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Covariance in models of loop quantum gravity: Gowdy systems

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arxiv 1507.00679 v1 pith:OWSITNGU submitted 2015-07-02 gr-qc hep-th

classification gr-qchep-th
keywords modelsgowdygravitylooppolarizedquantumsystemsabelianized
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Recent results in the construction of anomaly-free models of loop quantum gravity have shown obstacles when local physical degrees of freedom are present. Here, a set of no-go properties is derived in polarized Gowdy models, raising the question whether these systems can be covariant beyond a background treatment. As a side product, it is shown that normal deformations in classical polarized Gowdy models can be Abelianized.

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Cited by 1 Pith paper

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  1. Lessons for loop quantum gravity from emergent modified gravity

    gr-qc 2024-11 conditional novelty 6.0 of 10

    Emergent modified gravity rules out most proposed loop quantum gravity black-hole models and shows that mu0 and mu-bar holonomy schemes are canonically equivalent, so they are not physically distinct.

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