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Nuclear Physics in Astrophysics VIII

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

Session

RIBs in nuclear astrophysics 1

20 Jun 2017, 11:20
Sala conferenze (Laboratori Nazionali del Sud)

Sala conferenze

Laboratori Nazionali del Sud

Via S. Sofia 62 I-95123 Catania Italy

Presentation materials

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  1. 31. Beta decay spectroscopy studies of novae and x-ray bursts
    Chris Wrede (Michigan State University)
    20/06/2017, 11:20
    Explosive scenarios in astrophysics: observations, theory, and experiments
    Invited talk
    Nucleosynthesis and energy generation in classical novae and type I x-ray bursts are driven by nuclear reactions. Many of the thermonuclear rates have substantial uncertainties that preclude accurate comparisons between astronomical observations and astrophysical models. A program of beta decay measurements utilizing intense sources of rare isotopes adjacent to the proton drip line has been...
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  2. 66. Measurement of key resonance states for the $^{30}$P(p,$\gamma$)$^{31}$S reaction rate
    Dr Anu Kankainen (University of Jyväskylä)
    20/06/2017, 11:50
    Explosive scenarios in astrophysics: observations, theory, and experiments
    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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  3. 86. Constraining the 19Ne(p,γ)20Na Reaction Rate Using Direct Measurements at DRAGON
    Mr Ryan Wilkinson (University of Surrey)
    20/06/2017, 12:10
    Explosive scenarios in astrophysics: observations, theory, and experiments
    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. 79. Understanding the origin of ``nova'' grains and the $^{13}$N($\alpha$,p)$^{16}$O reaction
    Dr Nicolas de Séréville (IPN Orsay)
    20/06/2017, 12:30
    Explosive scenarios in astrophysics: observations, theory, and experiments
    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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  5. 57. Commissioning of the BRIKEN beta-delayed neutron detector for the study of exotic neutron-rich nuclei
    Alvaro Tolosa Delgado (IFIC (Instituto de Fisica Corpuscular))
    20/06/2017, 12:50
    Tools, techniques and facilities
    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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  6. 119. Isomer beam elastic scattering: 26mAl(p,p) for astrophysics
    Dr Daid Kahl (University of Edinburgh)
    20/06/2017, 13:10
    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 -0.35in \topmargin 0.305in \oddsidemargin...
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