Mirror reflections of a black hole

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dc.contributor.authorGood, Michael R. R.
dc.contributor.authorAnderson, Paul R.
dc.contributor.authorEvans, Charles R.
dc.date.accessioned2017-01-09T04:36:43Z
dc.date.available2017-01-09T04:36:43Z
dc.date.issued2016-09-12
dc.description.abstractAn exact correspondence between a black hole and an accelerating mirror is demonstrated. It is shown that for a massless minimally coupled scalar field, the same Bogolubov coefficients connecting the "in" and "out" states occur for a (1+1)-dimensional flat spacetime with a particular perfectly reflecting accelerating boundary trajectory and a (1+1)-dimensional curved spacetime in which a null shell collapses to form a black hole. Generalization of the latter to the (3+1)-dimensional case is discussed. The spectral dynamics is computed in both (1+1)-dimensional spacetimes along with the energy flux in the spacetime with a mirror. It is shown that the approach to equilibrium is monotonic, asymmetric in terms of the rate, and there is a specific time which characterizes the system when it is the most out of equilibrium.ru_RU
dc.identifier.citationGood, M. R. R., Anderson, P. R., & Evans, C. R. (2016). Mirror reflections of a black hole. Physical Review D - Particles, Fields, Gravitation and Cosmology, 94(6), [065010]. DOI: 10.1103/PhysRevD.94.065010ru_RU
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/2207
dc.language.isoenru_RU
dc.publisherPhysical Review D - Particles, Fields, Gravitation and Cosmologyru_RU
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectblack holeru_RU
dc.subjectmirrorru_RU
dc.subjectspace-timeru_RU
dc.titleMirror reflections of a black holeru_RU
dc.typeArticleru_RU

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