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“HIGH DENSITY ANTIMATTER domains contain antiprotons and antihelium.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

LOW DENSITY ANTIMATTER. “If the density is so low that nucleosynthesis is not possible, low density antimatter domains contain only antiprotons (and positrons).” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

THE SURPRISE. “In several cosmological scenarios, the appearance of domains with an antibaryon excess can be predicted.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

TYPES OF ANTIMATTER. “A classification of antimatter domains according to the densities, and to the type(s) of antimatter involved within the non-trivial baryosyntheses processes considered will be proposed.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

NEW APPROACH. “A chemical potential can be assigned for the boundary–interaction region, responsible for keeping baryons and antibaryons separated, as a function of the antimatter density. A baryon/antibaryon-symmetrical Universe with large domains is demonstrated not to be compatible with a γ-ray background; the difference in the amount of antimatter can therefore be ascribed to a possible contribution to the definition of the chemical potential.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

CALCULATIONS. “The realistic prediction of antihelium flux accessible to AMS02 experiment is now under way involving analysis of possible sources of energetic antinuclei from antimatter globular cluster and their propagation in galactic magnetic fields.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

ANTIMATTER SYNTHESIS. “Antimatter star evolution and activity can give rise to antinuclear components of cosmic rays and rough estimation of the corresponding antihelium flux, proportional to the ratio masses of antimatter to matter in our Galaxy, is about 10(−8) of the helium flux of cosmic rays.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

SMALLEST ANTIMATTER STAR. “The minimal mass of such a domain, surviving in a baryon asymmetrical Universe, is 10(3) M ⊙, and it can form a globular cluster of antimatter stars in our Galaxy.” (M ⊙ - solar units). https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

ANTIMATTER ISLANDS. “The evidence for antihelium component of cosmic rays cannot find explanation by natural astrophysical sources and can imply the existence of macroscopic antimatter regions in a baryon asymmetrical Universe.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn

EXOTIC CHEMISTRY. “Strong non-homogeneity in antibaryons might imply (probably as a necessary condition) strong non-homogeneity for baryons, and produce some exotic results in nucleosynthesis.” https://www.mdpi.com/2218-1997/7/9/347/htm View in LinkedIn