Cosmic microwave background spectrum and G-varying cosmology

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dc.contributor.authorNarlikar, J. V.
dc.contributor.authorRana, N. C.
dc.date.accessioned2012-03-15T08:36:07Z
dc.date.available2012-03-15T08:36:07Z
dc.date.issued1980-03-19
dc.description.abstractIt is shown that G-varying cosmologies provide a better fit to the observed data on cosmic microwave background, than the standard Friedmann models.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1522
dc.language.isoenen_US
dc.publisherElsevier Science Publishersen_US
dc.relation.ispartofseriesPhysics Letters;A77, No. 4, 1980
dc.subjectCosmic microwaveen_US
dc.subjectCosmologyen_US
dc.subjectG-varyingen_US
dc.titleCosmic microwave background spectrum and G-varying cosmologyen_US
dc.typeArticleen_US

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