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Quantum Gravity Foundations for Tsallis Holography in Rastall Theory

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    This paper presents a theoretical framework combining quantum gravity foundations with Tsallis non-extensive holography within Rastall modified gravity, yielding a rich phenomenology for dark energy, black hole thermodynamics, and early universe cosmology.

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    Key findings

    Tsallis holographic dark energy in Rastall gravity can mimic the predictions of the standard ΛCDM model.

    The Rastall parameter γ and the Tsallis non-extensivity parameter δ form a complementary parameter space constrained by observational data.

    The unified framework provides a viable and observationally testable avenue toward reconciling quantum mechanics with gravitation.

    Limitations & open questions

    Further observational data is needed to more tightly constrain the parameter space.

    The theoretical implications require further exploration, particularly in the context of quantum gravity.

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