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Enigmatic aspects of the early universe: possibility of a `pre-big bang phase'!

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dc.contributor.author Sivaram, C
dc.contributor.author Arun, K
dc.date.accessioned 2011-04-28T10:59:43Z
dc.date.available 2011-04-28T10:59:43Z
dc.date.issued 2011-05
dc.identifier.citation Astrophysics and Space Science, Vol. 333, No. 1, pp. 9-10 en
dc.identifier.uri http://hdl.handle.net/2248/5442
dc.description Restricted Access en
dc.description The original publication is available at springerlink.com
dc.description.abstract In this paper it is suggested that inclusion of mutual gravitational interactions among the particles in the early dense universe can lead to a ‘pre-big bang’ scenario, with particle masses greater than the Planck mass implying an accelerating phase of the universe, which then goes into the radiation phase when the masses fall below the Planck mass. The existence of towers of states of such massive particles (i.e. multiples of Planck mass) as implied in various unified theories, provides rapid acceleration in the early universe, similar to the usual inflation scenario, but here the expansion rate goes over ‘smoothly’ to the radiation dominated universe when temperature becomes lower than the Planck temperature. en
dc.language.iso en en
dc.publisher Springer en
dc.relation.uri http://dx.doi.org/10.1007/s10509-011-0670-5 en
dc.rights © Springer en
dc.subject Pre-big bang phase en
dc.subject Early universe en
dc.subject Klein-Kaluza tower of states en
dc.title Enigmatic aspects of the early universe: possibility of a `pre-big bang phase'! en
dc.type Article en


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