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Dimensional Transmutation in Particle Physics and Cosmology

<!--HTML-->Models with classical scale invariance (CSI) provides us with a dynamical origin for all masses (via dimensional transmutation) and can account for all evidence of beyond the standard model physics. Furthermore, a general theory with CSI is renormalizable (even in the gravity sector...

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Autor principal: Salvio, Alberto
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:http://cds.cern.ch/record/2657962
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author Salvio, Alberto
author_facet Salvio, Alberto
author_sort Salvio, Alberto
collection CERN
description <!--HTML-->Models with classical scale invariance (CSI) provides us with a dynamical origin for all masses (via dimensional transmutation) and can account for all evidence of beyond the standard model physics. Furthermore, a general theory with CSI is renormalizable (even in the gravity sector) and can solve the hierarchy problem. The price to pay is a classical ghost. The theory, however, admits quantizations that preserve unitarity and a Hamiltonian bounded from below. The solution of the hierarchy problem implies that the theory can be tested through inflationary data (indeed it predicts a (gravitational) isocurvature mode that could be observed in the next future). I will give an overview of CSI and introduce the subsequent talks on this subject.
id cern-2657962
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
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spelling cern-26579622022-11-02T22:34:49Zhttp://cds.cern.ch/record/2657962engSalvio, AlbertoDimensional Transmutation in Particle Physics and CosmologyScale invariance in particle physics and cosmologyTH institutes<!--HTML-->Models with classical scale invariance (CSI) provides us with a dynamical origin for all masses (via dimensional transmutation) and can account for all evidence of beyond the standard model physics. Furthermore, a general theory with CSI is renormalizable (even in the gravity sector) and can solve the hierarchy problem. The price to pay is a classical ghost. The theory, however, admits quantizations that preserve unitarity and a Hamiltonian bounded from below. The solution of the hierarchy problem implies that the theory can be tested through inflationary data (indeed it predicts a (gravitational) isocurvature mode that could be observed in the next future). I will give an overview of CSI and introduce the subsequent talks on this subject.oai:cds.cern.ch:26579622019
spellingShingle TH institutes
Salvio, Alberto
Dimensional Transmutation in Particle Physics and Cosmology
title Dimensional Transmutation in Particle Physics and Cosmology
title_full Dimensional Transmutation in Particle Physics and Cosmology
title_fullStr Dimensional Transmutation in Particle Physics and Cosmology
title_full_unstemmed Dimensional Transmutation in Particle Physics and Cosmology
title_short Dimensional Transmutation in Particle Physics and Cosmology
title_sort dimensional transmutation in particle physics and cosmology
topic TH institutes
url http://cds.cern.ch/record/2657962
work_keys_str_mv AT salvioalberto dimensionaltransmutationinparticlephysicsandcosmology
AT salvioalberto scaleinvarianceinparticlephysicsandcosmology