Quantum cosmology and the early universe

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dc.contributor.authorNarlikar, J. V.
dc.date.accessioned2012-03-25T11:06:37Z
dc.date.available2012-03-25T11:06:37Z
dc.date.issued1985-11-15
dc.description.abstractThe classical Friedmann cosmology is known to suffer from three major conceptual problems :' (i) spacetime singularity; (ii) particle horizons and (iii) flatness. It is shown that these problems may be resolved during the quantum era of the early universe. Recent attempts in this direction based on the quantization of the conformal degrees of freedom are reviewed here.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1615
dc.language.isoenen_US
dc.publisherItalian Physical Societyen_US
dc.relation.ispartofseriesThe Cosmic Background Radiation and Fundamental Physics (Proceedings of the Third Rome Meeting on Astrophysics). Ed. F. Melchiorri;199p., 1985
dc.subjectQuantumen_US
dc.subjectCosmologyen_US
dc.subjectUniverseen_US
dc.titleQuantum cosmology and the early universeen_US
dc.typeArticleen_US

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