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

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

2008-06-13

arxiv.org/abs/0806.2174v1

Int.J.Mod.Phys.E17:2194-2198,2008

Physics

Nuclear Physics

Nuclear Theory

5 pages, 2 figures, SOTANCP2008 Conference, Strasbourg, France, May 13-16, 2008, To appear in IJMPE

Scientific paper

10.1142/S0218301308011331

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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