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.
| Original language | English |
|---|---|
| Article number | 122 |
| Journal | Universe |
| Volume | 4 |
| Issue number | 11 |
| DOIs | |
| Publication status | Published - Nov 2018 |
Funding
Funding: This work was spported by state-targeted program “Center of Excellence for Fundamental and Applied Physics” (BR05236454) and the ORAU FY2018-SGP-1-STMM Faculty Development Competitive Research at Nazarbayev University (Grant No. 090118FD5350). This work was spported by state-targeted program “Center of Excellence for Fundamental and Applied Physics” (BR05236454) and the ORAU FY2018-SGP-1-STMM Faculty Development Competitive Research at Nazarbayev University (Grant No. 090118FD5350). M.R.R.G. thanks Yen Chin Ong, Aizhan Myrzakul, and Khalykbek Yelshibekov. M.R.R.G. also thanks Daniele Malafarina for clarifying points about the Penrose diagrams. The Ministry of Education and Science of the Republic of Kazakhstan are also acknowledged.
Keywords
- Black hole evaporation
- Information loss
- Remnants
ASJC Scopus subject areas
- General Physics and Astronomy
Fingerprint
Dive into the research topics of 'Spacetime continuity and quantum information loss'. Together they form a unique fingerprint.Cite this
- APA
- Standard
- Harvard
- Vancouver
- Author
- BIBTEX
- RIS