Vanishing of cosmological constant in nonfactorizable geometry

dc.contributor.authorPadmanabhan, T.
dc.contributor.authorShankaranarayanan, S.
dc.date.accessioned2012-03-12T13:31:46Z
dc.date.available2012-03-12T13:31:46Z
dc.date.issued2000-07-20
dc.description.abstractWe generalize the results of Randall and Sundrum to a wider class of four-dimensional space- times including the four-dimensional Schwarzschild background and de Sitter universe. We solve the equation for graviton propagation in a general four dimensional background and find an explicit solution for a zero mass bound state of the graviton. We find that this zero mass bound state is normalizable only if the cosmological constant is strictly zero, thereby providing a dynamical reason for the vanishing of cosmological constant within the context of this model. We also show that the results of Randall and Sundrum can be generalized without any modification to the Schwarzschild background.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1310
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;44/00
dc.subjectCosmological constant:Vanishingen_US
dc.subjectNonfactorizable geometryen_US
dc.titleVanishing of cosmological constant in nonfactorizable geometryen_US
dc.typePreprinten_US

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