Dr
Faïrouz Hammache
(IPN-Orsay)
22/06/2017, 16:50
Indirect methods in nuclear astrophysics
Invited talk
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Dr
Neven Soic
(Rudjer Boskovic Institute Zagreb Croatia)
22/06/2017, 17:20
Indirect methods in nuclear astrophysics
Invited talk
Detailed knowledge on complex spectroscopy of the $^{24}$Mg nucleus at excitation energies between 14 and 19 MeV has large impact on understanding of clustering in nuclei and on carbon - carbon burning, the $^{12}$C+$^{12}$C fusion, in massive stars. The $^{12}$C+$^{12}$C and $^{16}$O+$^{8}$Be cluster structures (threshold energies are 13.9 and 14.1 MeV respectively) become active in this...
Sebastiana Maria Puglia
(LNS)
22/06/2017, 17:50
Oral
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Mr
Jos Riley
(University of York)
22/06/2017, 18:10
Oral
Classical novae are the most common astrophysical thermonuclear explosion [1] and are thought to contribute noticeably to the galactic chemical evolution [2,3]. As one of the few environments that can be modeled primarily from experimental nuclear data, observations would provide a direct test for current hydrodynamic codes. 18F produced in the runaway is the strongest 𝛾-ray source [4]...
Dr
Vaclav Burjan
(Nuclear Physics Institute, CAS)
22/06/2017, 18:30
Oral
Nuclear Physics in Astrophysics 8, NPA8: 18-23 June 2017, Catania, Italy
The direct 18O(p; °)19F capture and the ANC method.
V. Burjan1, Z. Hons1, V. Kroha1, J. Mr¶azek1, ·S. Pisko·r1, A. M. Mukhamedzhanov2,
L. Trache2, R. E. Tribble2, M. La Cognata3, L. Lamia3, G. R. Pizzone3, S. Romano3,
C. Spitaleri3 and A. Tumino3;4
1 Nuclear Physics Institute of Czech Academy of Sciences, 250 68...
