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Scientific paper - Original scientific paper
The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars
Astrophysical Journal, 860 (2018), 1; 61. https://doi.org/10.3847/1538-4357/aac207
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 More authors...

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D'Agata, G., Pizzone, R., La Cognata, M., Indelicato, I., Spitaleri, C., Palmerini, S. ... Uroić, M. (2018). The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars. Astrophysical Journal, 860. (1). doi: 10.3847/1538-4357/aac207

D'Agata, G., et al. "The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars." Astrophysical Journal, vol. 860, no. 1, 2018. https://doi.org/10.3847/1538-4357/aac207

D'Agata, G., R.G. Pizzone, M. La Cognata, I. Indelicato, C. Spitaleri, S. Palmerini, O. Trippella, et al. "The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars." Astrophysical Journal 860, no. 1 (2018). https://doi.org/10.3847/1538-4357/aac207

D'Agata, G., et al. (2018) 'The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars', Astrophysical Journal, 860(1). doi: 10.3847/1538-4357/aac207

D'Agata G, Pizzone R, La Cognata M, Indelicato I, Spitaleri C, Palmerini S, and sur.. The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars. Astrophysical Journal [Internet]. 2018 [cited 2024 October 29];860(1). doi: 10.3847/1538-4357/aac207

G. D'Agata, et al., "The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars", Astrophysical Journal, vol. 860, no. 1, 2018. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:622288. [Accessed: 29 October 2024]

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Title (english)The 19F(α, p)22Ne Reaction at Energies of Astrophysical Relevance by Means of the Trojan Horse Method and Its Implications in AGB Stars
AuthorG. D'Agata
AuthorR.G. Pizzone
AuthorM. La Cognata
AuthorI. Indelicato
AuthorC. Spitaleri
AuthorS. Palmerini
AuthorO. Trippella
AuthorD. Vescovi
AuthorSaša Blagus
MBZ: 3964
AuthorS. Cherubini
AuthorP. Figuera
AuthorL. Grass
AuthorG.L. Guardo
AuthorM. Gulino
AuthorS. Hayakawa
AuthorR. Kshetri
AuthorL. Lamia
AuthorM. Lattuada
AuthorTea Mijatović
MBZ: 330335
AuthorMatko Milin
MBZ: 233723
AuthorĐuro Miljanić
MBZ: 31583
AuthorLovro Prepolec
MBZ: 326842
AuthorG.G. Rapisarda
AuthorS. Romano
AuthorM.L. Sergi
AuthorNatko Skukan
AuthorNeven Soić
MBZ: 184260
AuthorVedrana Tokić
MBZ: 340145
AuthorA. Tumino
AuthorMilivoj Uroić
MBZ: 221764
Author's institutionUniversity of Zagreb
Faculty of Science
(Department of Physics)
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Astronomy and Astrophysics
Abstract (english)
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.
Keywords (english)
Languageenglish
Publication typeScientific paper - Original scientific paper
Publication statusPublished
Peer reviewPeer review - international
Publication versionPublished version
Journal titleAstrophysical Journal
Numberingvol. 860, no. 1, 61
p-ISSN0004-637X
e-ISSN1538-4357
DOIhttps://doi.org/10.3847/1538-4357/aac207
URN:NBNurn:nbn:hr:217:622288
Publication2018
Document URLhttps://iopscience.iop.org/article/10.3847/1538-4357/aac207
Type of resourceText
Access conditionsOpen access
Terms of useLicence In copyright icon
Public note© 2018. The American Astronomical Society. Received 2018 January 16; Revised 2018 March 27; Accepted 2018 April 27; Published 2018 June 12.
Created on2020-02-29 22:03:10