Slope of the astrophysical S factor for the 7Li(p,γ)8Be reaction

M. Spraker, R. M. Prior, M. A. Godwin, B. J. Rice, E. A. Wulf, J. H. Kelley, D. R. Tilley, and H. R. Weller
Phys. Rev. C 61, 015802 – Published 17 December 1999
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Abstract

Polarized proton beams of 80 and 60 keV, and a biased target have been used to determine the slope of the astrophysical S factor for the 7Li(p,γ)8Be reaction from direct measurements at proton energies from 40 to 100 keV for capture to both the ground and the first excited states of 8Be. The results indicate a negativeslope for both cases. Vector analyzing power measurements at 90° were also obtained for proton energies from 40 to 80 keV. It is shown that the negative slope can be accounted for by considering the effect of the subthreshold resonance state at 16.6 MeV if the capture into this weakly bound, subthreshold state occurs at an effective radius of about 46 fm. The effect of this state increases the extrapolated value of the S factor at Ep=0 from the previous value of 0.3 keV b to the present value of 0.50 keV b.

  • Received 25 January 1999

DOI:https://doi.org/10.1103/PhysRevC.61.015802

©1999 American Physical Society

Authors & Affiliations

M. Spraker1,2, R. M. Prior1,2, M. A. Godwin2,3, B. J. Rice2,3, E. A. Wulf2,3, J. H. Kelley2,3, D. R. Tilley2,4, and H. R. Weller2,3

  • 1Department of Physics, North Georgia College and State University, Dahlonega, Georgia 30597
  • 2Triangle Universities Nuclear Laboratory, Duke Station, Durham, North Carolina 27708
  • 3Department of Physics, Duke University, Durham, North Carolina 27707
  • 4Department of Physics, North Carolina State University, Raleigh, North Carolina 27695

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Vol. 61, Iss. 1 — January 2000

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