Background independent quantizations: the scalar field I
arXiv:gr-qc/0508091 · doi:10.1088/0264-9381/23/9/001
Abstract
We are concerned with the issue of quantization of a scalar field in a diffeomorphism invariant manner. We apply the method used in Loop Quantum Gravity. It relies on the specific choice of scalar field variables referred to as the polymer variables. The quantization, in our formulation, amounts to introducing the `quantum' polymer *-star algebra and looking for positive linear functionals, called states. The assumed in our paper homeomorphism invariance allows to determine a complete class of the states. Except one, all of them are new. In this letter we outline the main steps and conclusions, and present the results: the GNS representations, characterization of those states which lead to essentially self adjoint momentum operators (unbounded), identification of the equivalence classes of the representations as well as of the irreducible ones. The algebra and topology of the problem, the derivation, all the technical details and more are contained in the paper-part II.
13 pages, minor corrections were made in the revised version
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- Polymer quantization of the free scalar field and its classical limit
- The Hole Argument for Covariant Theories
- Effective dynamics of the hybrid quantization of the Gowdy T^3 universe
- Background independent quantizations: the scalar field II
- Towards Loop Quantum Supergravity (LQSG) II. p-Form Sector
- Inflation from non-minimally coupled scalar field in loop quantum cosmology
- Quantum Hamiltonian for gravitational collapse
- Holonomy and inverse-triad corrections in spherical models coupled to matter
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- The Immirzi parameter from an external scalar field
- Singularity resolution from polymer quantum matter
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- Abelian 2+1D Loop Quantum Gravity Coupled to a Scalar Field