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Lower bound on the electroweak wall velocity from hydrodynamic instability

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arxiv 1412.8064 v2 pith:PANHX37T submitted 2014-12-27 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords electroweakdeflagrationsvelocitywallbaryogenesiscriticalextensionsmodel
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The subsonic expansion of bubbles in a strongly first-order electroweak phase transition is a convenient scenario for electroweak baryogenesis. For most extensions of the Standard Model, stationary subsonic solutions (i.e., deflagrations) exist for the propagation of phase transition fronts. However, deflagrations are known to be hydrodynamically unstable for wall velocities below a certain critical value. We calculate this critical velocity for several extensions of the Standard Model and compare with an estimation of the wall velocity. In general, we find a region in parameter space which gives stable deflagrations as well as favorable conditions for electroweak baryogenesis.

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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. Thin and thick bubble walls III: wall energy

    gr-qc 2025-01 conditional novelty 6.0 of 10

    The wall energy-momentum tensor is computed to next-to-next-to-leading order in the wall width, with a decomposition that assigns the potential barrier to the wall.

  2. Detecting gravitational waves from cosmological phase transitions with LISA: an update

    astro-ph.CO 2019-10 unverdicted novelty 4.0 of 10

    Updated LISA detection prospects for gravitational waves from phase transitions are derived from state-of-the-art sound-wave simulations, with a new web tool PTPlot provided for parameter scans.

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