Quantum Vacuum Instability Near Rotating Stars
arXiv:gr-qc/9212004 · doi:10.1103/PhysRevD.47.1557
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.
17 Pages, (accepted by PRD), (previously incorrect header files have been corrected)