|  Gauge Choices or Fixing | 
In General > s.a. gauge group / symmetry.
  * Motivation:
    In classical theories with gauge freedom, fixing the gauge is a useful way
    to do calculations keeping only physical degrees of freedom; Many approaches
    to the quantization of a field theory require gauge fixing.
  @ References: Pons IJMPA(96) [and singular Lagrangians].
  > Types of theories:
    see constrained systems.
In Gravity > s.a. coordinate systems;
  embedding; initial-value
  formulation; models [radial gauge];
  observables; time.
  * Harmonic coordinates / gauge:
    Ones such that \(\nabla^2 x^a = 0\); Alternatively, the densitized inverse metric
  is divergenceless, (|g|1/2
    gab),a = 0;
    > s.a. harmonic functions;
    Wikipedia page.
  * Synchronous gauge:
    Defined by \(h_{0a} = 0\), for metric perturbations.
  @ Various choices: Rovelli CQG(89) [fixed spatial volume element];
    Bartnik CQG(97)gq/96 [null quasi-spherical];
    Alcubierre & Massó PRD(98) [hyperbolic, pathologies];
    Hájíček & Kijowski PRD(00)gq/99 [covariant];
    Esposito & Stornaiolo gq/99-conf,
    NPPS(00)gq/99,
    CQG(00)gq/98  [family of gauges];
    Pons et al JMP(00) [Einstein-Yang-Mills, transformations];
    Pons CQG(01)gq [special relativity limit];
    Salisbury MPLA(03);
    Pretorius CQG(05)gq/04 [harmonic, numerical relativity];
    Leclerc CQG(07)gq [and FLRW models];
    Chen & Zhu PRD(11)-a1006 [true radiation gauge];
    Reiterer & Trubowitz a1104 [vielbein formalism].
  @ Dirac gauge: Bonazzola et al PRD(04)gq/03 [spherical coordinates];
    Cordero-Carrión et al PRD(08)-a0802.
  @ 2+1 dimensions: Menotti & Seminara AP(91) [radial].
  @ Quantum gravity: Avramidi et al NPPS(97) [axial];
    Hájíček gq/99-TX19;
    Mercuri & Montani IJMPD(04)gq/03 [kinematical action].
  @ Quantum cosmology: Shestakova in(07)-a0801 [dependence on gauge and interpretation].
  @ Various theories of gravity: da Rocha & Rodrigues AIP(10)-a0806 [as field theory in Minkowski space];
    > s.a. canonical general relativity and models
      in canonical general relativity; higher-order gravity;
      numerical relativity.
In Linearized Gravity
  > s.a. cosmological perturbations [longitudinal, comoving].
  * Einstein / de Donder /
    Hilbert / Fock gauge: Defined by \(h^{*a}{}^{}_{b,a} = 0\), where
    \(h^*_{ab}:= h^{~}_{ab} - {1\over2}\,\eta^{~}_{ab} h\) (transverse?); The
    gravitational counterpart to the Lorenz gauge; not conformally invariant.
  * Radiation gauge: In addition,
    h = 0 and h0i = 0
    with i = 1, 2, 3.
  * Remark: The TT condition can only
    be imposed on the constraint surface–so it is not, strictly speaking, a gauge.
  @ References: Esposito & Stornaiolo CQG(00)gq/98;
    Scaria & Chakraborty CQG(02)ht [Wigner's little group];
    Leclerc CQG(07)gq;
    Price & Wang AJP(08)oct [transverse traceless gauge].
Electromagnetism and Other Gauge Theories > s.a. Gribov Problem;
  gauge theory; quantum gauge thories.
  * Idea: Gauge fixing corresponds
    to picking a cross section of the appropriate fiber bundle; This can always be done
    locally, but a global gauge choice in the non-Abelian case beyond perturbation
    theory is a non-trivial problem, and it may be impossible (Gribov ambiguity).
  * Axial gauge: Given a 4-vector
    u, impose u · A = 0, or u ·
  A =  any g-valued function on spacetime; This fixes the gauge
    everywhere if gauge transformations have to go to the identity at infinity.
  * Coulomb gauge: Defined by ∇
    · A = 0 (in 3D); Implies that the scalar potential Φ
    is just the instantaneous Coulomb potential; Also known as radiation gauge.
  * Feynman gauge: The choice
    ζ = 1 in the electromagnetic Lagrangian.
  * Landau gauge: The choice
    ζ → 0 in the gauge term \(\cal L_{\rm G}\) of the
    electromagnetic Lagrangian.
  * Lorenz gauge: A gauge in which
    ∇a Aa
    = 0, or = (any g-valued function on spacetime),
    so ∇2Aa
    = Ja; The residual
    freedom is Aa
    \(\mapsto\) Aa
    + ∂a χ, with
    ∇2 χ = 0, and can be used to impose the Coulomb gauge;
    Note: It is named after Ludwig Valentin Lorenz, and not after the Hendrik Antoon Lorentz of the Lorentz
    transformations [@ see Iliev a0803].
  * Radial gauge: In Maxwell theory,
    xa Aa
    = 0; In Poincaré gauge theory, xa
    Γa = 0,
    xa ea = 0.
  @ General references: Itzykson & Zuber 80, p567;
    Jackson AJP(02)sep [general transformations, and causality];
    Castellani IJTP(04) [Dirac's views];
    Capri et al PRD(06) [interpolating];
    Heras AJP(07)feb
      [different gauges and retarded electric and magnetic fields];
    Leclerc CQG(07)gq;
    Frenkel & Rácz EJP(15)-a1407 [use of transverse projection operator for transformation between gauges];
    Reiss JPB(17)-a1609 [restrictions and practical consequences].
  @ Axial gauge: in Itzykson & Zuber 80, p566;
    in Cheng & Li 84, p254;
    Krasnansky a0806 [for QCD].
  @ Coulomb gauge:
    Brill & Goodman AJP(67)sep [causality];
    in Itzykson & Zuber 80, p576;
    Cronstrom ht/98 [Yang-Mills theory];
    Haller & Ren PRD(03) [and Weyl, for QCD];
    > s.a. yang-mills theory.
  @ Lorenz gauge: Jackson AJP(08)-a0708 [attribution];
    Rodrigues AACA(10)-a0801-conf [and Killing vector fields];
    Heras & Fernández-Anaya EJP(10) [potentials as physical quantities].
  @ Radial gauge: Modanese & Toller JMP(90);
    Magliaro et al PRD(07)-a0704 [compatibility with others].
  @ Other choices:
    Heras AP(06) [Kirchhoff gauge];
    Landshoff APA-a0810-in [non-covariant gauges];
    Maas PRD(16)-a1510 [Landau gauge, first Gribov region].
  > In specific theories: see dirac
    fields; electromagnetism; Gauge Theory of Gravity;
    yang-mills gauge theory.
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