Dark energy homogeneity in general relativity: Are we applying it correctly?

DOI10.1007/s10714-016-2047-0zbMath1338.83194arXiv1505.03436OpenAlexW1916497742MaRDI QIDQ291424

Didam G. A. Duniya

Publication date: 10 June 2016

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1505.03436

zbMATH Keywords

perturbationhomogeneitygeneral relativitypower spectrumdark energymatter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (4)

Probing beyond-Horndeski gravity on ultra-large scales ⋮ A resolution of a metric singularity associated with the introduction of Λ into static spherically symmetric systems ⋮ Observed galaxy power spectrum in cubic Galileon model ⋮ CMB and matter power spectra with non-linear dark-sector interactions

Cites Work

• Lensing and time-delay contributions to galaxy correlations
• Relativistic effect in galaxy clustering
• Isolating relativistic effects in large-scale structure
• Novel null-test for the Λ cold dark matter model with growth-rate data
• DARK ENERGY IN PRACTICE
• DYNAMICS OF DARK ENERGY
• Cosmological Imprint of an Energy Component with General Equation of State
• Notes on top-down languages
• Quintessence and supergravity

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