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Standard Model CP-violation and baryon asymmetry

Simply based on CP arguments, we argue against a Standard Model explanation of the baryon asymmetry of the universe in the presence of a first order phase transition. A CP-asymmetry is found in the reflection coefficients of quarks hitting the phase boundary created during the electroweak transition...

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Detalles Bibliográficos
Autores principales: Gavela, M.B., Hernandez, P., Orloff, J., Pene, O.
Lenguaje:eng
Publicado: 1994
Materias:
Acceso en línea:https://dx.doi.org/10.1142/S0217732394000629
http://cds.cern.ch/record/256026
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author Gavela, M.B.
Hernandez, P.
Orloff, J.
Pene, O.
author_facet Gavela, M.B.
Hernandez, P.
Orloff, J.
Pene, O.
author_sort Gavela, M.B.
collection CERN
description Simply based on CP arguments, we argue against a Standard Model explanation of the baryon asymmetry of the universe in the presence of a first order phase transition. A CP-asymmetry is found in the reflection coefficients of quarks hitting the phase boundary created during the electroweak transition. The problem is analyzed both in an academic zero temperature case and in the realistic finite temperature one. The building blocks are similar in both cases: Kobayashi-Maskawa CP-violation, CP-even phases in the reflection coefficients of quarks, and physical transitions due to fermion self-energies. In both cases an effect is present at order $\alpha_W^2$ in rate. A standard GIM behaviour is found as intuitively expected. In the finite temperature case, a crucial role is played by the damping rate of quasi-particles in a hot plasma, which is a relevant scale together with $M_W$ and the temperature. The effect is many orders of magnitude below what observation requires, and indicates that non standard physics is indeed needed in the cosmological scenario.
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institution Organización Europea para la Investigación Nuclear
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publishDate 1994
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spelling cern-2560262020-07-23T02:48:41Zdoi:10.1142/S0217732394000629http://cds.cern.ch/record/256026engGavela, M.B.Hernandez, P.Orloff, J.Pene, O.Standard Model CP-violation and baryon asymmetryParticle Physics - PhenomenologySimply based on CP arguments, we argue against a Standard Model explanation of the baryon asymmetry of the universe in the presence of a first order phase transition. A CP-asymmetry is found in the reflection coefficients of quarks hitting the phase boundary created during the electroweak transition. The problem is analyzed both in an academic zero temperature case and in the realistic finite temperature one. The building blocks are similar in both cases: Kobayashi-Maskawa CP-violation, CP-even phases in the reflection coefficients of quarks, and physical transitions due to fermion self-energies. In both cases an effect is present at order $\alpha_W^2$ in rate. A standard GIM behaviour is found as intuitively expected. In the finite temperature case, a crucial role is played by the damping rate of quasi-particles in a hot plasma, which is a relevant scale together with $M_W$ and the temperature. The effect is many orders of magnitude below what observation requires, and indicates that non standard physics is indeed needed in the cosmological scenario.Simply based on CP arguments, we argue against a Standard Model explanation of the baryon asymmetry of the universe in the presence of a first order phase transition. A CP-asymmetry is found in the reflection coefficients of quarks hitting the phase boundary created during the electroweak transition. The problem is analyzed both in an academic zero temperature case and in the realistic finite temperature one. The building blocks are similar in both cases: Kobayashi-Maskawa CP-violation, CP-even phases in the reflection coefficients of quarks, and physical transitions due to fermion self-energies. In both cases an effect is present at order $\alpha_W^2$ in rate. A standard GIM behaviour is found as intuitively expected. In the finite temperature case, a crucial role is played by the damping rate of quasi-particles in a hot plasma, which is a relevant scale together with $M_W$ and the temperature. The effect is many orders of magnitude below what observation requires, and indicates that non standard physics is indeed needed in the cosmological scenario.hep-ph/9312215CERN-TH-7081-93LPTHE-ORSAY-93-48HUTP-93-A036HD-THEP-93-45CERN-TH-7081-93HD-THEP-93-45HUTP-93-A-036LPTHE-93-48oai:cds.cern.ch:2560261994
spellingShingle Particle Physics - Phenomenology
Gavela, M.B.
Hernandez, P.
Orloff, J.
Pene, O.
Standard Model CP-violation and baryon asymmetry
title Standard Model CP-violation and baryon asymmetry
title_full Standard Model CP-violation and baryon asymmetry
title_fullStr Standard Model CP-violation and baryon asymmetry
title_full_unstemmed Standard Model CP-violation and baryon asymmetry
title_short Standard Model CP-violation and baryon asymmetry
title_sort standard model cp-violation and baryon asymmetry
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1142/S0217732394000629
http://cds.cern.ch/record/256026
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AT peneo standardmodelcpviolationandbaryonasymmetry