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

1997/06/05 by H. Beer, Peter J. Mohr, P. Mohr +15
Medicine · Physics and Astronomy · #FOS: Physical sciences #Nuclear Experiment (nucl-ex) #Nuclear Physics and Applications #Nuclear Theory (nucl-th) #Nuclear physics research studies #Radiation Therapy and Dosimetry #nucl-ex #nucl-th

paper · pdf · doi:10.48550/arxiv.nucl-ex/9706002

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

arxiv created 1997/06/05 · openalex publication_date 1997/06/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

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.

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