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Neutron Capture Cross Section Measurement ofSm151at the CERN Neutron Time of Flight Facility (n_TOF)

Authors :
I. Goncalves
C. Lamboudis
J. L. Tain
Thomas Rauscher
L. Tavora
M. Embid-Segura
D. Karadimos
Rene Reifarth
D. Cortina
Manuel Lozano
A.J.P.L. Policarpo
José M. Martínez-Val
F. Gramegna
P. Pavlopoulos
P. Rullhusen
J. Andrzejewski
M. Kerveno
F. Käppeler
M. Krtička
T. Papaevangelou
J. M. Quesada
Carlo Rubbia
A. Pavlik
José Manuel Perlado
L. Ferrant
Heinz Oberhummer
G. Cortes
C. Domingo-Pardo
V. Vlachoudis
Saed Dababneh
M. Rosetti
V. Konovalov
F. Voss
W.I. Furman
Alfredo Ferrari
R. Ferreira-Marques
Nicola Colonna
E. Gonzalez-Romero
S. Marrone
H. Alvarez-Pol
A. Plukis
A. Lindote
Subramanian Raman
J. Pancin
R. Gallino
J. Cox
C. Paradela
G. Aerts
V. Ketlerov
J. Marganiec
E. Griesmayer
P. M. Milazzo
E. Chiaveri
Laurent Tassan-Got
S. Lukic
S. Andriamonje
D. Cano-Ott
Michael Heil
P. F. Mastinu
Marco Pignatari
Roberto Capote
Ralf Plag
J. Benlliure
W. Rapp
H. Frais-Koelbl
M. Dahlfors
P. Vaz
Alberto Ventura
Aaron Couture
C. Pretel
F. Neves
E. Jericha
I. Duran
D. Villamarin
P. E. Koehler
E. Berthoumieux
A. Herrera-Martinez
R. C. Haight
Alberto Mengoni
A. Molina-Coballes
G. Vannini
F. Bečvář
L. Perrot
S. David
G. Tagliente
V. Chepel
J. Salgado
A. Poch
P. Baumann
Michael Wiescher
Yacine Kadi
C. Moreau
M. C. Vincente
J.C. Soares
S. Isaev
U. Abbondanno
F. Gunsing
A. J. M. Plompen
G. Rudolf
I. Lopes
P. Cennini
K. Wisshak
A. Goverdovski
F. Alvarez-Velarde
Gerald Badurek
R. Dolfini
M. Mosconi
C. Stephan
S. O'Brien
R. Terlizzi
H. Wendler
F. Calviño
H. Leeb
B. Haas
Source :
Physical Review Letters. 93
Publication Year :
2004
Publisher :
American Physical Society (APS), 2004.

Abstract

The Sm-151(n,gamma)Sm-152 cross section has been measured at the spallation neutron facility n_TOF at CERN in the energy range from 1 eV to 1 MeV. The new facility combines excellent resolution in neutron time-of-flight, low repetition rates, and an unsurpassed instantaneous luminosity, resulting in rather favorable signal/background ratios. The Sm-151 cross section is of importance for characterizing neutron capture nucleosynthesis in asymptotic giant branch stars. At a thermal energy of kT=30 keV the Maxwellian averaged cross section of this unstable isotope (t(1/2)=93 yr) was determined to be 3100+/-160 mb, significantly larger than theoretical predictions.

Details

ISSN :
10797114 and 00319007
Volume :
93
Database :
OpenAIRE
Journal :
Physical Review Letters
Accession number :
edsair.doi...........56b5690d92f432b5549c91df22d498ac