-a1608 [using the Hawking quasilocal mass, and varying cosmological acceleration];
    Arakida GRG(18)-a1708 [definition of the total deflection angle];
    Takizawa et al PRD(20)-a2001.
  @ With cosmological constant, other metrics: Freire et al GRG(01)gq/02 [with a conical defect].
  @ By planets: Kopeikin ap/03 [Jupiter];
    Crosta & Mignard CQG(06)ap/05 [and Gaia mission];
    Kopeikin & Makarov PRD(07)gq/06 [planetary multipoles];
    Malkin et al SSR(09)-a0907 [radio sources];
    Fomalont & Kopeikin IAU(07)-a0912 [VLBA results].
  @ Kerr metric:
    Iorio NCB(03)gq/02;
    Kraniotis CQG(05)gq [and Kerr-AdS];
    Edery & Godin GRG(06) [second-order, equatorial];
    Iyer & Hansen PRD(09) [equatorial];
    Iyer a1810 [asymmetry from frame dragging].
  @ Other isolated-object metrics: Ruggiero et al IJMPD(06) [rotating sources, and quadrupole moments];
    Sultana PRD(13) [Kerr-de Sitter];
    Hu et al AHEP(14)-a1312 [spherically  symmetric spacetime, with cosmological constant];
    Kraniotis GRG(14)-a1401 [Kerr-Newman and Kerr-Newman-AdS];
    Ahmadi & Sedaghatmanesh a1501 [binary system];
    Aghili et al GRG(17)-a1408,
    Piattella PRD-a1508,
    Univ(16)-a1609 [McVittie metric];
    Ono et al PRD(18)-a1806 [rotating wormhole];
    news cosmos(18)jun [galaxy ESO 325-G004, 450 Mly away];
    Hsiao et al PRD(20)-a1910 [Kerr-Newman black holes].
  @ In Weyl gravity: Edery & Paranjape PRD(98)ap/97 [and delay];
    Pireaux CQG(04),
    CQG(04)gq;
    Cattani et al PRD(13).
  @ Related topics: Durrer PRL(94) [in perturbed FLRW spacetime];
    Özer & Delice CQG(18)-a1708 [modified gravity with a cosmological term].
  @ Quantum-gravity motivated: Tso & Bailey PRD(11)-a1108 [with Lorentz symmetry violation];
    Bjerrum-Bohr et al PRL(15)-a1410 [in quantum gravity, one-loop gravitational amplitude];
    Xu & Yang JMP(18)-a1709 [higher-order theories].
Examples, Observations, Missions
  * LATOR: A proposed mission
    that would send two laser-transmitter spacecraft behind the Sun to measure the
    relative gravitational light bending of their signals using a hundred-meter-baseline
    optical interferometer, to be constructed on the ISS; Should allow a simultaneous
    determination of the orbit parameters of the spacecraft and of γ
    with an uncertainty of 2.4 × 10−9,
    a 6 × 10−9 determination of the
    solar quadrupole moment J2, and
    the first measurement of the second-order post-PPN parameter δ
    to an accuracy of about 10−3.
  @ LATOR mission: Turyshev et al CQG(04)gq/03-conf,
    NPPS(04)gq,
    ASR(07)gq/04-conf,
    IJMPD(04)gq-conf,
    ESA-gq/05,
    in(06)gq;
    Plowman & Hellings CQG(06)gq/05;
    Turyshev & Shao IJMPD(07)gq-proc.
  @ Related topics: Zschocke & Klioner a1007 [simplification, for Gaia astrometry mission];
    news pt(17)jun
      [weighing white dwarf Stein 2051 B with light];
    Bruns CQG(18)-a1802 [analysis of observations during the 2017-08-21 eclipse].
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