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Runaway Gravitational Production of Dark Photons

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arxiv 2403.15536 v1 pith:AVPCRNIX submitted 2024-03-22 hep-th astro-ph.COgr-qchep-ph

classification hep-thastro-ph.COgr-qchep-ph
keywords runawayproductiongravitationalnonminimalparticlethereabeliancompletion
verification ladder T0 review T1 audit T2 compute T3 formal

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We demonstrate that gravitational particle production (GPP) of a massive, Abelian, vector (Proca) field during inflation in the presence of nonminimal coupling to gravity may suffer from an instability which leads to runaway production of high-momentum modes. This is untenable unless there is some mechanism to regulate the runaway. We discuss the parameter space of the particle mass and nonminimal couplings where such a runaway occurs and possible ways to tame the runaway. We find that there is no obvious way to resolve the runaway in a UV completion or with kinetic mixing to the standard model.

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Forward citations

Cited by 5 Pith papers

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

  1. The effects of non Bunch-Davies initial conditions on gravitationally produced relics

    gr-qc 2026-03 conditional novelty 6.0 of 10

    Non-Bunch–Davies initial conditions can drastically change gravitationally produced vector dark matter abundances, opening a wider viable mass range.

  2. Constraining Dark Photon Dark Matter with Radio Silence from Soliton Mergers around Supermassive Black Holes

    hep-ph 2025-09 conditional novelty 6.0 of 10

    Non-observation of radio bursts from soliton mergers around supermassive black holes constrains dark photon solitons to make up less than about 1% of dark matter, with future surveys reaching 0.2%.

  3. Superheavy Dark Matter from the String Theory Axiverse

    hep-th 2025-04 conditional novelty 6.0 of 10

    Heavy axions from a simple string-theory compactification can be produced in large numbers by gravitational particle production at the end of inflation and can account for all dark matter, provided they remain stable ...

  4. A self-consistent Higgs-portal framework for dark matter--admixed neutron stars: Collider-motivated benchmarks meet multimessenger constraints

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    Adding heavy dark matter to neutron stars via nχ=FχnB softens the equation of state and lowers the maximum mass, but the vector interaction invoked is numerically negligible.

  5. Aspects of massive gauge fields

    hep-th 2025-05 conditional novelty 3.0 of 10

    A proceedings summary arguing that the massless limit of massive Yang-Mills is smooth via a Vainshtein-like mechanism, and that self-interactions make Proca and Kalb-Ramond strong-coupling behaviors differ, questionin...

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