Modificated activation method for measurement of the yield of the astrophysical reactions

The original version of the activation method is presented and yield of the astrophysical relevant reaction 1 2 C ( p , γ ) 1 3 N has been measured at the energy region 190–650 keV using this method. The rate of this reaction was calculated within the temperature region 0 . 0 1 ≤ T 9 ≤ 1 . 0 through...

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Hauptverfasser: Artemov, S. V., Igamov, S. B., Karakhodzhaev, A. A., Tojiboyev, O. R., Ergashev, F. Kh, Burtebayev, N., Kholbaev, I., Rumi, R. F., Eshkobilov, Sh. Kh, Khalikov, R. I.
Format: Tagungsbericht
Sprache:eng
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Zusammenfassung:The original version of the activation method is presented and yield of the astrophysical relevant reaction 1 2 C ( p , γ ) 1 3 N has been measured at the energy region 190–650 keV using this method. The rate of this reaction was calculated within the temperature region 0 . 0 1 ≤ T 9 ≤ 1 . 0 through the yield values. The possibility of improving the method for measuring very small yields or cross sections was demonstrated.
ISSN:2010-1945
2010-1945
DOI:10.1142/S2010194519600139