TY  - JOUR
A1  - Mazzone, Annamaria
A1  - Cristallo, Sergio
A1  - Aberle, Oliver
A1  - Alaerts, Gery
A1  - Alcayne, Victor
A1  - Amaducci, Simone
A1  - Andrzejewski, Józef
A1  - Audouin, Laurent
A1  - Babiano Suarez, Victor
A1  - Bacak, Michael
A1  - Barbagallo, Massimo
A1  - Bécares, Vicente
A1  - Bečvář, František
A1  - Bellia, Giorgio
A1  - Berthoumieux, Eric
A1  - Billowes, Jonathan
A1  - Bosnar, Damir
A1  - Brown, Adam S.
A1  - Busso, Maurizio
A1  - Caamaño, Manuel
A1  - Caballero Ontanaya, Luis
A1  - Calviani, Marco
A1  - Calviño Tavares, Francisco
A1  - Cano-Ott, Daniel
A1  - Casanovas Hoste, Adrià
A1  - Castelluccio, Donato Maurizio
A1  - Cerutti, Francesco
A1  - Chen, Yonghao
A1  - Chiaveri, Enrico
A1  - Clai, Giulia
A1  - Colonna, Nicola
A1  - Cortés Rossell, Guillem Pere
A1  - Cortés-Giraldo, Miguel Antonio
A1  - Cosentino, Luigi
A1  - Damone, Lucia Anna
A1  - Diakaki, Maria
A1  - Dietz, Mirco
A1  - Domingo-Pardo, César
A1  - Dressler, Rugard
A1  - Dupont, Emmeric
A1  - Durán, Ignacio
A1  - Eleme, Zinovia
A1  - Fernández Domínguez, Beatriz
A1  - Ferrari, Alfredo
A1  - Gonçalves, Isabel Maria Ferro
A1  - Finocchiaro, Paolo
A1  - Furman, Valter
A1  - Garg, Ruchi
A1  - Gawlik, Aleksandra
A1  - Gilardoni, Simone
A1  - Glodariu, Tudor
A1  - Göbel, Kathrin
A1  - González Romero, Enrique Miguel
A1  - Guerrero Sánchez, Carlos
A1  - Gunsing, Frank
A1  - Heinitz, Stephan
A1  - Heyse, Jan
A1  - Jenkins, David
A1  - Jericha, Erwin
A1  - Kadi, Yacine
A1  - Käppeler, Franz
A1  - Kimura, Atsushi
A1  - Kivel, Nikolay
A1  - Kokkoris, Michael
A1  - Kopatch, Yuri N.
A1  - Kopecky, Stefan
A1  - Krtička, Milan
A1  - Kurtulgil, Cem Deniz
A1  - Ladarescu, Ion
A1  - Lederer-Woods, Claudia
A1  - Lerendegui-Marco, Jorge
A1  - Lo Meo, Sergio
A1  - Lonsdale, Sarah-Jane
A1  - Macina, Daniela
A1  - Manna, Alice
A1  - Martínez, Trinitario
A1  - Masi, Alessandro
A1  - Massimi, Cristian
A1  - Mastinu, Pierfrancesco
A1  - Mastromarco, Mario
A1  - Matteucci, Francesca
A1  - Maugeri, Emilio Andrea
A1  - Mendoza Cembranos, Emilio
A1  - Mengoni, Alberto
A1  - Michalopoulou, Veatriki
A1  - Milazzo, Paolo Maria
A1  - Mingrone, Federica
A1  - Mucciola, Riccardo
A1  - Musumarra, Agatino
A1  - Negret, Alexandru
A1  - Nolte, Ralf
A1  - Ogállar Ruiz, Francisco
A1  - Oprea, Andreea
A1  - Patronis, Nikolas
A1  - Pavlik, Andreas
A1  - Perkowski, Jarosław
A1  - Piersanti, Luciano
A1  - Porras Sánchez, José Ignacio
A1  - Praena, Javier
A1  - Quesada Molina, José Manuel
A1  - Radeck, Désirée
A1  - Ramos Doval, Diego
A1  - Reifarth, René
A1  - Rochman, Dimitri
A1  - Rubbia, Carlo
A1  - Sabaté-Gilarte, Marta
A1  - Saxena, Alok
A1  - Schillebeeckx, Peter
A1  - Schumann, Dorothea
A1  - Smith, Alastair Gavin
A1  - Sosnin, Nikolay V.
A1  - Stamatopoulos, Athanasios
A1  - Tagliente, Giuseppe
A1  - Taı́n Enríquez, José Luis
A1  - Talip, Zeynep
A1  - Tarifeño-Saldivia, Ariel
A1  - Tassan-Got, Laurent
A1  - Torres-Sánchez, Pablo
A1  - Tsinganis, Andrea
A1  - Ulrich, Jiri
A1  - Urlaß, Sebastian
A1  - Valenta, Stanislav
A1  - Vannini, Gianni
A1  - Variale, Vincenzo
A1  - Vaz, Pedro
A1  - Ventura, Alberto
A1  - Vescovi, Diego
A1  - Vlachoudis, Vasilis
A1  - Vlastou, Rosa
A1  - Wallner, Anton
A1  - Woods, Philip John
A1  - Wynants, Ruud
A1  - Wright, Tobias  J.
A1  - Žugec, Petar
T1  - Measurement of the 154Gd(n,γ) cross section and its astrophysical implications
T2  - Physics Letters B
N2  - 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.
Y1  - 2020
UR  - http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/70199
UR  - https://nbn-resolving.org/urn:nbn:de:hebis:30:3-701998
SN  - 1873-2445
SN  - 0370-2693
VL  - 804
IS  - 135405
PB  - Elsevier
CY  - Amsterdam
ER  -