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Hamiltonian dynamics of linearly polarized Gowdy models coupled to massless scalar fields

J Fernando Barbero G1, Daniel Gómez Vergel2 and Eduardo J S Villaseñor3,4

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The purpose of this paper is to analyze in detail the Hamiltonian formulation for the compact Gowdy models coupled to massless scalar fields as a necessary first step toward their quantization. We will pay special attention to the coupling of matter and those features that arise for the {\bb S}^1\times{\bb S}^2 and {\bb S}^3 topologies that are not present in the well-studied {\bb T}^3 case—in particular the polar constraints that come from the regularity conditions on the metric. As a byproduct of our analysis we will get an alternative understanding, within the Hamiltonian framework, of the appearance of initial and final singularities for these models.


PACS

04.20.Fy Canonical formalism, Lagrangians, and variational principles

04.20.Dw Singularities and cosmic censorship

04.60.-m Quantum gravity

MSC

70S05 Lagrangian formalism and Hamiltonian formalism

83C20 Classes of solutions; algebraically special solutions, metrics with symmetries

83C75 Space-time singularities, cosmic censorship, etc.

83C05 Einstein's equations (general structure, canonical formalism, Cauchy problems)

Subjects

Gravitation and cosmology

Dates

Issue 23 (7 December 2007)

Received 23 July 2007, in final form 17 October 2007

Published 21 November 2007



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