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The Running Gravitational Couplings

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arxiv hep-th/9707239 v3 pith:HQRVBVQH submitted 1997-07-29 hep-th gr-qc

The Running Gravitational Couplings

classification hep-th gr-qc
keywords constantcosmologicalnewtonrunningscaleszeroaccountappreciably
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We compute the running of the cosmological constant and Newton's constant taking into account the effect of quantum fields with any spin between 0 and 2. We find that Newton's constant does not vary appreciably but the cosmological constant can change by many orders of magnitude when one goes from cosmological scales to typical elementary particle scales. In the extreme infrared, zero modes drive the cosmological constant to zero.

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Cited by 3 Pith papers

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

  1. Is there ghost and tachyon free bounce in UV complete gravity theory?

    gr-qc 2026-07 conditional novelty 6.0

    Ghost- and tachyon-free bounces in AID gravity require a negative cosmological constant; known positive-Λ solutions inevitably contain ghost radiation.

  2. Towards gauge independence in asymptotically safe quantum gravity

    hep-th 2026-07 conditional novelty 6.0

    In an essential proper-time scheme, gauge dependence of the flow for Newton's constant cancels order-by-order once redundant off-shell terms are absorbed by field redefinitions, leaving a gauge-independent non-Gaussia...

  3. Asymptotically safe quantum gravity and its phenomenology -- a review

    hep-th 2026-06 unverdicted novelty 1.0

    Review surveying progress toward realistic asymptotically safe quantum gravity with quantum scale symmetry and observational implications.