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First-order nonthermal phase transition after preheating

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arxiv hep-ph/9804425 v1 pith:AJJJRQWG submitted 1998-04-28 hep-ph astro-phgr-qchep-th

classification hep-phastro-phgr-qchep-th
keywords phasetransitionfieldfieldsfirst-orderfluctuationsinflatonnonthermal
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

During preheating after inflation, parametric resonance rapidly generates very large fluctuations of scalar fields. In models where the inflaton field $\phi$ oscillates in a double-well potential and interacts with another scalar field $X$, fluctuations of X can keep the \phi to -\phi symmetry temporarily restored. If the coupling of \phi to X is much stronger than the inflaton self-coupling, the subsequent symmetry breaking is a first-order phase transition. We demonstrate the existence of this nonthermal phase transition with lattice simulations of the full nonlinear dynamics of the interacting fields. In particular, we observe nucleation of an expanding bubble.

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

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    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 para...

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