Spacetime Continuity and Quantum Information Loss

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