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Main Authors: Dembitskaia, A. I., Weiss, Stephane, Khlopov, M. Yu., Krasnov, M. A.
Format: Preprint
Published: 2026
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Online Access:https://arxiv.org/abs/2601.15147
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author Dembitskaia, A. I.
Weiss, Stephane
Khlopov, M. Yu.
Krasnov, M. A.
author_facet Dembitskaia, A. I.
Weiss, Stephane
Khlopov, M. Yu.
Krasnov, M. A.
contents According to modern physics, our Universe is baryon-asymmetric. That phenomenon can not be described in the frameworks of the Standard Model of particle physics. Globally, the Universe consists of baryon matter. However, some scenarios can lead to the existence of local antimatter domains. In the research, the chemical evolution of such an isolated antimatter domain, surrounded by baryonic matter, is studied. The size of the domain is estimated according to the conditions of its survival in baryon surrounding, and the process of annihilation at its border is taken into account.
format Preprint
id arxiv_https___arxiv_org_abs_2601_15147
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Chemical evolution of antimatter domains in early Universe
Dembitskaia, A. I.
Weiss, Stephane
Khlopov, M. Yu.
Krasnov, M. A.
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
According to modern physics, our Universe is baryon-asymmetric. That phenomenon can not be described in the frameworks of the Standard Model of particle physics. Globally, the Universe consists of baryon matter. However, some scenarios can lead to the existence of local antimatter domains. In the research, the chemical evolution of such an isolated antimatter domain, surrounded by baryonic matter, is studied. The size of the domain is estimated according to the conditions of its survival in baryon surrounding, and the process of annihilation at its border is taken into account.
title Chemical evolution of antimatter domains in early Universe
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2601.15147