On structure formation from a small-scales-interacting dark sector

DOI10.1088/1475-7516/2019/04/042OpenAlexW3100538880WikidataQ128001733 ScholiaQ128001733MaRDI QIDQ5862652

Mahnaz Asghari, David F. Mota, Shahram Khosravi, Jose Beltrán Jiménez

Publication date: 9 March 2022

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

Full work available at URL: https://arxiv.org/abs/1902.05532

zbMATH Keywords

dark matter theorydark energy theorycosmological parameters from LSScosmological parameters from CMBR

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (6)

Is there evidence for CIDER in the Universe? ⋮ J-PAS: forecasts on interacting vacuum energy models ⋮ A null test of the equivalence principle using relativistic effects in galaxy surveys ⋮ On cosmological signatures of baryons-dark energy elastic couplings ⋮ Interacting tachyonic scalar field ⋮ Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids

Uses Software

• MontePython 3
• Monte Python

Cites Work

• Ghost dark energy with non-linear interaction term
• Cosmology and astrophysical constraints of Gauss-Bonnet dark energy
• 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.
• Cosmological parameters from SDSS and WMAP
• CMB and matter power spectra with non-linear dark-sector interactions
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The cosmological constant problem

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