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Evolution of evaporating Black Holes in a higher dimensional inflationary universe

dc.contributor.authorMbonye, Manasse R.en_US
dc.date.accessioned2011-11-15T16:02:52Z
dc.date.available2011-11-15T16:02:52Z
dc.date.issued1999-11-19en_US
dc.identifier.citationMbonye, Manasse R. (1999). "Evolution of evaporating Black Holes in a higher dimensional inflationary universe." AIP Conference Proceedings 493(1): 161-166. <http://hdl.handle.net/2027.42/87523>en_US
dc.identifier.otherAPCPCS-493-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87523
dc.description.abstractSpherically symmetric Black Holes of the Vaidya type are examined in an asymptotically de Sitter, higher dimensional spacetime. The various horizons are identified and located. The structure and dynamics of such horizons are studied. © 1999 American Institute of Physics.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleEvolution of evaporating Black Holes in a higher dimensional inflationary universeen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumPhysics Department, University of Michigan, Ann Arbor, Michigan 48109en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87523/2/161_1.pdf
dc.identifier.doi10.1063/1.1301580en_US
dc.identifier.sourceEighth Canadian conference on general relativity and relativistic astrophysicsen_US
dc.owningcollnamePhysics, Department of


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