Volume 63, Number 4, August 2003
|Page(s)||524 - 530|
|Published online||01 November 2003|
decay of and its possible astrophysical implications
Ruder Bošković Institute - Zagreb, Croatia
2 INFN-Laboratori Nazionali del Sud and Università di Catania - Catania, Italy
Accepted: 17 June 2003
The excitation energy spectrum has been obtained from coincidence measurements of the reaction at . The decay of the states at excitations between 10 and 16 into has been observed for the first time. Observed α-decay indicates possible cluster structure of the excited states. The influence of these states on the cross-section of the astrophysically important () and reactions is discussed and the results are compared with existing results.
PACS: 21.10.-k – Properties of nuclei; nuclear energy levels / 26.35.+c – Big Bang nucleosynthesis / 27.20.+n –
© EDP Sciences, 2003
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