Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/2181
Full metadata record
DC FieldValueLanguage
dc.contributor.authorJassal, H.K.-
dc.date.accessioned2020-11-25T06:27:43Z-
dc.date.available2020-11-25T06:27:43Z-
dc.date.issued2019-
dc.identifier.citationResonance, 24(3), pp. 273-287.en_US
dc.identifier.other10.1007/s12045-019-0779-3-
dc.identifier.urihttps://link.springer.com/article/10.1007/s12045-019-0779-3-
dc.identifier.urihttp://hdl.handle.net/123456789/2181-
dc.description.abstractObservational data has lead us to believe that the Universe is undergoing an accelerated expansion. This acceleration can only be driven by a component which has a negative pressure, the cosmological constant or other exotic models such as the ‘dark energy’. Understanding the nature of dark energy is the focus of many current studies, and its origin being unknown, these studies are largely focused on model building and constraining its parameters. In this article, we discuss how the accelerated expansion of the Universe is driven by dark energy and how dark energy parameters are constrained by observations.en_US
dc.language.isoenen_US
dc.publisherSpringer Linken_US
dc.subjectAccelerationen_US
dc.subjectUnderstandingen_US
dc.subjectEnergy parametersen_US
dc.titleThe Mystery of Dark Energy and Some Revelationsen_US
dc.typeArticleen_US
Appears in Collections:Research Articles

Files in This Item:
File Description SizeFormat 
Need to add pdf.odt8.63 kBOpenDocument TextView/Open


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