Physics Letters B (May 2020)

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

  • 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

Journal volume & issue
Vol. 804

Abstract

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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