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Infrared Properties of Quantum Gravity: UV/IR Mixing, Gravitizing the Quantum -- Theory and Observation

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arxiv 2202.06890 v1 pith:KDDTNFPC submitted 2022-02-14 hep-th gr-qc

classification hep-thgr-qc
keywords quantumgravitydiscussinfraredmixingphenomenologytheoryappearance
verification ladder T0 review T1 audit T2 compute T3 formal
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We discuss the possible appearance of several rather exotic phenomena in quantum gravity, including UV/IR mixing, novel modifications of infrared phenomenology that extend effective field theory approaches, and the relaxation of the usual notions of locality. We discuss the relevance of such concepts in quantum gravity for quantum information science, cosmology and general quantum gravity phenomenology.

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Cited by 6 Pith papers

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

  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. Geometric noise spectrum in interferometers

    hep-th 2026-01 conditional novelty 6.0 of 10

    The noise spectrum an interferometer would see from quantum spacetime jitter is computed for vacuum, thermal, squeezed, and scalar-backreaction states; all are Planck-suppressed.

  3. Information Metrics and Possible Limitations of Local Information Objectivity in Quantum Gravity

    gr-qc 2025-01 unverdicted novelty 6.0 of 10

    Quantum gravity may permit contextual deviations from the Fisher metric, inducing observer-dependent modifications to the Born rule.

  4. Quantum Spacetime, Quantum Gravity and Gravitized Quantum Theory

    gr-qc 2026-04 unverdicted novelty 5.0 of 10

    Quantum spacetime with a non-commutative dual explains the fixed Born rule of quantum theory and leads to gravitized quantum mechanics featuring dynamical probabilities and higher-order interference.

  5. Geometric noise spectrum in interferometers

    hep-th 2026-01 unverdicted novelty 5.0 of 10

    Computes UV-finite noise spectra in interferometers from graviton fluctuations in vacuum/thermal/squeezed states and from massless scalar vacuum stress-energy, all Planck-suppressed.

  6. 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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