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AstrophysicalS(E) factor of10B(p, α1)7Be at low energies

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Zeitschrift für Physik A Hadrons and Nuclei

Abstract

The absolute cross section of the fusion reaction 10B(p, α1γ)7 has been measured at the c.m. energy range E=48 to 159 keV via the 429 keV secondary γ-ray transition. The studies involved high proton currents and thick solid 10Btargets. The resulting cross sections have the same energy dependence as those of the 10B(p,α0)7Bereaction but they are lower by a factor 600.

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References

  1. Angulo, C., Engstler, S., Raimann, G., Rolfs, C., Schulte, W.H., and Somorjai, E., Z.Phys. A (1993) (in print).

  2. Wüstenbecker, S., Ebbing, H., Schulte, W. H., Baumeister, H., Becker, H. W., Cleff, B., Rolfs, C.S., Trautvetter, H. P., Mitchell, G. E., Schweitzer, J. Peterson, C. A.,Nucl. Instr. Meth. A279 (1989) 448.

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Authors and Affiliations

  1. Institut für Physik mit Ionenstrahlen, Ruhr-Universität, Postfach 102148, W-4630, Bochum 1, Germany

    C. Angulo, W. H. Schulte, D. Zahnow, G. Raimann & C. Rolfs

Authors
  1. C. Angulo
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  2. W. H. Schulte
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  3. D. Zahnow
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  4. G. Raimann
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  5. C. Rolfs
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Additional information

Supported in part by the Deutsche Forschungsgemeinschaft (Ro429/18-2 and Ro429/21-3), the Landesamt Nordrhein Westfalen (IVA5-10600387), and the Comision Intel-ministerial de Ciencia y Technologia (AEN90-0932).

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Angulo, C., Schulte, W.H., Zahnow, D. et al. AstrophysicalS(E) factor of10B(p, α1)7Be at low energies. Z. Physik A - Hadrons and Nuclei 345, 333–334 (1993). https://doi.org/10.1007/BF01280844

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  • DOI: https://doi.org/10.1007/BF01280844

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