Subthreshold resonance in the 6Li(d,α)4He reaction and its astrophysical implications

K. Czerski, A. Huke, H. Bucka, P. Heide, G. Ruprecht, and B. Unrau
Phys. Rev. C 55, 1517 – Published 1 March 1997
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Abstract

The total cross section of the 6Li(d,α)4He reaction has been measured for deuteron energies between 50 and 180 keV. From a detailed distorted-wave Born approximation analysis of the angular distributions and the excitation function up to 1 MeV it was possible to determine the strength of a subthreshold resonance that dominates the cross section at sub-Coulomb energies and contributes significantly to the increase of the astrophysical S factor at low energies. Consequently the electron screening energy we have determined for the 6Li(d,α)4He reaction is considerably smaller than the value given in previous works which overestimate the theoretical predictions. In addition the stellar reaction rate has been calculated up to a temperature of T9=3.

  • Received 4 June 1996

DOI:https://doi.org/10.1103/PhysRevC.55.1517

©1997 American Physical Society

Authors & Affiliations

K. Czerski, A. Huke, H. Bucka, P. Heide, G. Ruprecht, and B. Unrau

  • Technische Universität Berlin, Institut für Strahlungs- und Kernphysik, D-10623 Berlin, Germany

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Vol. 55, Iss. 3 — March 1997

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