The 14N+p is the bottleneck of the CNO cycle and determines the CNO neutrinos from the Sun. Those have been recently observed by Borexino and this information can be used to determine the CNO abundances in the Sun core. The new accelerator installed at the Gran Sasso National Laboratory can provide the cross section for this reaction in a wide energy range.
The 14N+p is the bottleneck of the CNO cycle and determines the CNO neutrinos from the Sun. Those have been recently observed by Borexino and this information can be used to determine the CNO abundances in the Sun core. The new accelerator installed at the Gran Sasso National Laboratory can provide the cross section for this reaction in a wide energy range.
Study of the 14N(p,g)15O reaction in a wide energy range in underground with LUNA
VIGOLO, ANNA
2022/2023
Abstract
The 14N+p is the bottleneck of the CNO cycle and determines the CNO neutrinos from the Sun. Those have been recently observed by Borexino and this information can be used to determine the CNO abundances in the Sun core. The new accelerator installed at the Gran Sasso National Laboratory can provide the cross section for this reaction in a wide energy range.| File | Dimensione | Formato | |
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https://hdl.handle.net/20.500.12608/51910