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

Nguyen Ngoc Duy, Le Hong Khiem
Author affiliations

Authors

  • Nguyen Ngoc Duy
  • Le Hong Khiem Institute of Physics, VAST

DOI:

https://doi.org/10.15625/0868-3166/21/2/114

Keywords:

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

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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Published

30-06-2011

How to Cite

[1]
N. N. Duy and L. H. Khiem, “Feasibility Study of Direct Measurement of Stellar Reaction <sup>22</sup>Mg(α,p)<sup>25</sup>Al”, Comm. Phys., vol. 21, no. 2, p. 169, Jun. 2011.

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Section

Papers
Published 30-06-2011

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