Unifying dark matter, dark energy and inflation with a fuzzy dark fluid

DOI10.1088/1475-7516/2021/01/033zbMath1484.83098arXiv2007.05376OpenAlexW3040754853MaRDI QIDQ5025280

J.-F. Coupechoux, Alexandre Arbey

Publication date: 1 February 2022

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

Full work available at URL: https://arxiv.org/abs/2007.05376

zbMATH Keywords

inflationdark matter theorydark energy theory

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Symmetry breaking in quantum theory (81R40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Dark matter and dark energy (83C56)

Related Items (1)

Palatini R ² quintessential inflation

Cites Work

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• \(f(R)\) theories
• Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
• A new type of isotropic cosmological models without singularity
• Quintessence: a review
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• Inflation, Dark Matter, and Dark Energy in the String Landscape
• Cosmological scalar fields and Big-Bang nucleosynthesis
• Theory challenges of the accelerating Universe
• Inflationary universe: A possible solution to the horizon and flatness problems

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