_{1}

^{*}

Charge equilibration has been recognized as a dominant process at the early stage of low-energy heavy-ion reactions. The production of exotic nuclei is suppressed under the appearance of charge equilibration, in which the proton-neutron ratios of the final reaction products are inevitably averaged. Therefore charge equilibration plays one of the most crucial roles in the synthesis of chemical elements. Focusing on how and when the charge equilibration takes place, zero sound propagation in femto-scale quantum liquids is explained.

This article is concerned with Fermionic property of heavy ions (many-nucleon systems with the size up to several 10-femtometers) colliding at the energy of a few MeV per nucleon. In the following, we refer to those collisions as low-energy heavy-ion collisions. Fusion is not necessarily achieved in the low-energy heavy-ion collisions, neither is fragmentation. Reaction dynamics and the resulting products can be drastically different depending on the impact parameter, the mass of colliding ions, and so on. Therefore the reaction mechanism of low-energy heavy-ion collisions is worth investigating to understand the production of chemical elements. This is deeply concerned with an open problem as for the existence and the origin of chemical elements including their production mechanism.

Charge equilibrium in heavy-ion reactions means the states with the proton-neutron ratio corresponding to the average of the colliding ions, and charge equilibration is the process leading towards charge equilibrium. The chemical property of final products can be different depending on whether charge equilibration appears or not. There is a relatively long research history for the charge equilibration. In fact many experiments of low-energy heavy-ion collisions were carried out in the 1960s. In those experiments most of the final products were reported to be in charge equilibrium, even when fragmentation takes place [

One of the most important features of charge equilibration is its rapidness taking as much as a few 10^{−22} s [^{−20} s), so that charge equilibration has been recognized as an inevitable and dominant process in low-energy heavy-ion reactions. The relation between charge equilibration and the isovector giant dipole resonance has been studied relatively well because of the correspondence in their time scales, but no decisive conclusion has ever been obtained. Indeed, including the question of “when does charge equilibration take place ?”, many things could not be explained merely by the isovector giant dipole resonance. For the theoretical research on the relation between charge equilibration and the isovector giant dipole resonance, the importance of dipole mode to charge distribution of a fissioning nucleus was pointed out by HillWheeler [

Let us denote a many-particle wave function by . It is assumed to satisfy

where denotes the Hamiltonian operator. The solution can be represented by under a suitable boundary condition, if does not de- pend on. Let the corresponding probability density be, and begin with the classic theory of sound propagation inside gases. Readers may wonder why sound propagation is related to charge equilibration, it will be clarified step by step. Let the equilibrium probability density be. If the fluctuation is added to the equilibrium:

a force arises from the gradient pressure. Here the essential property of sound propagation is extracted from the simplified linearized analysis. The equation of motion is given by

where and denote the velocity and the pressure, respectively. The pressure depends on both and the entropy. On the other hand, the equation of continuity is given by

The right hand side is approximated by to the lowest order. After differentiating this equation by, an equality is derived together with the divergence of Equation (1). If we further assume that is expanded with respect to at a fixed entropy, the lowest order contribution brings about

This is a wave equation for, where represents the propagation speed of the density. For example, is given by for the perfect Fermi gas in its ground state (), where means the Fermi velocity. This type of propagation is called first sound, which provides a picture for particles propagating with changing density.

On the other hand, we should pay attention to the propagation of particle without changing density. This type of propagation is called zero sound, which has a finite frequency even when the wave number is equal to zero (cf. zero point vibration). To understand zero sound, the linear response is considered for a given external field:

where denotes the number density operator. In particular, if we restrict ourselves to the impulsive perturbation, the linear response is

where denotes the retarded generalized dielectric function. The resonance frequency can be calculated by the pole of the integrand of the right hand side. Eventually we assume the phonon dispersion relation (), which reproduces the frequency of propagating wave, and is nonzero even when the wave number is equal to zero:

then the resonance frequency is obtained. Consequently the dispersion relation at long wave length becomes

where; and denote the mass and the Fermi wave number, respectively. Note that this relation is the representation in momentum space. The lower-limit of the velocity for zero sound is the Fermi velocity, because the non-damping mode can only exist when (see the denominator inside the logarithmic function). If is assumed in the limit, the left hand side becomes, and the propagation velocity of zero sound is represented using. For the weak-coupling limit ():

and for the strong-coupling limit ():

This shows that the propagation velocity of zero sound is almost equal to in the weak-coupling limit. It is just times faster than the previously seen first sound velocity of the perfect Fermi gas. A rather general discussion shows that zero sound is faster than first sound [7,8]. Roughly speaking, the matter waves without changing density propagate more easily than those with changing density, because the change in density possibly leads to the appearance of larger restoring force. Zero sound provides a picture of particle exchange within a quite short time (but not instantaneous).

Two different sound propagations in Fermi liquids have been discussed in terms of whether they entail the density change or not. In particular there exists zero sound in Fermionic many-body system, which is different from and faster than the ordinary sound. Zero sound has been known to arise from the collective dynamics of the Fermionic many-body systems. All the collective dynamics is actually based on the propagation of zero sound, while there are various representations (various modes) for the collective dynamics. One distinct difference between zero and first sounds is their relation to collisions between particles. First sound appears when the states are in local thermal equilibrium. This corresponds to the situation when the mean interparticle collision time is sufficiently smaller than the oscillation period of the propagating wave. Meanwhile zero sound is associated with the collective excitation mode, which disappears when there are many collisions between particles. This corresponds to the situation when the mean interparticle collision time is larger than the oscillation period of the propagating wave. Although such a collisionless energy regime is expected to be realized due to the Pauli principle, its validity should be confirmed for each individual physical system. Consequently zero sound is expected to be important to low-energy phenomena, while first sound becomes effective at higher energies. For the usage of the terminology low and high energies, we had better note that both sounds are scaled by (i.e. Fermi energy). For more details of sound propagation, see Section 5 of Ref. [

As a theoretical research on zero sound in Fermionic many-body systems, Landau’s Fermi liquid theory [10, 11] is well known, where zero sound propagation was actually seen in liquid ^{3}He [12,13]. However, there is no guarantee that such a sound plays a role in heavy-ion reactions. There are two essential differences between heavy-ion reactions and the ^{3}He case; the physical system consists of finite numbers of nucleons, and the event is accomplished within a finite time interval. That is to say, both size and time are highly restricted in heavy-ion reactions. Indeed, in the context of many-nucleon systems, the main interest of zero sound propagation was not in heavy-ion reactions but in nuclear vibrations (for example, see Ref. [

As an example of Fermionic many-body systems, we consider many-nucleon system. There are two types of nucleons, that is, protons and neutrons. Charge equilibration is the mixing of protons and neutrons due to the time evolution, therefore it is a kind of chemical mixing. Apart from such a chemical equilibration, there are several kinds of equilibration in heavy-ion reactions, that is, mass equilibration, momentum equilibration, and thermal equilibration. Among them charge equilibration (chemical equilibration) has drawn special attention because of its crucial role in the synthesis of chemical elements.

Let us consider the collision of two ions. The existence of an upper energy limit for charge equilibration has been pointed out by Iwata-Otsuka-Maruhn-Itagaki [

where identifies the two colliding ions, and means the energy in the laboratory frame. and, which satisfy, and, denote the masses of the two colliding ions, where, , and denote the proton and the neutron numbers of each colliding ion (labeled by), respectively. and are parameters introduced based on Ref. [15,16]. This formula provides an upper energy limit of charge equilibration, which arises from the nucleons propagating at the Fermi velocity. In heavy-ion collisions, there are four different Fermi velocities (Fermi energies), because there are two different kinds of nucleons and two colliding ions. The first term on the right hand side of Equation (3) calculates those four Fermi velocities. If only the Fermi velocities (for neutrons and protons) of the total merged system are taken, experimental results cannot be explained because the charge equilibration is accomplished before the formation of a compound nucleus (see the experimental comparison shown in Ref. [

The nucleons propagating at the Fermi velocity, which is represented by Equations (3) and (4), correspond to the propagation of zero sound. Indeed, according to the calculation of the mean free path of nucleons inside nuclear matter [

^{52}Ca (N/Z = 32/20) to ^{36}Ca (N/Z = 16/20). Cases with two different impact parameters and two different energies are compared. Because this heavy-ion reaction is classified to class II of the classification shown in ^{52}Ca and ^{36}Ca on the N-Z plane, its charge equilibration dynamics can be measured mostly by the flow of neutrons. The final products are different, where only the case with fm and E/A = 1.0 MeV results in fragmentation, while the other cases result in fusion. Despite such significant differences in final products, the propagation speed of charge equilibrating flow is almost the same. Indeed, the wave front of N/Z = 1.10 propagates 6.5 fm in 0.75 × 10^{−}^{22} s after the neck formation (the neck is formed at 6.0 × 10^{−}^{22} s for E/A = 1.0 MeV and 3.0 × 10^{−}^{22} s for E/A = 2.0 MeV). It shows that the propagation speed of charge equilibrating flow is in-

dependent of the incident energy (the relative velocity of collision) and the impact parameter, while the total neutrons included in neutron-rich flow depends highly on the incident energy. In particular the propagation speed of charge equilibrating flow is faster than the relative velocity of collision (

With respect to zero sound, what was clarified in Ref. [^{−}^{22} s, is realized as nucleon propagation without changing density. Third, there exists an upper energy limit for the fast charge equilibration, which corresponds to the energy limit at which zero sound can survive. For example, as is shown in Ref. [^{40}Ar + ^{58}Ni at E_{lab}/A = 7.0 MeV and ^{56}Fe + ^{165}Ho at E_{lab}/A = 8.3 MeV, and the disappearance of charge equilibration for ^{112}Sn + ^{124}Sn at E_{lab}/A = 50 MeV. For the terminology of “fast” charge equilibration, it takes into account the existence of another kind of charge equilibration that has nothing to do with zero sound propagation. Such charge equilibration, which appears at higher energies, is more related to the first sound. Therefore its process is relatively slow compared to the fast charge equilibration, and insufficient to lead to fusion or to charge equilibrium for most fragments. Charge equilibration at higher energies was also studied well (for example, see references [8-10,20-23] of Ref. [

As a remark, the previous research on charge equilibration with respect to the collective dynamics is mentioned. As is discussed, charge equilibration was studied in association with the isovector giant dipole resonance. Charge equilibration is sometimes related to the isovector dipole resonance, but not in all cases; i.e. the concept of resonance is too restrictive to explain charge equilibration. Nevertheless isovector giant dipole resonance means that the modes related to the composite nucleus play a role, it cannot explain the different upper energy limits for different reactions having exactly the same composite nucleus. In addition, an isovector mode different from the isovector giant dipole resonance sometimes appears (see

Apart from how and when charge equilibration takes place, here we see the reason why charge equilibration takes place. First of all, the propagation of zero sound is expected to be efficient to any kind of nucleon propagations and vibrations. The answer is obtained by clarifying the origin of charge equilibration. When the two ions have a contact during the heavy-ion collisions, large fluctuations appear in the shape and the internal structure. Zero sound is expected to contribute to stabilization by changing both the shape and the internal structure, which can be understood by the contribution of each term included in the Bethe-Weizsäcker mass formula [19,20]:

where the coefficients are given by MeV, MeV, MeV and MeV, respectively [

libration is closely related with zero sound propagation.

The propagation of charge equilibrating flow has been visualized, and a physical interpretation has been given to the fast charge equilibration; i.e., the fast charge equilibration is realized by zero sound propagation in which their propagation speeds coincide with each other. This means that the collective dynamics of the many-nucleon system and thus its Fermionic statistical property are essential to the fast charge equilibration. In this context the upper energy limit for the fast charge equilibration corresponds to the upper-limit energy for zero sound propagation to be effective. Consequently charge equilibration should be regarded as the exchange of nucleons (charge exchange), because zero sound does not necessarily entail density change.

The correspondence of zero sound propagation in femto-scale systems is not only the giant dipole resonance, but also the flow propagating almost at the Fermi velocity. Indeed, the similarity between neutron-rich flow shown in

As is discussed, the fast charge equilibration is not a process appearing only at a certain energy. The fast charge equilibration universally appears in low-energy heavy-ion reactions at energies lower than the upper energy limit, instead. Note that the fast charge equilibration process becomes operational only if the two colliding ions interact by the nuclear force.

This work is based on the collaboration with Profs. T. Otsuka, J. A. Maruhn, and N. Itagaki, and supported by the Helmholtz alliance HA216/EMMI. The author thanks to Prof. J. A. Maruhn for reading the manuscript carefully. Encouragement from Dr. C. Simenel at the initial stage of this research is acknowledged.