Dynamics of dark energy

EJ Copeland, M Sami, S Tsujikawa - International Journal of Modern …, 2006 - World Scientific
We review in detail a number of approaches that have been adopted to try and explain the
remarkable observation of our accelerating universe. In particular we discuss the arguments …

Cosmological constant—the weight of the vacuum

T Padmanabhan - Physics reports, 2003 - Elsevier
Recent cosmological observations suggest the existence of a positive cosmological constant
Λ with the magnitude Λ (Gℏ/c3)≈ 10− 123. This review discusses several aspects of the …

Quintom cosmology: theoretical implications and observations

YF Cai, EN Saridakis, MR Setare, JQ Xia - Physics Reports, 2010 - Elsevier
We review the paradigm of quintom cosmology. This scenario is motivated by the
observational indications that the equation-of-state of dark energy across the cosmological …

Jerk, snap and the cosmological equation of state

M Visser - Classical and Quantum Gravity, 2004 - iopscience.iop.org
Taylor expanding the cosmological equation of state around the current epoch is the
simplest model one can consider that does not make any a priori restrictions on the nature of …

Reconstructing dark energy

V Sahni, A Starobinsky - International Journal of Modern Physics D, 2006 - World Scientific
This review summarizes recent attempts to reconstruct the expansion history of the universe
and to probe the nature of dark energy. Reconstruction methods can be broadly classified …

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 …

WMAP constraints on low redshift evolution of dark energy

HK Jassal, JS Bagla… - Monthly Notices of the …, 2005 - academic.oup.com
The conceptual difficulties associated with a cosmological constant have led to the
investigation of alternative models in which the equation of state parameter, w= p/ρ, of the …

Phenomenological parameterization of quintessence

C Wetterich - Physics Letters B, 2004 - Elsevier
We propose a simple phenomenological parameterization of quintessence with a time-
varying equation of state. In particular, it accounts for the possibility of early dark energy. The …

[HTML][HTML] The reconstruction of constant jerk parameter with f (R, T) gravity

A Pradhan, G Goswami, A Beesham - Journal of High Energy Astrophysics, 2023 - Elsevier
In this work, we have developed an FLRW type model of a universe which displays transition
from deceleration in the past to the acceleration at the present. For this, we have considered …

Observational constraints on low redshift evolution of dark energy:<? format?> How consistent are different observations?

HK Jassal, JS Bagla, T Padmanabhan - Physical Review D—Particles, Fields …, 2005 - APS
The dark energy component of the Universe is often interpreted either in terms of a
cosmological constant or as a scalar field. A generic feature of the scalar field models is that …