Feasibility Study of Direct Measurement of Stellar Reaction 22Mg(α,p)25Al
Author affiliations
DOI:
https://doi.org/10.15625/0868-3166/21/2/114Keywords:
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.Downloads
Download data is not yet available.
Metrics
Metrics Loading ...
Downloads
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.
Issue
Section
Papers
License
Authors who publish with CIP agree with the following terms:- The manuscript is not under consideration for publication elsewhere. When a manuscript is accepted for publication, the author agrees to automatic transfer of the copyright to the editorial office.
- The manuscript should not be published elsewhere in any language without the consent of the copyright holders. Authors have the right to enter into separate, additional contractual arrangements for the non-exclusive distribution of the journal’s published version of their work (e.g., post it to an institutional repository or publish it in a book), with an acknowledgement of its initial publication in this journal.
- Authors are encouraged to post their work online (e.g., in institutional repositories or on their websites) prior to or during the submission process, as it can lead to productive exchanges or/and greater number of citation to the to-be-published work (See The Effect of Open Access).
Published 30-06-2011
