Abstract
Covariant jump conditions across a bubble wall, including surface tension and dissipation, for a nongravitational moving surface have been derived. Special situations, such as those associated with a domain wall, a dust shell, and a spherical boundary, are discussed. In particular, the cosmological QCD phase transition has been examined as a specific application of the general formalism. The possible mechanism of energy transport during the phase transition is studied, and a critical condition for neutrino conduction to dominate over the hydrodynamic flow has been obtained.
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.
