Vol. 21 No. 2 (2011)
Papers

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

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  • Nguyen Ngoc Duy,
  • Le Hong Khiem
Le Hong Khiem
Institute of Physics, VAST
DOI: https://doi.org/10.15625/0868-3166/21/2/114

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
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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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