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Real-Time History of the Cosmological Electroweak Phase Transition
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We study numerically the real-time history of the cosmological electroweak phase transition, as it may take place in the Standard Model or in MSSM for m_H < m_W according to recent lattice results. We follow the nucleated bubbles from the initial stages of acceleration and rapid growth, through collisions with compression waves resulting in slowing down and reheating to T_c, until the final stages of slow growth and evaporation. We find that collisions with compression waves may make the bubble walls oscillate in the radial direction, and that reheating to T_c takes generically place.
Forward citations
Cited by 2 Pith papers
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Bubble velocities in local equilibrium from a pseudopotential
Terminal bubble-wall velocities in local equilibrium can be found by requiring degenerate minima of a field-only pseudopotential, avoiding scalar equations of motion and profile or equation-of-state assumptions.
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Entropy production at electroweak bubble walls from scalar field fluctuations
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.
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