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arXiv · 0806.2174

Astrophysical S-factor for $^{16}$O+$^{16}$O within the adiabatic molecular picture

Alexis Diaz-Torres·Leandro Romero Gasques·Michael Wiescher
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Abstract

The astrophysical S-factor for $^{16}$O + $^{16}$O 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 $^{16}$O + $^{16}$O fusion cross section at deep sub-barrier energies.

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Alexis Diaz-Torres, Leandro Romero Gasques, Michael Wiescher. 2008-06-13. Astrophysical S-factor for $^{16}$O+$^{16}$O within the adiabatic molecular picture. https://doi.org/10.1142/s0218301308011331

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