Covariance in models of loop quantum gravity: Spherical symmetry

Martin Bojowald, Suddhasattwa Brahma, Juan D. Reyes

Research output: Contribution to journalArticle

31 Citations (Scopus)

Abstract

Spherically symmetric models of loop quantum gravity have been studied recently by different methods that aim to deal with structure functions in the usual constraint algebra of gravitational systems. As noticed by Gambini and Pullin, a linear redefinition of the constraints (with phase-space dependent coefficients) can be used to eliminate structure functions, even Abelianizing the more difficult part of the constraint algebra. The Abelianized constraints can then easily be quantized or modified by putative quantum effects. As pointed out here, however, the method does not automatically provide a covariant quantization, defined as an anomaly-free quantum theory with a classical limit in which the usual (off-shell) gauge structure of hypersurface deformations in space-time appears. The holonomy-modified vacuum theory based on Abelianization is covariant in this sense, but matter theories with local degrees of freedom are not. Detailed demonstrations of these statements show complete agreement with results of canonical effective methods applied earlier to the same systems (including signature change).

Original languageEnglish (US)
Article number045043
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume92
Issue number4
DOIs
StatePublished - Aug 31 2015

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gravitation
symmetry
algebra
quantum theory
degrees of freedom
signatures
anomalies
vacuum
coefficients

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Cite this

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Covariance in models of loop quantum gravity : Spherical symmetry. / Bojowald, Martin; Brahma, Suddhasattwa; Reyes, Juan D.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 92, No. 4, 045043, 31.08.2015.

Research output: Contribution to journalArticle

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