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

A new measurement of the 6Li(p,gamma)7Be cross section at LUNA

20 Jun 2017, 19:30
2h
Sala conferenze (Laboratori Nazionali del Sud)

Sala conferenze

Laboratori Nazionali del Sud

Via S. Sofia 62 I-95123 Catania Italy
Poster Stellar evolution and nucleosynthesis Poster session

Speaker

Rosanna Depalo (P)

Description

% % 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 +0.35in \evensidemargin -0.35in %\renewcommand{\rmdefault}{ptm} % to use Times font \long\def\TITLE#1{{\Large{\bf#1}}}\long\def\AUTHORS#1{ #1\\[3mm]} \long\def\AFFILIATION#1#2{$^{#1}\,$ #2\\} \begin{document} {\small \it Nuclear Physics in Astrophysics 8, NPA8: 18-23 June 2017, Catania, Italy} \vspace{12pt} \thispagestyle{empty} \begin{center} %%% %%% Title goes here. %%% \TITLE{A new measurement of the $^{6}$Li(p,$\gamma$)$^{7}$Be cross section at LUNA}\\[3mm] %%% %%% Authors and affiliations are next. The presenter should be %%% underlined as shown below. %%% \AUTHORS{R. Depalo$^{1,2}$ for the LUNA collaboration } %%% {\small \it \AFFILIATION{1}{Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, Padova, Italy} \AFFILIATION{2}{INFN - Sezione di Padova, Padova, Italy} } %%% \vspace{12pt} % Do not modify % Enter contact e-mail address here. \centerline{Contact email: {\it rdepalo@pd.infn.it}} \vspace{18pt} % Do not modify \end{center} %%% %%% Abstract proper starts here. %%% The detection of $^{6}$Li in stars is a powerful tool for understanding the Big Bang nucleosynthesis, as well as the early stellar structure and evolution.\\ In stars, lithium is quickly destroyed during the pre-main sequence and main sequence phases, at temperatures of about 2 MK. Theoretical predictions of lithium abundances in the stellar surface are strongly dependent on the input physics and in many cases non-standard processes are required to explain the observed abundances [1].\\ The $^{6}$Li depletion proceeds mainly through the $^{6}$Li(p,$\alpha$)$^{3}$He reaction. This reaction has been studied by many groups, and in order to explain the angular distribution of the emitted alpha particles, an R-matrix fit of the experimental data requires the contribution of both negative and positive parity excited states [2]. \\ Although the existence of positive parity excited states in $^{7}$Be has never been confirmed experimentally, a recent measurement of the $^{6}$Li(p,$\gamma$)$^{7}$Be cross section revealed a possible resonance-like structure at center of mass energy of 195 keV [3]. The observed S-factor is reproduced by an R-matrix fit assuming the existence of an excited state with E $\approx$ 5800 keV and J$^{\pi}$ = (1/2$^{+}$, 3/2$^{+}$).\\ A new measurement of the $^{6}$Li(p,$\gamma$)$^{7}$Be cross section at proton energies between 50 and 400 keV has been performed at the Laboratory for Underground Nuclear Astrophysics. The poster provides a description of the experimental setup and preliminary results of the data analysis. \bigskip {\small \noindent [1] E. Tognelli et al. A\&A \textbf{548}, A41 (2012)\\ \noindent [2] J. Cruz et al. J. Phys. G Nucl. Part. Phys. \textbf{35}, 014004 (2008)\\ \noindent [3] J. J. He et al. Phys. Lett. B \textbf{725}, 287-291 (2013)\\ %%% %%% End of abstract. %%% \end{document}

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