PARTICLE SPECTRUM OF THE REISSNER–NORDSTRÖM BLACK HOLE

Good, Michael R. R.; Ong, Yen Chin

PARTICLE SPECTRUM OF THE REISSNER–NORDSTRÖM BLACK HOLE

dc.contributor.author	Good, Michael R. R.
dc.contributor.author	Ong, Yen Chin
dc.date.accessioned	2021-01-27T03:27:06Z
dc.date.available	2021-01-27T03:27:06Z
dc.date.issued	2020-12-21
dc.description.abstract	The Reissner–Nordström black hole – moving mirror correspondence is solved. The beta coefficients reveal that charge makes a black hole radiate fewer particles (neutral massless scalars) per frequency. An old Reissner–Nordström black hole emits particles in an explicit Planck distribution with temperature corresponding to the surface gravity of its outer horizon.	en_US
dc.identifier.citation	Good, M. R. R., & Ong, Y. C. (2020). Particle spectrum of the Reissner–Nordström black hole. The European Physical Journal C, 80(12). https://doi.org/10.1140/epjc/s10052-020-08761-7	en_US
dc.identifier.issn	1434-6052
dc.identifier.uri	https://link.springer.com/article/10.1140/epjc/s10052-020-08761-7
dc.identifier.uri	https://doi.org/10.1140/epjc/s10052-020-08761-7
dc.identifier.uri	http://nur.nu.edu.kz/handle/123456789/5244
dc.language.iso	en	en_US
dc.publisher	SpringerOpen	en_US
dc.relation.ispartofseries	European Physical Journal C;80, Article number: 1169 (2020)
dc.rights	Attribution-NonCommercial-ShareAlike 3.0 United States	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-sa/3.0/us/	*
dc.subject	spectrum of the collapsing star	en_US
dc.subject	black hole	en_US
dc.subject	Schwarzschild limit	en_US
dc.subject	gravity	en_US
dc.subject	Research Subject Categories::NATURAL SCIENCES::Physics	en_US
dc.title	PARTICLE SPECTRUM OF THE REISSNER–NORDSTRÖM BLACK HOLE	en_US
dc.type	Article	en_US
workflow.import.source	science