Abstract
By taking advantage of the high efficiency of the Coulomb dissociation method, we studied the stellar 22Mg(p, γ)23Al reaction. The radiative width Γγ of the first excited state in 23Al was determined by measuring the intermediate-energy 23Al → 22Mg + p breakup process with a lead target.
Original language | English |
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Pages (from-to) | S1517-S1521 |
Journal | Journal of Physics G: Nuclear and Particle Physics |
Volume | 31 |
Issue number | 10 |
DOIs | |
Publication status | Published - 2005 Oct 1 |