Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2336
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dc.contributor.authorBorde, A-
dc.date.accessioned2008-05-22T06:14:06Z-
dc.date.available2008-05-22T06:14:06Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 4, pp. 571 - 577en
dc.identifier.urihttp://hdl.handle.net/2248/2336-
dc.description.abstractIt is often stated that topology change is impossible in classical general relativity. In particular, it appears to be widely believed that the pleasure of topology change comes at a fixed price: topology – changing space times must be singular. This perception is wrong. I discuss here both the kinematics and the dynamics of topology change, in order to clarify what precisely the obstacles are, and (with luck) to dispel a few of the more widespread misconceptions about this process. Some of the work presented here extends the work of Geroch and Tipler to a wider class of spacetimes, and some of it offers novelties – such as an explicit example of non-singular 2-dimensional topology change that have been claimed in the literature to be impossibleen
dc.format.extent559783 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25..571Ben
dc.subjectTopologyen
dc.subjectKinematicsen
dc.subjectDynamicsen
dc.titleHow impossible is topology change?en
dc.typeArticleen
Appears in Collections:BASI Publications

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