Horndeski under the quantum loupe
arXiv:2004.11655 · doi:10.1088/1475-7516/2020/10/010
Abstract
With recent constraints on the propagation speed of gravitational waves, the class of scalar-tensor theories has significantly been reduced. We consider one of the surviving models still relevant for cosmology and investigate its radiative stability. The model contains operators with explicit breaking of the Galileon symmetry and we study whether they harm the re-organization of the effective field theory. Within the regime of validity we establish a non-renormalization theorem and show explicitly that the quantum corrections, to one-loop, do not detune the classical Lagrangian generating suppressed counterterms. This is striking since the non-renormalization theorem is established in the presence of a genuine Galileon symmetry breaking term.
23 pages, 4 figures
References in corpus (13)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Resummation of Massive Gravity
- Dark Energy after GW170817: dead ends and the road ahead
- Strong constraints on cosmological gravity from GW170817 and GRB 170817A
- Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
- Multi-field galileons and higher co-dimension branes
- Non-Renormalization and Naturalness in a Class of Scalar-Tensor Theories
- Dark-Energy Instabilities induced by Gravitational Waves
- Cosmological constraints on dark energy in light of gravitational wave bounds
- Unification of Galileon Dualities
- Quantum Corrections in Galileons from Matter Loops
- One-loop renormalization in Galileon effective field theory
- Geometrized quantum Galileons
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- Quantum Stability of Generalized Proca Theories
- Quantum Corrections to Generic Branes: DBI, NLSM, and More
- Scalar-tensor cosmologies without screening
- Quantum stability of Proca-Nuevo
- On tachyonic stability priors for dark energy
- Beyond Horndeski interactions induced by quantum effects
- Large black-hole scalar charges induced by cosmology in Horndeski theories
- Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
- Infrared Sensitivity of Cosmological Probes in Horndeski Theory
- Dark energy constraints in light of theoretical priors