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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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Lenguaje: | eng |
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2016
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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 |
record_format | invenio |
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 |