What can classical gravity tell us about quantum structure of spacetime?

dc.contributor.authorPadmanabhan, T.
dc.date.accessioned2012-03-03T15:01:28Z
dc.date.available2012-03-03T15:01:28Z
dc.date.issued2011-09-12
dc.description.abstractSeveral features of classical gravity, combined with the existence of Davies-Unruh temperature of horizon s, support the following paradigm: Gravitational field equations in a wide class of theories, including Einstein ’s theory, should be viewed as describing the thermodynamic limit of the statistical mechanics of (as yet unknown) atoms of spacetime. I present the conceptual evidence for this emergent paradigm and discuss several facets of this approach.en_US
dc.identifier.urihttp://hdl.handle.net/11007/197
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.relation.ispartofseriesPapers, Lecture notes, Invited Contributions etc. in the arXive;Journal of Physics: Conference Series;Vol. 314, 2011
dc.subjectClassical gravityen_US
dc.subjectQuantum structureen_US
dc.subjectSpacetimeen_US
dc.titleWhat can classical gravity tell us about quantum structure of spacetime?en_US
dc.typeArticleen_US

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