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Preprint . 1992
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Quantum vacuum instability near rotating stars

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 15 Feb 1993Embargo end date: 01 Jan 1992 English Publisher:American Physical Society (APS)Journal:Physical Review D, volume 47, pages 1,557-1,562 (issn: 0556-2821, Copyright policy )
Authors: Matacz, A L; Ottewill, A C; Davies, P C W;

doi: 10.1103/physrevd.47.1557 , 10.48550/arxiv.gr-qc/9212004

pmid: 10015732

arXiv: gr-qc/9212004

Quantum vacuum instability near rotating stars

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)

Related Organizations
Keywords

FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), General Relativity and Quantum Cosmology

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    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 33
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    		 Top 10%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Top 10%
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    		 Average
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
33
Top 10%
Top 10%
Average
Green