Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5442
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dc.contributor.authorSivaram, C-
dc.contributor.authorArun, K-
dc.date.accessioned2011-04-28T10:59:43Z-
dc.date.available2011-04-28T10:59:43Z-
dc.date.issued2011-05-
dc.identifier.citationAstrophysics and Space Science, Vol. 333, No. 1, pp. 9-10en
dc.identifier.urihttp://hdl.handle.net/2248/5442-
dc.descriptionRestricted Accessen
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractIn 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.isoenen
dc.publisherSpringeren
dc.relation.urihttp://dx.doi.org/10.1007/s10509-011-0670-5en
dc.rights© Springeren
dc.subjectPre-big bang phaseen
dc.subjectEarly universeen
dc.subjectKlein-Kaluza tower of statesen
dc.titleEnigmatic aspects of the early universe: possibility of a `pre-big bang phase'!en
dc.typeArticleen
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