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The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry
Primordial Big-Bang Nucleosynthesis (BBN) tightly constrains the existence of any additional relativistic degrees of freedom at that epoch. However a large asymmetry in electron neutrino number shifts the chemical equilibrium between the neutron and proton at neutron freeze-out and allows such addit...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
1999
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1126-6708/1999/11/015 http://cds.cern.ch/record/397013 |
_version_ | 1780893948155265024 |
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author | March-Russell, John Murayama, Hitoshi Riotto, Antonio |
author_facet | March-Russell, John Murayama, Hitoshi Riotto, Antonio |
author_sort | March-Russell, John |
collection | CERN |
description | Primordial Big-Bang Nucleosynthesis (BBN) tightly constrains the existence of any additional relativistic degrees of freedom at that epoch. However a large asymmetry in electron neutrino number shifts the chemical equilibrium between the neutron and proton at neutron freeze-out and allows such additional particle species. Moreover, the BBN itself may also prefer such an asymmetry to reconcile predicted element abundances and observations. However, such a large asymmetry appears to be in conflict with the observed small baryon asymmetry if they are in sphaleron mediated equilibrium. In this paper we point out the surprising fact that in the Standard Model, if the asymmetries in the electron number and the muon number are equal (and opposite) and of the size required to reconcile BBN theory with observations, a baryon asymmetry of the Universe of the correct magnitude and sign is automatically generated within a factor of two. This small remaining discrepancy is naturally remedied in the supersymmetric Standard Model. |
id | cern-397013 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1999 |
record_format | invenio |
spelling | cern-3970132023-03-14T18:45:15Zdoi:10.1088/1126-6708/1999/11/015http://cds.cern.ch/record/397013engMarch-Russell, JohnMurayama, HitoshiRiotto, AntonioThe Small Observed Baryon Asymmetry from a Large Lepton AsymmetryParticle Physics - PhenomenologyPrimordial Big-Bang Nucleosynthesis (BBN) tightly constrains the existence of any additional relativistic degrees of freedom at that epoch. However a large asymmetry in electron neutrino number shifts the chemical equilibrium between the neutron and proton at neutron freeze-out and allows such additional particle species. Moreover, the BBN itself may also prefer such an asymmetry to reconcile predicted element abundances and observations. However, such a large asymmetry appears to be in conflict with the observed small baryon asymmetry if they are in sphaleron mediated equilibrium. In this paper we point out the surprising fact that in the Standard Model, if the asymmetries in the electron number and the muon number are equal (and opposite) and of the size required to reconcile BBN theory with observations, a baryon asymmetry of the Universe of the correct magnitude and sign is automatically generated within a factor of two. This small remaining discrepancy is naturally remedied in the supersymmetric Standard Model.Primordial Big-Bang Nucleosynthesis (BBN) tightly constrains the existence of any additional relativistic degrees of freedom at that epoch. However a large asymmetry in electron neutrino number shifts the chemical equilibrium between the neutron and proton at neutron freeze-out and allows such additional particle species. Moreover, the BBN itself may also prefer such an asymmetry to reconcile predicted element abundances and observations. However, such a large asymmetry appears to be in conflict with the observed small baryon asymmetry if they are in sphaleron mediated equilibrium. In this paper we point out the surprising fact that in the Standard Model, if the asymmetries in the electron number and the muon number are equal (and opposite) and of the size required to reconcile BBN theory with observations, a baryon asymmetry of the Universe of the correct magnitude and sign is automatically generated within a factor of two. This small remaining discrepancy is naturally remedied in the supersymmetric Standard Model.hep-ph/9908396CERN-TH-99-218LBNL-44140UCB-PTH-99-30LBL-44140CERN-TH-99-218oai:cds.cern.ch:3970131999-08-19 |
spellingShingle | Particle Physics - Phenomenology March-Russell, John Murayama, Hitoshi Riotto, Antonio The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry |
title | The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry |
title_full | The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry |
title_fullStr | The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry |
title_full_unstemmed | The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry |
title_short | The Small Observed Baryon Asymmetry from a Large Lepton Asymmetry |
title_sort | small observed baryon asymmetry from a large lepton asymmetry |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1088/1126-6708/1999/11/015 http://cds.cern.ch/record/397013 |
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