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Dimensional Transmutation in Gravity and Cosmology

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arxiv 2012.11608 v2 pith:AWVF4SUM submitted 2020-12-21 hep-th astro-ph.COgr-qc

classification hep-thastro-ph.COgr-qc
keywords gravityscaledimensionalmasstermstransmutationachievedaction
verification ladder T0 review T1 audit T2 compute T3 formal
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We review (and extend) the analysis of general theories of all interactions (gravity included) where the mass scales are due to dimensional transmutation. Quantum consistency requires the presence of terms in the action with four derivatives of the metric. It is shown, nevertheless, how unitary is achieved and the classical Ostrogradsky instabilities can be avoided. The four-derivative terms also allow us to have a UV complete framework and a naturally small ratio between the Higgs mass and the Planck scale. Moreover, black holes of Einstein gravity with horizons smaller than a certain (microscopic) scale are replaced by horizonless ultracompact objects that are free from any singularity and have interesting phenomenological applications. We also discuss the predictions that can be compared with observations of the microwave background radiation anisotropies and find that this scenario is viable and can be tested with future data. Finally, how strong phase transitions can emerge in models of this type with approximate scale symmetry and how to test them with GW detectors is reviewed and explained.

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Cited by 2 Pith papers

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

  1. Primordial Gravitational Waves in Quadratic Gravity

    gr-qc 2025-02 unverdicted novelty 6.0 of 10

    In quadratic gravity, the inflationary tensor power spectrum is suppressed by (1 + 2H_*^2/m_gh^2)^{-1}, which restores the standard consistency relation r = -8n_t.

  2. Supercooled Phase Transitions with Radiative Symmetry Breaking

    hep-ph 2026-02 unverdicted novelty 3.0 of 10

    Supercooled phase transitions from radiative symmetry breaking can be described, at leading and next-to-leading order, by formulas depending only on three or four parameters (χ0, β̄, g, and g̃ at NLO).

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