Speaker
Maxim Grigoryev
Description
We are studying the thermodynamic properties of the Kiselev black hole for the equation-of-state parameter $\omega \in (0, 1]$. In this case, the black hole possesses two horizons, and we examine the behavior of the Hawking temperature during the processes of evaporation and accretion of charged particles. We have shown that as the mass of the black hole increases, the temperature does not always decrease but may also slightly increase.
Author
Co-author
Vitalii Vertogradov
(Herzen State Pedagogical University of Russia)
