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Spacetime Continuity and Quantum Information Loss

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dc.contributor.author Good, Michael R. R.
dc.date.accessioned 2019-04-25T10:06:28Z
dc.date.available 2019-04-25T10:06:28Z
dc.date.issued 2018-11-09
dc.identifier.citation Good, M.R.R. Spacetime Continuity and Quantum Information Loss. Universe 2018, 4, 122. en_US
dc.identifier.uri http://dx.doi.org/10.3390/universe4110122
dc.identifier.uri http://nur.nu.edu.kz/handle/123456789/3854
dc.description.abstract Continuity across the shock wave of two regions in the metric during the formation of a black hole can be relaxed in order to achieve information preservation. A Planck scale sized spacetime discontinuity leads to unitarity (a constant asymptotic entanglement entropy) by restricting the origin of coordinates (moving mirror) to be timelike. Moreover, thermal equilibration occurs and total evaporation energy emitted is finite. en_US
dc.language.iso en en_US
dc.publisher MDPI en_US
dc.rights Attribution-NonCommercial-ShareAlike 3.0 United States *
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/3.0/us/ *
dc.subject black hole evaporation en_US
dc.subject information loss en_US
dc.subject remnants en_US
dc.title Spacetime Continuity and Quantum Information Loss en_US
dc.type Article en_US
workflow.import.source science

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