Ultracompact (R<3 M) objects in general relativity

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2706

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DC Field	Value	Language
dc.contributor.author	Iyer, B.R.	-
dc.contributor.author	Vishveshwara, C.V.	-
dc.contributor.author	Dhurandhar, S.V.	-
dc.date.accessioned	2007-06-11T09:25:39Z	-
dc.date.available	2007-06-11T09:25:39Z	-
dc.date.issued	1985-03	-
dc.identifier.citation	Classical and Quantum Gravity, 1985, Vol.2, p219-228	en
dc.identifier.issn	0264-9381	-
dc.identifier.uri	http://hdl.handle.net/2289/2706	-
dc.description	Restricted Access.	en
dc.description.abstract	The authors investigate the possible existence of ultracompact objects, i.e., configurations with radii less than three times the mass in geometrical units. Within the framework of core envelope models for a comparatively low value of the fiducial (p/ rho c2) at the interface, stable ultracompact objects with causal cores are in fact found to be possible. On the other hand available equations of state valid at higher densities when used throughout the star lead invariably to configurations with radii greater than 3 M. It is also shown that within the framework of core-envelope models stability requirements do not bring down the mass limit.	en
dc.format.extent	481080 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	IOP Publishing Ltd.	en
dc.relation.uri	http://dx.doi.org/10.1088/0264-9381/2/2/013	en
dc.rights	1985 IOP Publishing Ltd.	en
dc.title	Ultracompact (R<3 M) objects in general relativity	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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