Asymmetric Dark Matter in Baryon Asymmetrical Universe
New heavy particles with electroweak charges arise in extensions of the standard model. They should take part in sphaleron transitions in the early Universe, which balance baryon asymmetry with the excess of new charged particles. If electrically charged with charge <inline-formula><math xm...
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| Format: | Article |
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MDPI AG
2024-03-01
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| Series: | Symmetry |
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| Online Access: | https://www.mdpi.com/2073-8994/16/3/311 |
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| author | Vitaly A. Beylin Maxim Yu. Khlopov Danila O. Sopin |
| author_facet | Vitaly A. Beylin Maxim Yu. Khlopov Danila O. Sopin |
| author_sort | Vitaly A. Beylin |
| collection | DOAJ |
| description | New heavy particles with electroweak charges arise in extensions of the standard model. They should take part in sphaleron transitions in the early Universe, which balance baryon asymmetry with the excess of new charged particles. If electrically charged with charge <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>−</mo><mn>2</mn><mi>n</mi></mrow></semantics></math></inline-formula>, they bind with <i>n</i> nuclei of primordial helium in dark atoms of dark matter. This makes it possible to find the ratio of densities of asymmetric dark matter and baryonic matter. Examples of the model with new, successive, and stable generation of quarks and leptons and the minimal walking technicolor model are considered. |
| first_indexed | 2024-04-24T17:48:18Z |
| format | Article |
| id | doaj.art-5ea54c379d09465ea5bcc0a025cd5f55 |
| institution | Directory Open Access Journal |
| issn | 2073-8994 |
| language | English |
| last_indexed | 2024-04-24T17:48:18Z |
| publishDate | 2024-03-01 |
| publisher | MDPI AG |
| record_format | Article |
| series | Symmetry |
| spelling | doaj.art-5ea54c379d09465ea5bcc0a025cd5f552024-03-27T14:05:27ZengMDPI AGSymmetry2073-89942024-03-0116331110.3390/sym16030311Asymmetric Dark Matter in Baryon Asymmetrical UniverseVitaly A. Beylin0Maxim Yu. Khlopov1Danila O. Sopin2Virtual Institute of Astroparticle Physics, 75018 Paris, FranceVirtual Institute of Astroparticle Physics, 75018 Paris, FranceInstitute of Nuclear Physics and Technology, National Research Nuclear University “MEPHI”, 31 Kashirskoe Chaussee, 115409 Moscow, RussiaNew heavy particles with electroweak charges arise in extensions of the standard model. They should take part in sphaleron transitions in the early Universe, which balance baryon asymmetry with the excess of new charged particles. If electrically charged with charge <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>−</mo><mn>2</mn><mi>n</mi></mrow></semantics></math></inline-formula>, they bind with <i>n</i> nuclei of primordial helium in dark atoms of dark matter. This makes it possible to find the ratio of densities of asymmetric dark matter and baryonic matter. Examples of the model with new, successive, and stable generation of quarks and leptons and the minimal walking technicolor model are considered.https://www.mdpi.com/2073-8994/16/3/311cosmoparticle physicswalking technicolorstable multiple charged particlessphaleron transitionsbaryon asymmetrynew stable quarks |
| spellingShingle | Vitaly A. Beylin Maxim Yu. Khlopov Danila O. Sopin Asymmetric Dark Matter in Baryon Asymmetrical Universe Symmetry cosmoparticle physics walking technicolor stable multiple charged particles sphaleron transitions baryon asymmetry new stable quarks |
| title | Asymmetric Dark Matter in Baryon Asymmetrical Universe |
| title_full | Asymmetric Dark Matter in Baryon Asymmetrical Universe |
| title_fullStr | Asymmetric Dark Matter in Baryon Asymmetrical Universe |
| title_full_unstemmed | Asymmetric Dark Matter in Baryon Asymmetrical Universe |
| title_short | Asymmetric Dark Matter in Baryon Asymmetrical Universe |
| title_sort | asymmetric dark matter in baryon asymmetrical universe |
| topic | cosmoparticle physics walking technicolor stable multiple charged particles sphaleron transitions baryon asymmetry new stable quarks |
| url | https://www.mdpi.com/2073-8994/16/3/311 |
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