Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7338
Title: Dark energy constraints on masses and sizes of large scale cosmic structures
Authors: Rebecca, L
Arun, K
Sivaram, C
Issue Date: Jul-2018
Publisher: Springer
Citation: Astrophysics and Space Science, Vol. 363, 149
Abstract: The 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.
Description: Restricted Access
The original publication is available at springerlink.com
URI: http://hdl.handle.net/2248/7338
ISSN: 0004-640X
???metadata.dc.rights???: © Springer
???metadata.dc.relation.uri???: https://doi.org/10.1007/s10509-018-3371-5
Appears in Collections:IIAP Publications

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