Chameleon scalar field in LRS Bianchi type I cosmological model

DOI10.1134/S0202289316010059zbMath1342.83524OpenAlexW2333900106MaRDI QIDQ2628757

Ashutosh Singh, R. Chaubey, Rakesh Raushan

Publication date: 15 July 2016

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0202289316010059

zbMATH Keywords

cosmological modelcold dark matteranisotropicLRS Bianchi type IChameleon scalar fieldFriedmann-Robertson-Walker cosmological model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)

Related Items (1)

Cosmic acceleration and ekpyrotic bounce with Chameleon field

Cites Work

• Unnamed Item
• Cosmological constant -- the weight of the vacuum
• Role of chameleon field in accelerating universe
• The cosmological constant and dark energy
• COSMIC DYNAMICS IN CHAMELEON COSMOLOGY
• 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
• Inflationary universe: A possible solution to the horizon and flatness problems
• Dynamical Systems in Cosmology
• The Large Scale Structure of Space-Time

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