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Shape of dark energy: Constraining its evolution with a general parametrization

Dong Ha Lee ^1,*, Weiqiang Yang^2,†, Eleonora Di Valentino ^1,‡, Supriya Pan^3,4,§, and Carsten van de Bruck^1,∥

¹School of Mathematical and Physical Sciences, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom
²Department of Physics, Liaoning Normal University, Dalian 116029, People’s Republic of China
³Department of Mathematics, Presidency University, 86/1 College Street, Kolkata 700073, India
⁴Institute of Systems Science, Durban University of Technology, Durban 4000, Republic of South Africa

^*Contact author: dhlee1@sheffield.ac.uk
^†Contact author: d11102004@163.com
^‡Contact author: e.divalentino@sheffield.ac.uk
^§Contact author: supriya.maths@presiuniv.ac.in
^∥Contact author: c.vandebruck@sheffield.ac.uk

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Articles Citing

Shape of dark energy: Constraining its evolution with a general parametrization

Modifying ΛCDM dynamics via out-of-equilibrium axions: Reconciling SH0ES and DESI H0 values

Field Theory Vacuum and Entropic Dark Energy Models

Cosmological preference for a positive neutrino mass at 2.7σ: A joint analysis of DESI DR2, DESY5, and DESY1 data

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Dark energy and neutrinos along the cosmic expansion history

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Revisiting CPL with sign-switching density: To cross or not to cross the NECB

Thermodynamic reconstruction in observationally constrained dynamical dark energy models

Observational constraints on the modified cosmology inspired by string T-duality

Parametrizing dark energy at the density level: A two-parameter alternative to the Chevallier-Polarski-Linder parametrization

Dissecting the Hubble tension: Insights from a diverse set of sound-horizon-free H0 measurements

When one-parameter dark energy makes neutrinos physical again

Late-time emergence of dark energy and its interaction with dark matter

Model-independent late-Universe measurements of H0 and ΩK with the parametrization based on cosmic age-improved inverse distance ladder

Intertwined constraints in extended cosmologies: Dark energy, curvature, neutrinos, and inflation

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the w 0 wa CDM framework

Beyond CPL: Evidence for dynamical dark energy in three-parameter models

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