Energetics of midvelocity emissions in peripheral heavy ion collisions at Fermi energies
arXiv:nucl-ex/0405032 · doi:10.1103/PhysRevLett.93.232701
Abstract
Peripheral and semi-peripheral collisions have been studied in the system 93Nb+93Nb at 38 AMeV. The evaporative and midvelocity components of the light charged particle and intermediate mass fragment emissions have been carefully disentangled. In this way it was possible to obtain the average amount not only of charge and mass, but also of energy, pertaining to the midvelocity emission, as a function of an impact parameter estimator. This emission has a very important role in the overall balance of the reaction, as it accounts for a large fraction of the emitted mass and for more than half of the dissipated energy. As such, it may give precious clues on the microscopic mechanism of energy transport from the interaction zone toward the target and projectile remnants.
arXiv comment4 pages, 3 figures, RevTex4 style
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Cited by in corpus (6)
- Correlations between emission timescale of fragments and isospin dynamics in Sn+Ni and Sn+Ni reactions at 35 AMeV
- IMF isotopic properties in semi-peripheral collisions at Fermi energies
- Particle and light fragment emission in peripheral heavy ion collisions at Fermi energies
- Comparison of AMD calculations with experimental data for peripheral collisions of 93Nb+93Nb,116Sn at 38 MeV/nucleon
- Distinctive features of Coulomb-related emissions in peripheral heavy ion collisions at Fermi energies
- Size and asymmetry of the reaction entrance channel: influence on the probability of neck production