Astrophysical neutron capture rates in s- and r-process nucleosynthesis

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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.
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

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Nuclear Experiment, Nuclear Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/81371

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/nucl-ex/9706002
 http://arxiv.org/abs/nucl-ex/9706002

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arXiv