Measurement of the 154Gd(n,γ) cross section and its astrophysical implications

The neutron capture cross section of 154Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67% in 154Gd. The capture measurement, performed with four C6D6 scintillation detector...

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Main Authors: A. Mazzone, S. Cristallo, O. Aberle, G. Alaerts, V. Alcayne, S. Amaducci, J. Andrzejewski, L. Audouin, V. Babiano-Suarez, M. Bacak, M. Barbagallo, V. Bécares, F. Bečvář, G. Bellia, E. Berthoumieux, J. Billowes, D. Bosnar, A.S. Brown, M. Busso, M. Caamaño, L. Caballero, M. Calviani, F. Calviño, D. Cano-Ott, A. Casanovas, D.M. Castelluccio, F. Cerutti, Y.H. Chen, E. Chiaveri, G. Clai, N. Colonna, G.P. Cortés, M.A. Cortés-Giraldo, L. Cosentino, L.A. Damone, M. Diakaki, M. Dietz, C. Domingo-Pardo, R. Dressler, E. Dupont, I. Durán, Z. Eleme, B. Fernández-Domíngez, A. Ferrari, I. Ferro-Gonçalves, P. Finocchiaro, V. Furman, R. Garg, A. Gawlik, S. Gilardoni, T. Glodariu, K. Göbel, E. González-Romero, C. Guerrero, F. Gunsing, S. Heinitz, J. Heyse, D.G. Jenkins, E. Jericha, Y. Kadi, F. Käppeler, A. Kimura, N. Kivel, M. Kokkoris, Y. Kopatch, S. Kopecky, M. Krtička, D. Kurtulgil, I. Ladarescu, C. Lederer-Woods, J. Lerendegui-Marco, S. Lo Meo, S.-J. Lonsdale, D. Macina, A. Manna, T. Martínez, A. Masi, C. Massimi, P.F. Mastinu, M. Mastromarco, F. Matteucci, E. Maugeri, E. Mendoza, A. Mengoni, V. Michalopoulou, P.M. Milazzo, F. Mingrone, R. Mucciola, A. Musumarra, A. Negret, R. Nolte, F. Ogállar, A. Oprea, N. Patronis, A. Pavlik, J. Perkowski, L. Piersanti, I. Porras, J. Praena, J.M. Quesada, D. Radeck, D. Ramos Doval, R. Reifarth, D. Rochman, C. Rubbia, M. Sabaté-Gilarte, A. Saxena, P. Schillebeeckx, D. Schumann, A.G. Smith, N. Sosnin, A. Stamatopoulos, G. Tagliente, J.L. Tain, Z. Talip, A.E. Tarifeño-Saldivia, L. Tassan-Got, P. Torres-Sánchez, A. Tsinganis, J. Ulrich, S. Urlass, S. Valenta, G. Vannini, V. Variale, P. Vaz, A. Ventura, D. Vescovi, V. Vlachoudis, R. Vlastou, A. Wallner, P.J. Woods, R. Wynants, T.J. Wright, P. Žugec
Format: Article
Language:English
Published: Elsevier 2020-05-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269320302094
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author A. Mazzone
S. Cristallo
O. Aberle
G. Alaerts
V. Alcayne
S. Amaducci
J. Andrzejewski
L. Audouin
V. Babiano-Suarez
M. Bacak
M. Barbagallo
V. Bécares
F. Bečvář
G. Bellia
E. Berthoumieux
J. Billowes
D. Bosnar
A.S. Brown
M. Busso
M. Caamaño
L. Caballero
M. Calviani
F. Calviño
D. Cano-Ott
A. Casanovas
D.M. Castelluccio
F. Cerutti
Y.H. Chen
E. Chiaveri
G. Clai
N. Colonna
G.P. Cortés
M.A. Cortés-Giraldo
L. Cosentino
L.A. Damone
M. Diakaki
M. Dietz
C. Domingo-Pardo
R. Dressler
E. Dupont
I. Durán
Z. Eleme
B. Fernández-Domíngez
A. Ferrari
I. Ferro-Gonçalves
P. Finocchiaro
V. Furman
R. Garg
A. Gawlik
S. Gilardoni
T. Glodariu
K. Göbel
E. González-Romero
C. Guerrero
F. Gunsing
S. Heinitz
J. Heyse
D.G. Jenkins
E. Jericha
Y. Kadi
F. Käppeler
A. Kimura
N. Kivel
M. Kokkoris
Y. Kopatch
S. Kopecky
M. Krtička
D. Kurtulgil
I. Ladarescu
C. Lederer-Woods
J. Lerendegui-Marco
S. Lo Meo
S.-J. Lonsdale
D. Macina
A. Manna
T. Martínez
A. Masi
C. Massimi
P.F. Mastinu
M. Mastromarco
F. Matteucci
E. Maugeri
E. Mendoza
A. Mengoni
V. Michalopoulou
P.M. Milazzo
F. Mingrone
R. Mucciola
A. Musumarra
A. Negret
R. Nolte
F. Ogállar
A. Oprea
N. Patronis
A. Pavlik
J. Perkowski
L. Piersanti
I. Porras
J. Praena
J.M. Quesada
D. Radeck
D. Ramos Doval
R. Reifarth
D. Rochman
C. Rubbia
M. Sabaté-Gilarte
A. Saxena
P. Schillebeeckx
D. Schumann
A.G. Smith
N. Sosnin
A. Stamatopoulos
G. Tagliente
J.L. Tain
Z. Talip
A.E. Tarifeño-Saldivia
L. Tassan-Got
P. Torres-Sánchez
A. Tsinganis
J. Ulrich
S. Urlass
S. Valenta
G. Vannini
V. Variale
P. Vaz
A. Ventura
D. Vescovi
V. Vlachoudis
R. Vlastou
A. Wallner
P.J. Woods
R. Wynants
T.J. Wright
P. Žugec
author_facet A. Mazzone
S. Cristallo
O. Aberle
G. Alaerts
V. Alcayne
S. Amaducci
J. Andrzejewski
L. Audouin
V. Babiano-Suarez
M. Bacak
M. Barbagallo
V. Bécares
F. Bečvář
G. Bellia
E. Berthoumieux
J. Billowes
D. Bosnar
A.S. Brown
M. Busso
M. Caamaño
L. Caballero
M. Calviani
F. Calviño
D. Cano-Ott
A. Casanovas
D.M. Castelluccio
F. Cerutti
Y.H. Chen
E. Chiaveri
G. Clai
N. Colonna
G.P. Cortés
M.A. Cortés-Giraldo
L. Cosentino
L.A. Damone
M. Diakaki
M. Dietz
C. Domingo-Pardo
R. Dressler
E. Dupont
I. Durán
Z. Eleme
B. Fernández-Domíngez
A. Ferrari
I. Ferro-Gonçalves
P. Finocchiaro
V. Furman
R. Garg
A. Gawlik
S. Gilardoni
T. Glodariu
K. Göbel
E. González-Romero
C. Guerrero
F. Gunsing
S. Heinitz
J. Heyse
D.G. Jenkins
E. Jericha
Y. Kadi
F. Käppeler
A. Kimura
N. Kivel
M. Kokkoris
Y. Kopatch
S. Kopecky
M. Krtička
D. Kurtulgil
I. Ladarescu
C. Lederer-Woods
J. Lerendegui-Marco
S. Lo Meo
S.-J. Lonsdale
D. Macina
A. Manna
T. Martínez
A. Masi
C. Massimi
P.F. Mastinu
M. Mastromarco
F. Matteucci
E. Maugeri
E. Mendoza
A. Mengoni
V. Michalopoulou
P.M. Milazzo
F. Mingrone
R. Mucciola
A. Musumarra
A. Negret
R. Nolte
F. Ogállar
A. Oprea
N. Patronis
A. Pavlik
J. Perkowski
L. Piersanti
I. Porras
J. Praena
J.M. Quesada
D. Radeck
D. Ramos Doval
R. Reifarth
D. Rochman
C. Rubbia
M. Sabaté-Gilarte
A. Saxena
P. Schillebeeckx
D. Schumann
A.G. Smith
N. Sosnin
A. Stamatopoulos
G. Tagliente
J.L. Tain
Z. Talip
A.E. Tarifeño-Saldivia
L. Tassan-Got
P. Torres-Sánchez
A. Tsinganis
J. Ulrich
S. Urlass
S. Valenta
G. Vannini
V. Variale
P. Vaz
A. Ventura
D. Vescovi
V. Vlachoudis
R. Vlastou
A. Wallner
P.J. Woods
R. Wynants
T.J. Wright
P. Žugec
author_sort A. Mazzone
collection DOAJ
description The neutron capture cross section of 154Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67% in 154Gd. The capture measurement, performed with four C6D6 scintillation detectors, has been complemented by a transmission measurement performed at the GELINA time-of-flight facility (JRC-Geel), thus minimising the uncertainty related to sample composition. An accurate Maxwellian averaged capture cross section (MACS) was deduced over the temperature range of interest for s process nucleosynthesis modelling. We report a value of 880(50) mb for the MACS at kT=30 keV, significantly lower compared to values available in literature. The new adopted 154Gd(n,γ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models. Keywords: s process, 154Gd, Neutron time of flight, n_TOF
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spelling doaj.art-87f984be47724ffaab22cf97fb9ec04f2022-12-21T18:50:44ZengElsevierPhysics Letters B0370-26932020-05-01804Measurement of the 154Gd(n,γ) cross section and its astrophysical implicationsA. Mazzone0S. Cristallo1O. Aberle2G. Alaerts3V. Alcayne4S. Amaducci5J. Andrzejewski6L. Audouin7V. Babiano-Suarez8M. Bacak9M. Barbagallo10V. Bécares11F. Bečvář12G. Bellia13E. Berthoumieux14J. Billowes15D. Bosnar16A.S. Brown17M. Busso18M. Caamaño19L. Caballero20M. Calviani21F. Calviño22D. Cano-Ott23A. Casanovas24D.M. Castelluccio25F. Cerutti26Y.H. Chen27E. Chiaveri28G. Clai29N. Colonna30G.P. Cortés31M.A. Cortés-Giraldo32L. Cosentino33L.A. Damone34M. Diakaki35M. Dietz36C. Domingo-Pardo37R. Dressler38E. Dupont39I. Durán40Z. Eleme41B. Fernández-Domíngez42A. Ferrari43I. Ferro-Gonçalves44P. Finocchiaro45V. Furman46R. Garg47A. Gawlik48S. Gilardoni49T. Glodariu50K. Göbel51E. González-Romero52C. Guerrero53F. Gunsing54S. Heinitz55J. Heyse56D.G. Jenkins57E. Jericha58Y. Kadi59F. Käppeler60A. Kimura61N. Kivel62M. Kokkoris63Y. Kopatch64S. Kopecky65M. Krtička66D. Kurtulgil67I. Ladarescu68C. Lederer-Woods69J. Lerendegui-Marco70S. Lo Meo71S.-J. Lonsdale72D. Macina73A. Manna74T. Martínez75A. Masi76C. Massimi77P.F. Mastinu78M. Mastromarco79F. Matteucci80E. Maugeri81E. Mendoza82A. Mengoni83V. Michalopoulou84P.M. Milazzo85F. Mingrone86R. Mucciola87A. Musumarra88A. Negret89R. Nolte90F. Ogállar91A. Oprea92N. Patronis93A. Pavlik94J. Perkowski95L. Piersanti96I. Porras97J. Praena98J.M. Quesada99D. Radeck100D. Ramos Doval101R. Reifarth102D. Rochman103C. Rubbia104M. Sabaté-Gilarte105A. Saxena106P. Schillebeeckx107D. Schumann108A.G. Smith109N. Sosnin110A. Stamatopoulos111G. Tagliente112J.L. Tain113Z. Talip114A.E. Tarifeño-Saldivia115L. Tassan-Got116P. Torres-Sánchez117A. Tsinganis118J. Ulrich119S. Urlass120S. Valenta121G. Vannini122V. Variale123P. Vaz124A. Ventura125D. Vescovi126V. Vlachoudis127R. Vlastou128A. Wallner129P.J. Woods130R. Wynants131T.J. Wright132P. Žugec133Istituto Nazionale di Fisica Nucleare, Bari, Italy; Consiglio Nazionale delle Ricerche, Bari, ItalyIstituto Nazionale di Fisica Nazionale, Perugia, Italy; Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, ItalyEuropean Organisation for Nuclear Research (CERN), SwitzerlandEuropean Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, BelgiumCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainINFN Laboratori Nazionali del Sud, Catania, Italy; Dipartimento di Fisica e Astronomia, Università di Catania, ItalyUniversity of Lodz, PolandIPN, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, FranceInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainEuropean Organisation for Nuclear Research (CERN), Switzerland; Technische Universität Wien, Austria; CEA Saclay, Irfu, Université Paris-Saclay, Gif-sur-Yvette, FranceEuropean Organisation for Nuclear Research (CERN), Switzerland; Istituto Nazionale di Fisica Nucleare, Bari, ItalyCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainCharles University, Prague, Czech RepublicINFN Laboratori Nazionali del Sud, Catania, Italy; Dipartimento di Fisica e Astronomia, Università di Catania, ItalyCEA Saclay, Irfu, Université Paris-Saclay, Gif-sur-Yvette, FranceUniversity of Manchester, United KingdomDepartment of Physics, Faculty of Science, University of Zagreb, CroatiaUniversity of York, United KingdomIstituto Nazionale di Fisica Nazionale, Perugia, Italy; Dipartimento di Fisica e Geologia, Università di Perugia, ItalyUniversity of Santiago de Compostela, SpainInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainEuropean Organisation for Nuclear Research (CERN), SwitzerlandUniversitat Politècnica de Catalunya, SpainCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainUniversitat Politècnica de Catalunya, SpainIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Bologna, ItalyEuropean Organisation for Nuclear Research (CERN), SwitzerlandIPN, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, FranceUniversity of Manchester, United Kingdom; Universidad de Sevilla, Spain; European Organisation for Nuclear Research (CERN), SwitzerlandIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Bari, ItalyUniversitat Politècnica de Catalunya, SpainUniversidad de Sevilla, SpainINFN Laboratori Nazionali del Sud, Catania, ItalyIstituto Nazionale di Fisica Nucleare, Bari, Italy; Dipartimento di Fisica, Università degli Studi di Bari, ItalyNational Technical University of Athens, GreeceSchool of Physics and Astronomy, University of Edinburgh, United KingdomInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainPaul Scherrer Institut (PSI), Villigen, SwitzerlandCEA Saclay, Irfu, Université Paris-Saclay, Gif-sur-Yvette, FranceUniversity of Santiago de Compostela, SpainUniversity of Ioannina, GreeceUniversity of Santiago de Compostela, SpainEuropean Organisation for Nuclear Research (CERN), SwitzerlandInstituto Superior Técnico, Lisbon, PortugalINFN Laboratori Nazionali del Sud, Catania, ItalyJoint Institute for Nuclear Research (JINR), Dubna, RussiaSchool of Physics and Astronomy, University of Edinburgh, United KingdomUniversity of Lodz, PolandEuropean Organisation for Nuclear Research (CERN), SwitzerlandHoria Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH), Bucharest, Magurele, RomaniaGoethe University Frankfurt, GermanyCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainUniversidad de Sevilla, SpainCEA Saclay, Irfu, Université Paris-Saclay, Gif-sur-Yvette, FrancePaul Scherrer Institut (PSI), Villigen, SwitzerlandEuropean Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, BelgiumUniversity of York, United KingdomTechnische Universität Wien, AustriaEuropean Organisation for Nuclear Research (CERN), SwitzerlandKarlsruhe Institute of Technology, Campus North, IKP, 76021 Karlsruhe, GermanyJapan Atomic Energy Agency (JAEA), Tokai-mura, JapanPaul Scherrer Institut (PSI), Villigen, SwitzerlandNational Technical University of Athens, GreeceJoint Institute for Nuclear Research (JINR), Dubna, RussiaEuropean Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, BelgiumCharles University, Prague, Czech RepublicGoethe University Frankfurt, GermanyInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainSchool of Physics and Astronomy, University of Edinburgh, United KingdomUniversidad de Sevilla, SpainIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Bologna, ItalySchool of Physics and Astronomy, University of Edinburgh, United KingdomEuropean Organisation for Nuclear Research (CERN), SwitzerlandIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, ItalyCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainEuropean Organisation for Nuclear Research (CERN), SwitzerlandIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, Italy; Corresponding author at: Dipartimento di Fisica e Astronomia, Università di Bologna, Italy.Istituto Nazionale di Fisica Nucleare, Sezione di Legnaro, ItalyEuropean Organisation for Nuclear Research (CERN), Switzerland; University of Manchester, United KingdomIstituto Nazionale di Fisica Nazionale, Trieste, Italy; Dipartimento di Fisica, Università di Trieste, ItalyPaul Scherrer Institut (PSI), Villigen, SwitzerlandCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), SpainIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Bologna, ItalyNational Technical University of Athens, GreeceIstituto Nazionale di Fisica Nazionale, Trieste, ItalyEuropean Organisation for Nuclear Research (CERN), SwitzerlandIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, ItalyINFN Laboratori Nazionali del Sud, Catania, Italy; Dipartimento di Fisica e Astronomia, Università di Catania, ItalyHoria Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH), Bucharest, Magurele, RomaniaPhysikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, GermanyUniversity of Granada, SpainHoria Hulubei National Institute of Physics and Nuclear Engineering (IFIN-HH), Bucharest, Magurele, RomaniaUniversity of Ioannina, GreeceUniversity of Vienna, Faculty of Physics, Vienna, AustriaUniversity of Lodz, PolandIstituto Nazionale di Fisica Nazionale, Perugia, Italy; Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, ItalyUniversity of Granada, SpainUniversity of Granada, SpainUniversidad de Sevilla, SpainPhysikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, GermanyIPN, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, FranceGoethe University Frankfurt, GermanyPaul Scherrer Institut (PSI), Villigen, SwitzerlandEuropean Organisation for Nuclear Research (CERN), SwitzerlandUniversidad de Sevilla, Spain; European Organisation for Nuclear Research (CERN), SwitzerlandBhabha Atomic Research Centre (BARC), IndiaEuropean Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, BelgiumPaul Scherrer Institut (PSI), Villigen, SwitzerlandUniversity of Manchester, United KingdomUniversity of Manchester, United KingdomNational Technical University of Athens, GreeceIstituto Nazionale di Fisica Nucleare, Bari, ItalyInstituto de Física Corpuscular, CSIC - Universidad de Valencia, SpainPaul Scherrer Institut (PSI), Villigen, SwitzerlandUniversitat Politècnica de Catalunya, SpainEuropean Organisation for Nuclear Research (CERN), Switzerland; National Technical University of Athens, Greece; IPN, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, FranceUniversity of Granada, SpainEuropean Organisation for Nuclear Research (CERN), SwitzerlandPaul Scherrer Institut (PSI), Villigen, SwitzerlandEuropean Organisation for Nuclear Research (CERN), Switzerland; Helmholtz-Zentrum Dresden-Rossendorf, GermanyCharles University, Prague, Czech RepublicIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Bari, ItalyInstituto Superior Técnico, Lisbon, PortugalIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, ItalyIstituto Nazionale di Fisica Nazionale, Perugia, Italy; Gran Sasso Science Institute, L'Aquila, Italy; Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, ItalyEuropean Organisation for Nuclear Research (CERN), SwitzerlandNational Technical University of Athens, GreeceAustralian National University, Canberra, AustraliaSchool of Physics and Astronomy, University of Edinburgh, United KingdomEuropean Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, BelgiumUniversity of Manchester, United KingdomDepartment of Physics, Faculty of Science, University of Zagreb, CroatiaThe neutron capture cross section of 154Gd was measured from 1 eV to 300 keV in the experimental area located 185 m from the CERN n_TOF neutron spallation source, using a metallic sample of gadolinium, enriched to 67% in 154Gd. The capture measurement, performed with four C6D6 scintillation detectors, has been complemented by a transmission measurement performed at the GELINA time-of-flight facility (JRC-Geel), thus minimising the uncertainty related to sample composition. An accurate Maxwellian averaged capture cross section (MACS) was deduced over the temperature range of interest for s process nucleosynthesis modelling. We report a value of 880(50) mb for the MACS at kT=30 keV, significantly lower compared to values available in literature. The new adopted 154Gd(n,γ) cross section reduces the discrepancy between observed and calculated solar s-only isotopic abundances predicted by s-process nucleosynthesis models. Keywords: s process, 154Gd, Neutron time of flight, n_TOFhttp://www.sciencedirect.com/science/article/pii/S0370269320302094
spellingShingle A. Mazzone
S. Cristallo
O. Aberle
G. Alaerts
V. Alcayne
S. Amaducci
J. Andrzejewski
L. Audouin
V. Babiano-Suarez
M. Bacak
M. Barbagallo
V. Bécares
F. Bečvář
G. Bellia
E. Berthoumieux
J. Billowes
D. Bosnar
A.S. Brown
M. Busso
M. Caamaño
L. Caballero
M. Calviani
F. Calviño
D. Cano-Ott
A. Casanovas
D.M. Castelluccio
F. Cerutti
Y.H. Chen
E. Chiaveri
G. Clai
N. Colonna
G.P. Cortés
M.A. Cortés-Giraldo
L. Cosentino
L.A. Damone
M. Diakaki
M. Dietz
C. Domingo-Pardo
R. Dressler
E. Dupont
I. Durán
Z. Eleme
B. Fernández-Domíngez
A. Ferrari
I. Ferro-Gonçalves
P. Finocchiaro
V. Furman
R. Garg
A. Gawlik
S. Gilardoni
T. Glodariu
K. Göbel
E. González-Romero
C. Guerrero
F. Gunsing
S. Heinitz
J. Heyse
D.G. Jenkins
E. Jericha
Y. Kadi
F. Käppeler
A. Kimura
N. Kivel
M. Kokkoris
Y. Kopatch
S. Kopecky
M. Krtička
D. Kurtulgil
I. Ladarescu
C. Lederer-Woods
J. Lerendegui-Marco
S. Lo Meo
S.-J. Lonsdale
D. Macina
A. Manna
T. Martínez
A. Masi
C. Massimi
P.F. Mastinu
M. Mastromarco
F. Matteucci
E. Maugeri
E. Mendoza
A. Mengoni
V. Michalopoulou
P.M. Milazzo
F. Mingrone
R. Mucciola
A. Musumarra
A. Negret
R. Nolte
F. Ogállar
A. Oprea
N. Patronis
A. Pavlik
J. Perkowski
L. Piersanti
I. Porras
J. Praena
J.M. Quesada
D. Radeck
D. Ramos Doval
R. Reifarth
D. Rochman
C. Rubbia
M. Sabaté-Gilarte
A. Saxena
P. Schillebeeckx
D. Schumann
A.G. Smith
N. Sosnin
A. Stamatopoulos
G. Tagliente
J.L. Tain
Z. Talip
A.E. Tarifeño-Saldivia
L. Tassan-Got
P. Torres-Sánchez
A. Tsinganis
J. Ulrich
S. Urlass
S. Valenta
G. Vannini
V. Variale
P. Vaz
A. Ventura
D. Vescovi
V. Vlachoudis
R. Vlastou
A. Wallner
P.J. Woods
R. Wynants
T.J. Wright
P. Žugec
Measurement of the 154Gd(n,γ) cross section and its astrophysical implications
Physics Letters B
title Measurement of the 154Gd(n,γ) cross section and its astrophysical implications
title_full Measurement of the 154Gd(n,γ) cross section and its astrophysical implications
title_fullStr Measurement of the 154Gd(n,γ) cross section and its astrophysical implications
title_full_unstemmed Measurement of the 154Gd(n,γ) cross section and its astrophysical implications
title_short Measurement of the 154Gd(n,γ) cross section and its astrophysical implications
title_sort measurement of the 154gd n γ cross section and its astrophysical implications
url http://www.sciencedirect.com/science/article/pii/S0370269320302094
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