Recent cosmological observations have posed a challenge for traditional theories of gravity: what is the force driving the accelerated expansion of the universe? What if dark energy or …
F Pace, JC Waizmann… - Monthly Notices of the …, 2010 - academic.oup.com
We study the spherical collapse model for several dark-energy scenarios using the fully non- linear differential equation for the evolution of the density contrast within homogeneous …
We study the growth of perturbations in an expanding Newtonian universe with Bose- Einstein condensate (BEC) dark matter. We first ignore special relativistic effects and derive …
We review dark energy models that can present non-negligible fluctuations on scales smaller than Hubble radius. Both linear and nonlinear evolutions of dark energy fluctuations …
LR Abramo, RC Batista, L Liberato… - Journal of Cosmology …, 2007 - iopscience.iop.org
We study non-linear structure formation in the presence of dark energy. The influence of dark energy on the growth of large-scale cosmological structures is exerted both through its …
T Harko - Monthly Notices of the Royal Astronomical Society, 2011 - academic.oup.com
We consider the global cosmological evolution and the evolution of the density contrast in the Bose–Einstein condensate dark matter model, in the framework of a post-Newtonian …
PH Chavanis - The European physical journal plus, 2014 - Springer
We construct models of universe with a generalized equation of state p=(αρ+kρ^1+1/n)c^2 having a linear component and a polytropic component. Concerning the linear equation of …
N Komatsu, S Kimura - Physical Review D, 2014 - APS
We study two types of entropic-force models in a homogeneous, isotropic, spatially flat, matter-dominated universe. The first type is a Λ (t) type similar to Λ (t) CDM (varying-lambda …
Oliver Piattella Page 1 UNITEXT for Physics Oliver Piattella Lecture Notes in Cosmology Page 2 UNITEXT for Physics Series editors Paolo Biscari, Dipartimento di Fisica, Politecnico di …