scholarly journals Effects of shear and rotation on the spherical collapse model for clustering dark energy

2014 ◽  
Vol 445 (1) ◽  
pp. 648-659 ◽  
Author(s):  
Francesco Pace ◽  
Ronaldo C. Batista ◽  
Antonino Del Popolo
Keyword(s):  
Dark Energy ◽  
Spherical Collapse ◽  
Collapse Model

Improvements in the Spherical Collapse Model and Dark Energy Cosmologies

2014 ◽  
Vol 23 (3-4) ◽  
Author(s):  
A. Del Popolo
Keyword(s):  
Shear Stress ◽  
Angular Momentum ◽  
Dark Energy ◽  
Spherical Symmetry ◽  
Linear Density ◽  
Spherical Collapse ◽  
Collapse Model ◽  
Density Threshold ◽  
Stress Influence

AbstractIn the present paper, we study how the effects of deviations from spherical symmetry of a system, produced by angular momentum, and shear stress, influence typical parameters of the spherical collapse model, like the linear density threshold for collapse of the non-relativistic component (

scholarly journals On the implementation of the spherical collapse model for dark energy models

2017 ◽  
Vol 2017 (10) ◽  
pp. 040-040 ◽  
Author(s):  
Francesco Pace ◽  
Sven Meyer ◽  
Matthias Bartelmann
Keyword(s):  
Dark Energy ◽  
Energy Models ◽  
Spherical Collapse ◽  
Collapse Model

THE INFLUENCE OF DARK ENERGY ON THE LARGE SCALE STRUCTURE FORMATION

2010 ◽  
Vol 25 (11n12) ◽  
pp. 874-884 ◽  
Author(s):  
SEOKCHEON LEE
Keyword(s):  
Dark Energy ◽  
Equation Of State ◽  
Structure Formation ◽  
Poisson Distribution ◽  
Large Scale ◽  
Density Perturbation ◽  
Spherical Collapse ◽  
Collapse Model ◽  
Small Scales ◽  
Large Scale Structure Formation

Inhomogeneity at small scales (Mpcs) of our universe is manifest from observations. In regions smaller than 8h-1 Mpc galaxies tend to cluster instead of showing a Poisson distribution. The properties of the spherical collapse model which approximately depicts this nonlinearity of the density perturbation are investigated when there exits dark energy. The evolution of a spherical perturbation depends only on the initial critical overdensity threshold for the collapse, δc and its value approaches to 1.58 instead of the conventionally known 1.69 independent of the value of the equation of state of dark energy.

scholarly journals On the spherical collapse model in dark energy cosmologies

2004 ◽  
Vol 421 (1) ◽  
pp. 71-81 ◽  
Author(s):  
D. F. Mota ◽  
C. van de Bruck
Keyword(s):  
Dark Energy ◽  
Spherical Collapse ◽  
Collapse Model

scholarly journals Spherical collapse model and cluster formation beyond theΛcosmology: Indications for a clustered dark energy?

2009 ◽  
Vol 80 (4) ◽  
Author(s):  
Spyros Basilakos ◽  
Juan Carlos Bueno Sanchez ◽  
Leandros Perivolaropoulos
Keyword(s):  
Dark Energy ◽  
Cluster Formation ◽  
Spherical Collapse ◽  
Collapse Model
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