Formation and Search of Large Scale Antimatter Regions
A. V. Grobov, S. G. Rubin
TL;DR
This paper explores how large antimatter regions can form and evolve into galaxies with unique anti-nuclei compositions, providing insights into antimatter distribution in the universe.
Contribution
It introduces a mechanism for generating large antimatter regions that survive to modern times and evolve into galaxies with distinctive antimatter signatures.
Findings
Large antimatter regions can persist and evolve into galaxies.
Galaxies with high antimatter density contain anti-helium and anti-deuterium.
Antimatter domain sizes exceed critical thresholds for survival.
Abstract
In the present paper we discuss a generation of large antimatter regions with sizes exceeding the critical surviving size. In the modern epoch domains with high antimatter density evolve to single galaxies with a peculiar content of anti-helium and anti-deuterium.
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