کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1854530 1035840 2011 6 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
p-process nucleosynthesis: Activation experiments
موضوعات مرتبط
مهندسی و علوم پایه فیزیک و نجوم فیزیک هسته ای و انرژی بالا
پیش نمایش صفحه اول مقاله
p-process nucleosynthesis: Activation experiments
چکیده انگلیسی

For the astrophysical p   process a complex reaction network has to be solved. In the order of 10,000 theoretically predicted reaction rates are needed for simulations of this network. For reactions involving αα particles or protons, the predictions in the framework of the Hauser–Feshbach (HF) model were found to deviate from experimental results partially by a factor of 55 or even more. To optimize the predictive power of the applied HF codes, the nuclear physics input has to be improved. For this purpose, the reactions 166Er(α,n) and 169Tm(p,n) as well as the reaction 170Yb(γ,n) have been measured with the activation method at low energies. The data can provide a further test of HF predictions but can also be used to optimize input parameters of the afore mentioned codes. Preliminary results of the experiments are presented and compared to theoretical predictions using the standard settings of the HF codes NON-SMOKER and TALYS.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Progress in Particle and Nuclear Physics - Volume 66, Issue 2, April 2011, Pages 379–384
نویسندگان
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