18–23 Jun 2017
Laboratori Nazionali del Sud
Europe/Rome timezone

Session

r-process 2

19 Jun 2017, 14:30
Sala conferenze (Laboratori Nazionali del Sud)

Sala conferenze

Laboratori Nazionali del Sud

Via S. Sofia 62 I-95123 Catania Italy

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  1. Stephane Goriely (Universite Libre de Bruxelles)
    19/06/2017, 14:30
    Invited talk
    The r-process nucleosynthesis and related nuclear challenges S. Goriely Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, Belgium Contact email: sgoriely@astro.ulb.ac.be The rapid neutron-capture process, or r-process, is known to be of fundamental importance for explaining the origin of approximately half of the A > 60 stable nuclei observed in nature. In...
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  2. Dr Jesús Casal (ECT*)
    19/06/2017, 15:00
    Indirect methods in nuclear astrophysics
    Oral
  3. Georgios Perdikakis (Central Michigan University)
    19/06/2017, 15:20
    Oral
    % % 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 ...
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  4. Clemens Wolf (Goethe-University Frankfurt)
    19/06/2017, 15:40
    Oral
    The $^{23}$Al(p,$\gamma$)$^{24}$Si stellar reaction rate has a significant impact of the light-curve emitted in X-ray bursts. Theoretical calculation shows that the reaction rate is mainly determined by the properties of direct capture as well as low-lying 2$^{+}$ states and a possible 4$^{+}$ state in $^{24}$Si. Currently, there is little experimental information on the properties of these...
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