Further Direct Approaches to the Nuclear Reactions in the Sun

Details Further Direct Approaches to the Nuclear Reactions in the Sun Further Direct Approaches to the Nuclear Reactions in the Sun

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..603g&link_type=abstract

Nuclear Physics A, v. 621, p. 603-606.

Physics

Nuclear Physics

Scientific paper

Nuclear fusion reactions play a key role in the understanding of energy production, neutrino emission and nucleosynthesis of the elements in stars. The direct measurement of the cross section of these reactions at the relevant energies is usually hampered by cosmic radiation, beam induced background and/or the radioactivity of the nuclei involved. This contribution presents the work of the LUNA (Laboratory for Underground Nuclear Astrophysics) and the NABONA (Napoli Bochum Nuclear Astrophysics) collaborations on new solutions applied to these old problems.

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