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PARTICLE SPECTRUM OF THE REISSNER–NORDSTRÖM BLACK HOLE

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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.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.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.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


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