Astrophysical neutron capture rates in s- and r-process nucleosynthesis
核实验
2007-05-23 v1 核理论
摘要
Astrophysical neutron capture rates of light and heavy nuclei have been measured and calculated. For the measurements the activation technique was applied at the 3.75 MV Karlsruhe Van de Graaff accelerator, and at the Geel electron linear accelerator (GELINA) the time-of-flight (TOF) method was used. The calculations were performed using direct and compound nuclear capture models.
引用
@article{arxiv.nucl-ex/9706002,
title = {Astrophysical neutron capture rates in s- and r-process nucleosynthesis},
author = {H. Beer and P. Mohr and H. Oberhummer and T. Rauscher and P. Mutti and F. Corvi and P. V. Sedyshev and Yu. P. Popov},
journal= {arXiv preprint arXiv:nucl-ex/9706002},
year = {2007}
}
备注
10 pages, uses LaTeX2e with epsf.sty and camready.sty (included), 10 postscript figures with psfig (included), Proceedings of the International Seminar on Interaction of Neutrons with Nuclei, 14.-17 May 1997, Dubna, Russia