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
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$^3$.
@article{TMF_1973_17_2_a1,
author = {V. I. Man'ko and M. A. Markov},
title = {Properties of fridmons and the early stage of evolution of the universe $10^{-6}-10^{-5}$},
journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
pages = {160--164},
year = {1973},
volume = {17},
number = {2},
language = {ru},
url = {http://geodesic.mathdoc.fr/item/TMF_1973_17_2_a1/}
}
TY - JOUR
AU - V. I. Man'ko
AU - M. A. Markov
TI - Properties of fridmons and the early stage of evolution of the universe $10^{-6}-10^{-5}$
JO - Teoretičeskaâ i matematičeskaâ fizika
PY - 1973
SP - 160
EP - 164
VL - 17
IS - 2
UR - http://geodesic.mathdoc.fr/item/TMF_1973_17_2_a1/
LA - ru
ID - TMF_1973_17_2_a1
ER -
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/
[1] M. A. Markov, ZhETF, 51 (1966), 878
[2] S. Hawking, Month. Notic. Roy. Astron. Soc., 152 (1971), 75 | DOI
[3] M. A. Markov, Ann. Phys., 59 (1970), 109 | DOI
[4] M. A. Markov, V. P. Frolov, TMF, 3 (1970), 3
[5] G. V. Domogatskii, I. M. Zheleznykh, YaF, 10 (1969), 1238
[6] Ya. B. Zeldovich, UFN, 89 (1966), 647 | DOI
[7] L. D. Landau, E. M. Lifshits, Teoriya polya, «Nauka», 1967 | MR | Zbl
[8] V. A. Berezin, M. A. Markov, TMF, 12 (1972), 153
[9] L. Parker, Phys. Rev. Lett., 21 (1968), 562 ; 28 (1972), 705 ; Phys. Rev., 183 (1969), 1057 ; Phys. Rev., 3D (1971), 346 | DOI | DOI | DOI | Zbl
[10] K. Suga, H. Sakuyama , S. Kawaguchi, T. Hara, Phys. Rev. Lett., 27 (1972), 1604 | DOI