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Three-α-particle reactions in kinematical star conditions

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Abstract

The10B(d, αα)4He reaction was studied at energies between 4.2 and 6.6 MeV in kinematical plane-star conditions with special emphasis on sequential processes through the8Be state of 11.4 MeV. The results are compared with predictions of the Quebert model.

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Authors and Affiliations

  1. Ruder Bošković Institute, P.O. Box 1016, 41001, Zagreb, Croatia

    M. Bogovac, Đ. Miljanić, D. Rendić & M. Zadro

  2. Istituto Nazionale di Fisica Nucleare, I-95129, Catania, Laboratorio Nazionale del Sud, Italy

    G. Calvi, M. Lattuada, F. Riggi & C. Spitaleri

Authors
  1. M. Bogovac
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  2. G. Calvi
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  3. M. Lattuada
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  4. Đ. Miljanić
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  5. D. Rendić
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  6. F. Riggi
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  7. C. Spitaleri
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  8. M. Zadro
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Dedicated to Profs. Erich Schmid and Ivo Šlaus on the occasion of their 60th birthdays

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Bogovac, M., Calvi, G., Lattuada, M. et al. Three-α-particle reactions in kinematical star conditions. Few-Body Systems 12, 191–199 (1992). https://doi.org/10.1007/BF01074815

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  • DOI: https://doi.org/10.1007/BF01074815

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