14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June PRE-EQUILIBRIUM (EXCITON) MODEL AND THE HEAVY-ION REACTIONS WITH CLUSTER EMISSION E. Běták Inst. of Physics, Slovak Acad. Sci., Bratislava, Slovakia J. Cseh ATOMKI, Debrecen, Hungary

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June Motivation 2.Consistency of the exciton model – master eq. approach 3.Coalescence and Iwamoto-Harada model for cluster emission in its density formulation 4.Extensions of the Iwamoto-Harada model 5. Cluster emission with angular momentum variables 6.Cluster emission from heavy-ion collisions

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June MOTIVATION Candidates for hyperdefomed nuclei are expected to be formed (relatively easily) in (light) heavy-ion reactions at not too high energy (say, incident energy of few tens or as a maximum few hundreds of MeV). Some combinations of colliding ions have been suggested. The question is, which energies seem to be favourable for their creation. We aim to get some hints for this process, and illustrate it on the 20Ne + 20Ne -> 36 Ar (plus something: α, 2n+2p, n+p+d, …) The production cross section serves as the main indiucator. Therefore we applied statistical pre-equilibrium model with additions suitable to this aim.

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June CONSISTENCY OF THE EXCITON MODEL - MASTER EQUATIONS APPROACH Master equations are capable to describe the whole process in time from the very creation of the composite system through its equilibration up to the decay of compound nucleus within a single formalism, not mixing various approaches. Using the density-dependent formulation of the so-called Iwamoto- Harada model (Dobes and Betak, 5 years before I+H) for cluster emission, pick-up as well as knock-out can be included. Obviously, one pays for the single approach with the lost of majority details, like details of the structures in spectra, but the cross sections describe the average trends rather satisfactorilly. A technical handicap remains: the set of master equations is huge, but we have a suitable algorithm to solve it.

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June COALESCENCE MODEL FOR CLUSTER EMISSION Kalbach (Cline, Kalbach-Cline, Kalbach-Walker), Ribanský & Obložinský Emision rate (nucleons): Coalescence clusters:

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June coalescence IH model IHB model knock-out COALESCENCE (IWAMOTO-HARADA) MODEL FOR CLUSTER EMISSION IN ITS DENSITY FORMULATION

Generalized (coalescence + pickup) Iwamoto & Harada, Dobeš & Běták, Bisplinghoff EMISSION RATE PROPORTIONAL to the CLUSTER FORMATION PROBABILITY SINGLE-CLUSTER DENSITY INVERSELY PROPORTIONAL to the CLUSTER FORMATION PROBABILITY THEREFORE the result is PARAMETERLESS ! 7

 Bisplinghoff Pickup limited by the binding energy of nucleons in the cluster (i.e. about 28 MeV for alphas and 2 MeV for deuterons)  Now Limitation due to binding energy for all clusters Only low-exciton configurations with pickup (CN limit!) Thermal “blurring” considered Admixture allowed for all potential well (Heisenberg uncertainty relation) Possibility of knockout (initial stage only) for alphas 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June

9 Calculations without spin (old) a) deuterons

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June Bb) alphas

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June c) α-knockout admixtures from the fit to the data

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June Cluster emission with with angular momentum variables

Spin variables: Coupling of nucleons to form a coalescence or pickup cluster may be – in a very rough approximation – considered included in the formation probability. Therefore, no additional couplings appear in the emission rates and the only place affected by the angular momentum are different transition coefficients and via competitions to other (nucleon,γ) channels. Exception: knock-out – α-particle is not formed during reaction, but it is already present in the target nucleus. 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June Primary nucleon, deuteron, alpha and gamma energy spectra (gammas with cascades) from 197Au+p at 62 MeV

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June

HEAVY IONS – INITIAL CONFIGURATION (without spin variables today) Cindro et al.: for lower energies, where 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June

HEAVY IONS – CLUSTER BREAKUP Kalbach Walker, www-nds.iaea.org/fendl3/docs/dBreakupRCM2.pdf where the normalizatoion factor is only weakly sensitive to the projectile. We use this as very rough initial approximation. 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June

14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June P r e l i m i n a r y 20 Ne + 20 Ne

CONCLUSIONS Clusterization itself parameterless Effective only at initial stages, what enables proper equilibrium (compound nucleus) limit Thermal blurring of nucleons allowed Pickup (IHB) generalized to all types of clusters  For strongly bound ejectiles knockout possible: Included angular momentum, but the couplings of nucleons to form a cluster are hidden in cluster formation probability Introduction of spin variables enhances the cluster emission compared to spin-independent case. (It plays similar role as deformation according to Blann & Komoto) All calculations presented here are just with default parameters (level densities, inverse c.s., transition matrix element). Possibility to indicate various contributing mechanisms leading to the same (nearly equilibrated) composite system, and to select the most suitable conditions for structure studies, like existence of hyperdeformed nucli. Further effort: heavy ions, cluster emission, pre-equilibrium with some elements of direct reactions and spin variables tgogether within one formalism 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June

Thank you 14th Internat. Conf. Nucl. Reaction Mechanisms, Varenna, 19th June