Direct Measurements of the Astrophysical (α, n) and (p, n) Reactions by Using Low-Energy Light Neutron-Rich Rnb

Details Direct Measurements of the Astrophysical (α, n) and (p, n) Reactions by Using Low-Energy Light Neutron-Rich Rnb Direct Measurements of the Astrophysical (α, n) and (p, n) Reactions by Using Low-Energy Light Neutron-Rich Rnb

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..316i&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astronomy

1

Scientific paper

An experimental program to measure reaction cross sections of (α, n) and (p, n) reactions on light neutron-rich nuclei by using low-energy radioactive nuclear beams is in progress at Tandem accelerator facility of Japan Atomic Energy Research Institute. Exclusive measurements of 8Li(α, n)11B and 16N(α, n)19F reaction cross sections have been performed successfully. Their excitation functions together with the experimental method are presented.

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