Thawing in a coupled quintessence model

DOI10.1007/S10714-016-2125-3zbMath1380.83306arXiv1508.06022OpenAlexW3105793181MaRDI QIDQ682432

H. Mohseni Sadjadi, Matin Honardoost, Hamid Reza Sepangi

Publication date: 2 February 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1508.06022

zbMATH Keywords

cosmologydark matterdark energycoupled quintessencethawing model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)

Related Items (5)

Constant-roll, cosmic acceleration, and massive neutrinos ⋮ Symmetron with a non-minimal kinetic term ⋮ Symmetry breaking, and the effect of matter density on neutrino oscillation ⋮ Cosmic acceleration and de Sitter expansion in hybrid mass varying neutrino model ⋮ Symmetron and de Sitter attractor in a teleparallel model of cosmology

Uses Software

• DLMF

Cites Work

• Unnamed Item
• Cosmological constant -- the weight of the vacuum
• The general property of dynamical quintessence field
• Quintessence: a review
• Quintessence with O ( N ) symmetry
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• The cosmological constant
• Interacting quintessence

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