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Gravity-gauge Anomaly Constraints on the Energy-momentum Tensor

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arxiv 2312.13222 v2 pith:SDBZV7QI submitted 2023-12-20 hep-th gr-qchep-ph

classification hep-thgr-qchep-ph
keywords constraintssymmetryanomaliesanomalybreakingdimensionalenergy-momentumexplicit
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We derive constraints on the four dimensional energy-momentum tensor from gravitational and gauge anomalies. Our work can be considered an extension of Duff's analysis [1] to include parity-odd terms and explicit symmetry breaking. The constraints imply the absence of the parity-odd $R\tilde R$ and $F\tilde F$ terms, for theories whose symmetries are compatible with dimensional regularisation, in a model-independent way. Remarkably, even in the case of explicit symmetry breaking the $\Box R$-anomaly is found to be finite and unambiguous after applying the symmetry constraints. We compute mixed gravity-gauge anomalies at leading order and deduce phenomenological consequences for vector bosons associated with global chiral symmetries.

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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. Effective scalaron--photon interaction in $f(R)$ gravity

    hep-th 2026-06 unverdicted novelty 7.0 of 10

    In the Jordan-frame treatment of f(R) gravity the scalaron-photon effective coupling vanishes for m much less than loop-particle masses because the classical-trace diagrams cancel the Fujikawa anomaly term.

  2. Interactions of the scalaron dark matter in $f (R)$ gravity

    astro-ph.CO 2025-05 conditional novelty 5.0 of 10

    For scalaron dark matter in f(R) gravity, the two-photon decay rate is confirmed at one loop, the resulting extragalactic background spectrum is derived, and the thermal scalaron abundance is shown to be negligible.

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