5 dark matter and dark energy

V Sahni - The Physics of the Early Universe, 2004 - Springer
I briefly review our current understanding of dark matter and dark energy. The first part of this
review focusses on issues pertaining to dark matter including observational evidence for its …

Observational constraints on dynamical dark energy models

O Avsajanishvili, GY Chitov, T Kahniashvili, S Mandal… - Universe, 2024 - mdpi.com
Scalar field ϕ CDM models provide an alternative to the standard Λ CDM paradigm, while
being physically better motivated. Dynamical scalar field ϕ CDM models are divided into two …

Dark energy

M Li, XD Li, S Wang, Y Wang - Communications in theoretical …, 2011 - iopscience.iop.org
Dark Energy - IOPscience Skip to content IOP Science home Accessibility Help Search all
IOPscience content Search Article Lookup Select journal (required) Volume number: Issue …

Cosmological constant and vacuum energy: old and new ideas

J Sola - Journal of Physics: Conference Series, 2013 - iopscience.iop.org
The cosmological constant (CC) term in Einstein's equations, Λ, was first associated to the
idea of vacuum energy density. Notwithstanding, it is well-known that there is a huge, in fact …

Constraints on holographic dark energy from type Ia supernova observations

X Zhang, FQ Wu - Physical Review D—Particles, Fields, Gravitation, and …, 2005 - APS
In this paper, we use the type Ia supernovae data to constrain the holographic dark energy
model proposed by Li. We also apply a cosmic age test to this analysis. We consider in this …

Dark energy and gravity

T Padmanabhan - General Relativity and Gravitation, 2008 - Springer
I review the problem of dark energy focussing on cosmological constant as the candidate
and discuss what it tells us regarding the nature of gravity. Section 1 briefly overviews the …

[HTML][HTML] On the possible running of the cosmological “constant”

IL Shapiro, J Sola - Physics Letters B, 2009 - Elsevier
Despite the many outstanding cosmological observations leading to a strong evidence for a
non-vanishing cosmological constant (CC) term Λ in the gravitational field equations, the …

Hubble expansion and structure formation in time varying vacuum models

S Basilakos, M Plionis, J Sola - … Review D—Particles, Fields, Gravitation, and …, 2009 - APS
We investigate the properties of the FLRW flat cosmological models in which the vacuum
energy density evolves with time, Λ (t). Using different versions of the Λ (t) model, namely …

[HTML][HTML] Holographic Chaplygin gas model

MR Setare - Physics Letters B, 2007 - Elsevier
Holographic Chaplygin gas model - ScienceDirect Skip to main contentSkip to article
Elsevier logo Journals & Books Help Search My account Sign in View PDF Download full …

Interacting holographic generalized Chaplygin gas model

MR Setare - Physics Letters B, 2007 - Elsevier
In this Letter we consider a correspondence between the holographic dark energy density
and interacting generalized Chaplygin gas energy density in FRW universe. Then we …