Cosmological evolution with interaction between dark energy and dark matter

YL Bolotin, A Kostenko, OA Lemets… - International Journal of …, 2015 - World Scientific
In this review we consider in detail different theoretical topics associated with interaction in
the dark sector. We study linear and nonlinear interactions which depend on the dark matter …

Dark energy

M Li, XD Li, S Wang, Y Wang - Communications in theoretical …, 2011 - iopscience.iop.org
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Constraints on the dark side of the universe and observational Hubble parameter data

TJ Zhang, C Ma, T Lan - Advances in Astronomy, 2010 - Wiley Online Library
This paper is a review on the observational Hubble parameter data that have gained
increasing attention in recent years for their illuminating power on the dark side of the …

A unified dark energy model from a vanishing speed of sound with emergent cosmological constant

O Luongo, H Quevedo - International Journal of Modern Physics D, 2014 - World Scientific
The problem of the cosmic acceleration is here revisited by using the fact that the adiabatic
speed of sound can be assumed to be negligible small. Within the context of general …

Testing the phenomenological interacting dark energy with observational H(z) data

S Cao, N Liang, ZH Zhu - Monthly Notices of the Royal …, 2011 - academic.oup.com
In order to test the possible interaction between dark energy and dark matter, we investigate
observational constraints on a phenomenological scenario, in which the ratio between the …

[HTML][HTML] Reconstruction and constraining of the jerk parameter from OHD and SNe Ia observations

ZX Zhai, MJ Zhang, ZS Zhang, XM Liu, TJ Zhang - Physics Letters B, 2013 - Elsevier
Compared with the plentiful researches of the Hubble parameter and deceleration factor, the
third time derivative of the scale factor a (t) in the FRW cosmology, namely, the jerk …

[HTML][HTML] Hubble parameter data constraints on dark energy

Y Chen, B Ratra - Physics Letters B, 2011 - Elsevier
We use Hubble parameter versus redshift data from Stern et al.(2010)[1] and Gaztañaga et
al.(2009)[2] to place constraints on model parameters of constant and time-evolving dark …

Cosmic equation of state from combined angular diameter distances: Does the tension with luminosity distances exist?

S Cao, ZH Zhu - Physical Review D, 2014 - APS
Using relatively complete observational data concerning four angular diameter distance
(ADD) measurements and combined SN+ GRB observations representing current luminosity …

Combined constraints on modified Chaplygin gas model from cosmological observed data: Markov Chain Monte Carlo approach

J Lu, L Xu, Y Wu, M Liu - General Relativity and Gravitation, 2011 - Springer
Abstract We use the Markov Chain Monte Carlo method to investigate a global constraints
on the modified Chaplygin gas (MCG) model as the unification of dark matter and dark …

[图书][B] Dark energy

M Li, X Li, S Wang, Y Wang - 2014 - books.google.com
This book introduces the current state of research on dark energy. It consists of three parts.
The first part is for preliminary knowledge, including general relativity, modern cosmology …