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On a Model of Variable Curvature that Mimics the Observed Universe Acceleration

https://doi.org/10.2139/ssrn.5050314
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The European Physical Journal C
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Explicit cosmological coarse graining via spatial averaging
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Curvature dominance dark energy model in f(R)-gravity
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Nontrivial geometries: Bounds on the curvature of the universe
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An exponential equation of state of dark energy in the light of 2018 CMB Planck data
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Challenges for $\Lambda$CDM: An update
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Exact Solutions of Einstein's Field Equations
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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
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Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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What Do We Really Know about Cosmic Acceleration?
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Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
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emcee : The MCMC Hammer
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ΛCDM-Rastall cosmology revisited: constraints from a recent Quasars datasample
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What is flat ΛCDM, and may we choose it?
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The Astrophysical Journal
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Journal of Cosmology and Astroparticle Physics
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The Astrophysical Journal Letters
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Critical assessment of some inhomogeneous pressure Stephani models
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Analytical solutions for two inhomogeneous cosmological models with energy flow and dynamical curvature
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Exploring the Expansion History of the Universe
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The cosmological constant problem
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WMAP constraints on low redshift evolution of dark energy
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Dark side of the universe in the Stephani cosmology
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Modified gravity with an exponential function of curvature
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Classical and Quantum Gravity
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ACCELERATING UNIVERSES WITH SCALING DARK MATTER
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General Relativity and Gravitation
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f(R) Theories
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Soviet Physics—USPEKHI
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Astrophysical Journal
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Test of the FLRW Metric and Curvature with Strong Lens Time Delays
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The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample
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Strong Lensing Modeling in Galaxy Clusters as a Promising Method to Test Cosmography. I. Parametric Dark Energy Models
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Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
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A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s −1 Mpc −1 Uncertainty from the Hubble Space Telescope and the SH0ES Team
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