Evolution of thick domain walls in de Sitter universe

preprint2016arXivOpen access

Abstract

We consider thick domain walls in a de Sitter universe following paper by Basu and Vilenkin. However, we are interested not only in stationary solutions found therein, but also investigate the general case of domain wall evolution with time. When the wall thickness parameter, δ0δ_0, is smaller than H−1/2H^{-1}/\sqrt{2}, where HH is the Hubble parameter in de Sitter space-time, then the stationary solutions exist, and initial field configurations tend with time to the stationary ones. However, there are no stationary solutions for δ0≥H−1/2δ_0 \geq H^{-1}/\sqrt{2}. We have calculated numerically the rate of the wall expansion in this case and have found that the width of the wall grows exponentially fast for δ0≫H−1δ_0 \gg H^{-1}. An explanation for the critical value δ0c=H−1/2δ_{0c} = H^{-1}/\sqrt{2} is also proposed.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.