SOME QUANTUM THERMAL-PROPERTIES OF UNIFORMLY ACCELERATING AND ROTATING BLACK-HOLES

Quantum thermal aspects of a uniformly accelerating and rotating black hole are briefly discussed. The location of event horizons and their corresponding thermal temperatures are given and some special cases of interest are analyzed. We find that a rotating black hole with m(2) = a(2) can be stabilized quantum-mechanically against Hawking radiation by uniform acceleration, i.e., it has no Hawking radiation as seen by asymptotic inertial observers.