Coulomb breakup of 17Ne from the viewpoint of nuclear astrophysics
Paper in proceeding, 2012
By the Coulomb breakup of 17Ne, the time-reversed reaction 15O(2p,γ)17Ne has been studied. This reaction might play an important role in the rp process, as a break-out reaction of the hot CNO cycle. The secondary 17Ne ion beam with an energy of 500 MeV/nucleon has been dissociated in a Pb target. The reaction products have been detected with the LAND-R3B experimental setup at GSI. The preliminary differential and integral Coulomb dissociation cross section sCoul has been determined, which then will be converted into a photo-absorption cross section sphoto, and a two-proton radiative capture cross section σcap. Additionally, information about the structure of the 17Ne, a potential two-proton halo nucleus, will be received. The analysis is in progress. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
Author
J. Marganiec
Helmholtz
F. Aksouh
Helmholtz
The French Alternative Energies and Atomic Energy Commission (CEA)
Y. Aksyutina
Helmholtz
H. Alvarez-Pol
Universidade de Santiagode Compostela
T. Aumann
Technische Universität Darmstadt
Helmholtz
S. Beceiro-Novo
Universidade de Santiagode Compostela
C.A. Bertulani
Texas A&M University
K. Boretzky
Helmholtz
M. Borge
CSIC - Instituto de Estructura de la Materia (IEM)
M. Chartier
University of Liverpool
A. Chatillon
Helmholtz
L. V. Chulkov
Helmholtz
D. Cortina-Gil
Universidade de Santiagode Compostela
I. A. Egorova
Joint Institute for Nuclear Research (JINR)
H. Emling
Helmholtz
O. Ershova
Goethe University Frankfurt
Helmholtz
Christian Forssén
Chalmers, Fundamental Physics
L. M. Fraile
CERN
Complutense University
H. O. U. Fynbo
Aarhus University
D. Galaviz
CSIC - Instituto de Estructura de la Materia (IEM)
H. Geissel
Helmholtz
L Grigorenko
Joint Institute for Nuclear Research (JINR)
M. Heil
Helmholtz
D.H.H. Hoffmann
Technische Universität Darmstadt
J. Hoffmann
Helmholtz
Håkan T Johansson
Chalmers, Fundamental Physics
Björn Jonson
Chalmers, Fundamental Physics
C. Karagiannis
Helmholtz
O. Kiselev
Helmholtz
J.V. Kratz
Johannes Gutenberg University Mainz
R. Kulessa
Jagiellonian University in Kraków
N. Kurz
Helmholtz
C. Langer
Goethe University Frankfurt
Helmholtz
Mattias Lantz
Uppsala University
Krister Larsson
Helmholtz
T. Le Bleis
Helmholtz
Technical University of Munich
R.C. Lemmon
University of Liverpool
A. O. Lindahl
Y. Litvinov
Helmholtz
K. Mahata
Bhabha Atomic Research Centre (BARC)
Helmholtz
C. Muntz
Goethe University Frankfurt
Thomas Nilsson
Chalmers, Fundamental Physics
C. Nociforo
Helmholtz
Göran Hugo Nyman
Chalmers, Fundamental Physics
W. Ott
Helmholtz
V. Panin
Helmholtz
Technische Universität Darmstadt
Y. L. Parfenova
Joint Institute for Nuclear Research (JINR)
S. Paschalis
Technische Universität Darmstadt
University of Liverpool
A. Perea
CSIC - Instituto de Estructura de la Materia (IEM)
R. Plag
Goethe University Frankfurt
Helmholtz
R. Reifarth
Goethe University Frankfurt
Helmholtz
A. Richter
Technische Universität Darmstadt
C. Rodriguez-Tajes
National Research Centre "Kurchatov Institute"
Universidade de Santiagode Compostela
D. Rossi
Johannes Gutenberg University Mainz
Helmholtz
G. Schrieder
Technische Universität Darmstadt
N. B. Shulgina
National Research Centre "Kurchatov Institute"
H. Simon
Helmholtz
J. Stroth
Goethe University Frankfurt
K. Summerer
Helmholtz
J. T. Taylor
University of Liverpool
O. Tengblad
CSIC - Instituto de Estructura de la Materia (IEM)
Elisabeth Tengborn
F. Wamers
Technische Universität Darmstadt
Helmholtz
H. Weick
Helmholtz
C. Wimmer
Helmholtz
Goethe University Frankfurt
Mikhail Zhukov
Chalmers, Fundamental Physics
Proceedings of Science
18248039 (eISSN)
12th International Symposium on Nuclei in the Cosmos, NIC 2012
, Australia,
, Australia,
Subject Categories
Accelerator Physics and Instrumentation
Subatomic Physics
Organic Chemistry