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Conserved charges in Chern-Simons modified theory and memory effects

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arxiv 2112.13049 v3 pith:HPJJJ6XO submitted 2021-12-24 gr-qc hep-phhep-th

classification gr-qchep-phhep-th
keywords chargesmemorychern-simonsconservedfieldformalismmodifiedscalar
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In this work, conserved charges and fluxes at the future null infinity are determined in the asymptotically flat spacetime for Chern-Simons modified gravity. The flux-balance laws are used to constrain the memory effects. For tensor memories, the Penrose's conformal completion method is used to analyze the asymptotic structures and asymptotic symmetries, and then, conserved charges for the Bondi-Metzner-Sachs algebra are constructed with the Wald-Zoupas formalism. These charges take very similar forms to those in Brans-Dicke theory. For the scalar memory, Chern-Simons modified gravity is rewritten in the first-order formalism, and the scalar field is replaced by a 2-form field dual to it. With this dual formalism, the scalar memory is described by the vacuum transition induced by the large gauge transformation of the 2-form field.

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Cited by 3 Pith papers

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

  1. Constraining superluminal Einstein-\AE{}ther gravity through gravitational memory

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    Tensor displacement memory in Einstein-Aether gravity diverges at a critical angle when aether scalar or vector waves travel faster than tensor gravitational waves, motivating a conjecture excluding superluminal Einst...

  2. Gravitational Memory in Generalized Proca Gravity

    gr-qc 2025-08 conditional novelty 6.0 of 10

    The displacement memory formula for Generalized Proca gravity is derived for a massive Lorentz-invariant branch and a massless Lorentz-violating branch, with the dispersive branch requiring a frequency-integrated treatment.

  3. Signatures of asymmetry: Gravitational wave memory and the parity violation

    gr-qc 2025-05 conditional novelty 6.0 of 10

    This paper derives that the integrated cosmological memory of gravitational waves in Chern-Simons gravity yields a polarization-dependent difference that could, for optimistic parameters, be testable by next-generatio...

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