Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 김성원 | * |
dc.date.accessioned | 2017-01-05T02:01:23Z | - |
dc.date.available | 2017-01-05T02:01:23Z | - |
dc.date.issued | 2003 | * |
dc.identifier.issn | 0556-2821 | * |
dc.identifier.other | OAK-1426 | * |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/233736 | - |
dc.description.abstract | The condition R = 0, where R is the four-dimensional scalar curvature, is used for obtaining a large class (with an arbitrary function of r) of static, spherically symmetric Lorentzian wormhole solutions. The worm-holes are globally regular and traversable, can have throats of arbitrary size and can be both symmetric and asymmetric. These solutions may be treated as possible wormhole solutions in a brane world since they satisfy the vacuum Einstein equations on the brane where effective stress-energy is induced by interaction with the bulk gravitational field. Some particular examples are discussed. © 2003 The American Physical Society. | * |
dc.language | English | * |
dc.title | Possible wormholes in a brane world | * |
dc.type | Article | * |
dc.relation.issue | 6 | * |
dc.relation.volume | 67 | * |
dc.relation.index | SCOPUS | * |
dc.relation.journaltitle | Physical Review D | * |
dc.identifier.doi | 10.1103/PhysRevD.67.064027 | * |
dc.identifier.wosid | WOS:000182105200056 | * |
dc.identifier.scopusid | 2-s2.0-0038746719 | * |
dc.author.google | Bronnikov K.A. | * |
dc.author.google | Kim S.-W. | * |
dc.contributor.scopusid | 김성원(55862533800;57194851458) | * |
dc.date.modifydate | 20240601081000 | * |