2022MNRAS.511L..82Y


Query : 2022MNRAS.511L..82Y

2022MNRAS.511L..82Y - Mon. Not. R. Astron. Soc., 511, L82-L86 (2022/March-3)

Surface tension of cosmic voids as a possible source for dark energy.

YUSOFI E., KHANPOUR M., KHANPOUR B., RAMZANPOUR M.A. and MOHSENZADEH M.

Abstract (from CDS):

The cosmological constant is estimated by considering the surface tension of supervoids in a void-dominated cosmic fluid by which we can get a possible source of dark energy. Looking at voids as bubbles, we define the concept of surface tension which is shown to have an almost constant value for supervoids that are enclosed by superclusters. The surface tensions of voids are computed by dimensional method for galaxies and superclusters with different values for each group. At large scale which vast voids are dominant the positive cosmological constants obtained of order (≃ +10–52 m–2), which are very close to those given by Planck.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): dark energy - large-scale structure of Universe - cosmology: theory

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 Z 526-12 AG? 03 53 02.4589142328 +35 35 22.174136556   14.4       ~ 152 0
3 NAME CAELUM SUPERCL SCG 04 43 -33.5           ~ 8 0
4 NAME Local Supercluster SCG 12 31 +12.4           ~ 566 0
5 NAME CrB Supercluster SCG 15 25 +29.5           ~ 148 0
6 NAME Laniakea Supercluster SCG ~ ~           ~ 61 0

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