Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7338
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dc.contributor.authorRebecca, L-
dc.contributor.authorArun, K-
dc.contributor.authorSivaram, C-
dc.date.accessioned2018-08-08T06:07:43Z-
dc.date.available2018-08-08T06:07:43Z-
dc.date.issued2018-07-
dc.identifier.citationAstrophysics and Space Science, Vol. 363, 149en_US
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/7338-
dc.descriptionRestricted Accessen_US
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractThe requirement that their gravitational binding self-energy density must at least equal the background repulsive dark energy density for large scale cosmic structures implies a mass-radius relation of {M} / {R2} ≈ 1 g/{cm2}, as pointed out earlier. This relation seems to hold true for primeval galaxies as well as those at present epoch. This could set constraints on the nature and evolution of dark energy. Besides, we also set constraints on the size of galaxy clusters and superclusters due to the repulsive cosmological dark energy. This could indicate as to why large scale cosmic structures much larger than ˜200 Mpc are not seen.en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.urihttps://doi.org/10.1007/s10509-018-3371-5-
dc.rights© Springer-
dc.titleDark energy constraints on masses and sizes of large scale cosmic structuresen_US
dc.typeArticleen_US
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