A POSSIBLE LATE TIME ΛCDM-LIKE BACKGROUND COSMOLOGY IN RELATIVISTIC MOND THEORY

DOI10.1142/S021827180901490XzbMath1168.83344arXivastro-ph/0504130OpenAlexW3123882180MaRDI QIDQ3394756

No author found.

Publication date: 8 September 2009

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0504130

zbMATH Keywords

dark energyrelativistic MONDteves

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• Cosmological constant -- the weight of the vacuum
• DYNAMICS OF DARK ENERGY
• Cosmological dynamics of scalar fields with O( N ) symmetry
• Quintessence with O ( N ) symmetry
• 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
• Cosmological Imprint of an Energy Component with General Equation of State

This page was built for publication: A POSSIBLE LATE TIME ΛCDM-LIKE BACKGROUND COSMOLOGY IN RELATIVISTIC MOND THEORY