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Gravitational waves from axions annihilation through quantum field theory

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arxiv 2306.12375 v2 pith:XZ3HZCT7 submitted 2023-06-21 hep-ph

classification hep-ph
keywords axionsgravitationalannihilationblackcalculatedecayholekerr
verification ladder T0 review T1 audit T2 compute T3 formal

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We use the scattering method to calculate the gravitational wave from axions annihilation in the axion cloud formed by the superradiance process around the Kerr black hole. We consider axions annihilating to gravitons as a three-body decay process and then calculate the corresponding decay width. In this approach, we can simply obtain the radiation power of gravitational wave and give the analytical approximate result with the spin effects of the Kerr black hole. Our study can also provide a cross-check to the numerical results in the traditional method.

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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. Perturbing Gravitational Atoms: Negative Love, Resonant Tides and Shifted Resonances

    gr-qc 2026-07 accept novelty 7.0 of 10

    Spinning gravitational atoms have negative static Love numbers enhanced by O(10²–10³) over non-spinning clouds, with internal perturbations shifting binary resonances.

  2. Preheating Axions in String Cosmology

    hep-th 2024-11 conditional novelty 6.0 of 10

    Preheating of closed-string axions in fibre inflation can overproduce dark matter, yielding new upper bounds on the axion mass and constraints on model parameters.

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