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It is suggested, on the basis of a simplified model of nucleon-antinucleon interaction, that a spatial separation of baryons and antibaryons might occur in the blackbody radiation at very high temperatures, typically larger than $kT=350$ MeV. Some applications to astrophysical data, like the matter density of the universe and a mechanism for quasistellar objects, are sketched.
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Roland Omnès (1969) studied this question.
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