Black Hole - Moving Mirror I: An Exact Correspondence

dc.contributor.authorAnderson, Paul R.
dc.contributor.authorGood, Michael R.R.
dc.contributor.authorEvans, Charles R.
dc.contributor.institutionSchool of Sciences and Humanities
dc.date.accessioned2016-01-08T10:27:26Z
dc.date.available2016-01-08T10:27:26Z
dc.date.issued2015
dc.description.abstractAn exact correspondence is shown between a new moving mirror trajectory in (1+1)D and a spacetime in (1+1)D in which a black hole forms from the collapse of a null shell. It is shown that the Bogolubov coe cients between the \in" and \out" states are identical and the exact Bogolubov coe cients are displayed. Generalization to the (3+1)D black hole case is discussed.
dc.identifier.citationAnderson, P. R., Good, M. R., & Evans, C. R. (2018). Black hole—Moving mirror I: An exact correspondence. In The Fourteenth Marcel Grossmann Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories: Proceedings of the MG14 Meeting on General Relativity, University of Rome “La Sapienza”, Italy, 12–18 July 2015 (pp. 1701-1704).
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/1006
dc.language.isoen
dc.subjectphysics
dc.subjectblack holes
dc.titleBlack Hole - Moving Mirror I: An Exact Correspondence
dc.typeArticle

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