<sup>26</sup>Si + α resonant scattering measurement for the astrophysical <sup>26</sup>Si(α, p)<sup>29</sup>P reaction rate
ORAL
Abstract
The 26Si(α, p)29P reaction is considered to have astrophysical importance such as impact on X-ray burst light curves, or on the abundance of 26Al known as a galactic gamma ray source. The cross section of this reaction has, however, never been measured directly, and there was only a study of 30S resonances via limited information from the 28Si(3He, n)30S and 32S(p, t)30S reactions. We have performed both the 26Si(α, p)29P reaction direct measurement and the 26Si(α, α)26Si resonant scattering measurement in inverse kinematics to determine the reaction cross section at higher energies and to obtain alpha resonance information in the 30S compound system, respectively. The experiment employed the thick-gas-target inverse-kinematics method with a 26Si radioactive isotope (RI) produced at the Center-for-the-Nuclear-Study RI Beam Separator (CRIB) of the University of Tokyo. In the presentation, we will discuss the α resonant scattering result, which covers the excitation energy range of Ex = 12–16 MeV and was analyzed by R-matrix fit, to update the 26Si(α, p)29P thermal reaction rate.
*This work was supported by JSPS KAKENHI No. 18K13556.
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Presenters
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Seiya Hayakawa
- Center for Nuclear Study, the University of Tokyo