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dc.contributor.author Das, Saurya
dc.contributor.author Ramadevi, P.
dc.contributor.author Yajnik, U. A.
dc.contributor.author Sule, A.
dc.date.accessioned 2016-02-16T19:22:45Z
dc.date.available 2016-02-16T19:22:45Z
dc.date.issued 2003
dc.identifier.citation Das, S., Ramadevi, P., Yajnik, U. A., & Sule, A. (2002). Quantum mechanical spectra of charged black holes. Physics Letters B, 565, 201-206. doi:10.1016/S0370-2693(03)00673-7 en_US
dc.identifier.uri https://hdl.handle.net/10133/4415
dc.description Sherpa Romeo green journal. Open access article. Creative Commons Attribution License (CC BY) applies. en_US
dc.description.abstract It has been argued by several authors, using different formalisms, that the quantum mechanical spectrum of black hole horizon area is discrete and uniformly spaced. Recently it was shown that two such approaches, namely the one involving quantization on a reduced phase space, and the algebraic approach of Bekenstein and Gour are equivalent for spherically symmetric, neutral black holes (hep-th/0202076). That is, the observables of one can be mapped to those of the other. Here we extend that analysis to include charged black holes. Once again, we find that the ground state of the black hole is a Planck size remnant. en_US
dc.language.iso en_CA en_US
dc.publisher Elsevier en_US
dc.subject Black holes en_US
dc.subject Quantum mechanical spectra en_US
dc.subject Charged black holes en_US
dc.title Quantum mechanical spectra of charged black holes en_US
dc.type Article en_US
dc.description.peer-review Yes en_US
dc.publisher.institution University of New Brunswick en_US
dc.publisher.institution Indian Institute of Technology Bombay en_US


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