DSpace Repository

Spacetime Continuity and Quantum Information Loss

Show simple item record

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


Files in this item

The following license files are associated with this item:

This item appears in the following Collection(s)

Show simple item record

Attribution-NonCommercial-ShareAlike 3.0 United States Except where otherwise noted, this item's license is described as Attribution-NonCommercial-ShareAlike 3.0 United States

Video Guide

Submission guideSubmission guide

Submit your materials for publication to

NU Repository Drive

Browse

My Account

Statistics