1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7193
Full metadata record
DC FieldValueLanguage
dc.contributor.authorArun, K-
dc.contributor.authorGudennavar, S. B-
dc.contributor.authorPrasad, A-
dc.contributor.authorSivaram, C-
dc.date.accessioned2020-11-17T14:42:43Z-
dc.date.available2020-11-17T14:42:43Z-
dc.date.issued2018-01-
dc.identifier.citationAdvances in Space Research, Vol. 61, No. 1, pp. 567-570en_US
dc.identifier.issn0273-1177-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7193-
dc.descriptionRestricted Access © Elsevier B.V. https://doi.org/10.1016/j.asr.2017.08.006en_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. 2017 COSPAR. Published by Elsevier Ltd. All rights reserved.en_US
dc.language.isoenen_US
dc.publisherElsevier B.Ven_US
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

Files in This Item:
File Description SizeFormat 
Alternate Models to Dark Energy.pdf
  Restricted Access		Restricted Access377.75 kBAdobe PDFView/Open Request a copy
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.