2022/02/01 by Aref'eva, Irina, Volovich, Igor
#FOS: Physical sciences #High Energy Physics - Theory (hep-th)
paper · doi:10.48550/arxiv.2202.00548
The problem of complete evaporation of Schwarzschild black holes raised by Hawking is that one has an explosion of the temperature T=1/8πM for vanishing black hole mass M. We consider the Reissner-Nordstrom black hole and note that if mass M and charge QM-C M3, C>0 for small M then the complete evaporation of black holes without blow-up of temperature is possible. We describe curves on the surface of state equations such that the motion along them provides complete evaporation. The radiation entropy follows the Page curve and vanishes at the end of evaporation. Similar results for rotating Kerr, Schwarzschild-de-Sitter and Reissner-Nordstrom-(Anti)-de-Sitter black holes are discussed.