Anisotropic cosmological model in presence of holographic dark energy and quintessence

DOI10.1007/s40995-017-0263-4zbMath1380.83322OpenAlexW2693834078MaRDI QIDQ1696120

B. Mishra, G. C. Samanta

Publication date: 14 February 2018

Published in: Iranian Journal of Science and Technology. Transaction A: Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s40995-017-0263-4

zbMATH Keywords

general relativityequation of stateholographic dark energyBianchi type-III space-time

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (2)

Bianchi type-III holographic dark energy model with quintessence ⋮ Sharma–Mittal holographic dark energy model in conharmonically flat space-time

Cites Work

• Bianchi type-III cosmological models with anisotropic dark energy (DE) in lyra geometry
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• Dissipative future universe without big rip
• Cosmic accelerated expansion and the entropy-corrected holographic dark energy
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• Bulk-brane interaction and holographic dark energy
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• Bianchi type-I anisotropic dark energy model with constant deceleration parameter
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• Bianchi type-III dark energy model in \(f(R,T)\) gravity
• Holographic dark energy with time varying \(n^2\) parameter in non-flat universe
• Universe filled with dark energy (DE) from a wet dark fluid (WDF) in \(f(R,T)\) gravity
• Dark energy models with variable equation of state parameter
• Bianchi type III anisotropic dark energy models with constant deceleration parameter
• SOME BIANCHI TYPE-V MODELS OF ACCELERATING UNIVERSE WITH DARK ENERGY
• DYNAMICS OF DARK ENERGY
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Cosmological parameters from SDSS and WMAP
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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