English

Dynamics of Totally Constrained Systems II. Quantum Theory

General Relativity and Quantum Cosmology 2010-11-19 v2

Abstract

In this paper a new formulation of quantum dynamics of totally constrained systems is developed, in which physical quantities representing time are included as observables. In this formulation the hamiltonian constraints are imposed on a relative probability amplitude functional Ψ\Psi which determines the relative probability for each state to be observed, instead of on the state vectors as in the conventional Dirac quantization. This leads to a foliation of the state space by linear manifolds on each of which Ψ\Psi is constant, and dynamics is described as linear mappings among acausal subspaces which are transversal to these linear manifolds. This is a quantum analogue of the classical statistical dynamics of totally constrained systems developed in the previous paper. It is shown that if the von Neumann algebra \C\C generated by the constant of motion is of type I, Ψ\Psi can be consistently normalizable on the acausal subspaces on which a factor subalgebra of \C\C is represented irreducibly, and the mappings among these acausal subspaces are conformal. How the formulation works is illustrated by simple totally constrained systems with a single constraint such as the parametrized quantum mechanics, a relativistic free particle in Minkowski and curved spacetimes, and a simple minisuperspace model. It is pointed out that the inner product of the relative probability amplitudes induced from the original Hilbert space picks up a special decomposition of the wave functions to the positive and the negative frequency modes.

Keywords

Cite

@article{arxiv.gr-qc/9507037,
  title  = {Dynamics of Totally Constrained Systems II. Quantum Theory},
  author = {Hideo Kodama},
  journal= {arXiv preprint arXiv:gr-qc/9507037},
  year   = {2010}
}

Comments

57 pages, some unexpected control codes in the original file, which may cause errors for some LaTeX compilers, were removed