APPARENT VERSUS TRUE VALUE OF THE COSMOLOGICAL CONSTANT

DOI10.1142/S0218271811020688zbMath1263.85073arXiv1208.3911OpenAlexW1976050956MaRDI QIDQ4914248

Pisin Chen, Antonio Enea Romano

Publication date: 18 April 2013

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

Full work available at URL: https://arxiv.org/abs/1208.3911

zbMATH Keywords

cosmological constantsupernovaedark energylarge scale inhomogeneities

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Radiative transfer in astronomy and astrophysics (85A25) Astrophysical cosmology (85A40)

Related Items (3)

Spherically-symmetric solutions in general relativity using a tetrad-based approach ⋮ Improved results on delay-dependent \(H_\infty \) control for uncertain systems with time-varying delays ⋮ Degeneracy in the spectrum and bispectrum among featured inflaton potentials

Cites Work

• Can the acceleration of our universe be explained by the effects of inhomogeneities?
• Effect of Inhomogeneity on Cosmological Models
• Solving the Inverse Problem with Inhomogeneous Universes
• 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
• Can Inhomogeneities Accelerate the Cosmic Volume Expansion?
• Spherically Symmetrical Models in General Relativity

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