Abstract
We consider theories with late-time phase transitions that lead to the formation of energetically soft domain wall effects. These transitions occur in the vacuum state of a weakly coupled scalar field which is not in thermal equilibrium. The spatial properties and distribution of these domain walls are computed using percolation theory. Assuming spherical collapse of matter, the percolation results are used to accurately predict the richness distribution of Abell clusters.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
