Vol. 21 No. 2 (2011)
Papers

Feasibility Study of Direct Measurement of Stellar Reaction <sup>22</sup>Mg(α,p)<sup>25</sup>Al

Le Hong Khiem
Institute of Physics, VAST

Published 30-06-2011

Keywords

  • X-rays burst,
  • CRIB,
  • 22Mg ,
  • αp-process,
  • nuclear astrophysics.

How to Cite

Duy, N. N., & Khiem, L. H. (2011). Feasibility Study of Direct Measurement of Stellar Reaction <sup>22</sup>Mg(α,p)<sup>25</sup>Al. Communications in Physics, 21(2), 169. https://doi.org/10.15625/0868-3166/21/2/114

Abstract

The stellar reaction 22Mg(α,p)25Al plays an important role for understanding the nucleosynthesis of stars. It has never investigated yet. We are planning to study this reaction in environment of X-rays burst with temperature T9 = 1÷3 GK using invert kinematics and thick target method. This paper shows a design for direct investigation of this reaction by simulation method. This design is necessary for experimental setup and for confirmation of the feasibility of the experiment.

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