|  Quantum Geometrodynamics: Dynamics in Superspace | 
The Program in General > s.a. canonical general relativity
  and ADM formulation [classical version]; canonical quantum gravity.
  * Idea: Geometrodynamics is
    the program for canonical quantum gravity based on superspace and the dynamics
    given there by the Wheeler-DeWitt equation; A 4-geometry is represented by a
    classical set of points C of superspace, contained in it as a hypersurface;
    The set of 3D geometries contains the time information; Initial data consists of
    a neighborhood in C, from which the Einstein equation gives C.
  * Problems: Mainly interpretational,
    such as What is the meaning of Ψ(q, φ)? We need an inner
    product for Ψs before we say that |Ψ|2
    is a probability.
Kinematics: Superspace
  > s.a. canonical quantum gravity; regge
  calculus [simplicial superspace]; topology change.
  * Idea: Superspace is a reduced
    configuration space for a Hamiltonian formulation of gravity, in which a point
    is a diffeomorphism equivalence class of Riemannian metrics on a spacelike
    hypersurface Σ: S(Σ):= Riem(Σ)/Diff(Σ).
  * Constraints: This choice of
    configuration space eliminates the diffeomorphism constraint, but the scalar
    one (coming from the gauge arbitrariness in choosing a slicing of spacetime)
    remains, and becomes the dynamical equation.
  * Topology: S(Σ)
    is not a manifold, but is made up out of a finite number of manifolds (strata).
  * Extended: Glue together copies of
    the same space [@ DeWitt (70)].
  * Grand: Need singular geometries.
  * Minisuperspace: Impose enough
    symmetries to get finite number of degrees of freedom.
  @ Structure of superspace: & Peres < 79; Fischer in(70);
    in Brill in(72); Reula pr(GR12);
    Christodoulakis & Zanelli pr(89);
    Giulini HPA(95)gq/93,
    PRD(95)gq/93;
    Fischer & Moncrief GRG(96) [including conformal superspace];
    Giulini GRG(09)-a0902;
    Gomes JMP(11);
    Liu a1509
      [Gromov's ε-approximation topology].
  @ Supermetric: Pekonen JGP(87);
    Szydłowski JMP(99);
    Schmidt gq/01-proc;
    Hehl & Kiefer GRG(18)-a1711 [comparison with the 4th-rank constitutive tensors in electrodynamics and elasticity theory].
  @ Minisuperspace: Misner in(72);
    Kuchař & Ryan in(86);
    Kiefer AP(91);
    Kerbrat et al RPMP(92);
    Saremi gq/01;
    > s.a. gowdy spacetimes.
  @ Related topics: Jacobson in(88) [self-dual representation];
    Rainer gq/96-conf [locally homogeneous];
    Barbour & Ó Murchadha a1009 [conformal superspace];
    > s.a. Configuration Space; riemannian geometry.
States: Wave Functionals
  > s.a. time in quantum gravity.
  * Idea: States are functionals
    Ψ[qab,φ]
    of metrics (and matter fields) belonging to an appropriate space; Notice that
    these states will end up without a time dependence, since they must satisfy the
    constraints; Instead, time can be taken as one of the components of
    qab.
  @ Inner product: DeWitt PR(67);
    Tsamis & Woodard PRD(87);
    Christodoulakis & Zanelli CQG(87);
    Vilenkin PRD(89).
Dynamics: Wheeler-DeWitt Equation > s.a. 3D quantum gravity;
  cosmological constant; FLRW quantum cosmology;
  lattice gravity [discretized].
  * Idea: The "zero-energy"
    Schrödinger-like equation one gets as the operator version of the scalar constraint,
    by replacing q and p by their coordinate representation operators
    (multiplication operator and −i\(\hbar\)(δ/δq), respectively),
    and acting with it on a wave functional
    Ψ[qab, φ].
  * Expression: For the dynamics of gravity
    coupled to a field φ, it is
{−Gabcd (δ2/δqab δqcd) + q1/2[–3R + 2Λ + (16πG)−1 T00(iδ/δφ, φ)]} Ψ(q, φ) = 0 ,
up to linear derivative terms depending on the choice of factor ordering, where the supermetric, with "signature" (−, +, +, +, +, +) –the minus sign coming from the conformal mode– and thought of as a 6 × 6 matrix, is defined by
Gabcd = \(1\over2\)q−1/2 (qac qbd + qad qbc − qab qcd) .
  @ General references:
    Woodard CQG(93);
    Jackiw gq/95 [modified];
    Błaut & Kowalski-Glikman gq/96 [solutions, and quantum potential];
    Norbury EJP(98)phy [II, from Newtonian physics];
    Soo CQG(07)gq [in terms of gauge-invariant 3-geometry elements];
    Sawayama a0904 [small universe];
    Cherkas & Kalashnikov DANB-a1406 [near small scale factors, discrete vs continuum spectrum];
    Rovelli CQG(15)-a1506 [rev].
  @ Related topics: Gurzadyan & Kocharyan JETP(87),
    Kocharyan CMP(91) [stability of cosmological models];
    Dereli et al PLB(94) [as spinor equation, including degenerate metrics and signature change];
    Mehta a1912 [in null-foliated spacetimes].
References > s.a. quantum cosmology [measure, third quantization];
  semiclassical quantum gravity; supergravity;
  supersymmetric field theories.
  @ General: Wheeler 62;
    Baierlein et al PR(62);
    Fletcher in(62);
    Marzke & Wheeler in(64);
    Wheeler in(64);
    DeWitt PR(67);
    Wheeler  in(68);
    Wheeler 68;
    Brill & Gowdy RPP(70);
    DeWitt in(70);
    Fischer in(70);
    Misner in(72);
    Christodoulou & Francaviglia AAST(76);
    Shestakova a0801-proc,
    MG12(12)-a0911 [problems and approaches to their solution];
    Kiefer GRG(09)-a0812 [overview];
    Shestakova G&C(19)-a1912 [and gauge invariance].
  @ Operator ordering:
    Hawking & Page NPB(86);
    Kontoleon & Wiltshire PRD(99)gq/98;
    Hall GRG(05)gq/04-in [from "exact uncertainty"];
    Huang et al EPJC(16)-a1505 [and the existence of a classical universe].
  @ And time evolution:
    Kheyfets & Miller gq/94,
    IJMPA(00);
    Cosgrove CQG(96)gq/95 [time slicings and consistency];
    Gil-Medrano JMP(96);
    Gentle et al IJMPA(04)gq/03,
    George et al gq/03-proc [constraints and true degrees of freedom];
    Ita et al PTEP(15)-a1501 [with intrinsic time].
  @ Relationships: Kubota et al PLB(04) [Wheeler-DeWitt and AdS-cft];
    Gielen Sigma(11)-a1111 [and connection dynamics].
  @ WKB approximation: Gerlach PR(69); Horiguchi NCB(96).
  @ Related topics: Parentani NPB(97)gq/96 [and Green functions for matter fields];
    Carroll gq/05
      [uncertainties and statistical geometrodynamics];
    Nelson & Sakellariadou PLB(08)-a0709 [quantum corrections and effective matter];
    Pedram & Jalalzadeh PRD(08) [signature change with fluids]].
  @ Generalizations: Shestakova G&C(99)gq/00,
    G&C(05) [extended phase space],
    G&C(00)gq [and cosmological constant],
    in(10)-a0810;
    Belinchón IJMPD(02)gq/01 [varying constants];
    Brännlund et al CQG(14)-a1312 [topology and volume effects];
    Faizal IJMPA(14)-a1406,
    IJMPA(15)-a1503 [deformed canonical commutation relations];
    Anderson a1412 [space of spaces].
    Based on modified gravity:
    see phenomenology [with non-linear correction]; lattice gravity
    and regge calculus [discrete versions]; modified approaches
    [scalar-tensor].
 Based on modified gravity:
    see phenomenology [with non-linear correction]; lattice gravity
    and regge calculus [discrete versions]; modified approaches
    [scalar-tensor].
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