The existence of macroscopic regions with antibaryon excess in the baryon a
symmetric Universe with general baryon excess is the possible consequence o
f practically all models of baryosynthesis, Diffusion of matter and antimat
ter to the border of antimatter domains defines the minimal scale of the an
timatter domains surviving to the present time. A model of diffused antiwor
ld is considered, in which the density within the surviving antimatter doma
ins is too low to form gravitationally bound objects. The possibility to te
st this model by measurements of cosmic gamma ray fluxes is discussed. The
expected gamma ray flux is found to be acceptable for modern cosmic gamma r
ay detectors and for those planned for the near future. (C) 2000 Elsevier S
cience B.V. All rights reserved.