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Поисковые слова: arp 220
Cosmological Gene project: Introduction IntroductionParticipantsInstrumentationAntenna

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