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s-process branching at W185 revised

P. Mohr, T. Shizuma, H. Ueda, S. Goko, A. Makinaga, K. Y. Hara, T. Hayakawa, Y.-W. Lui, H. Ohgaki, and H. Utsunomiya
Phys. Rev. C 69, 032801(R) – Published 29 March 2004

Abstract

The neutron capture cross section of the unstable s-process branching nucleus W185 has been derived from experimental data of the inverse W186(γ,n)W185 photodisintegration taken with monochromatic photon beams from laser Compton scattering. The result of σ=553±60mb at kT=30keV leads to a relatively high effective neutron density in the classical s process of Nn=4.7×108cm3. A realistic model for the s process in thermally pulsing asymptotic giant branch stars overestimates the abundance of Os186 significantly because of the relatively small neutron capture cross section of W185.

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  • Received 3 February 2004

DOI:https://doi.org/10.1103/PhysRevC.69.032801

©2004 American Physical Society

Authors & Affiliations

P. Mohr1,2,*, T. Shizuma3, H. Ueda4, S. Goko4, A. Makinaga4, K. Y. Hara4, T. Hayakawa3,5, Y.-W. Lui6, H. Ohgaki7, and H. Utsunomiya4

  • 1Institut für Kernphysik, Technische Universität Darmstadt, Schlossgartenstraße 9, D-64289 Darmstadt, Germany
  • 2Strahlentherapie, Diakoniekrankenhaus Schwäbisch Hall, D-74523 Schwäbisch Hall, Germany
  • 3Advanced Photon Research Center, Japan Atomic Energy Research Institute, Tokai, Ibaraki 319-1195, Japan
  • 4Department of Physics, Konan University, 8-9-1 Okamoto, Higashinada, Kobe 658-8501, Japan
  • 5National Astronomical Observatory, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan
  • 6Cyclotron Institute, Texas A & M University, College Station, Texas 77843, USA
  • 7Institute of Advanced Energy, Kyoto University, Gokanosho, Uji, Kyoto 611-0011, Japan

  • *Electronic address: WidmaierMohr@compuserve.de

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Issue

Vol. 69, Iss. 3 — March 2004

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