Quantum mechanical spectra of charged black holes

dc.contributor.authorDas, Saurya
dc.contributor.authorRamadevi, P.
dc.contributor.authorYajnik, U. A.
dc.contributor.authorSule, A.
dc.date.accessioned2016-02-16T19:22:45Z
dc.date.available2016-02-16T19:22:45Z
dc.date.issued2003
dc.descriptionSherpa Romeo green journal. Open access article. Creative Commons Attribution License (CC BY) applies.en_US
dc.description.abstractIt 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.description.peer-reviewYesen_US
dc.identifier.citationDas, 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)00673-7en_US
dc.identifier.urihttps://hdl.handle.net/10133/4415
dc.language.isoen_CAen_US
dc.publisherElsevieren_US
dc.publisher.institutionUniversity of New Brunswicken_US
dc.publisher.institutionIndian Institute of Technology Bombayen_US
dc.subjectBlack holesen_US
dc.subjectQuantum mechanical spectraen_US
dc.subjectCharged black holesen_US
dc.titleQuantum mechanical spectra of charged black holesen_US
dc.typeArticleen_US
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