Abstract
We analyze the accretion of phantom energy by primordial black holes along with radiation accretion and Hawking evaporation to determine their course of evolution throughout the history of the universe. We find a well‐defined transition in accretion regimes during the matter‐dominated era and investigate the competition between Hawking evaporation and phantom energy accretion as two processes that decrease the black hole mass. The final stages of black hole evaporation are greatly affected by these effects, and suggest a detailed thermodynamical analysis of the phantom fluid itself.
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.
