Alternate Models to Dark Energy

dc.contributor.author	Arun, K
dc.contributor.author	Gudennavar, S. B
dc.contributor.author	Prasad, A
dc.contributor.author	Sivaram, C
dc.date.accessioned	2020-11-17T14:42:43Z
dc.date.available	2020-11-17T14:42:43Z
dc.date.issued	2018-01
dc.identifier.citation	Advances in Space Research, Vol. 61, No. 1, pp. 567-570	en_US
dc.identifier.issn	0273-1177
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7193
dc.description	Restricted Access © Elsevier B.V. https://doi.org/10.1016/j.asr.2017.08.006	en_US
dc.description.abstract	One 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.iso	en	en_US
dc.publisher	Elsevier B.V	en_US
dc.subject	Dark energy	en_US
dc.subject	Dark matter	en_US
dc.subject	Varying gravitational constant	en_US
dc.subject	Varying proton mass	en_US
dc.title	Alternate Models to Dark Energy	en_US
dc.type	Article	en_US