Dirac equation in Kasner spacetime with local rotational symmetry

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3233

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DC Field	Value	Language
dc.contributor.author	Iyer, B.R.	-
dc.date.accessioned	2007-07-09T11:18:17Z	-
dc.date.available	2007-07-09T11:18:17Z	-
dc.date.issued	1985-11	-
dc.identifier.citation	Physics Letters A, 1985, Vol.112, p313-315	en
dc.identifier.issn	0375-9601	-
dc.identifier.uri	http://hdl.handle.net/2289/3233	-
dc.description	Restricted Access.	en
dc.description.abstract	The particular Kasner spacetime in which exact solutions for the Dirac equation were presented by Shishkin and Andrushkevich is known to be Minkowski spacetime in Rindler-like coordinates. We obtain decoupled equations for the Dirac equation in Kasner spacetime with local rotational symmetry and show that these in general are much more complicated.	en
dc.format.extent	125923 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Elsevier B.V.	en
dc.relation.uri	http://dx.doi.org/10.1016/0375-9601(85)90348-2	en
dc.rights	1985 Elsevier B.V.	en
dc.title	Dirac equation in Kasner spacetime with local rotational symmetry	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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