Akira Ono
Tohoku University Sendai, JAPAN
Abstract
It has been known that light clusters, such as $\alpha$ particles and
deuterons, are copiously formed in heavy-ion collisions in various
conditions. For example, in Au + Au central collisions at several
hundred MeV/nucleon, about 80\% of protons in the system are bound in
clusters and heavier fragments. This fact suggests that cluster
correlations may play important roles during the dynamical evolution
of heavy-ion collisions. Understanding of clusters may be also very
important when we try to get information on symmetry energy from
heavy-ion collisions.
Transport models should be carefully constructed in order to allow the
appearance of cluster correlations with the correct probabilities
during the time evolution of reactions. In the case of the AMD
approach, the two-nucleon collision process has been generalized by
allowing one or both of the colliding nucleons $N_1$ and $N_2$ to form
clusters with surrounding particles as $N_1+N_2+B_1+B_2\rightarrow
C_1+C_2$. We consider clusters ($C_1$ and $C_2$) up to $\alpha$
particles, and they are represented by placing Gaussian wave packets
at the same phase space point.
In this presentation, I will discuss the effects of cluster
correlations in heavy-ion collision dynamics. For neutron-rich
reaction systems, a typical effect of cluster formation, in particular
$\alpha$-cluster formation, is to enhance the neutron-proton asymmetry
of the rest of the system, i.e., $(N-2n_\alpha)/(Z-2n_\alpha) > N/Z$
when $N>Z$. This is at least partly responsible for the enhancement
of the neutron-proton (or triton-${}^3\mathrm{He}$) spectrum ratio at
low velocities in the center-of-mass frame of expanding and
fragmenting neutron-rich systems. Another effect of cluster
correlations in expanding systems is that nucleons and clusters cease
interacting with each other earlier than in the case without cluster
correlations where nucleons continue to interact until a relatively
late time. As a consequence, the spectra of emitted particles carry
direct information at an earlier time in the case of strong cluster
correlations. In central collisions of neutron-rich nuclei at 300
MeV/nucleon, the AMD calculation with cluster correlations shows that
the symmetry energy effect on the neutron-proton dynamics at the
compression stage is rather directly reflected in the neutron-proton
spectra in the final state.