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Photons from dark photon solitons via parametric resonance

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arxiv 2301.11470 v2 pith:XSGHJUOS submitted 2023-01-27 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords darkphotonssolitonsvectorradiationelectromagneticparametricpolarization
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Wave-like dark matter made of spin-1 particles (dark photons) is expected to form ground state clumps called "vector solitons", which can have different polarizations. In this work, we consider the interaction of dark photons with photons, expressed as dimension-6 operators, and study the electromagnetic radiation that arises from an isolated vector soliton due to parametric resonant amplification of the ambient electromagnetic field. We characterize the directional dependence and polarization of the outgoing radiation, which depends on the operator as well as the polarization state of the underlying vector soliton. We discuss the implications of this radiation for the stability of solitons and as a possible channel for detecting mergers of vector solitons through astrophysical observations.

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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. 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%.

  2. Ultralight fuzzy dark matter review

    astro-ph.CO 2025-07 unverdicted novelty 1.0 of 10

    A review of fuzzy dark matter that surveys the models, wave phenomenology, numerical methods, and current observational mass constraints of ultralight dark matter.

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