Some consequences of quadratic gravity for the early universe

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2513

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.contributor.author	Campanelli, M	-
dc.date.accessioned	2008-06-26T10:48:23Z	-
dc.date.available	2008-06-26T10:48:23Z	-
dc.date.issued	1992-06	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 192, No. 1, pp. 141 - 144	en
dc.identifier.issn	0004-640X (Print) 1572-946X (Online)	-
dc.identifier.uri	http://hdl.handle.net/2248/2513	-
dc.description.abstract	The hypothesis that gravity at very high energies and, hence, around the Planck epoch in the early universe is described by an action quadratic in the curvature, asymptotically free in the coupling is explored. It is shown that the flatness and horizon problems can be resolved in this framework without invoking inflation	en
dc.format.extent	375224 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer Netherlands	en
dc.relation.uri	http://www.springerlink.com/content/r715583k353j7564/	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1992Ap%26SS.192..141S	en
dc.subject	BIG BANG COSMOLOGY	en
dc.subject	GRAVITATION, UNIVERSE	en
dc.subject	ASYMPTOTIC PROPERTIES	en
dc.subject	FLATNESS	en
dc.subject	GRAVITATION THEORY	en
dc.subject	HORIZON	en
dc.title	Some consequences of quadratic gravity for the early universe	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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