| dc.contributor.author | Sermutlu, E. | en_US |
| dc.date.accessioned | 2016-02-08T10:45:02Z | |
| dc.date.available | 2016-02-08T10:45:02Z | |
| dc.date.issued | 1998 | en_US |
| dc.identifier.issn | 0264-9381 | |
| dc.identifier.uri | http://hdl.handle.net/11693/25454 | |
| dc.description.abstract | We 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.iso | English | en_US |
| dc.source.title | Classical and Quantum Gravity | en_US |
| dc.relation.isversionof | http://dx.doi.org/10.1088/0264-9381/15/6/004 | en_US |
| dc.title | The first law of black-hole thermodynamics for black holes in string theory | en_US |
| dc.type | Article | en_US |
| dc.department | Department of Mathematics | |
| dc.citation.spage | 1449 | en_US |
| dc.citation.epage | 1461 | en_US |
| dc.citation.volumeNumber | 15 | en_US |
| dc.citation.issueNumber | 6 | en_US |
| dc.identifier.doi | 10.1088/0264-9381/15/6/004 | en_US |
