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arXiv · gr-qc/9212004

Quantum Vacuum Instability Near Rotating Stars

A L Matacz·A C Ottewill·P C W Davies
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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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A L Matacz, A C Ottewill, P C W Davies. 1992-12-08. Quantum Vacuum Instability Near Rotating Stars. https://doi.org/10.1103/physrevd.47.1557

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