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Dark energy evolution from quantum gravity

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arxiv 2407.03465 v2 pith:AZPSFHFH submitted 2024-07-03 gr-qc astro-ph.COhep-th

Dark energy evolution from quantum gravity

classification gr-qc astro-ph.COhep-th
keywords darkenergyquantumgravityscaleevolutionneutrinodynamical
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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If an ultraviolet fixed point renders quantum gravity renormalizable, the effective potential for a singlet scalar field -- the cosmon -- can be computed according to the corresponding scaling solution of the renormalization group equations. We associate the largest intrinsic mass scale generated by the flow away from the fixed point with the scale of present dark energy density or even smaller. This results in a highly predictive scenario for the evolution of dynamical dark energy. It solves the cosmological constant problem dynamically, and may be called "quantum gravity quintessence". A first setting without quantum scale symmetry violation in the neutrino sector could explain the present amount of dark energy, but fails for the constraints on its time evolution. In contrast, a logarithmic scale symmetry violation in the beyond standard model sector responsible for the neutrino masses induces a non-vanishing cosmon-neutrino coupling in the Einstein frame. This yields a cosmology similar to growing neutrino quintessence, which could be compatible with present observations. The small number of unknown parameters turns the scaling solution for quantum gravity into a fundamental explanation of dynamical dark energy which can be falsified.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Fermi scale from quantum gravity scaling solution

    hep-th 2026-01 conditional novelty 5.0

    The Fermi/Planck ratio is claimed to be predictable from the analyticity of the quantum-gravity scaling solution for the cosmon-Higgs coupling, with numerics showing the coupling flows to a tiny, near-critical value.