Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS

DOI10.1088/1475-7516/2021/11/060zbMath1487.85021arXiv2104.13455OpenAlexW3215139807MaRDI QIDQ5062312

Javier E. Gonzalez, Micol Benetti, Rodrigo von Marttens, Jailson S. Alcaniz

Publication date: 15 March 2022

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

Full work available at URL: https://arxiv.org/abs/2104.13455

zbMATH Keywords

dark energy theorycosmological parameters from LSScosmological parameters from CMBR

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Diffraction, scattering (78A45) Geometrodynamics and the holographic principle (83E05) Quantum optics (81V80) Electromagnetic fields in general relativity and gravitational theory (83C50) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Radiative transfer in astronomy and astrophysics (85A25) Dark matter and dark energy (83C56)

Related Items (2)

What is flat ΛCDM, and may we choose it? ⋮ Effect of peculiar velocities of inhomogeneities on the shape of gravitational potential in spatially curved universe

Cites Work

• Inflationary universe: A possible solution to the horizon and flatness problems
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