Parametrized Theories  

In General > s.a. symplectic structures; time.
* Idea: Theories with time as a dynamical variable; t is a function of and the theory is invariant under '().
* Hamiltonian formulation: We need to introduce Lagrange multipliers to get a Hamiltonian formulation; These theories have as a common feature that H is a constraint, and vanishes (on shell); The reduced phase space gives the space of histories.
@ General references: Hájícek pr(87), PRD(88), JMP(89); Hájícek NPPS(97)gq/96 [time evolution and observables]; Fulop et al IJTP(99) [reparametrization as gauge]; Muslih IJMMS(02)mp/01 [Lagrangian and Hamiltonian]; Albrecht & Iglesias PRD(08)-a0708 [clock ambiguity]; Castrillón et al JPA(08) [parametrization method with a background metric].
@ Relational theories: Anderson CQG(08)-a0706 [foundations]; Gryb CQG(09)-a0810.

Barbour-Bertotti Models > s.a. mach's principle.
* Idea: A relational class of models, with action of the type

S = [–V(x) i mi (dxi/dt)2]1/2 d .

@ General references: Barbour Nat(74)may, NCB(75); Barbour & Bertotti NCB(77), PRS(82); in Smolin pr(88); Gergely CQG(00)gq, & McKain CQG(00)gq; Pooley & Brown BJPS(02) [relationalist implications].
@ Quantization: Barbour & Smolin pr(88); Rovelli pr(88), in(91) [group quantization]; in Smolin pr(88); Gryb a0804 [and time].

Non-Relativistic Point Particle > s.a. particle models.
* Action: It is of the type

S = (pa dxa/dtN H) d ,

with constraint H = p2/2m + V(x) and N = Lagrange multiplier (= dt/d); Gives a parabolic superhamiltonian.
* Applications: Often used as a test model for proposed solution to the problem of time in quantum gravity.
@ General references: Hartle & Kuchar JMP(84) [path integrals]; Anderson CQG(06)gq/05, CQG(06)gq/05 [relational particle models].
@ Time: Elze & Schipper PRD(02)gq [stochastic]; Gambini et al in(03)gq [from discrete formulation].

Free Relativistic Point Particle > s.a. particle models.
* Action: One possible form is of the type

S = (pa dxa/dtN H) d ,   with constraint   H = (p2+m2)/2m ,

which gives a hyperbolic superhamiltonian; We fix x(1) = x1, x(2) = x2, and vary the trajectory in between; The meaning of the Lagrange multiplier is related to a 1D metric on the world-line.
* Alternative: A Lagrangian invariant under reparametrizations ' = f(), df/d > 0, with f(1) = 1, f(2) = 2 is

L = –m [gab (dxa/dt)(dxb/dt)]1/2 .

@ Invariant time formulation: Fanchi FP(93).
@ Quantum theory: Hartle & Kuchar PRD(86) [path integrals]; Fanchi 93.

Field Theories > s.a. diffeomorphisms [parametrized Maxwell theory]; string theory.
* Minkowski space field theory: The theory can be parametrized by treating the 'embedding variables' which describe the foliation as dynamical variables to be varied in the action, in addition to the scalar field; Yields a parabolic superhamiltonian; > s.a. constrained systems [quantization].
@ Scalar field: Isham & Kuchar AP(85); Kuchar PRD(89) [on a cylinder]; Varadarajan PRD(04) [path-integral quantization], PRD(07) [Dirac quantization, lqg techniques].
@ Gravity: Kuchar in(81); [> s.a. canonical general relativity].

Quantization > s.a. quantization of constrained systems.
@ General references: Hájícek JMP(95)gq/94, et al JMP(95)gq/94 [group quantization]; Ruffini PhD(95)gq/05; Ashworth PRA(98)qp/96 [coherent state]; Muslih NCB(00); De Cicco & Simeone IJMPA(99)gq/01 [path integral]; Savvidou & Anastopoulos CQG(00) [histories]; Montesinos GRG(01) [evolving constants]; > s.a. histories quantum mechanics.
@ H = 0 approach: Wang CQG(03)gq [FRW spacetime + scalar]; Nikolic gq/03.
@ In quantum cosmology: Blyth & Isham PRD(75) [use H1/2].
@ Quantum observables: Marolf CQG(95)gq/94.
@ Parametrized non-relativistic quantum mechanics: Hartle & Kuchar in(84); Hartle CQG(96)gq/95 [time]; Hartle & Marolf PRD(97)gq [decoherent histories]; Lawrie & Epp PRD(96)gq/95 [interpretation]; Colosi a0711 [Pegg-Barnett phase operator formalism].
@ And quantum gravity: Gaioli & García-Álvarez GRG(94)gq/98 [and quantum gravity]; Gambini & Porto PRD(01)gq [generally covariant theories]; Anderson CQG(07)gq/06.


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