(48) The absolute difference between the two determinations is, ∆H ΛCDM 0 =73.57−69.45=4.12 km s −1 Mpc−1

Hubble T ension in theΛCDM Model Using theΛCDM model constraints obtained in Table (II), we have HΛCDM 0 (CC+SN) =73

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gr-qc · 2026-04-11 · unverdicted · novelty 3.0

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.

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Polytropic $f(Q)$ cosmology and its implications for the $H_0$ tension gr-qc · 2026-04-11 · unverdicted · none · ref 5
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.