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arxiv: astro-ph/9602095 · v1 · submitted 1996-02-19 · 🌌 astro-ph · gr-qc· hep-ph

Preheating and symmetry restoration in collisions of vacuum bubbles

classification 🌌 astro-ph gr-qchep-ph
keywords collisionsrestorationsymmetryphasebubblebubblesinflationnumbers
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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.

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