Observational constraints on modified CPL models for dark energy

DOI10.1142/S0219887824500506MaRDI QIDQ6492694

Subenoy Chakraborty, Gopal Sardar

Publication date: 25 April 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

cosmologydark energyCPL model

Mathematics Subject Classification ID

Differential geometry (53-XX) Relativity and gravitational theory (83-XX)

Cites Work

• \(f(R)\) theories
• Estimating the dimension of a model
• Crossing the phantom divide with dissipative normal matter in the Israel-Stewart formalism
• First evidence that non-metricity \(f(Q)\) gravity could challenge \(\Lambda\)CDM
• On the theory and applications of modern cosmography
• Cosmological degeneracy versus cosmography: A cosmographic dark energy model
• The cosmological constant and dark energy
• Modified Gravity and Cosmology
• RECONSTRUCTING DARK ENERGY
• Connecting early and late universe by f(R) gravity
• A UNIFIED DARK ENERGY MODEL FROM A VANISHING SPEED OF SOUND WITH EMERGENT COSMOLOGICAL CONSTANT
• Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field
• A new look at the statistical model identification

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