Properties of fridmons and the early stage of evolution of the universe $10^{-6}-10^{-5}$
Teoretičeskaâ i matematičeskaâ fizika, Tome 17 (1973) no. 2, pp. 160-164 Cet article a éte moissonné depuis la source Math-Net.Ru

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In the framework of the model of a hot universe, estimates are made of the possible concentration of fridmons (fundamental particles with mass $10^{-6}-10^{-5}$ g) in the early stages of evolution of the universe. It is shown that the matter density at the time of “quenching” of the fridmons is $10^{85}$ g/sm$^3$.
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     title = {Properties of fridmons and the early stage of evolution of the universe $10^{-6}-10^{-5}$},
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V. I. Man'ko; M. A. Markov. Properties of fridmons and the early stage of evolution of the universe $10^{-6}-10^{-5}$. Teoretičeskaâ i matematičeskaâ fizika, Tome 17 (1973) no. 2, pp. 160-164. http://geodesic.mathdoc.fr/item/TMF_1973_17_2_a1/

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