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Quadratic Gravity

Adding terms quadratic in the curvature to the Einstein-Hilbert action renders gravity renormalizable. This property is preserved in the presence of the most general renormalizable couplings with (and of) a generic quantum field theory (QFT). The price to pay is a massive ghost, which is due to the...

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Autor principal: Salvio, Alberto
Lenguaje:eng
Publicado: 2018
Materias:
Acceso en línea:https://dx.doi.org/10.3389/fphy.2018.00077
http://cds.cern.ch/record/2318415
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author Salvio, Alberto
author_facet Salvio, Alberto
author_sort Salvio, Alberto
collection CERN
description Adding terms quadratic in the curvature to the Einstein-Hilbert action renders gravity renormalizable. This property is preserved in the presence of the most general renormalizable couplings with (and of) a generic quantum field theory (QFT). The price to pay is a massive ghost, which is due to the higher derivatives that the terms quadratic in the curvature imply. In this paper the quadratic gravity scenario is reviewed including recent progress on the related stability problem of higher derivative theories. The renormalization of the theory is also reviewed and the final form of the full renormalization group equations in the presence of a generic renormalizable QFT is presented. The theory can be extrapolated up to infinite energy through the renormalization group if all matter couplings flow to a fixed point (either trivial or interacting). Moreover, besides reviewing the above-mentioned topics some further insight on the ghost issue and the infinite energy extrapolation is provided. There is the hope that in the future this scenario might provide a phenomenologically viable and UV complete relativistic field theory of all interactions.
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publishDate 2018
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spelling cern-23184152022-07-21T09:26:31Zdoi:10.3389/fphy.2018.00077http://cds.cern.ch/record/2318415engSalvio, AlbertoQuadratic Gravityhep-thParticle Physics - Theorygr-qcGeneral Relativity and CosmologyAdding terms quadratic in the curvature to the Einstein-Hilbert action renders gravity renormalizable. This property is preserved in the presence of the most general renormalizable couplings with (and of) a generic quantum field theory (QFT). The price to pay is a massive ghost, which is due to the higher derivatives that the terms quadratic in the curvature imply. In this paper the quadratic gravity scenario is reviewed including recent progress on the related stability problem of higher derivative theories. The renormalization of the theory is also reviewed and the final form of the full renormalization group equations in the presence of a generic renormalizable QFT is presented. The theory can be extrapolated up to infinite energy through the renormalization group if all matter couplings flow to a fixed point (either trivial or interacting). Moreover, besides reviewing the above-mentioned topics some further insight on the ghost issue and the infinite energy extrapolation is provided. There is the hope that in the future this scenario might provide a phenomenologically viable and UV complete relativistic field theory of all interactions.arXiv:1804.09944CERN-TH-2018-099oai:cds.cern.ch:23184152018-04-26
spellingShingle hep-th
Particle Physics - Theory
gr-qc
General Relativity and Cosmology
Salvio, Alberto
Quadratic Gravity
title Quadratic Gravity
title_full Quadratic Gravity
title_fullStr Quadratic Gravity
title_full_unstemmed Quadratic Gravity
title_short Quadratic Gravity
title_sort quadratic gravity
topic hep-th
Particle Physics - Theory
gr-qc
General Relativity and Cosmology
url https://dx.doi.org/10.3389/fphy.2018.00077
http://cds.cern.ch/record/2318415
work_keys_str_mv AT salvioalberto quadraticgravity