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exotic nuclei structure and reaction noyaux exotiques ... - IPN - IN2P3

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for peripheral ones. In experiments radial collective<br />

energy was recognized, in most of the cases, from<br />

comparisons of kinetic properties of fragments with<br />

models/ simulations.The mean relative velocity<br />

between fragments, β rel , independent of the reference<br />

frame, allows to compare radial collective<br />

energy for both types of sources (QF or QP). The<br />

effect of the source size (Coulomb contribution on<br />

fragment velocities) can be removed by using a<br />

simple normalization which takes into account,<br />

event by event, the Coulomb influence, in velocity<br />

space, of the mean fragment charge.<br />

All the quantitative information concerning the evolution<br />

of radial energy, E R , with excitation energy<br />

for both types of sources is presented in figure 1.<br />

At an excitation energy of about 5 AMeV, the β rel<br />

Figure 2: Left <strong>and</strong> right sides refer respectively to the<br />

mean charge of the heaviest fragment of partitions<br />

, <strong>and</strong> to the generalized asymmetry in charge of<br />

the fragment partitions without the heaviest one,<br />

Az\{Z1}, (see text) as a function of the reduced fragment<br />

multiplicity, Mfrag/, for different total excitation<br />

per nucleon of the sources. Full squares, open <strong>and</strong><br />

full circles st<strong>and</strong> respectively for QF sources <strong>and</strong> QP<br />

sources produced at 80 <strong>and</strong> 100 AMeV incident energies.<br />

values corrected from Coulomb effects <strong>and</strong> corresponding<br />

to QF <strong>and</strong> QP sources are similar. We<br />

have also added the E R values published by the<br />

ISIS collaboration [3] corresponding to the π - +Au<br />

<strong>reaction</strong>s which provide sources equivalent to the<br />

QP ones in terms of excitation energy range <strong>and</strong><br />

size. The observed evolution of E R for such sources<br />

is almost the same as for QP sources. For hadron-induced<br />

<strong>reaction</strong>s the thermal pressure is the<br />

only origin of radial expansion, which indicates that<br />

it is the same for QP sources. To be fully convincing,<br />

an estimate of the part of the radial collective<br />

energy due to thermal pressure calculated with the<br />

EES model [4] for an excited nucleus identical to<br />

QF sources produced at 50 AMeV incident energy<br />

is also reported (open square) in figure 1.<br />

We have shown that radial collective energy is essentially<br />

produced by thermal pressure in semi-<br />

peripheral heavy-ion collisions as it is in hadroninduced<br />

<strong>reaction</strong>s. For QF sources produced in<br />

central heavy-ion collisions the contribution<br />

from the compression-expansion cycle becomes<br />

more <strong>and</strong> more important as the incident energy<br />

increases. Those observations show that the radial<br />

collective energy does influence the fragment partitions.<br />

Moreover it is observed that, at fixed total<br />

excitation energy per nucleon, the evolution of the<br />

average fragment multiplicity normalized to the<br />

source charge/size = is fixed by<br />

the value of the radial collective energy: when E R<br />

increases more fragments are produced.<br />

Scalings of partitions<br />

Does the intensity of the radial collective energy<br />

also govern the details of fragment partitions, namely<br />

the relative charge/size of fragments in partitions.<br />

One can first consider the evolution of the<br />

size of the heaviest fragment, for given total excitation<br />

energies, with the reduced fragment multiplicities<br />

M frag /. On the left panel of figure 2 average<br />

values of the heaviest fragment charge for QP<br />

<strong>and</strong> QF sources are reported: they follow exactly<br />

the same evolution. Finally the division of<br />

the charge among other fragments is investigated<br />

using the generalized asymmetry in charge<br />

of the fragment partitions. One can re-calculate the<br />

generalized asymmetry by removing Z 1 from partitions,<br />

noted A Z \{Z 1 }. The results, displayed in figure<br />

2 (right panel) do not depend on the source type<br />

at a given total excitation energy <strong>and</strong> a given reduced<br />

fragment multiplicity. Note that the general<br />

asymmetry follows a linear trend except for the<br />

lower reduced fragment mutiplicity which corresponds<br />

to M frag =2; indeed in that case, after removing<br />

Z 1 , only one fragment is available for the<br />

asymmetry calculation <strong>and</strong> in each event the heavier<br />

Z of the partition below Z equal 5 was taken.<br />

Such a result shows the subtle role played by the<br />

radial collective energy. It influences the overall<br />

degree of fragmentation but it does not affect the<br />

relative size of fragments in partitions for fixed reduced<br />

fragment multiplicities. Those scalings represent<br />

a benchmark against which models describing<br />

fragmentation of finite systems should be tested.<br />

In particular the peculiar role of the freeze-out<br />

volume in reproducing or not those scalings must<br />

be investigated.<br />

References<br />

[1] B. Borderie <strong>and</strong> M. F. Rivet, Prog. Part. Nucl. Phys. 61, 551,<br />

2008.<br />

[2] E. Bonnet et al. (INDRA <strong>and</strong> ALADIN Collaborations), Nucl.<br />

Phys. A, 1., 2009.<br />

[3] L. Beaulieu et al., Phys. Rev. C 64, 064604, 2001.<br />

[4] W. A. Friedman, Phys. Rev. C 42, 667, 1990.<br />

[5] E. Bonnet et al. (INDRA <strong>and</strong> ALADIN Collaborations), submitted<br />

to Phys. Rev. Lett.<br />

107

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