English

Dynamical criterion for biased domain-wall formation

High Energy Physics - Phenomenology 2026-06-29 v1 Cosmology and Nongalactic Astrophysics

Abstract

In the presence of a bias term, the conventional condition for forming a domain-wall network is pfv>pc0.31p_{\rm fv}>p_c\simeq 0.31, with pfv/(1pfv)=exp(ΔV(0)/Vb(0))p_{\rm fv}/(1-p_{\rm fv})=\exp(-\Delta V(0)/V_b(0)), where pfvp_{\rm fv} is the false-vacuum fraction immediately after the phase transition, ΔV(0)\Delta V(0) is the zero-temperature energy splitting between the false and true vacua and Vb(0)V_b(0) is the zero-temperature barrier height measured from the true vacuum. This criterion, however, cannot be generally valid, since it is insensitive to the dynamics of the phase transition. In this work, we derive a dynamical criterion for domain wall formation in the presence of a bias term. We evaluate pfvp_{\rm fv} at the freeze-out temperature of the false-vacuum correlation volumes TfoT_{\rm fo}, obtaining a substantially stricter criterion. The same dynamical picture also yields a necessary consistency condition for applying scaling-regime gravitational-wave estimates, Tfo>TannT_{\rm fo}>T_{\rm ann}, where TannT_{\rm ann} is the annihilation temperature inferred from the scaling-regime dynamics.

Cite

@article{arxiv.2606.30094,
  title  = {Dynamical criterion for biased domain-wall formation},
  author = {Wen-Yuan Ai},
  journal= {arXiv preprint arXiv:2606.30094},
  year   = {2026}
}

Comments

12 pages, 2 figures