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Ms Gwenaelle Gilardy (University of Notre Dame)20/06/2017, 19:30PosterAt the end of its life, a massive star collapses into a neutron star. The neutrino flux released during the collapse is so significant that the probability of a neutrino interacting with a nucleus is enhanced enough to have an influence on element nucleosynthesis [1]. The origins of light elements, specifically $^{11}B$, is not fully understood. The $\nu$-process has been proposed as a...Go to contribution page
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Rosanna Depalo (P)20/06/2017, 19:30Stellar evolution and nucleosynthesisPoster% % 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 Tamás Szücs (MTA Atomki)20/06/2017, 19:30Poster% % 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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Prof. Tatyana Belyaeva (Universidad Autonoma del Estado de Mexico)20/06/2017, 19:30Indirect methods in nuclear astrophysicsPoster% % 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 Juan Carlos Morales-Rivera (Universidad Autónoma del Estado de México), Prof. Tatyana Belyaeva (Universidad Autonoma del Estado de Mexico)20/06/2017, 19:30Indirect methods in nuclear astrophysicsPoster% % Nuclear Physics in Astrophysics 8 template for abstract % % Format: LaTeX2e. % \documentclass[11pt]{article} \usepackage{graphicx} % % PAGE LAYOUT: % \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset -0.35in \topmargin 0.305in \oddsidemargin +0.35in \evensidemargin...Go to contribution page
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Diego Vescovi (PG)20/06/2017, 19:30PosterThe nucleosynthesis of 7Li represents one of the most crucial problems in nuclear astrophysics. The 7Li abundances of several atrophysical sites are hard to be reproduced: in particular, the 7Li abundance observed in the solar photosphere appears to be about 100 times lower than in meteorites. Recently, a new model for non-convective mixing mechanism induced by magnetohydrodynamics (MHD) was...Go to contribution page
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Dr Svetlana Chesnevskaya (IFIN-HH (ELI-NP))20/06/2017, 19:30Nuclear astrophysics with lasersPosterS. Chesnevskaya1, C.Matei1, D.L. Balabanski1, D.M. Filipescu1, D.G. Ghita1, A. Rotaru1, A. State1, Y. Xu1 G.L. Guardo2, M. La Cognata2, D. Lattuada2, C. Spitaleri2 1. ELI-NP/ IFIN-HH, 30 Reactorului Street, 077125 Magurele, Romania 2. INFN, Laboratori Nazionali del Sud, Via Santa Sofia 62, 95123 Catania, Italy Position-sensitive silicon strip detectors represent one of the best...Go to contribution page
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Mr Matthew Williams (University of York / TRIUMF)20/06/2017, 19:30Tools, techniques and facilitiesPosterThe electromagnetic mass analyser (EMMA) is a new vacuum-mode recoil mass spectrometer located at the ISAC-II facility at TRIUMF, Vancouver, Canada. Assembly of the spectrometer was completed in 2016, and it received first beam in December 2016. The first in-beam test consisted of an 80 MeV 36Ar beam impinged on a 4.46 μm 197Au foil. The initial test proved to be very successful, with the...Go to contribution page
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Dr Tatyana Belyaeva (Universidad Autónoma del Estado de México)20/06/2017, 19:30Poster\thispagestyle{empty} \begin{center} %%% %%% Title goes here. %%% \TITLE{Critial interaction and strong-absorption distances for the $^{7}$Li $+$ $^{58}$Ni system }\\[3mm] %%% %%% Authors and affiliations are next. The presenter should be %%% underlined as shown below. %%% \AUTHORS{P. Amador-Valenzuela$^{1}$, E.F. Aguilera$^1$, E. Martinez-Quiroz$^1$, D. Lizcano$^1$, J.C....Go to contribution page
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Oscar Trippella (PG)20/06/2017, 19:30Indirect methods in nuclear astrophysicsPoster% % 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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Giovanni Francesco Ciani (GSSI)20/06/2017, 19:30PosterHeaviest nuclei (A > 58) are synthesized by sequential neutron capture reactions. There are two main processes, depending on their time scale compared with the beta decay lifetime: these are the so called slow (s) and rapid (r) processes. Both produce about half of the stable isotopes beyond iron in the Universe [1]. Focusing on the s process, these take place in low mass (1 − 3M⊙) Asymptotic...Go to contribution page
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Prof. J.E. Horvath (IAG-USP, Sao Paulo, Brazil)20/06/2017, 19:30Poster\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:...Go to contribution page
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Ms Laetitia Canete (University of Jyväskylä)20/06/2017, 19:30Tools, techniques and facilitiesPoster% Format: LaTeX2e. % % canete.tex % % \documentstyle[11pt]{article} \textheight=9.9in \textwidth=6.3in \voffset -0.85in \hoffset -0.35in \topmargin 0.305in \oddsidemargin +0.35in \evensidemargin -0.35in \long\def\TITLE#1{{\Large{\bf#1}}}\long\def\AUTHORS#1{ #1\\[3mm]} \long\def\AFFILIATION#1#2{$^{#1}\,$ #2\\} \begin{document} {\small \it ...Go to contribution page
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Mr Laszlo Csedreki (INFN LNGS)20/06/2017, 19:30PosterNuclear Physics in Astrophysics 8, NPA8: 18-23 June 2017, Catania, Italy Introduction of the new LUNA experimental setup for high precision measurement of 13C(α,n)16O reaction for astrophysical purposes L. Csedreki1, G. F. Ciani2, I. Kochanek1 for the LUNA collaboration 1 INFN, Laboratori Nazionali del Gran Sasso LNGS, Assergi, Italy 2 Gran Sasso Science Institute, L’Aquila Contact...Go to contribution page
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Mrs Aleksandra Cvetinović (INFN-LNS Catania)20/06/2017, 19:30PosterFor nucleosynthesis calculations precise reaction rates should be known at energies close to the Gamow peak. Accurate measurements of nuclear reactions performed at these energies [1-5] shows an unexpected enhancement of the cross section at the lowest measurable energies that is attributed to the presence of atomic electrons in the target. In order to observe the bare nuclear cross section,...Go to contribution page
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Carmen Altana (LNS)20/06/2017, 19:30PosterThe future availability of high-intensity laser facilities capable of delivering tens of Petawatts of power (e.g. ELI-NP) into small volumes of matter at high repetition rates will give the unique opportunity to investigate nuclear reactions and fundamental interactions under the extreme plasma conditions realized by laser-matter interactions. Nuclear reactions of astrophysical interest are...Go to contribution page
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Mr Stefan Fiebiger (Goethe University Frankfurt)20/06/2017, 19:30Stellar evolution and nucleosynthesisPoster% % 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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Ms Magdalena Skurzok (Jagiellonian University)20/06/2017, 19:30PosterSearch for Deeply Bound Kaonic Nuclear States in AMADEUS experiment M. Skurzok1,2, C. Curceanu2, L. Fabbietti3,4, R. del Grande2,5, P. Moskal1, K. Piscicchia2,6, A. Scordo2, D. L. Sirghi2, Oton Vazquez Doce3,4 1 Institute of Physics, Jagiellonian University, 30-059 Krakow, Poland 2 INFN, Laboratori Nazionali di Frascati, 00044 Frascati, Italy 3 Excellence Cluster Origin and...Go to contribution page
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Dr Aliya Nurmukhanbetova (National Laboratory Astana, Nazarbayev University, Astana, 010000,Kazakhstan), Mr Dosbol Nauruzbayev (National Laboratory Astana, Nazarbayev University, Astana, 010000,Kazakhstan)20/06/2017, 19:30Poster% 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...Go to contribution page
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Prof. Sandrine Courtin (IPHC Strasbourg)20/06/2017, 19:30PosterThe STELLA (STELlar LAboratory) experimental station for the measurement of sub-barrier light heavy ion fusion cross sections has been commissioned at the Androm\`{e}de accelerator at IPN, Orsay. These measurements can yield both insight into nuclear cluster effects~[1] and the $S$-factors at energies of astrophysical interest. In particular, $^{12}$C+$^{12}$C fusion was identified as a key...Go to contribution page
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Mr Heinrich Wilsenach (TU-Dresden, IKTP)20/06/2017, 19:30Stellar evolution and nucleosynthesisPoster% % 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 Ivano Lombardo (Università di Napoli Federico II and INFN - Sez. Napoli)20/06/2017, 19:30PosterThe study of $^{13}$C structure allows to understand the effects of clusterization in light non-self-conjugated nuclei. The possible presence of rotational bands built on molecular states has been suggested in several papers [1,2]. Furthermore, in recent times, some theoretical papers [3,4] predicted the possible existence of states corresponding to the coupling of a valence neutrons to the...Go to contribution page
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Prof. Rene Reifarth (Goethe University Frankfurt)20/06/2017, 19:30PosterIsomers are metastable states of atomic nuclei. Their half-lifes are about 100 to 1000 times longer than those of the excited nuclear states with prompt g-emissions. If the conditions in an application change on the time scale of isomers' half lifes, their abundances have to be tracked explicitly. The high temperatures under stellar conditions enable the population of higher-lying states...Go to contribution page
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Emily Kading (Graduate Student)20/06/2017, 19:30Big Bang nucleosynthesis and the early universePoster% % 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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