Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69...31m&link_type=abstract
Astrophysics and Space Science, Volume 69, Issue 1, pp.31-43
Astronomy and Astrophysics
Astrophysics
2
Scientific paper
On the basis of the solutions obtained in the previous paper, the changes in the scenario of the standard model of the Big Bang are found. The chaos degree (constrainst on fluctuation spectra) is obtained, which could be still preserved by the initially completely chaotic Universe at the time of light elements nucleosynthesist es. The time boundaries of hadron and lepton eras and the time the electron neutrinos and neutrons become ‘frozen’ in reactions of weak interaction may be shifted up to 1.4 times. The corresponding temperatures may shift off from the standard ones 0.88 times if the mean-square level of fluctuations is close to unity. If the density of the energy of fluctuations concentrated in the short-wave region of the spectrum is less than 1.5{ɛ/-}, the nucleosynthesis leads to a helium abundance coinciding with the observe one. If at the timet es the maximum of the spectral density of the energy is in the long-wave region, that is λmax ≫ct es the level of the chaos during the period of nucleosynthesis is restricted to ν≲1.76 (where ν˜∫|C K |2 d3 K,C K is Fourier component of the amplitude of metric fluctuations). In particular, the protogalactic vortical disturbances with a wide spectrum Δ ≳ 4 × 103 Ω-1(Δ = ΔK/K, Ω = ϱ/ϱcrit) are compatible with the observed helium abundance.
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