Experimental study of the O-15(2p, gamma) Ne-17 cross section by Coulomb Dissociation for the rp process
Paper in proceeding, 2016

The time-reversed reaction O-15(2p, gamma) Ne-17 has been studied by the Coulomb dissociation technique. Secondary 17Ne ion beams at 500 AMeV have been produced by fragmentation reactions of Ne-20 in a beryllium production target and dissociated on a secondary Pb target. The incoming beam and the reaction products have been identified with the kinematically complete LAND-(RB)-B-3 experimental setup at GSI. The excitation energy prior to decay has been reconstructed by using the invariant-mass method. The preliminary differential and integral Coulomb Dissociation cross sections (sigma(Coul)) have been calculated, which provide a photoabsorption (sigma(photo)) and a radiative capture cross section (sigma(cap)). Additionally, important information about the nuclear structure of the Ne-17 nucleus will be obtained. The analysis is in progress.

RADII

CAPTURE

Author

J. Marganiec

EMMI

F. Wamers

Technische Universität Darmstadt

F. Aksouh

Helmholtz

Y. Aksyutina

Helmholtz

H. Alvarez Pol

Universidade de Santiagode Compostela

T. Aumann

Technische Universität Darmstadt

S. Beceiro

Universidade de Santiagode Compostela

C. Bertulani

Texas A&M University

K. Boretzky

Helmholtz

M. J. Borge

CSIC - Instituto de Estructura de la Materia (IEM)

M. Chartier

University of Liverpool

A. Chatillon

Helmholtz

L. Chulkov

Helmholtz

D. Cortina-Gil

Universidade de Santiagode Compostela

I. Egorova

Dubna International University

H. Emling

Helmholtz

O. Ershova

Helmholtz

Christian Forssen

Chalmers, Physics, Subatomic and Plasma Physics

L. M. Fraile

CERN

H. Fynbo

Aarhus University

D. Galaviz

CSIC - Instituto de Estructura de la Materia (IEM)

H. Geissel

Helmholtz

L. Grigorenko

Dubna International University

M. Heil

Helmholtz

D. H. H. Hoffmann

Technische Universität Darmstadt

J. Hoffmann

Technische Universität Darmstadt

Håkan T Johansson

Chalmers, Physics, Subatomic and Plasma Physics

Björn Jonson

Chalmers, Physics, Subatomic and Plasma Physics

M. Karakoc

Akdeniz University

C. Karagiannis

Helmholtz

O. Kiselev

Helmholtz

J. V. Kratz

Johannes Gutenberg University Mainz

R. Kulessa

Jagiellonian University in Kraków

N. Kurz

Helmholtz

C. Langer

Helmholtz

Mattias Lantz

Chalmers, Physics, Subatomic and Plasma Physics

Kristian Larsson

Chalmers, Physics, Subatomic and Plasma Physics

T. Le Bleis

Helmholtz

R. Lemmon

University of Liverpool

Y. A. Litvinov

Helmholtz

K. Mahata

Helmholtz

C. Muntz

Goethe University Frankfurt

Thomas Nilsson

Chalmers, Physics, Subatomic and Plasma Physics

C. Nociforo

Helmholtz

Göran Hugo Nyman

Chalmers, Physics, Subatomic and Plasma Physics

W. Ott

Helmholtz

V. Panin

Helmholtz

Y. Parfenova

Dubna International University

S. Paschalis

Technische Universität Darmstadt

A. Perea

CSIC - Instituto de Estructura de la Materia (IEM)

R. Plag

Helmholtz

R. Reifarth

Helmholtz

A. Richter

Technische Universität Darmstadt

K. Riisager

Aarhus University

C. R. Tajes

Universidade de Santiagode Compostela

D. Rossi

Helmholtz

G. Schrieder

Technische Universität Darmstadt

Natalia Shulgina

Chalmers, Physics, Subatomic and Plasma Physics

H. Simon

Helmholtz

J. Stroth

Goethe University Frankfurt

K. Suemmerer

Helmholtz

J. Taylor

University of Liverpool

Olof Tengblad

Chalmers, Physics, Subatomic and Plasma Physics

Elisabeth Tengborn

Chalmers, Physics, Subatomic and Plasma Physics

H. Weick

Helmholtz

M. Wiescher

University of Notre Dame

C. Wimmer

Helmholtz

Mikhail Zhukov

Chalmers, Physics, Subatomic and Plasma Physics

Journal of Physics: Conference Series

17426588 (ISSN) 17426596 (eISSN)

Vol. 665 1 012046

6th Nuclear Physics in Astrophysics, NPA 2013
Lissabon, Portugal,

Subject Categories

Subatomic Physics

Physical Sciences

Astronomy, Astrophysics and Cosmology

Roots

Basic sciences

DOI

10.1088/1742-6596/665/1/012046

More information

Latest update

7/2/2021 7