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.
Original language | English (US) |
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Pages (from-to) | 1557-1562 |
Number of pages | 6 |
Journal | Physical Review D |
Volume | 47 |
Issue number | 4 |
DOIs | |
State | Published - 1993 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)