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Pygmy dipole resonance in 124Sn populated by inelastic scattering of 17O

Authors :
A. Pullia
J. Eberth
Sunniva Siem
D. R. Napoli
N. Karkour
S. Lunardi
A. Giaz
D. S. Judson
K. Mazurek
Elena Litvinova
A. Gottardo
P. Molini
Roman Gernhäuser
F. Recchia
S. Ceruti
Begoña Quintana
R. Avigo
D. Bazzacco
R. Nicolini
P. Bednarczyk
Roberto Menegazzo
M. Kmiecik
D. Mengoni
A. Bracco
S. Brambilla
P. A. Söderström
L. Charles
M. Zieblinski
P. Désesquelles
A. I. Morales
Marco Bellato
J. Grebosz
G. Benzoni
Luna Pellegri
O. Wieland
B. Birkenbach
J. Simpson
C. Michelagnoli
O. Stezowski
C. A. Ur
Bo Cederwall
S. Leoni
M.D. Salsac
G. de Angelis
A. Maj
E. Farnea
Ch. Theisen
J. J. Valiente Dobon
Roberto Isocrate
C. Boiano
Herbert Hess
M. Krzysiek
F. Camera
M. Ciemala
Andreas Görgen
S. Bottoni
E. G. Lanza
N. Blasi
B. Siebeck
F. C. L. Crespi
A. Gadea
D. Bortolato
P. Reiter
V. Vandone
B. Million
J. Jolie
A. Jungclaus
SCOAP
Source :
Physics Letters B, Digital.CSIC. Repositorio Institucional del CSIC, instname, Physics Letters B, Vol 738, Iss, Pp 519-523 (2014)
Publication Year :
2014
Publisher :
Elsevier BV, 2014.

Abstract

L. Pellegri et al. ; 5 pags. ; 6 figs. ; open access article under the CC BY license. Funded by SCOAP3<br />© 2014 The Authors. The γ decay from the high-lying states of 124Sn was measured using the inelastic scattering of 17O at 340 MeV. The emitted γ rays were detected with high resolution with the AGATA demonstrator array and the scattered ions were detected in two segmented δE-E silicon telescopes. The angular distribution was measured both for the γ rays and the scattered 17O ions. An accumulation of E1 strength below the particle threshold was found and compared with previous data obtained with (γ, γ') and (α, α'γ) reactions. The present results of elastic scattering, and excitation of E2 and E1 states were analysed using the DWBA approach. From this comprehensive description the isoscalar component of the 1- excited states was extracted. The obtained values are based on the comparison of the data with DWBA calculations including a form factor deduced using a microscopic transition density.<br />Grant No. 2011/03/B/ST2/01894; (iii) the National Superconducting Cyclotron Laboratory at MSU; (iv) the US NSF Grant PHY-1204486; and the German BMBF under Grant 06KY9136.

Details

ISSN :
03702693
Volume :
738
Database :
OpenAIRE
Journal :
Physics Letters B
Accession number :
edsair.doi.dedup.....54873166938c7533f901f59728159a68
Full Text :
https://doi.org/10.1016/j.physletb.2014.08.029