| dc.contributor.author | Strominger, Andrew | |
| dc.contributor.author | Vafa, Cumrun | |
| dc.date.accessioned | 2019-09-22T18:34:25Z | |
| dc.date.issued | 1996 | |
| dc.identifier.citation | Strominger, Andrew, and Cumrun Vafa. 1996. “Microscopic Origin of the Bekenstein-Hawking Entropy.” Physics Letters B 379 (1–4): 99–104. https://doi.org/10.1016/0370-2693(96)00345-0. | |
| dc.identifier.issn | 0370-2693 | |
| dc.identifier.issn | 1873-2445 | |
| dc.identifier.uri | http://nrs.harvard.edu/urn-3:HUL.InstRepos:41385003 | * |
| dc.description.abstract | The Bekenstein-Hawking area-entropy relation S-BH = A/4 is derived for a class of five-dimensional extremal black holes in string theory by counting the degeneracy of BPS soliton bound states. | |
| dc.language.iso | en_US | |
| dc.publisher | Elsevier | |
| dash.license | LAA | |
| dc.title | Microscopic origin of the Bekenstein-Hawking entropy | |
| dc.type | Journal Article | |
| dc.description.version | Accepted Manuscript | |
| dc.relation.journal | Physics Letters, B | |
| dash.depositing.author | Vafa, C.::4e237a95963132b39101a21b3da5ddb2::600 | |
| dc.date.available | 2019-09-22T18:34:25Z | |
| dash.workflow.comments | 1Science Serial ID 79201 | |
| dc.identifier.doi | 10.1016/0370-2693(96)00345-0 | |
| dash.source.volume | 379;43104 | |
| dash.source.page | 99-104 | |
