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Solving the Standard Model Problems in Softened Gravity

The Higgs naturalness problem is solved if the growth of Einstein's gravitational interaction is softened at an energy $ \lesssim 10^{11}\,$GeV (softened gravity). We work here within an explicit realization where the Einstein-Hilbert Lagrangian is extended to include terms quadratic in the cur...

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Autor principal: Salvio, Alberto
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.94.096007
http://cds.cern.ch/record/2205472
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author Salvio, Alberto
author_facet Salvio, Alberto
author_sort Salvio, Alberto
collection CERN
description The Higgs naturalness problem is solved if the growth of Einstein's gravitational interaction is softened at an energy $ \lesssim 10^{11}\,$GeV (softened gravity). We work here within an explicit realization where the Einstein-Hilbert Lagrangian is extended to include terms quadratic in the curvature and a non-minimal coupling with the Higgs. We show that this solution is preserved by adding three right-handed neutrinos with masses below the electroweak scale, accounting for neutrino oscillations, dark matter and the baryon asymmetry. The smallness of the right-handed neutrino masses (compared to the Planck scale) and the QCD $\theta$-term are also shown to be natural. We prove that a possible gravitational source of CP violation cannot spoil the model, thanks to the presence of right-handed neutrinos. Starobinsky inflation can occur in this context, even if we live in a metastable vacuum.
id cern-2205472
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2016
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spelling cern-22054722023-10-04T07:45:41Zdoi:10.1103/PhysRevD.94.096007http://cds.cern.ch/record/2205472engSalvio, AlbertoSolving the Standard Model Problems in Softened GravityParticle Physics - PhenomenologyThe Higgs naturalness problem is solved if the growth of Einstein's gravitational interaction is softened at an energy $ \lesssim 10^{11}\,$GeV (softened gravity). We work here within an explicit realization where the Einstein-Hilbert Lagrangian is extended to include terms quadratic in the curvature and a non-minimal coupling with the Higgs. We show that this solution is preserved by adding three right-handed neutrinos with masses below the electroweak scale, accounting for neutrino oscillations, dark matter and the baryon asymmetry. The smallness of the right-handed neutrino masses (compared to the Planck scale) and the QCD $\theta$-term are also shown to be natural. We prove that a possible gravitational source of CP violation cannot spoil the model, thanks to the presence of right-handed neutrinos. Starobinsky inflation can occur in this context, even if we live in a metastable vacuum.The Higgs naturalness problem is solved if the growth of Einstein’s gravitational interaction is softened at an energy ≲1011  GeV (softened gravity). We work here within an explicit realization where the Einstein-Hilbert Lagrangian is extended to include terms quadratic in the curvature and a nonminimal coupling with the Higgs. We show that this solution is preserved by adding three right-handed neutrinos with masses below the electroweak scale, accounting for neutrino oscillations, dark matter and the baryon asymmetry. The smallness of the right-handed neutrino masses (compared to the Planck scale) and the QCD θ-term are also shown to be natural. We prove that a possible gravitational source of CP violation cannot spoil the model, thanks to the presence of right-handed neutrinos. Inflation is approximately described by the Starobinsky model in this context and can occur even if we live in a metastable vacuum.The Higgs naturalness problem is solved if the growth of Einstein's gravitational interaction is softened at an energy $ \lesssim 10^{11}\,$GeV (softened gravity). We work here within an explicit realization where the Einstein-Hilbert Lagrangian is extended to include terms quadratic in the curvature and a non-minimal coupling with the Higgs. We show that this solution is preserved by adding three right-handed neutrinos with masses below the electroweak scale, accounting for neutrino oscillations, dark matter and the baryon asymmetry. The smallness of the right-handed neutrino masses (compared to the Planck scale) and the QCD $\theta$-term are also shown to be natural. We prove that a possible gravitational source of CP violation cannot spoil the model, thanks to the presence of right-handed neutrinos. Inflation is approximately described by the Starobinsky model in this context, and can occur even if we live in a metastable vacuum.arXiv:1608.01194CERN-TH-2016-176CERN-TH-2016-176oai:cds.cern.ch:22054722016-08-03
spellingShingle Particle Physics - Phenomenology
Salvio, Alberto
Solving the Standard Model Problems in Softened Gravity
title Solving the Standard Model Problems in Softened Gravity
title_full Solving the Standard Model Problems in Softened Gravity
title_fullStr Solving the Standard Model Problems in Softened Gravity
title_full_unstemmed Solving the Standard Model Problems in Softened Gravity
title_short Solving the Standard Model Problems in Softened Gravity
title_sort solving the standard model problems in softened gravity
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.94.096007
http://cds.cern.ch/record/2205472
work_keys_str_mv AT salvioalberto solvingthestandardmodelproblemsinsoftenedgravity