CONSTRAINTS ON DARK ENERGY FROM THE OBSERVED EXPANSION OF OUR COSMIC HORIZON

DOI10.1142/S0218271809014984zbMath1168.85308arXiv0711.4181WikidataQ56979989 ScholiaQ56979989MaRDI QIDQ3395540

Fulvio Melia

Publication date: 5 September 2009

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

Full work available at URL: https://arxiv.org/abs/0711.4181

zbMATH Keywords

cosmologygravitationdark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Astrophysical cosmology (85A40)

Related Items (1)

Spherically-symmetric solutions in general relativity using a tetrad-based approach

Cites Work

• On the potentials yielding cosmological scaling solutions
• Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
• Visual Horizons in World Models
• Scaling solutions in Robertson-Walker spacetimes
• 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

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