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NLO friction in symmetry restoring phase transitions

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arxiv 2405.19447 v1 pith:5ZPAIDJU submitted 2024-05-29 hep-ph astro-ph.COhep-th

classification hep-phastro-ph.COhep-th
keywords phasepressurefrictionsymmetrytransitionswallcaseemission
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abstract

Interactions between bubbles/domain walls and the surrounding medium are a topic of active research, particularly as they apply to friction effects on accelerated expansion during first-order phase transitions. In this paper, we analyze for the first time friction pressure on relativistic walls in phase transitions where gauge symmetry is restored, particularly motivated by the observation that this pressure can, in principle, be negative at leading order, since some particles lose mass by definition as they cross into the new phase. We find, however, that at NLO, the soft emission of vectors from a charged current leads to positive pressure scaling as the wall's Lorentz boost factor $\gamma_w$, similar to the case of gauge symmetry breaking. Contrary to the latter case, we find that the dominant contribution in single emission is safe from IR divergences and exhibits a much stronger dependence on the wall shape. Finally, we argue that in any phase transition, no multi-particle process on the wall can impart negative pressure greater than the leading order result, in the asymptotic limit of large velocity.

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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. Direct Detection of Cosmic Walls with Paleo Detectors

    hep-ph 2025-05 conditional novelty 6.0 of 10

    Ancient minerals could preserve parallel damage tracks left by a passing cosmic wall, enabling a direct search for these rare objects with paleo detectors.

  2. Populating dark sectors with relativistic bubble walls

    hep-ph 2024-12 conditional novelty 3.0 of 10

    Relativistic bubble walls can pair-produce dark matter much heavier than the phase transition scale, which then free-streams as warm dark matter.

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