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dc.contributor.authorSermutlu, E.en_US
dc.date.accessioned2016-02-08T10:45:02Z
dc.date.available2016-02-08T10:45:02Z
dc.date.issued1998en_US
dc.identifier.issn0264-9381
dc.identifier.urihttp://hdl.handle.net/11693/25454
dc.description.abstractWe investigate thermodynamical properties of four- and five-dimensional black-hole solutions of toroidally compactified string theory. We find an explicit expression for the first law of black-hole thermodynamics. We calculate the temperature T, angular velocity Ω and the electromagnetic potentials Φi on the horizon using two different methods.en_US
dc.language.isoEnglishen_US
dc.source.titleClassical and Quantum Gravityen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0264-9381/15/6/004en_US
dc.titleThe first law of black-hole thermodynamics for black holes in string theoryen_US
dc.typeArticleen_US
dc.departmentDepartment of Mathematics
dc.citation.spage1449en_US
dc.citation.epage1461en_US
dc.citation.volumeNumber15en_US
dc.citation.issueNumber6en_US
dc.identifier.doi10.1088/0264-9381/15/6/004en_US


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