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.
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container_volume 49
creator 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.
description 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.
doi_str_mv 10.1142/S2010194519600139
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subjects Activation
Energy measurement
title Modificated activation method for measurement of the yield of the astrophysical reactions
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