Why does the universe expand?

dc.contributor.authorPadmanabhan, T.
dc.date.accessioned2012-03-03T15:02:18Z
dc.date.available2012-03-03T15:02:18Z
dc.date.issued2010-06-17
dc.description.abstractThe purpose of the paper is fivefold: (a) Argue that the question in the title can be presented in a meaningful manner and that it requires an answer. (b) Discuss the conventional answers and explain why they are unsatisfactory. (c) Suggest that a key ingredient in the answer could be the instability arising due to the ‘wrong’ sign in the Hilbert action for the kinetic energy term corresponding to expansion factor. (d) Describe how this idea connects up with another peculiar feature of our universe, viz. it spontaneously became more and more classical in the course of evolution. (e) Provide a speculative but plausible scenario, based on the thermodynamic per- spective of gravity, in which one has the hope for relating the thermodynamic and cosmological arrows of time.en_US
dc.identifier.urihttp://hdl.handle.net/11007/203
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.ispartofseriesGeneral Relativity and Gravitation;Vol. 42, 2010
dc.subjectCosmological arrow of timeen_US
dc.subjectThermosynamical arrow of timeen_US
dc.subjectHorizon thermodynamicsen_US
dc.subjectEquipartitionen_US
dc.titleWhy does the universe expand?en_US
dc.typeArticleen_US

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