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Rostov-na-Donu, Russia

Bazhutov Yu.N.,Ionosphere and Radiowave Propagation Institute IZMIRAN | Parkhomov A.G.,RAS Research Center Kurchatov Institute | Vereshkov G.M.,Federal South University h
Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011 | Year: 2011

Earlier on 18-th European Cosmic Ray Symposium we had been presented results on detection of high daily variations (∼100%, 7s ) for events caused by the high ionization cosmic ray component, passing through a telescope "Doch-4A". On 22-th European Cosmic Ray Symposium we had been presented results from the scintillation spectrometric telescopes "Doch-4M" running during (2001-2006) of large season & daily variations of the high ionization cosmic ray component. For the first time it was observed for the high ionization cosmic ray component statistically convincing evidence (7.3s statistical errors) for the effect of season variations with the variation amplitude A∼ 30% and for daily variations (3.5s , A∼35%). Here these results are interpreted in framework of Erzion model by elastic scattering of high energy neutral Erzions (E>10GeV), detected by telescope "Doch-4M", on thermolized space neutral Erzions around Sun, proposed as one of component of dark matter objects. For such interpretation we must proposed the dark matter density equal to 10 -11g/cm2. Source

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