1988
DOI: 10.1103/physrevlett.61.927
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Selective Parity Transitions and Dinuclear Orbiting ofC12+Mg

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Cited by 38 publications
(25 citation statements)
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“…like angular dependence -characteristic of a long-lived, orbiting, dinuclear complex. Similar results have been obtained for 20 Ne + 12 C system [12,13], where resonance-like behaviour was also found in the excitation functions for several outgoing channels, which was similar to the observation made for symmetric 16 O + 16 O system [25,26,27,28]. Enhancements of large angle, binary reaction yields have also been observed in somewhat heavier 28 Si + 28 Si, 24 Mg + 24 Mg systems [1], where significant non resonant background yield was observed at higher excitation energies.…”
Section: Introductionsupporting
confidence: 89%
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“…like angular dependence -characteristic of a long-lived, orbiting, dinuclear complex. Similar results have been obtained for 20 Ne + 12 C system [12,13], where resonance-like behaviour was also found in the excitation functions for several outgoing channels, which was similar to the observation made for symmetric 16 O + 16 O system [25,26,27,28]. Enhancements of large angle, binary reaction yields have also been observed in somewhat heavier 28 Si + 28 Si, 24 Mg + 24 Mg systems [1], where significant non resonant background yield was observed at higher excitation energies.…”
Section: Introductionsupporting
confidence: 89%
“…[13] and assuming the excitation energy division follows the mass ratio [1]) are in qualitative agreement with the experimental results obtained at 9 MeV/nucleon by Rae et al [41] for the sequential decay of 20 Ne + 12 C. It was found that even at the highest excitation energy, secondary decay of Si * and Al * do not reach up to N; the contribution of primary Mg * , Na * decay to Z ≤ 7 were estimated to be < ∼ 1% of the primary yield and that of Ne * decay to N, C, B yield were estimated to be ∼ 10-20%, ∼ 15-20% and ∼ 30-50% of the primary yield, respectively. Nearly ∼ 40-45% of the primary O * produced through binary exit channel 16 O + 16 O decays to C. The secondary decay yields from the primary excited fragments are shown in Fig. 9 for different bombarding energies.…”
Section: A Contribution From Secondary Decay Of Heavier Fragmentsmentioning
confidence: 99%
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