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

Nguyen Ngoc Duy; Le Hong Khiem

doi:10.15625/0868-3166/21/2/114

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 22Mg(α,p)25Al”, Comm. Phys., vol. 21, no. 2, p. 169, Jun. 2011.

IEEE

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Issue

Vol. 21 No. 2 (2011)

Section

Papers

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