Resonance neutron-capture cross sections of stable magnesium isotopes and their astrophysical implications

  • C. Massimi
  • , P. Koehler
  • , S. Bisterzo
  • , N. Colonna
  • , R. Gallino
  • , F. Gunsing
  • , F. Kaeppeler
  • , G. Lorusso
  • , A. Mengoni
  • , M. Pignatari
  • , G. Vannini
  • , U. Abbondanno
  • , G. Aerts
  • , H. Alvarez
  • , F. Alvarez-Velarde
  • , S. Andriamonje
  • , J. Andrzejewski
  • , P. Assimakopoulos
  • , L. Audouin
  • , G. Badurek
  • M. Barbagallo, P. Baumann, F. Becvar, F. Belloni, M. Bennett, E. Berthoumieux, M. Calviani, F. Calvino, D. Cano-Ott, R. Capote, C. Carrapico, A. Carrillo de Albornoz, P. Cennini, V. Chepel, E. Chiaveri, G. Cortes, A. Couture, J. Cox, M. Dahlfors, S. David, I. Dillmann, R. Dolfini, C. Domingo-Pardo, W. Dridi, I. Duran, C. Eleftheriadis, M. Embid-Segura, L. Ferrant, A. Ferrari, T. Rauscher, N TOF Collaboration

Research output: Contribution to journalArticlepeer-review

63 Citations (Scopus)

Abstract

We have measured the neutron capture cross sections of the stable magnesium isotopes Mg-24,Mg-25,Mg-26 in the energy range of interest to the s process using the neutron time-of-flight facility n_TOF at CERN. Capture events from a natural metal sample and from samples enriched in Mg-25 and Mg-26 were recorded using the total energy method based on (C6H6)-H-2 detectors. Neutron resonance parameters were extracted by a simultaneous resonance shape analysis of the present capture data and existing transmission data on a natural isotopic sample. Maxwellian-averaged capture cross sections for the three isotopes were calculated up to thermal energies of 100 keV and their impact on s-process analyses was investigated. At 30 keV the new values of the stellar cross section for Mg-24, Mg-25, and Mg-26 are 3.8 +/- 0.2 mb, 4.1 +/- 0.6 mb, and 0.14 +/- 0.01 mb, respectively.

Original languageEnglish
Article number044615
Number of pages15
JournalPhysical Review C (nuclear physics)
Volume85
Issue number4
DOIs
Publication statusPublished - 20 Apr 2012

Keywords

  • NUCLEAR
  • WAVE
  • RADIATIVE-CAPTURE
  • DIPOLE TRANSITIONS
  • GIANT BRANCH STARS
  • MASSIVE STARS
  • OF-FLIGHT FACILITY
  • S-PROCESS NUCLEOSYNTHESIS
  • REACTION-RATES
  • EVOLUTION

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