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

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dc.creatorDiaz-Torres, Alexis
dc.creatorGasques, Leandro Romero
dc.creatorWiescher, Michael
dc.date2008-06-13
dc.date.accessioned2026-07-07T12:32:18Z
dc.date.available2026-07-07T12:32:18Z
dc.descriptionThe 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.
dc.description5 pages, 2 figures, SOTANCP2008 Conference, Strasbourg, France, May 13-16, 2008, To appear in IJMPE
dc.identifierhttps://arxiv.org/abs/0806.2174
dc.identifierhttp://arxiv.org/abs/0806.2174
dc.identifierInt.J.Mod.Phys.E17:2194-2198,2008
dc.identifierdoi:10.1142/S0218301308011331
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216740
dc.subjectNuclear Theory
dc.titleAstrophysical S-factor for $^{16}$O+$^{16}$O within the adiabatic molecular picture
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