AGB nucleosynthesis: The 19F(α, p)22Ne reaction at astrophysical energies (CROSBI ID 650616)
Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
D'Agata, G. ; Pizzone, R.G., Spitaleri, C. ; Blagus, Saša ; Figuera, P. ; Grassi, L. ; Guardo, G.L. ; Gulino, M. ; Hayakawa, S. ; Indelicato, I. ; Kshetri, R. ; La Cognata, M. ; Lamia, L. ; Lattuada, M. ; Mijatović, Tea ; Milin, Matko ; Miljanić, Đuro ; Prepolec, Lovro ; Sergi, M.L. ; Skukan, Natko ; Soić, Neven ; Tokić, Vedrana ; Tumino, A. ; Uroić, Milivoj
engleski
AGB nucleosynthesis: The 19F(α, p)22Ne reaction at astrophysical energies
Learning how 19F is produced and destructed in AGB-stars is crucial. Fluorine abundance is in fact important, given that it is strongly tied to standard and extra-mixing processes taking place in AGB-stars. This kind of objects are considered to be the main sources of fluorine in galactic environment, in which experimental abundances are far overestimated. For this reason the reaction 19F(α, p)22Ne, that represents the main destruction channel in He-rich environment, was studied at energies corresponding to T~2·10^8 K.
nuclear reactions ; nuclear structure
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Podaci o prilogu
080001-1-080001-5.
2017.
objavljeno
Podaci o matičnoj publikaciji
Exotic nuclei and nuclear/particle astrophysics (VI). Physics with small accelerators: Proceedings of Carpathian Summer School of Physics 2016 (CSSP16)
Trache, L. ; Ghita, D.G.
Melville (NY): American Institute of Physics (AIP)
Podaci o skupu
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predavanje
29.02.1904-29.02.2096
