A measurement of the Ne-22(n, gamma)Ne-23 capture cross section at a stellar temperature of kT = 25 keV
A measurement of the Ne-22(n, gamma)Ne-23 capture cross section at a stellar temperature of kT = 25 keV
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kT = 25 keV 恒星温度下 Ne-22(n, gamma)Ne-23 俘获截面的测量
DOI:
10.1086/170518
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发表时间:
1991
期刊:
影响因子:
--
通讯作者:
F. Kaeppeler
中科院分区:
文献类型:
--
作者:
H. Beer;G. Rupp;F. Voss;F. Kaeppeler
The capture cross section of 22 Ne has been determined by a fast cyclic activation technique. The measurements were carried out at the Karlsruhe 3.75 MV pulsed Van de Graaff accelerator using the 7 Li(p, n) reaction close to the reaction threshold to generate neutrons with a distribution resembling a Maxwell spectrum of kT=25 keV. The activation samples consisted of a mixture of enriched 22 Ne (99.9%) and natural Kr-gas contained in stainless steel spheres (20 mm diameter and 0.5 mm wall thickness). The activity of the samples was counted with a high-resolution Ge(Li) detector via the characteristic 439 keV 23 Ne γ-ray line. The 22 Ne capture cross section at kT=25 keV was found to be 66.0±5.0 μbarn