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H0 tension in Tsallis and Renyi statistics

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arxiv 2501.02457 v1 pith:SQDP2WZF submitted 2025-01-05 gr-qc

Naser Sadeghnezhad This is my paper · ORCID
classification gr-qc
keywords renyistatisticstsallistensionastrophysicalattemptsconstraincosmological
topics The Hubble Tension
open problems The Hubble Tension
verification ladder T0 review T1 audit T2 compute T3 formal
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Motivated by recent attempts to study the implications of Tsallis and Renyi statistics in gravitational, cosmological, and astrophysical systems, the possible relationships between H0 tension and generalized statistics are explored. It is obtained that, in the light of H0 tension, the energytime uncertainty relations in Tsallis and Renyi statistics constrain the values of Tsallis and Renyi parameters. Hence, the way to find the footprints of non-extensivity in the universe is paved.

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Cited by 1 Pith paper

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  1. The case for a low dark matter density in dynamical dark energy model from local probes

    astro-ph.CO 2025-01 conditional novelty 5.0 of 10

    A Bayesian combination of local probes shows that a low matter density can accommodate local H0 and sigma8 values in LCDM when the BAO sound horizon is left free, but dynamical dark energy still faces tensions with Pa...

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