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A heuristic hypothesis about domination of Bose-Einstein statistics in theearly Universe is suggested. The possibility of Bose-Einstein condensation(BEC) of primordial baryon-antibaryon pairs is considered. In accordance withthis postulation enormous masses in the order of galactic mass may beaccumulated within the cosmic scales. At the certain threshold value of thematter density the structural bosons decay into fermions and the sharpbreakdown of quantum-mechanical symmetry of the particles wave functionsoccurs. Then, due to the Pauli principle of exclusion a large-scale phasetransition occurs because of enormous pressure jump of the matter. Thisphenomenon might cause Cosmological Bang at the beginning stage of the MatterEra. As a mechanism of accumulation of galactic mass much larger than theconfiguration with structural bosons, a hypothetical BEC of elementary bosons(gauge bosons $W^{\pm}$ and $Z^{0})$ is discussed as well.

Cosmological Bang within Matter Era. Is the Generation of Galactic-Scale Mass Possible?