Reanalysis shows DESI-preferred w0wa models reduce local H0 by 0.5-2.5 km s^{-1} Mpc^{-1} relative to LambdaCDM.
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A single f(Q, L_m) gravity model with HRDE produces Starobinsky-like inflation at high curvature and late-time acceleration, with RGUP corrections keeping n_s and r consistent with Planck while shifting the running of the spectral index.
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The DESI results impact the local determination of $H_0$
Reanalysis shows DESI-preferred w0wa models reduce local H0 by 0.5-2.5 km s^{-1} Mpc^{-1} relative to LambdaCDM.
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Cosmology of f(Q,L_m) gravity with Holographic Ricci Dark Energy: Early-Time Inflation and Late-Time Acceleration and RGUP Corrected Observables
A single f(Q, L_m) gravity model with HRDE produces Starobinsky-like inflation at high curvature and late-time acceleration, with RGUP corrections keeping n_s and r consistent with Planck while shifting the running of the spectral index.