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Physics Research International
Volume 2014 (2014), Article ID 619360, 10 pages
How Much Asymmetry of Colliding Pair Affects Nuclear Dynamics at Balance Point?
Department of Physics, GSSDGS Khalsa College, Patiala 147001, India
Received 5 May 2014; Accepted 21 July 2014; Published 20 August 2014
Academic Editor: Rajeev K. Puri
Copyright © 2014 Supriya Goyal. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Using the quantum molecular dynamics model, we study the nuclear dynamics at the balance energy of mass asymmetric colliding nuclei by keeping the total mass of the system fixed and by varying the mass asymmetry (, where and are the masses of the target and projectile, resp.) of the reaction. In particular, we study the various quantities like average and maximum density and temperature, collision rate, participant-spectator matter, anisotropic ratio, relative momentum, and their mass asymmetry and mass dependence. Our results indicate sizeable effect of mass asymmetry on these quantities.
It is now well established that collective transverse flow of the nucleons is a signature of the interaction and can provide information about the equation of state (EoS) as well as nucleon-nucleon (nn) cross-section of the nuclear matter. Extensive studies have been done over the past three decades on the sensitivity of collective transverse flow towards the nuclear EoS, nn cross-section, and entrance channel parameters such as incident energy of projectile, size of the system (), and colliding geometry (i.e., impact parameter) [1–9]. The disappearance of flow is predicted to appear at some incident energy, which is termed as balance energy () . This balance energy has been subjected to extensive theoretical and experimental calculations to know its accurate value as well as its mass and impact parameter dependence [11–22].
Recently, the sensitivity of collective transverse flow and towards the mass asymmetry of the reaction has been carried out at different colliding geometries by keeping the total mass of the system fixed [20–22]. It has been found that almost independent of total system mass as well as colliding geometry, mass asymmetry has a uniform effect on the collective transverse flow and its disappearance . This study was motivated from the recent observations by FOPI collaboration on the mass asymmetric reactions of + and + [23, 24]. They observe that flow in asymmetric reactions is a key observation for investigating the reaction dynamics. The difference between the reaction dynamics for symmetric and asymmetric reactions is attributed to the different role played by excitation energy in these reactions. In symmetric reactions most of the excitation energy is deposited in the form of compressional energy, whereas an asymmetric reaction deposits it in the form of thermal energy . Therefore, in the present paper, this study is further extended for the central collisions to see the effect of mass asymmetry of the reaction on the nuclear dynamics at the balance energy. Similar work has been carried out by Sood and Puri  for the nearly symmetric and symmetric reactions at the balance energy, but the role of mass asymmetry in the participant-spectator matter, average and maximum density and temperature, net collisions, anisotropic ratio, relative momentum, and the mass dependence of these quantities is not taken care of. This has been taken care of in the present study. The study is made within the framework of quantum molecular dynamics (QMD) model [12–18, 20–22, 25–44], which is explained in Section 2. Results and discussion are explained in Section 3 and finally we summarize the results in Section 4.
2. The Model
The quantum molecular dynamics model [12–18, 20–22, 25–44] simulates the reaction on an event by event basis. Here each nucleon is represented by a Gaussian wave packet with a width of centered around the mean position and mean momentum . Here each nucleon is represented by a coherent state of the form The Wigner distribution of a system with nucleons is given by with .
The center of each Gaussian (in the coordinate and momentum space) is chosen by the Monte Carlo procedure. The momentum of nucleons (in each nucleus) is chosen between zero and local Fermi momentum [; is the potential energy of nucleon ]. Naturally, one has to take care that the nuclei, thus generated, have right binding energy and proper root mean square radii.
The centroid of each wave packet is propagated using the classical equations of motion: where the Hamiltonian is given by Our total interaction potential reads as with with fm and MeV.
The static (local) Skyrme interaction can further be parameterized as Here , , and are the parameters that define equation of state. The momentum-dependent interaction is obtained by parameterizing the momentum dependence of the real part of the optical potential. The final form of the potential reads as Here = 1.57 MeV and . A parameterized form of the local plus momentum-dependent interaction (MDI) potential (at zero temperature) is given by The parameters , , and in above equation must be readjusted in the presence of momentum-dependent interactions so as to reproduce the ground state properties of the nuclear matter. The set of parameters corresponding to different equations of state can be found in .
3. Results and Discussion
For the present analysis, we simulated the reactions of (), (), (), and () for = 40, (), (), (), and () for = 80, (), (), (), and () for = 160, and (), (), (), and () for = 240, at their corresponding theoretical balance energies (taken from ). The balance energies at which these reactions are simulated were calculated using a momentum-dependent soft equation of state with standard energy-dependent cugnon cross-section and reduced impact parameter ( = , where ; is the radius of projectile or target) of 0.25. The values of parameters used in (9) for momentum-dependent soft equation of state are compressibility , , , , , and . The reactions are followed uniformly up to 500 fm/c.
In Figure 1, we display the / (left column) and / (right column) as a function of the reaction time. The values of and are calculated within a sphere of radius 2 fm around the center of mass. The density is then computed at each time step during the reaction using The results are displayed by varying from 0.1 to 0.7 for different mass ranges; that is, = 40, 80, 160, and 240. It is clear from the figure that the maximal value of / decreases with increase in . A similar trend can be seen for the evolution of / at all mass ranges. This is due to the decrease in the interaction region with increase in mass asymmetry of the reaction. Further, one should note that for nearly symmetric reactions with = 0.1, the values of / and / are comparable for the heavy systems, indicating the wide and uniform formation of dense matter in the central region of 2 fm radius. This is similar to what predicted in . However, a nonhomogeneous nature of the dense matter is seen for lighter systems at all asymmetries. For each mass range, as increases and for each , as decreases, the incident energy increases. Therefore, for each , the reactions with larger asymmetries and for each , the systems with smaller , finishes much earlier. Similarly, the peak values of the densities are also delayed for reactions of heavy colliding nuclei and smaller asymmetries. Also, one should note that the time of saturation increases with increase in .
Similar to Figure 1, we display the net collision rate as a function of the reaction time in Figure 2. It is directly connected with the density. Due to the decrease in interaction volume with increase in mass asymmetry of colliding nuclei, the net collision rate decreases with increase in and the interactions among nucleons also cease earlier. This is observed for all system mass ranges. As expected, with increase in system mass, opposite trend is observed for each . This behavior is also evident from the density profile (see Figure 1).
It is well known that balance energy represents a counterbalancing between the attractive and repulsive forces; therefore, this fact should also be reflected in quantities like spectator and participant matter. In Figure 3, we display the normalized spectator (a, b) and participant (c, d) matter as a function of reaction time. The results are displayed for different asymmetries by keeping the total mass of the system fixed as = 80 and 240. All nucleons having experienced at least one collision are termed as participant and the remaining matter is termed as spectator matter. One can also define spectator and participant matter in terms of rapidity distribution; however, the results are similar for both definitions, as shown in . From the figure, one clearly sees that at the start of the reaction, all nucleons constitute spectator matter; therefore, no participant matter exists at initial time (i.e., fm/c). Due to decrease in the number of nn collisions with increase in , the spectator (participant) matter increases (decreases) with increase in . Similar behavior is seen for different system masses.
In Figure 4, we display the time evolution of relative momentum (a) and anisotropy ratio (b) for different and . The anisotropy ratio is defined as [38–44] This anisotropy ratio is an indicator of the global equilibrium of the system as it does not depend on the local density. The full global equilibrium averaged over large number of events will correspond to = 1. The second quantity, the relative momentum of two colliding spheres, is defined as [38–44] where Here and are the momentum and density experienced by the th particle and stands either for target or projectile. As noted, this quantity measures deviation from a single Fermi sphere and hence represents local equilibrium. Such a concept of local equilibrium is commonly used in the hydrodynamical model. Obviously, with the passage of the time, density in a central sphere will decrease due to lesser and lesser nucleons and, as a result, will also decrease. On the other hand, no such density dependence exists for . The anisotropy ratio will saturate after the finishing of the reaction. From the figure, we see that decreases as the reaction proceeds, while ratio increases and saturates after the high dense phase is over. Due to increase in incident energy with , thermalization is little bit better achieved for larger . Similar behavior is observed for each fixed system mass. However, for each , due to high density obtained in heavier systems, the thermalization is better achieved compared to lighter colliding nuclei.
Temperature is one of the associated quantities linked with a dense matter. In principle, one can define true temperature only for a thermalized and equilibrated matter. Since in heavy-ion collisions the matter is nonequilibrated, one cannot talk of temperature. One can only look in terms of the local environment. In our case, we follow the description of the temperature as given in [45–47]. The extraction of the temperature is based on the local density approximation; that is, one deduces the temperature in a volume element surrounding the position of each particle at a given time step [45–47]. In present case each local volume element of nuclear matter in coordinate space and time has some temperature defined by the diffused edge of the deformed Fermi distribution consisting of two colliding Fermi spheres, which is typical for a nonequilibrium momentum distribution in heavy-ion collisions. In this formalism which is dubbed the hot Thomas-Fermi approach [45–47], one determines extensive quantities such as the density and kinetic energy as well as entropy with the help of momentum distributions at a given temperature. Using this formalism, we also extracted the average and maximum temperature within a central sphere of 2 fm radius as described in the case of density.
In Figure 5, we display the mass dependence of the maximal values of , , , and as well as the final stage value of (allowed) nn collisions and spectator/participant matter. For the nearly symmetric reaction having = 0.1, the dependence is similar to that shown in . All the quantities follow a power law behavior . The values of power factor are displayed in the figure. It shows that the dependence of temperature reached in the central region is in sharp contradiction to the evolution of density reached in the central region because the dependence of maximal value of and is very weak on system mass for all while weak dependence on system mass is seen in case of temperature. This is due to the fact that the temperature depends also on the kinetic energy (i.e., excitation energy) of the system [45–47]. For a given colliding geometry, the maximal value of and also depends on the bombarding energy rather than on the size of the interacting source . Since, in our case, we have carried out the study at balance energy, which varies with the system mass, this in turn leads to dependence of temperature on the system mass due to the variation in the bombarding energy. At a fixed bombarding energy, dependence could be different. For nn collisions, one sees a linear enhancement with the system mass for each . Naturally, at a fixed energy, the nn collisions should scale as  and it is seen for each . The spectator and participant matter are nearly independent of the mass of the system for each .
In Figure 6, we display the mass asymmetry dependence of the maximal values of , , , and as well as the final stage value of (allowed) nn collisions and spectator/participant matter. The results are displayed for different mass ranges. Lines are the linear fits . We find a clear dependence of quantities on . The dependence of maximal value of and on decreases with increase in system mass while in case of and ; different trend is seen which is due to the same reason as explained in earlier paragraph, while for nn collisions an opposite trend is observed. The nn collisions also decrease with increase in , but due to larger interaction volume in heavier systems, heavier colliding nuclei show large dependence. Obviously, the spectator matter and the participant matter will behave oppositely. For each system mass, the spectator (participant) matter increases (decreases) with increase in and similar to density; the dependence decreases with increase in total mass of the system. From this figure, it is clear that mass asymmetry of the reaction has a significant role in the nuclear dynamics of the reaction. Therefore, while studying various phenomenon in the intermediate energy heavy-ion collisions, one should take care of the mass asymmetry of the reaction.
We studied the nuclear dynamics (particularly, average and maximum temperature and density, collision rate, participant-spectator matter, anisotropic ratio, relative momentum, and their mass asymmetry and mass dependence) at the balance energy of mass asymmetric reactions by keeping the total mass of the system fixed as 40, 80, 160, and 240 and varying the mass asymmetry of the reaction from 0.1 to 0.7. A sizeable effect of mass asymmetry on these quantities is observed. Therefore one cannot ignore the presence of mass asymmetry of reaction while studying the various phenomena of intermediate energy heavy-ion reactions.
Conflict of Interests
The author declares that there is no conflict of interests regarding the publication of this paper.
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