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Quantum Gravity Phenomenology in the Infrared

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arxiv 2104.00802 v2 pith:NAFCASWW submitted 2021-04-01 gr-qc hep-th

classification gr-qchep-th
keywords quantumgravityinfrareduniverseallowsconsequencesevolutionfundamental
verification ladder T0 review T1 audit T2 compute T3 formal
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Quantum gravity effects are traditionally tied to short distances and high energies. In this essay we argue that, perhaps surprisingly, quantum gravity may have important consequences for the phenomenology of the infrared. We center our discussion around a conception of quantum gravity involving a notion of quantum spacetime that arises in metastring theory. This theory allows for an evolution of a cosmological Universe in which string-dual degrees of freedom decouple as the Universe ages. Importantly such an implementation of quantum gravity allows for the inclusion of a fundamental length scale without introducing the fundamental breaking of Lorentz symmetry. The mechanism seems to have potential for an entirely novel source for dark matter/energy. The simplest observational consequences of this scenario may very well be residual infrared modifications that emerge through the evolution of the Universe.

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Cited by 2 Pith papers

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  1. A Cosmological Uncertainty Relation and Late-Universe Acceleration

    astro-ph.CO 2026-04 unverdicted novelty 6.0 of 10

    A deformed uncertainty relation for the universe scale factor modifies the Friedmann equation to yield late-universe acceleration or a bounce according to the sign of a single free exponent.

  2. A Cosmological Uncertainty Relation and Late-Universe Acceleration

    astro-ph.CO 2026-04 unverdicted novelty 4.0 of 10

    Deformed commutation relation for the cosmic scale factor modifies the Friedmann equation to produce late-time dark energy with w > -1 or a non-singular bounce as a horizon-scale quantum gravity effect, without new pa...

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