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.
The corresponding Hubble constant estimates are, H f(Q) 0 (CC+SN) =72.41 +0.56 −0.60 km s−1 Mpc−1, (52) H f(Q) 0 (BAO+CMB) =68.19 +0.37 −0.34 km s−1 Mpc−1
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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.