Physics Letters B (May 2017)

Neutron spectroscopy of 26Mg states: Constraining the stellar neutron source 22Ne(α,n)25Mg

  • C. Massimi,
  • S. Altstadt,
  • J. Andrzejewski,
  • L. Audouin,
  • M. Barbagallo,
  • V. Bécares,
  • F. Bečvář,
  • F. Belloni,
  • E. Berthoumieux,
  • J. Billowes,
  • S. Bisterzo,
  • D. Bosnar,
  • M. Brugger,
  • M. Calviani,
  • F. Calviño,
  • D. Cano-Ott,
  • C. Carrapiço,
  • D.M. Castelluccio,
  • F. Cerutti,
  • E. Chiaveri,
  • L. Cosentino,
  • M. Chin,
  • G. Clai,
  • N. Colonna,
  • G. Cortés,
  • M.A. Cortés-Giraldo,
  • S. Cristallo,
  • M. Diakaki,
  • C. Domingo-Pardo,
  • I. Duran,
  • R. Dressler,
  • C. Eleftheriadis,
  • A. Ferrari,
  • P. Finocchiaro,
  • K. Fraval,
  • S. Ganesan,
  • A.R. García,
  • G. Giubrone,
  • I.F. Gonçalves,
  • E. González-Romero,
  • E. Griesmayer,
  • C. Guerrero,
  • F. Gunsing,
  • A. Hernández-Prieto,
  • D.G. Jenkins,
  • E. Jericha,
  • Y. Kadi,
  • F. Käppeler,
  • D. Karadimos,
  • N. Kivel,
  • P. Koehler,
  • M. Kokkoris,
  • S. Kopecky,
  • M. Krtička,
  • J. Kroll,
  • C. Lampoudis,
  • C. Langer,
  • E. Leal-Cidoncha,
  • C. Lederer,
  • H. Leeb,
  • L.S. Leong,
  • S. Lo Meo,
  • R. Losito,
  • A. Mallick,
  • A. Manousos,
  • J. Marganiec,
  • T. Martínez,
  • P.F. Mastinu,
  • M. Mastromarco,
  • E. Mendoza,
  • A. Mengoni,
  • P.M. Milazzo,
  • F. Mingrone,
  • M. Mirea,
  • W. Mondelaers,
  • A. Musumarra,
  • C. Paradela,
  • A. Pavlik,
  • J. Perkowski,
  • M. Pignatari,
  • L. Piersanti,
  • A. Plompen,
  • J. Praena,
  • J.M. Quesada,
  • T. Rauscher,
  • R. Reifarth,
  • A. Riego,
  • M.S. Robles,
  • C. Rubbia,
  • M. Sabaté-Gilarte,
  • R. Sarmento,
  • A. Saxena,
  • P. Schillebeeckx,
  • S. Schmidt,
  • D. Schumann,
  • G. Tagliente,
  • J.L. Tain,
  • D. Tarrío,
  • L. Tassan-Got,
  • A. Tsinganis,
  • S. Valenta,
  • G. Vannini,
  • I. Van Rijs,
  • V. Variale,
  • P. Vaz,
  • A. Ventura,
  • M.J. Vermeulen,
  • V. Vlachoudis,
  • R. Vlastou,
  • A. Wallner,
  • T. Ware,
  • M. Weigand,
  • C. Weiß,
  • R. Wynants,
  • T. Wright,
  • P. Žugec

DOI
https://doi.org/10.1016/j.physletb.2017.02.025
Journal volume & issue
Vol. 768, no. C
pp. 1 – 6

Abstract

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This work reports on accurate, high-resolution measurements of the 25Mg(n,γ)26Mg and 25Mg(n,tot) cross sections in the neutron energy range from thermal to about 300 keV, leading to a significantly improved 25Mg(n,γ)26Mg parametrization. The relevant resonances for n+25Mg were characterized from a combined R-matrix analysis of the experimental data. This resulted in an unambiguous spin/parity assignment of the corresponding excited states in 26Mg. With this information experimental upper limits of the reaction rates for 22Ne(α,n)25Mg and 22Ne(α,γ)26Mg were established, potentially leading to a significantly higher (α,n)/(α,γ) ratio than previously evaluated. The impact of these results has been studied for stellar models in the mass range 2 to 25 M⊙.

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