Measurement of the Sm-151(n,gamma)Sm-152 cross section at n_TOF

  • S. Marrone
  • , U. Abbondanno
  • , G. Aerts
  • , F. Alvarez-Velarde
  • , H. Alvarez-Pol
  • , S. Andriamonje
  • , J. Andrzejewski
  • , C. Badurek
  • , P. Baumann
  • , F. Becvar
  • , J. Benlliure
  • , E. Berthoumieux
  • , F. Calvino
  • , D. Cano-Ott
  • , R. Capote
  • , P. Cennini
  • , V. Chepel
  • , E. Chiaveri
  • , N. Colonna
  • , G. Cortes
  • D. Cortina, A. Couture, J. Cox, S. Dababneh, M. Dahlfors, S. David, R. Dolfini, C. Domingo-Pardo, R.B. Duran, M. Embid-Segura, L. Ferrant, A. Ferrari, R. Ferreira-Marques, H. Frais-Koelbl, W. Furman, I. F. Goncalves, R. Gallino, E. Gonzalez-Romero, A. Goverdovski, F. Gramegna, E. Griesmayer, F. Gunsing, B. Haas, R. Haight, M. Heil, A. Herrera-Martinez, S. Isaev, E. Jericha, F. Kappeler, Y. Kadi, D. Karadimos, M. Kerveno, V. Ketlerov, P. Koehler, V. Konovalov, M. Krticka, C. Lamboudis, H. Leeb, A. Lindote, I. Lopes, M. Lozano, S. Lukic, J. Marganiec, J. Martinez-Val, P. Mastinu, A. Mengoni, P.M. Milazzo, A. Molina-Coballes, C. Moreau, M. Mosconi, F. Neves, H. Oberhummer, S. O'Brien, J. Pancin, T. Papaevangelou, C. Paradela, A. Pavlik, P. Pavlopoulos, J. M. Perlado, L. Perrot, M. Pignatari, R. Plag, A. Plompen, A. Plukis, A. Poch, A. Policarpo, C. Pretel, J. Quesada, S. Raman, W. Rapp, T. Rauscher, R. Reifarth, M. Rosetti, C. Rubbia, G. Rudolf, P. Rullhusen, J. Salgado, J. C. Soares, C. Stephan, G. Tagliente, J. L. Tain, L. Tassan-Got, L. Tavora, R. Terlizzi, G. Vannini, P. Vaz, A. Ventura, D. Villamarin, M.C. Vincente, V. Vlachoudis, F. Voss, H. Wendler, M. Wiescher, K. Wisshak

Research output: Contribution to journalArticlepeer-review

7 Citations (Scopus)

Abstract

The Sm-151(n,gamma) Sm-152 cross section, which is important for the interpretation of the Sm-151 branching as an s-process thermometer, was measured from 1 eV up to 1 MeV at the innovative n-TOF facility at CERN. Based on these data, the Maxwellian-averaged cross section at kT=30 keV is found to be 3100 +/- 160 nib. This value can be used to constrain the thermodynamical conditions in Asymptotic Giant Branch (AGB) stars during He-shell burning.

Original languageEnglish
Pages (from-to)533-536
Number of pages4
JournalNuclear Physics A
Volume758
DOIs
Publication statusPublished - 25 Jul 2005
Event8th International Symposium on Nucle in the Cosmos (NIC8) - Vancouver, Canada
Duration: 19 Jul 200423 Jul 2004

Keywords

  • S-PROCESS
  • NUCLEOSYNTHESIS
  • NEUTRON-CAPTURE

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