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Bubble wall velocity: heavy physics effects

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arxiv 2010.02590 v3 pith:DKVYU33X submitted 2020-10-06 hep-ph

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

We analyse the dynamics of the relativistic bubble expansion during the first order phase transition focusing on the ultra relativistic velocities $\gamma\gg 1$. We show that fields much heavier than the scale of the phase transition can significantly contribute to the friction and modify the motion of the bubble wall leading to interesting phenomenological consequences. NLO effects on the friction due to the soft vector field emission are reviewed as well.

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Forward citations

Cited by 6 Pith papers

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

  1. Can the universe be matter-dominated after a supercooled first-order phase transition?

    hep-ph 2026-07 conditional novelty 7.0 of 10

    After a supercooled first-order phase transition, the scalar field's equation of state is set by the bubble-wall Lorentz factor γ*, and matter domination is delayed until a/a* ≃ γ* in the free-streaming limit.

  2. Entropy production at electroweak bubble walls from scalar field fluctuations

    hep-ph 2025-07 conditional novelty 7.0 of 10

    Scalar fluctuations produce a nonvanishing entropy discontinuity across an electroweak bubble wall even in the zero-friction limit, showing LTE-based wall velocity upper bounds cannot be saturated.

  3. Particle Production via Rippled Bubble Walls

    hep-ph 2026-07 conditional novelty 6.0 of 10

    A rippled bubble wall produces heavy particles resonantly when the momentum transfer matches the ripple frequency, potentially raising dark-matter abundance by orders of magnitude.

  4. Tunnelling out of Starobinsky inflation: Raising the spectral tilt

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    A first-order phase-transition exit from a displaced Starobinsky branch truncates ~12 e-folds, shifting the spectral tilt from n_s≈0.965 to ≈0.973 at r≈2×10⁻³.

  5. 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.

  6. Mineral Detection of Neutrinos and Dark Matter 2025 Proceedings

    physics.ins-det 2025-08 unverdicted novelty 4.0 of 10

    A workshop proceedings presenting 20 status reports on mineral detectors as passive, long-exposure nuclear recoil detectors for dark matter, neutrinos, and cosmic rays.

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