Asymmetric Dark Matter in Baryon Asymmetrical Universe

Author:

Beylin Vitaly A.1ORCID,Khlopov Maxim Yu.123ORCID,Sopin Danila O.2ORCID

Affiliation:

1. Virtual Institute of Astroparticle Physics, 75018 Paris, France

2. Institute of Nuclear Physics and Technology, National Research Nuclear University “MEPHI”, 31 Kashirskoe Chaussee, 115409 Moscow, Russia

3. Research Institute of Physics, Southern Federal University, Stachki 194, 344090 Rostov on Don, Russia

Abstract

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 −2n, they bind with n 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.

Funder

Ministry of Science and Higher Education of the Russian Federation

MEPHI program on Prioritet 2030

Publisher

MDPI AG

Reference61 articles.

1. Beylin, V., Khlopov, M., Kuksa, V., and Volchanskiy, N. (2020). New Physics of Strong Interaction and Dark Universe. Universe, 6.

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3. Belotsky, K., Khlopov, M., and Shibaev, K. (2008). Stable quarks of the 4th family?. arXiv.

4. Possible manifestations of the existence of a fourth-generation neutrino;Golubkov;J. Exp. Theor. Phys.,1999

5. Beylin, V., Khlopov, M., and Sopin, D. (2023). Charge Asymmetry of New Stable Families in Baryon Asymmetrical Universe. Symmetry, 15.

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