dc.contributor.author |
Borde, A |
|
dc.date.accessioned |
2008-05-22T06:14:06Z |
|
dc.date.available |
2008-05-22T06:14:06Z |
|
dc.date.issued |
1997 |
|
dc.identifier.citation |
BASI, Vol. 25, No. 4, pp. 571 - 577 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2336 |
|
dc.description.abstract |
It 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 impossible |
en |
dc.format.extent |
559783 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1997BASI...25..571B |
en |
dc.subject |
Topology |
en |
dc.subject |
Kinematics |
en |
dc.subject |
Dynamics |
en |
dc.title |
How impossible is topology change? |
en |
dc.type |
Article |
en |