Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6859
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dc.contributor.authorSivaram, C-
dc.contributor.authorArun, K-
dc.contributor.authorKiren, O. V-
dc.contributor.authorSivaram, C-
dc.date.accessioned2020-11-11T01:23:07Z-
dc.date.available2020-11-11T01:23:07Z-
dc.date.issued2018-06-
dc.identifier.citationTheoretical Physics, Vol. 3, No. 2, pp. 43-50en_US
dc.identifier.issn2519-9633-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6859-
dc.descriptionOpen Access © Isaac Scientific Publishing Co.; https://doi.org/10.22606/tp.2018.32004en_US
dc.description.abstractIt was little over a hundred years ago that Einstein introduced the ‘cosmological constant’ in his General Theory of Relativity in order to obtain a static universe, to conform to the philosophical view of the universe at that time. What Einstein subsequently dubbed as the ‘biggest blunder’ of his life (after Hubble’s discovery of the expanding universe) has come back in vogue in cosmology. Here we look at the evolution of the concept of the cosmological constant from its inception to it possibly making up close to about 70% of the energy density of the universe.en_US
dc.language.isoenen_US
dc.publisherIsaac Scientific Publishingen_US
dc.subjectGeneral Theory of Relativityen_US
dc.subjectDark energyen_US
dc.subjectCosmological constanten_US
dc.subjectExpanding universeen_US
dc.subjectCosmologyen_US
dc.titleHundred Years of Einstein's Cosmological Constanten_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

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