Quantum Vacuum Instability Near Rotating Stars
A L Matacz, A C Ottewill, P C W Davies
Abstract
We discuss the Starobinskii-Unruh process for the Kerr black hole. We show how this effect is related to the theory of squeezed states. We then consider a simple model for a highly relativistic rotating star and show that the Starobinskii-Unruh effect is absent.
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