RADIATION FROM AN INERTIAL MIRROR HORIZON
| dc.contributor.author | Good, Michael | |
| dc.contributor.author | Abdikamalov, Ernazar | |
| dc.date.accessioned | 2021-07-01T13:15:56Z | |
| dc.date.available | 2021-07-01T13:15:56Z | |
| dc.date.issued | 2020-08 | |
| dc.description.abstract | The purpose of this study is to investigate radiation from asymptotic zero acceleration motion where a horizon is formed and subsequently detected by an outside witness. A perfectly reflecting moving mirror is used to model such a system and compute the energy and spectrum. The trajectory is asymptotically inertial (zero proper acceleration)—ensuring negative energy flux (NEF), yet approaches light-speed with a null ray horizon at a finite advanced time. We compute the spectrum and energy analytically. | en_US |
| dc.identifier.citation | Good, M., & Abdikamalov, E. (2020). Radiation from an Inertial Mirror Horizon. Universe, 6(9), 131. doi:10.3390/universe6090131 | en_US |
| dc.identifier.issn | 2218-1997 | |
| dc.identifier.uri | http://nur.nu.edu.kz/handle/123456789/5506 | |
| dc.language.iso | en | en_US |
| dc.publisher | Universe | 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 | Type of access: Open Access | en_US |
| dc.subject | acceleration radiation | en_US |
| dc.subject | moving mirrors | en_US |
| dc.subject | QFT in curved spacetime | en_US |
| dc.subject | horizons | en_US |
| dc.subject | dynamical Casimir effect | en_US |
| dc.subject | black holes | en_US |
| dc.subject | Hawking radiation | en_US |
| dc.subject | negative energy flux | en_US |
| dc.title | RADIATION FROM AN INERTIAL MIRROR HORIZON | en_US |
| dc.type | Article | en_US |
| workflow.import.source | science |