Polytropic f(Q) cosmology with power-law f(Q) produces exact solutions whose Bayesian fits to data yield a specific status for the H0 tension.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 2years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
An f(R,T) gravity model in anisotropic spacetime is reconstructed via a variable deceleration parameter and tightly constrained by Hubble and Pantheon+ data, reproducing the deceleration-to-acceleration transition and approaching de Sitter expansion.
citing papers explorer
-
Polytropic $f(Q)$ cosmology and its implications for the $H_0$ tension
Polytropic f(Q) cosmology with power-law f(Q) produces exact solutions whose Bayesian fits to data yield a specific status for the H0 tension.
-
Anisotropic Cosmology with interacting Dark Energy in f(R,T) Gravity: A Data-Constrained & independent Approach
An f(R,T) gravity model in anisotropic spacetime is reconstructed via a variable deceleration parameter and tightly constrained by Hubble and Pantheon+ data, reproducing the deceleration-to-acceleration transition and approaching de Sitter expansion.