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Baryon asymmetry of the universe in the minimal standard model
We calculate the baryon asymmetry of the Universe which would arise during a first order electroweak phase transition due to minimal standard model processes. It agrees in sign and magnitude with the observed baryonic excess, for resonable KM parameters and m$_t$ in the expected range, and plausible...
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
1993
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| Materias: | |
| Acceso en línea: | http://cds.cern.ch/record/249421 |
| _version_ | 1780885440686981120 |
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| author | Farrar, Glennys R. Shaposhnikov, M.E. |
| author_facet | Farrar, Glennys R. Shaposhnikov, M.E. |
| author_sort | Farrar, Glennys R. |
| collection | CERN |
| description | We calculate the baryon asymmetry of the Universe which would arise during a first order electroweak phase transition due to minimal standard model processes. It agrees in sign and magnitude with the observed baryonic excess, for resonable KM parameters and m$_t$ in the expected range, and plausible values of bubble velocity and other high temperature effects. A detailed version of this work (77pp) is being simultaneously submitted to the net. A shortened version of this recently appeared in Phys. Rev. Lett. {\bf 70}, 2833, 1993. |
| id | cern-249421 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 1993 |
| record_format | invenio |
| spelling | cern-2494212021-07-15T01:54:07Zhttp://cds.cern.ch/record/249421engFarrar, Glennys R.Shaposhnikov, M.E.Baryon asymmetry of the universe in the minimal standard modelParticle Physics - TheoryWe calculate the baryon asymmetry of the Universe which would arise during a first order electroweak phase transition due to minimal standard model processes. It agrees in sign and magnitude with the observed baryonic excess, for resonable KM parameters and m$_t$ in the expected range, and plausible values of bubble velocity and other high temperature effects. A detailed version of this work (77pp) is being simultaneously submitted to the net. A shortened version of this recently appeared in Phys. Rev. Lett. {\bf 70}, 2833, 1993.We calculate the baryon asymmetry of the Universe which would arise during a first order electroweak phase transition due to minimal standard model processes. It agrees in sign and magnitude with the observed baryonic excess, for resonable KM parameters and m$_t$ in the expected range, and plausible values of bubble velocity and other high temperature effects. A detailed version of this work (77pp) is being simultaneously submitted to the net. A shortened version of this recently appeared in Phys. Rev. Lett. {\bf 70}, 2833, 1993.hep-ph/9305274RU-93-10CERN-TH-6729-92CERN-TH-6729-93RU-93-10oai:cds.cern.ch:2494211993 |
| spellingShingle | Particle Physics - Theory Farrar, Glennys R. Shaposhnikov, M.E. Baryon asymmetry of the universe in the minimal standard model |
| title | Baryon asymmetry of the universe in the minimal standard model |
| title_full | Baryon asymmetry of the universe in the minimal standard model |
| title_fullStr | Baryon asymmetry of the universe in the minimal standard model |
| title_full_unstemmed | Baryon asymmetry of the universe in the minimal standard model |
| title_short | Baryon asymmetry of the universe in the minimal standard model |
| title_sort | baryon asymmetry of the universe in the minimal standard model |
| topic | Particle Physics - Theory |
| url | http://cds.cern.ch/record/249421 |
| work_keys_str_mv | AT farrarglennysr baryonasymmetryoftheuniverseintheminimalstandardmodel AT shaposhnikovme baryonasymmetryoftheuniverseintheminimalstandardmodel |