A New Measurement of the 8Li(α,n)11B Reaction for Astrophysical Interest

Details A New Measurement of the 8Li(α,n)11B Reaction for Astrophysical Interest A New Measurement of the 8Li(α,n)11B Reaction for Astrophysical Interest

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..847..374d&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Hori

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Interaction And Reaction Cross Sections, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments

Scientific paper

The 8Li(α,n)11B reaction has been measured directly and exclusively in the energy region of Ecm=0.45-1.75 MeV by using highly efficient detector system covering Ecm= 0.56 MeV, which corresponds to the Gamow window at T9=1. This experiment has been performed in the condition of inverse kinematics by using low-energy radioactive 8Li beam at the Tandem accelerator facility of Japan Atomic Energy Research Institute. The reaction cross section obtained in the present measurement is consistent with that of the previous exclusive measurements within the errors in an overlapping energy region, but is less than half of that of the inclusive measurements, in particular for lower energy region.

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