2008
DOI: 10.1016/j.physletb.2008.05.007
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Prompt dipole radiation in fusion reactions

Abstract: The prompt γ -ray emission is investigated in the 16 A MeV energy region by means of the 36,40Ar + 96,92Zr fusion reactions leading to a compound nucleus in the vicinity of 132Ce. The dynamical nature\ud of this radiation is confirmed. We show that the prompt γ radiation has an angular distribution pattern\ud consistent with a dipole oscillation along the symmetry axis of the dinuclear system. The data are\ud compared with calculations based on a collective bremsstrahlung analysis of the reaction dynamics

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Cited by 30 publications
(43 citation statements)
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“…Our data therefore suggest that the DD γ-emission time scale is confined at the beginning of the reaction, in agreement with our previous results [8] for evaporation events and with theoretical expectations [4]. By taking into account the an DD γ-ray angular distribution (a 2 = -1) for evaporation events and the response function of the experimental setup, the DD yield, integrated over energy and over angle, is (1.2 ± 0.2)*10 −3 .…”
Section: Resultssupporting
confidence: 93%
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“…Our data therefore suggest that the DD γ-emission time scale is confined at the beginning of the reaction, in agreement with our previous results [8] for evaporation events and with theoretical expectations [4]. By taking into account the an DD γ-ray angular distribution (a 2 = -1) for evaporation events and the response function of the experimental setup, the DD yield, integrated over energy and over angle, is (1.2 ± 0.2)*10 −3 .…”
Section: Resultssupporting
confidence: 93%
“…It is interesting to note that E DD is lower than the centroid energy of the GDR built on the ground state of a nucleus of similar mass, E GDR = 14 MeV. This result confirms the high deformation of the emitting source at the moment of the DD γ emission, in agreement with expectations [2,3] and with our previous works [7,8].…”
Section: Resultssupporting
confidence: 91%
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