exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3
exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3
exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3
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difference comes from the opposite evolution of<br />
the fragment multiplicity—see below.<br />
Figure 2: Same as figure 1, for the light charged<br />
particle (Z≤2) multiplicities. All statistical<br />
errors amount to 0.04.<br />
As appears in the table, the composite system with<br />
N/Z=1.385 has been formed by three different entrance<br />
channels. It is interesting to note that, within<br />
the error bars, the measured multiplicities are the<br />
same. This confirms that the selected quasi-fusion<br />
sources have lost the entrance channel memory<br />
<strong>and</strong> reached a high degree of equilibration [1].<br />
fragments.<br />
As already noted for total <strong>and</strong> lcp multiplicities, the<br />
fragment multiplicity is independent of the entrance<br />
channel mass asymmetry for a given composite<br />
system.<br />
Some indications of the evolution of the multiplicities<br />
with the neutron-richness of the system were<br />
already noted in [3,4] . The independence of the<br />
entrance channel for a given N/Z is however an<br />
original new result.<br />
Dynamical simulations<br />
The <strong>reaction</strong> dynamics can be followed by solving<br />
the BNV transport equation that describes the evolution<br />
of the one-body distribution function according<br />
to the nuclear mean-field <strong>and</strong> two-body collisions<br />
. The compressibility modulus is K=200 MeV,<br />
And the free nucleon-nucleon cross-section with its<br />
energy, angular <strong>and</strong> isospin dependence is used.<br />
Two different prescriptions for the symmetry energy<br />
term [5] are chosen: an asy-stiff one (linear<br />
increase of the potential symmetry term with density)<br />
or an asy-soft term roughly varying as the<br />
square root of the density.<br />
The first results, obtained for 124 Xe+ 112 Sn <strong>and</strong><br />
136 Xe+ 124 Sn at 45 MeV/nucleon, show the same<br />
relative increase of the fragment number at the<br />
end of the BNV calculation (i.e. before deexcitation<br />
<strong>and</strong> filter by the experimental apparatus)<br />
as observed experimentally. The asy-stiffness of<br />
the EOS does not influence the fragment multiplicity<br />
for the neutron poor system, while slightly more<br />
fragments are produced in the asy-stiff case for the<br />
neutron-rich one.<br />
References<br />
[1] F. Gagnon-Moisan et al., Proceedings of the IWM2009.<br />
[2] G. Tabacaru et al., Eur. Phys. J. A 18, 103, 2003.<br />
[3] J. F. Dempsey et al., Phys. Rev. C 54, 1710, 1996.<br />
[4] G. J. Kunde et al., Phys. Rev. Lett. 77, 2897, 1996.<br />
[4] V. Baran et al., Nucl. Phys. A703, 603, 2002.<br />
Figure 3: Same as figure 1, for the fragment<br />
(Z≥5) multiplicities. Statistical errors are<br />
0.02.<br />
The multiplicities for fragments (Z≥5) are displayed<br />
in figure 3. Conversely to lcp multiplicities, they<br />
only slightly increase (by about 5%) with the incident<br />
energy. Indeed the systems become more<br />
fragmented at higher energies, <strong>and</strong> the charge of<br />
the products becomes smaller [2]. Thus a larger<br />
number of them have a charge smaller than 5,<br />
which is the lower limit for our “fragment” definition.<br />
The interesting point is the increase of the<br />
fragment multiplicity for neutron-rich systems. M frag<br />
increases by about 8% when N/Z sys increases from<br />
1.27 to 1.5. This larger fragment number can be<br />
attributed to the larger quantity of available neutrons,<br />
which helps the formation of more stable<br />
105