pith. sign in

Can topological defects be formed during preheating ?

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

1 Pith paper citing it
abstract

We study the dynamics of a scalar field \Phi with the potential g(|\Phi|^2-\eta^2)^2/2 (g=self-coupling constant, \eta=symmetry breaking scale) after inflation and make clear whether topological defects can ever be formed during preheating. In particular, we pay attention to GUT defects (\eta \sim 10^{15}GeV - 10^{17}GeV), and consider three types of fluctuations. The first one is produced due to parametric resonance, the second is due to the negative curvature of the potential, and the last is created during inflation. We search for the parameter region that nonthermal fluctuations of the scalar field produced through the parametric resonant decay of its homogeneous part do not lead to defect formation. We find that this region is rather wide, and the GUT defects are not produced after inflation. This fact shows that the positiveness of the effective mass square of the field and production of large fluctuations whose amplitude is as large as that of homogeneous mode are not enough conditions for full symmetry restoration.

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.

citing papers explorer

Showing 1 of 1 citing paper.

  • Dark Matter Freeze-in from a $Z^\prime$ Reheaton hep-ph · 2025-11-04 · unverdicted · none · ref 50 · 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.