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dc.contributor.authorPandey, Biswajit-
dc.date.accessioned2021-05-26T11:40:42Z-
dc.date.available2021-05-26T11:40:42Z-
dc.date.issued2019-03-
dc.identifier.urihttps://vbudspace.lsdiscovery.in/xmlui/handle/123456789/57-
dc.description.abstractWe propose an alternative physical mechanism to explain the observed accelerated expansion of the Universe based on the configuration entropy of the cosmic web and its evolution. We show that the sheets, filaments, and clusters in the cosmic web act as sinks whereas the voids act as the sources of information. The differential entropy of the cosmic velocity field increases with time and also acts as a source of entropy. The growth of non-linear structures and the emergence of the cosmic web may lead to a situation where the overall dissipation rate of information at the sinks is about to dominate the generation rate of information from the sources. Consequently, the Universe either requires a dispersal of the overdense non-linear structures or an accelerated expansion of the underdense voids to prevent a violation of the second law of thermodynamics. The dispersal of the sheets, filaments, and clusters is not a viable option due to the attractive nature of gravity but the repulsive and outward peculiar gravitational acceleration at the voids makes it easier to stretch them at an accelerated rate. We argue that this accelerated expansion of the voids inside the cosmic web may mimic the behaviour of dark energyen_US
dc.language.isoenen_US
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
dc.relation.ispartofseriesMNRASL 485, L73–L77 (2019);-
dc.subjectmethods: analytical – cosmology: dark energy – cosmology: theory – large-scale structure of Universeen_US
dc.titleConfiguration entropy of the cosmic web: can voids mimic the dark energy?en_US
dc.title.alternativeRoyal Astronomical Societyen_US
dc.typeArticleen_US
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