Hard Gammas from Low-Energy Heavy-Ion Collisions

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Single-particle radiative mechanism of $γ$ emission embedded into the pre-equilibrium exciton model is used to calculate the $γ$ emission from a decay of $^{160}$Er$^{*}$ created in two different ways. The initial stage of a reaction is described using momentum-space overlaps of colliding nuclei. We can reproduce the main features of the observed $γ$ energy spectra including the fact that the spectrum observed in more symmetric combination is slightly harder than in the other case.
7 pages, LaTeX file followed by 1 PostScript Figure To be published in "Acta Physica Slovaca"(fax (+42-7)376085)

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