Pregled bibliografske jedinice broj: 1049138
Toward a reassessment of the 19 F(p, α0) 16 O reaction rate at astrophysical temperatures
Toward a reassessment of the 19 F(p, α0) 16 O reaction rate at astrophysical temperatures // Physics letters. B, 748 (2015), 178-182 doi:10.1016/j.physletb.2015.06.073 (međunarodna recenzija, članak, znanstveni)
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Naslov
Toward a reassessment of the 19 F(p, α0) 16 O reaction rate at astrophysical temperatures
Autori
Lombardo, I. ; Dell'Aquila, Daniele ; Di Leva, A. ; Indelicato, I. ; La Cognata, M. ; La Commara, M. ; Ordine, A. ; Rigato, V. ; Romoli, M. ; Rosato, E. ; Spadaccini, G. ; Spitaleri, C. ; Tumino, A. ; Vigilante, M.
Izvornik
Physics letters. B (0370-2693) 748
(2015);
178-182
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
Nuclear Structure ; Nuclear Clustering ; Light nuclei ; Nuclear astrophysics
Sažetak
The 19F(p, α0)16O reaction at low energies plays an important role in fundamental physics. In particular in nuclear astrophysics it represents, together with the 19F(p, γ)20Ne reaction, the crossing point between the CNO and the NeNa cycles in stars. Further, in hydrogen-rich stellar environments, it is the most important fluorine destruction channel. In this paper we report new measurements on the 19F(p, α0)16O reaction at deeply sub-Coulomb energies (0.2-0.6 MeV), a region where, despite the key role of this reaction, very few and old data are reported. The deduced astrophysical S-factor is ≈1.5-2 times larger than currently adopted extrapolations with possibly important astrophysical consequences.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus