A PARAMETRIZED VARIABLE DARK ENERGY MODEL: STRUCTURE FORMATION AND OBSERVATIONAL CONSTRAINTS

DOI10.1142/S0218271806009170zbMath1130.85009arXivastro-ph/0508323OpenAlexW2102968569MaRDI QIDQ3426980

Sohrab Rahvar, M. Sadegh Movahed, S. Arbabi Bidgoli

Publication date: 14 March 2007

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0508323

zbMATH Keywords

cosmologyFriedmann-Robertson-Walker modelsstructure formationobservational constraintsquintessence modeltheory dark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Galactic and stellar structure (85A15) Astrophysical cosmology (85A40)

Related Items (2)

Observational constraints with recent data on the DGP modified gravity ⋮ AN INVERSE f(R) GRAVITATION FOR COSMIC SPEED UP, AND DARK ENERGY EQUIVALENT

Cites Work

• 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
• The cosmological constant problem

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