Pregled bibliografske jedinice broj: 960488
The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars
The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars // The Astrophysical journal, 860 (2018), 1; 61, 11 doi:10.3847/1538-4357/aac207 (međunarodna recenzija, članak, znanstveni)
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Naslov
The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars
Autori
D'Agata, G. ; Pizzone, R.G. ; La Cognata, M. ; Indelicato, I. ; Spitaleri, C. ; Palmerini, S. ; Trippella, O. ; Vescovi, D. ; Blagus, Saša ; Cherubini, S. ; Figuera, P. ; Grass, L. ; Guardo, G.L. ; Gulino, M. ; Hayakawa, S. ; Kshetri, R. ; Lamia, L. ; Lattuada, M. ; Mijatović, Tea ; Milin, Matko ; Miljanić, Đuro ; Prepolec, Lovro ; Rapisarda, G.G. ; Romano, S. ; Sergi, M.L. ; Skukan, Natko ; Soić, Neven ; Tokić, Vedrana ; Tumino, A. ; Uroić, Milivoj
Izvornik
The Astrophysical journal (0004-637X) 860
(2018), 1;
61, 11
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
asymptotic giant branch ; thermonuclear reaction-rates ; wolf-rayet stars ; cross-sections ; fluorine ; f-19 ; nucleosynthesis ; abundances ; resonances ; CNO
Sažetak
The main source of F-19 in the universe has not yet been clearly identified and this issue represents one of the unanswered questions of stellar modeling. This lack of knowledge can be due to the F-19(alpha, p)Ne-22 reaction cross-section that has proven to be difficult at low energies: direct measurements stop only at about similar to 660 keV, leaving roughly half of the astrophysical relevant energy region (from 200 keV to 1.1 MeV) explored only by R-matrix calculations. In this work, we applied the Trojan Horse Method to the quasi-free three-body Li-6(F-19, p(22)Ne)d reaction performed at E-beam = 6 MeV in order to indirectly study the F-19(alpha, p)Ne-22 reaction in the sub-Coulomb energy region. In this way, we obtained the cross-section and the reaction rate in the temperature region of interest for astrophysics and free from electron screening effects. A brief analysis of the impact of the new measured reaction rate in AGB star nucleosynthesis is also presented.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Institut "Ruđer Bošković", Zagreb,
Prirodoslovno-matematički fakultet, Zagreb
Profili:
Lovro Prepolec
(autor)
Vedrana Tokić
(autor)
Đuro Miljanić
(autor)
Milivoj Uroić
(autor)
Tea Mijatović
(autor)
Matko Milin
(autor)
Saša Blagus
(autor)
Neven Soić
(autor)
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