Astrophysical S-Factor for 16 0+ 16 0 within the Adiabatic Molecular Picture
Date
2008
Authors
Diaz-Torres, Alexis
Gasques, Leandro Romero
Wiescher, M.
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World Scientific Publishing Company
Abstract
The astrophysical S-factor for 16O+16O is investigated within the adiabatic molecular picture. It very well explains the available experimental data. The collective radial mass causes a pronounced resonant structure in the S-factor excitation function, providing a motivation for measuring the 16O+16O fusion cross section at deep sub-barrier energies
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International Journal of Modern Physics E - Nuclear Physics
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Journal article
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2037-12-31