Vector field as a quintessence partner
From MaRDI portal
Publication:3159012
DOI10.1088/0264-9381/21/13/014zbMath1061.83078arXivgr-qc/0402095OpenAlexW2084494415MaRDI QIDQ3159012
Publication date: 1 February 2005
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0402095
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (15)
Inflation and late time acceleration designed by Stueckelberg massive photon ⋮ Bianchi type-III cosmological models with anisotropic dark energy (DE) in lyra geometry ⋮ Kerr–anti-de Sitter/de Sitter black hole in perfect fluid dark matter background ⋮ Scalar–tensor teleparallel gravity with boundary term by Noether symmetries ⋮ EVOLUTION OF THE MAGNETIC COMPONENT IN YANG–MILLS CONDENSATE DARK ENERGY MODELS ⋮ Joule–Thomson expansion of RN-AdS black hole immersed in perfect fluid dark matter ⋮ Bianchi type-III magnetized wet dark fluid cosmological model in general relativity ⋮ Cosmological models with Yang-Mills fields ⋮ On a Ströbel-inspired \(k(t)\) FLRW ansatz in a class of metric \(F(R)\) models ⋮ Modelling cosmic acceleration in modified Yang-Mills theory ⋮ Bianchi type III models with anisotropic dark energy ⋮ Cosmological evolution of interacting dark energy in Lorentz violation ⋮ Cosmology with a nonminimally coupled Yang-Mills field ⋮ Inflation driven by massive vector fields with derivative self-interactions ⋮ ATTRACTOR SOLUTION IN COUPLED YANG–MILLS FIELD DARK ENERGY MODELS
This page was built for publication: Vector field as a quintessence partner
