Probing the imprints of generalized interacting dark energy on the growth of perturbations

DOI10.1088/1475-7516/2017/11/001OpenAlexW2736563828MaRDI QIDQ5021618

Jurgen Mifsud, Carsten Van De Bruck

Publication date: 13 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1707.07667

zbMATH Keywords

modified gravitycosmological perturbation theorydark energy theoryintegrated Sachs-Wolfe effect

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (6)

Redshift space distortions in the presence of non-minimally coupled dark matter ⋮ Disformal invariance of cosmological observables ⋮ Testing the equivalence principle on cosmological scales using the odd multipoles of galaxy cross-power spectrum and bispectrum ⋮ Transient weak gravity in scalar-tensor theories ⋮ Finite-time cosmological singularities and the possible fate of the universe ⋮ Scalar field dark matter and dark energy: a hybrid model for the dark sector

Uses Software

• CLASS

Cites Work

• Republication of: Perturbations of a cosmological model and angular variations of the microwave background. Edited and with commentary by George Ellis and with notes on Sachs-Wolfe integration by Jürgen Ehlers. With brief autobiographies by Sachs and Wolfe.
• DYNAMICS OF DARK ENERGY
• Cosmological evolution with interaction between dark energy and dark matter
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Interacting quintessence

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