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Nuclear Physics in Astrophysics VIII

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

Session

Indirect methods 1

22 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. 142. THM measurements in nuclear astrophysics: recent results and future perspectives
    Livio Lamia (LNS)
    22/06/2017, 14:30
    Invited talk
    Experimental nuclear astrophysics aims at measuring astrophysically relevant burning reaction cross sections at the corresponding Gamow energy. However, in spite of the improvements for measuring low-energy nuclear reaction cross sections, the Gamow energy region peak often remains far to be fully explored mainly in the case of charged-particles induced reactions. In such cases, both Coulomb...
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  2. 59. Reaction production + AMS: An alternative method to study (d,alpha)26Al and (p,gamma)26Al reactions at low energies
    LUIS ARMANDO ACOSTA SANCHEZ (CT)
    22/06/2017, 15:00
    Tools, techniques and facilities
    Invited talk
    It is well known the importance in Astrophysics of the reactions regarding 26Al. This radioisotope is presented for instance, in the stars where there is H, C and Ne fusion at high temperatures; as well it can be found inside meteorites where it can be deposited or to be created in situ [1]. Considering the importance of the 26Al nuclei, in this work are presented the rst results...
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  3. 18. Cross section measurement of 14N(p,gamma)15O using the activation method
    Dr György Gyürky (Institute for Nuclear Research (Atomki)
    22/06/2017, 15:30
    Indirect methods in nuclear astrophysics
    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. 93. Measurement of β-delayed protons from decay of 31Cl covering the Gamow window of 30P(p,γ)31S at typical nova temperatures
    Dr Antti Saastamoinen (Cyclotron Insitute, Texas A&M University)
    22/06/2017, 15:50
    Explosive scenarios in astrophysics: observations, theory, and experiments
    Oral
    The thermonuclear runaway in classical novae proceeds through radiative proton capture re- actions (p,γ) involving proton rich sd-shell nuclei close to the dripline. Many of the capture reactions at typical peak nova temperatures of 0.2-0.4 GK are dominated by resonant capture. Therefore, the key parameters in understanding the astrophysical reaction rates are the energies, decay widths and...
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