EFFECTS OF f(R) DARK ENERGY ON DISSIPATIVE ANISOTROPIC COLLAPSING FLUID

DOI10.1142/S0217732310034195zbMath1208.83130arXiv1008.2678OpenAlexW2086241016MaRDI QIDQ3086209

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Publication date: 30 March 2011

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1008.2678

zbMATH Keywords

dynamical equations\(f(R)\) theorydissipative anisotropic fluid

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (8)

Newtonian and post Newtonian expansionfree fluid evolution in \(f(R)\) gravity ⋮ Shear-free radiating collapse model via Karmarkar condition in f(R) gravity ⋮ Cosmological evolution for dark energy models in \(f(T)\) gravity ⋮ EXPANSIONFREE FLUID EVOLUTION AND SKRIPKIN MODEL IN f(R) THEORY ⋮ Effects of charge on dynamical instability of spherical collapse in \(f(R,T)\) gravity ⋮ Dissipative planar gravitational collapse in f(G) gravity ⋮ F(T) MODELS WITHIN BIANCHI TYPE-I UNIVERSE ⋮ Exact solutions of Bianchi type \(V\) spacetime in \(f(R,T)\) gravity

Cites Work

• EFFECTS OF ELECTROMAGNETIC FIELD ON GRAVITATIONAL COLLAPSE
• GRAVITATIONAL PERFECT FLUID COLLAPSE WITH COSMOLOGICAL CONSTANT
• PLANE SYMMETRIC GRAVITATIONAL COLLAPSE
• 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
• Spherical symmetry in f ( R )-gravity
• On Continued Gravitational Contraction
• Dynamics of viscous dissipative plane symmetric gravitational collapse

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