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Introduction to the Effective Field Theory Description of Gravity

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arxiv gr-qc/9512024 v1 pith:3KYSNCML submitted 1995-12-11 gr-qc hep-phhep-th

John F. Donoghue (Univ. of Massachusetts , Amherst) This is my paper · ORCID
classification gr-qchep-phhep-th
keywords theoryeffectivefielddescriptiongravityintroductionquantumenergies
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This is a pedagogical introduction to the treatment of general relativity as a quantum effective field theory. Gravity fits nicely into the effective field theory description and forms a good quantum theory at ordinary energies.

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Cited by 7 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 39 citations worldwide. Full citation record

  1. Black hole mergers beyond general relativity: a self-force approach

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    Self-force theory is extended to compute merger and ringdown waveforms in beyond-GR black hole binaries under the extreme mass-ratio approximation, with first calculations of self-force corrections to the merger waveform.

  2. Quantum gravity and matter fields in a general background gauge

    hep-th 2026-03 unverdicted novelty 6.0 of 10

    One-loop effective action for quantum gravity plus matter is computed off-shell in a general background gauge, shown to be gauge-independent on-shell per the DeWitt-Kallosh theorem, and used to establish non-renormali...

  3. Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes

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    A second-order RG-improved Schwarzschild-(A)dS metric is derived and its scalar QNMs are shown to depend weakly on the free parameter ζ, with consistent results from WKB, shooting, and matrix-pencil time-domain analysis.

  4. Towards the consistent perturbative expansion in discrete gravity

    gr-qc 2026-01 conditional novelty 5.0 of 10

    A mixed finite-difference action plus a principal-value soft synchronous gauge is claimed to make lattice gravity perturbation theory reproduce continuum gravity at small momenta.

  5. Leading effective field theory corrections to the Kerr metric at all spins

    gr-qc 2025-12 unverdicted novelty 5.0 of 10

    Numerical solutions show that leading effective-field-theory corrections to the Kerr metric grow with spin and are largest near extremality.

  6. Observer Time from Causality in Perturbative Quantum Gravity

    hep-th 2025-06 conditional novelty 5.0 of 10

    A lightbulb-and-mirror protocol defines diffeomorphism-invariant elapsed proper time, and its leading quantum gravity correction makes the time a noncommuting quantum operator.

  7. Response of interferometers to the vacuum of quantum gravity

    hep-th 2024-09 unverdicted novelty 5.0 of 10

    Standard low-energy quantum gravity via effective graviton QFT predicts interferometer length variations of order the Planck length (~10^{-35} m), with no divergences indicating breakdown.

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