Looking for interactions in the cosmological dark sector

DOI10.1088/1475-7516/2019/12/023OpenAlexW2969865127MaRDI QIDQ5066993

Saulo Carneiro, Willian Miranda, Humberto A. Borges, Cássio Pigozzo, Micol Benetti, Jailson S. Alcaniz

Publication date: 31 March 2022

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

Full work available at URL: https://arxiv.org/abs/1908.07213

zbMATH Keywords

dark energy theorycosmological parameters from LSScosmological parameters from CMBR

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (3)

Addressing the cosmological \(H_0\) tension by the Heisenberg uncertainty ⋮ J-PAS: forecasts on interacting vacuum energy models ⋮ Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models

Cites Work

• Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
• Can the cosmological dark sector be modeled by a single scalar field?
• Dynamical system analysis of interacting models
• Quintessence or Phoenix?
• Inhomogeneous vacuum energy
• Probing the independence within the dark sector in the fluid approximation
• An alternative to quintessence
• Interacting quintessence
• Non-adiabatic Chaplygin gas

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