تم الدراسة للتفاعل 24Mg(3He,t)24Al عند E(3He)=420 MeV. تم الحصول على دقة انطلاقية بقيمة 35 كيلو فولت. يتم استخراج قوى Gamow-Teller لمستويات معينة في 24Al باستخدام علاقة تجريبية حديثة للتناسب بين قوى Gamow-Teller وخطوط الانحدار المختلطة في نقطة صفر لنقل الحزمة. إلا أنه تم العثور على اختلافات صغيرة لبعض التثاقلات الضعيفة، تم الحصول على اتفاق جيد مع بيانات 24Mg(p,n) السابقة والحسابات الهيكلية للنووية التي تستخدم التفاعلات USDA/B في مساحة النموذج الصحافي sd. تم قياس انطلاقية التثاقل لعدد من المستويات في 24Al التي تؤثر على تحديد معدل التفاعل 23Mg(p,gamma)24Al الحراري. وتظهر النتائج متطابقة مع اثنين من التفاعلات الثالثة (3He,t) التي تم تنفيذها في طاقات حزمة أقل بكثير. ومع ذلك، تم العثور على وضعية جديدة عند Ex(24Al)=2.605(10) MeV وهي الوضعية الثالثة أعلى من انطلاقية فصل البروتون.
The 24Mg(3He,t)24Al reaction has been studied at E(3He)=420 MeV. An energy resolution of 35 keV was achieved. Gamow-Teller strengths to discrete levels in 24Al are extracted by using a recently developed empirical relationship for the proportionality between Gamow-Teller strengths and differential cross sections at zero momentum transfer. Except for small discrepancies for a few weak excitations, good agreement with previous 24Mg(p,n) data and nuclear-structure calculations using the USDA/B interactions in the sd shell-model space is found. The excitation energy of several levels in 24Al of significance for determination of the 23Mg(p,gamma)24Al thermonuclear reaction rate were measured. Results are consistent with two of the three previous (3He,t) measurements, performed at much lower beam energies. However, a new state at Ex(24Al)=2.605(10) MeV was found and is the third state above the proton separation energy.
Gamow-Teller transitions from 24Mg to 24Na were studied via the (t,3He) reaction at 115 AMeV using a secondary triton beam produced via fast fragmentation of 150 AMeV 16O ions. Compared to previous (t,3He) experiments at this energy that employed a p
Differential cross sections for transitions of known weak strength were measured with the (3He,t) reaction at 420 MeV on targets of 12C, 13C, 18O, 26Mg, 58Ni, 60Ni, 90Zr, 118Sn, 120Sn and 208Pb. Using this data, it is shown the proportionalities betw
Electron capture and beta decay play important roles in the evolution of pre-supernovae stars and their eventual core collapse. These rates are normally predicted through shell-model calculations. Experimentally determined strength distributions from
Charge-exchange reactions are an important tool for determining weak-interaction rates. They provide stringent tests for nuclear structure models necessary for modeling astrophysical environments such as neutron stars and core-collapse supernovae. In
The proportionality between differential cross sections at vanishing linear momentum transfer and Gamow-Teller transition strength, expressed in terms of the textit{unit cross section} ($hat{sigma}_{GT}$) was studied as a function of target mass numb