Anisotropic dark energy transit cosmological models with time-dependent ω(t) and redshift-dependent ω(z) EoS parameter

DOI10.1142/S0219887818500196zbMath1387.83134OpenAlexW2754714249MaRDI QIDQ4602868

Dinesh Chandra Maurya

Publication date: 7 February 2018

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0219887818500196

zbMATH Keywords

dark energyvariable deceleration parameteranisotropic modelsaccelerating universeBianchi type-I universeredshift-dependent EoS parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

• Unnamed Item
• Unnamed Item
• Dark energy model in anisotropic Bianchi type-III space-time with variable eos parameter
• Some exact Bianchi type-V perfect fluid cosmological models with heat flow and decaying vacuum energy density \(\Lambda \): expressions for some observable quantities
• Bianchi type-I anisotropic dark energy model with constant deceleration parameter
• Variable equation of state for generalized dark energy model
• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• Bianchi type III models with anisotropic dark energy
• Genesis of dark energy: Dark energy as consequence of release and two-stage tracking of cosmological nuclear energy
• Exact spatially homogeneous cosmologies
• Can modified gravity explain accelerated cosmic expansion?
• Generalized Chaplygin gas model: dark energy -- dark matter unification and CMBR con\-straints
• Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
• Dark energy models with variable equation of state parameter
• A study of angular size-redshift relation for models in which Λ decays as the energy density
• Dark energy models in LRS Bianchi type-II space-time in the new perspective of time-dependent deceleration parameter
• DYNAMICS OF DARK ENERGY
• RECONSTRUCTING DARK ENERGY
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Λ-CDM UNIVERSE: A PHENOMENOLOGICAL APPROACH WITH MANY POSSIBILITIES
• Cosmological parameters from SDSS and WMAP
• Consistent modified gravity: dark energy, acceleration and the absence of cosmic doomsday
• CURVATURE QUINTESSENCE
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Cosmological Imprint of an Energy Component with General Equation of State
• LOCALLY ROTATIONALLY SYMMETRIC BIANCHI TYPE-I COSMOLOGICAL MODEL IN f(T) GRAVITY: FROM EARLY TO DARK ENERGY DOMINATED UNIVERSE
• BIANCHI TYPE-II COSMOLOGICAL MODELS WITH CONSTANT DECELERATION PARAMETER
• THE MINIMAL CURVATURE OF THE UNIVERSE IN MODIFIED GRAVITY AND CONFORMAL ANOMALY RESOLUTION OF THE INSTABILITIES

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