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On the degrees of freedom count on singular phase space submanifolds

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arxiv 2311.10690 v5 pith:TXHNX4CJ submitted 2023-11-17 hep-th gr-qcmath-phmath.MP

classification hep-thgr-qcmath-phmath.MP
keywords aroundgravityphasesingularspacetheretopicwere
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abstract

I discuss singular loci in the phase spaces of theories which lack globally well-defined numbers of dynamical modes. This is a topic which appears quite often in the recent literature on modified gravity. In particular, there were discussions about $R^2$ gravity around Minkowski space. It is a relatively simple case, and still there were some confusions. It clearly shows that one should be very accurate when trying to understand a potentially problematic theory through perturbations around a simply looking background. At the same time, many modern teleparallel approaches are laden with even more severe issues. Therefore, it is a topic which is certainly worth carefully thinking about.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Propagating degrees of freedom on maximally-symmetric backgrounds in $f(R)$ theories of gravity

    gr-qc 2024-12 accept novelty 7.0 of 10

    For all degenerate f(R) models, the linearized spectrum on maximally symmetric backgrounds is empty: no graviton and no scalaron.

  2. Weak Gravity Limit in Newer General Relativity

    gr-qc 2024-12 conditional novelty 6.0 of 10

    In Newer GR, stable tensor and vector sectors force one coefficient combination to its GR value, and the STEGR-plus-gradient-squared model carries 3/2 new dynamical modes, not 1.

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