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Preheating and symmetry restoration in collisions of vacuum bubbles

1 Pith paper cite this work. Polarity classification is still indexing.

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abstract

In first-order inflation a phase transition is completed by the collisions of expanding true-vacuum bubbles. If bubble collisions produce large numbers of soft scalar particles carrying quantum numbers associated with a spontaneously broken symmetry, then symmetry restoration may occur in a ``pre-heating'' phase in a manner similar to symmetry restoration in the pre-heating phase of slow-roll inflation. Since bubble collisions lead to inhomogeneities, there is the possibility of inhomogeneous symmetry restoration where restoration occurs only in the regions of wall collisions.

fields

hep-ph 1

years

2025 1

verdicts

UNVERDICTED 1

representative citing papers

Dark Matter Freeze-in from a $Z^\prime$ Reheaton

hep-ph · 2025-11-04 · unverdicted · novelty 5.0

Dark matter freezes in from non-thermal Z' decays before reheating ends in an inflationary model with a secluded U(1)_D gauge sector, Z' reheaton, and lattice treatment of non-perturbative effects, opening viable parameter space with GW probes.

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  • Dark Matter Freeze-in from a $Z^\prime$ Reheaton hep-ph · 2025-11-04 · unverdicted · none · ref 46 · internal anchor

    Dark matter freezes in from non-thermal Z' decays before reheating ends in an inflationary model with a secluded U(1)_D gauge sector, Z' reheaton, and lattice treatment of non-perturbative effects, opening viable parameter space with GW probes.