Ms
Gwenaelle Gilardy
(University of Notre Dame)
20/06/2017, 19:30
Poster
At 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...
Rosanna Depalo
(P)
20/06/2017, 19:30
Stellar evolution and nucleosynthesis
Poster
%
% 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 ...
Dr
Tamás Szücs
(MTA Atomki)
20/06/2017, 19:30
Poster
%
% 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 ...
Prof.
Tatyana Belyaeva
(Universidad Autonoma del Estado de Mexico)
20/06/2017, 19:30
Indirect methods in nuclear astrophysics
Poster
%
% 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 ...
Mr
Juan Carlos Morales-Rivera
(Universidad Autónoma del Estado de México), Prof.
Tatyana Belyaeva
(Universidad Autonoma del Estado de Mexico)
20/06/2017, 19:30
Indirect methods in nuclear astrophysics
Poster
%
% 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...
Dr
Svetlana Chesnevskaya
(IFIN-HH (ELI-NP))
20/06/2017, 19:30
Nuclear astrophysics with lasers
Poster
S. 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...
Mr
Matthew Williams
(University of York / TRIUMF)
20/06/2017, 19:30
Tools, techniques and facilities
Poster
The 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...
Dr
Tatyana Belyaeva
(Universidad Autónoma del Estado de México)
20/06/2017, 19:30
Poster
\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....
Oscar Trippella
(PG)
20/06/2017, 19:30
Indirect methods in nuclear astrophysics
Poster
%
% 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 ...
Giovanni Francesco Ciani
(GSSI)
20/06/2017, 19:30
Poster
Heaviest 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...
Prof.
J.E. Horvath
(IAG-USP, Sao Paulo, Brazil)
20/06/2017, 19:30
Poster
\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:...
Ms
Laetitia Canete
(University of Jyväskylä)
20/06/2017, 19:30
Tools, techniques and facilities
Poster
% 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 ...
Mr
Laszlo Csedreki
(INFN LNGS)
20/06/2017, 19:30
Poster
Nuclear 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...
Mrs
Aleksandra Cvetinović
(INFN-LNS Catania)
20/06/2017, 19:30
Poster
For 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,...
Carmen Altana
(LNS)
20/06/2017, 19:30
Poster
The 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...
Mr
Stefan Fiebiger
(Goethe University Frankfurt)
20/06/2017, 19:30
Stellar evolution and nucleosynthesis
Poster
%
% 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 ...
Ms
Magdalena Skurzok
(Jagiellonian University)
20/06/2017, 19:30
Poster
Search 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...
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, 19:30
Poster
% 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...
Prof.
Sandrine Courtin
(IPHC Strasbourg)
20/06/2017, 19:30
Poster
The 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...
Mr
Heinrich Wilsenach
(TU-Dresden, IKTP)
20/06/2017, 19:30
Stellar evolution and nucleosynthesis
Poster
%
% 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 ...
Dr
Ivano Lombardo
(Università di Napoli Federico II and INFN - Sez. Napoli)
20/06/2017, 19:30
Poster
The 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...
Prof.
Rene Reifarth
(Goethe University Frankfurt)
20/06/2017, 19:30
Poster
Isomers 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...
Emily Kading
(Graduate Student)
20/06/2017, 19:30
Big Bang nucleosynthesis and the early universe
Poster
%
% 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 ...
