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• W3081920847 abstract "$^{25}mathrm{Mg}(p,ensuremath{gamma})^{26}mathrm{Al}$ is the most important reaction in the Mg-Al cycle in the hydrogen burning regions of stars. Its cross sections at stellar energies are essential to understand the issues of radioactive $^{26}mathrm{Al}$ in the galaxy and meteorites. The 57.7 keV resonance dominate the $^{25}mathrm{Mg}(p,ensuremath{gamma})^{26}mathrm{Al}$ astrophysical reaction rates at relative low temperature, but it is very difficult to measure its resonance strength directly, and the indirect measurement results deviate by a factor of about 2 by far. In this work, the angular distributions of $^{25}mathrm{Mg}(^{7}mathrm{Li},^{6}mathrm{He})^{26}mathrm{Al}$ leading to 6.364 MeV and eleven low-lying states in $^{26}mathrm{Al}$ have been measured by the Q3D magnetic spectrometer of the HI-13 tandem accelerator. The spectroscopic factors were derived and used to deduce the proton width and 57.7 keV resonance strength. The astrophysical $^{25}mathrm{Mg}(p,ensuremath{gamma})^{26}mathrm{Al}$ reaction rates at stellar energies have been updated by using the present result." @default.
• W3081920847 created "2020-09-08" @default.
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• W3081920847 date "2020-08-27" @default.
• W3081920847 modified "2023-10-14" @default.
• W3081920847 title "Indirect measurement of the 57.7 keV resonance strength for the astrophysical <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mi>γ</mml:mi></mml:math> -ray source of the <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mrow><mml:mmultiscripts><mml:mi>Mg</mml:mi><mml:mprescripts /><mml:none /><mml:mn>25</mml:mn></mml:mmultiscripts><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Al</mml:mi><mml:…" @default.
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• W3081920847 doi "https://doi.org/10.1103/physrevc.102.025804" @default.
• W3081920847 hasPublicationYear "2020" @default.
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