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Zeitschrift für Physik A Hadrons and Nuclei

, Volume 352, Issue 4, pp 353–354 | Cite as

Comment on the7Li(p, γ)8Be reaction at energies of astrophysical interest

  • H. R. Weller
  • R. M. Chasteler
Short Note

Abstract

The results of two recent publication are reconsidered. These papers argue that the p-wave effects seen in the7Li(p, γ)8Be reaction belowEp=80 keV can be accounted for by considering the low-energy tail of the p-wave resonance atEp=441 keV. It is shown that the cross section and analyzing power data require an order-of-magnitude more p-wave strength when considered together.

PACS

25.40.Lw 24.70.+s 95.30.Cq 

References

  1. 1.
    R.M. Chasteler, H.R. Weller, D.R. Tilley, and R.M. Prior, Phys. Rev. Lett.72 (1994) 3949.Google Scholar
  2. 2.
    C. Rolfs and R.W. Kavanagh, Z. Phys. A350 (1994) 93.Google Scholar
  3. 3.
    D. Zahnowet al., submitted for publicationGoogle Scholar
  4. 4.
    R.G. Seyler and H.R. Weller, Phys. Rev.C20 (1979) 453.Google Scholar
  5. 5.
    B. Mainsbridge, Nucl. Phys.21 (1960) 1.Google Scholar
  6. 6.
    F.C. Barker, Aust. J. Phys.33 (1980) 159.Google Scholar

Copyright information

© Springer-Verlag 1995

Authors and Affiliations

  • H. R. Weller
    • 1
  • R. M. Chasteler
    • 1
  1. 1.Nuclear LaboratoryDuke University and Triangle UniversitiesDurhamUSA

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