Kerr-Newman Black Holes and Negative Temperatures ()
ABSTRACT
The application of the Unruh procedure to the Rindler approximation of the Kerr-Newman metric in the neighborhood of the event and Cauchy horizons leads, unambiguously, to the well-known positive Hawking (black hole) temperature at the outer horizon, but to a negative (white hole) temperature at the inner horizon. Some consequences for the heat capacities and the status of the third law of thermodynamics are also discussed.
Share and Cite:
Socolovsky, M. (2022) Kerr-Newman Black Holes and Negative Temperatures.
Journal of High Energy Physics, Gravitation and Cosmology,
8, 940-947. doi:
10.4236/jhepgc.2022.84065.
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