Cosmological Gene project: Introduction

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The list of "Project Team" CMBA experiments, 1968-1998

year	motivation	results
1968	J.Silk predictions for protogalaxies	Anisotropy by factor 10 less than predicted
1969	M.Rees prediction for polarization of CMB	At small scales polarization less than 0.001%
1973	Ya.Zeldovich pankaces and Daucourt grav. noise predictions	less than predicted
1975	3 Russian approaches: adiabatic, vector and tensor type perturbations	Anisotropy by factor 3-5 less than all the predictions
1980	Neutrino Universe prediction based on Moscow University neutrino mass estimates	Better agreement, but less than predicted by factor 2 even for very late epoch of the galaxies formation
1981- 1995	Check of Inflation predictions	Discovery of strong extra noise at horizon scales but difficult to interpret ("Experiment Cold", Parijskij, Korolkov, 1986; all references may be found there connected with CMBA experiments made by PROJECT group in 1968-1986).
1997	Spectrum of the CMBA	First strong confirmation of the Black Body spectrum of CMBA at sub-degrees scales by comparison of the RATAN-600 longest wavelengths (7.6cm) measurements with SK and MSAM results at MM waves ("Dark Ages of the Universe", Parijskij et al, 1998)
1997-	Development of the "Sakharov oscillations" ("Cosmological Gene") project at RATAN-600 using near field zone atmosphere filtration theory	New information on the small scale Galactic noise which extends the Galactic Window to 30 GHz. The beginning of the next generation RATAN-600CMBA project