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Dr Faïrouz Hammache (IPN-Orsay)22/06/2017, 16:50Indirect methods in nuclear astrophysicsInvited talk% % Nuclear Physics in Astrophysics 8 template for abstract % % Format: LaTeX2e. % % Rename this file to name.tex, where `name' is the family name % of the first author, and edit it to produce your abstract. % \documentstyle[11pt]{article} % % PAGE LAYOUT: % \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset ...Go to contribution page
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Dr Neven Soic (Rudjer Boskovic Institute Zagreb Croatia)22/06/2017, 17:20Indirect methods in nuclear astrophysicsInvited talkDetailed 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...Go to contribution page
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Sebastiana Maria Puglia (LNS)22/06/2017, 17:50Oral% % Nuclear Physics in Astrophysics 8 template for abstract % % Format: LaTeX2e. % % Rename this file to name.tex, where `name' is the family name % of the first author, and edit it to produce your abstract. % \documentstyle[11pt]{article} % % PAGE LAYOUT: % \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset ...Go to contribution page
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Mr Jos Riley (University of York)22/06/2017, 18:10OralClassical 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]...Go to contribution page
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Dr Vaclav Burjan (Nuclear Physics Institute, CAS)22/06/2017, 18:30OralNuclear 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...Go to contribution page
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