Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7226
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dc.contributor.authorArun, K-
dc.contributor.authorGudennavar, S. B-
dc.contributor.authorPrasad, A-
dc.contributor.authorSivaram, C-
dc.date.accessioned2018-01-12T09:08:17Z-
dc.date.available2018-01-12T09:08:17Z-
dc.date.issued2018-01-01-
dc.identifier.citationAdvances in Space Research, Vol. 61, No. 1, pp. 567-570en_US
dc.identifier.issn0273-1177-
dc.identifier.urihttp://hdl.handle.net/2248/7226-
dc.descriptionRestricted Accessen_US
dc.description.abstractOne of the unresolved questions currently in cosmology is that of the non-linear accelerated expansion of the universe. This has been attributed to the so called Dark Energy (DE). The accelerated expansion of the universe is deduced from measurements of Type Ia supernovae. Here we propose alternate models to account for the Type Ia supernovae measurements without invoking dark energy.en_US
dc.language.isoenen_US
dc.publisherElsevier B.Ven_US
dc.relation.urihttps://doi.org/10.1016/j.asr.2017.08.006-
dc.rights© Elsevier B.V.-
dc.subjectDark energyen_US
dc.subjectDark matteren_US
dc.subjectVarying gravitational constanten_US
dc.subjectVarying proton massen_US
dc.titleAlternate models to dark energyen_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

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