Research Article | Open Access

Gao-Feng Wei, Guo-Qiang He, Xin-Wei Cao, Yi-Xin Lu, "Impact Parameter Dependence of Ratio in Probing the Nuclear Symmetry Energy Using Heavy-Ion Collisions", *Advances in High Energy Physics*, vol. 2016, Article ID 9317873, 8 pages, 2016. https://doi.org/10.1155/2016/9317873

# Impact Parameter Dependence of Ratio in Probing the Nuclear Symmetry Energy Using Heavy-Ion Collisions

**Academic Editor:**Frank Filthaut

#### Abstract

The impact parameter dependence of ratio is examined in heavy-ion collisions at 400 MeV/nucleon within a transport model. It is shown that the sensitivity of ratio on symmetry energy shows a transition from central to peripheral collisions; that is, the stiffer symmetry energy leads to a larger ratio in peripheral collisions while the softer symmetry energy always leads this ratio to be larger in central collisions. After checking the kinematic energy distribution of ratio, we found this transition of sensitivity of ratio to symmetry energy is mainly from less energetic pions; that is, the softer symmetry energy gets the less energetic pions to form a smaller ratio in peripheral collisions while these pions generate a larger ratio in central collisions. Undoubtedly, the softer symmetry energy can also lead more energetic pions to form a larger ratio in peripheral collisions. Nevertheless, considering that most of pions are insufficiently energetic at this beam energy, we therefore suggest the ratio as a probe of the high-density symmetry energy effective only in central at most to midcentral collisions, thereby avoiding the possible information of low-density symmetry energy carried in ratio from peripheral collisions.

The determination of density-dependent nuclear symmetry energy is one of the hot topics in isospin physics due to its importance in understanding the structure of radiative nuclei in nuclear physics [1–5] and the evolution of massive stars and properties of neutron stars in nuclear astrophysics [6–10]. Presently, although many useful experimental observables [11–20] have been proposed to determine the nuclear symmetry energy, the knowledge regarding the nuclear symmetry energy is still far lacking except for the relative determination of nuclear symmetry energy at saturation density from empirical liquid-drop mass formula [14, 21]. For example, by comparing the ratio with the FOPI experimental data [22], the Boltzmann-Uehling-Uhlenbeck (BUU) [23] and Boltzmann-Langevin (BL) [24] communities favor a supersoft symmetry energy, but the quantum molecular dynamics (QMD) [25] community suggests a superstiff symmetry energy. Therefore, much more efforts need to be made to better determine the nuclear symmetry energy at both supersaturation and subsaturation densities.

Heavy-ion collisions induced by neutron-rich nuclei as an important tool are commonly used to study the density dependence of nuclear symmetry energy [26–31]. Usually, a higher compressive density formed in central heavy-ion collisions with the softer symmetry energy gets the ratio to be larger compared to the case of stiffer symmetry energy. However, the densities formed in heavy-ion collisions always experience a broad range from subsaturation to supersaturation densities. Therefore, one has to evaluate the influence of the high-density (low-density) matter phase on observable when probing the symmetry energy at subsaturation (supersaturation) density using heavy-ion collisions due to the formation of supersaturation (subsaturation) density matter. Certainly, the influence of low-density matter phase is inevitable using heavy-ion collisions to probe high-density symmetry energy due to the densities formed at the final reaction stage always lower than the saturation density; therefore, one has to select those of reaction production without experiencing the final reaction stage such as preequilibration neutron-proton ratio. On the other hand, as shown recently, the pion potential has opposite effects on ratio compared to the effect of symmetry energy on it and thus decreases the sensitivity of ratio to symmetry energy [32, 33]. Moreover, the modification of pion production threshold can even invert the sensitivity of ratio to symmetry energy [34]. Actually, impact parameter as a factor can also influence the compressive density of participating region and thus may even invert the sensitivity of ratio to symmetry energy in peripheral collisions as mentioned in our recent work about the influence of neutron-skin thickness on the ratio in heavy-ion collisions [35]. Therefore, it is necessary to systematically check the impact parameter dependence of ratio in probing the symmetry energy using heavy-ion collisions and show the corresponding reasons and which energy range of pion does get the sensitivity of ratio to symmetry energy reversal. This is the main purpose of the present study.

The present study is based on an isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model [36]. In this model, an isospin-dependent mean-field is used to model the nuclear interaction; its expression is defined as follows:In the above, is the nucleon number density and is the isospin asymmetry of the nuclear medium; denotes the neutron (proton) density, the isospin is for neutrons and for protons, and is the local phase space distribution function. The expressions and values of the parameters , , , , , , and can be found in [37, 38], and they lead to the binding energy of −16 MeV, incompressibility 212 MeV for symmetric nuclear matter, and symmetry energy MeV at saturation density , respectively, while parameter is used to mimic the different forms of symmetry energy predicted by various many-body theories without changing any properties of symmetric nuclear matter and the value of symmetry energy at saturation density . Shown in Figure 1 is the density dependence of symmetry energy with a softer setting and stiffer one .

Now let us check the impact parameter dependence of ratio in probing the symmetry energy. Within the IBUU transport model for heavy-ion collision at the intermediate energy, almost all the pions are produced from the decay of resonances. Therefore, the dynamic pion ratio, that is, , can be defined asDue to the fact that all the resonances will eventually decay at the final reaction stage, it is thus the ratio that will naturally become the ratio. Shown in Figures 2 and 3 are the time evolution of ratio and rapidity distribution of ratio from central to peripheral Pb + Pb collisions at the beam energy of 400 MeV/nucleon. Similar to previous results [23, 25], the dynamic ratio and final ratio are more sensitive to the symmetry energy at the central heavy-ion collision compared to the case of peripheral heavy-ion collision and larger with a softer symmetry energy setting compared to the case of the stiffer setting . However, it can be seen that no matter the dynamic ratio or the rapidity distribution of final ratio on the symmetry energy shows a transition from central to peripheral collisions; that is, the stiffer symmetry energy leads to a larger ratio in peripheral collisions while the softer symmetry energy obviously gets this ratio to be larger in central collisions. On the other hand, it is well known that the increasing of impact parameter will directly change the participant numbers and thus the pion multiplicities and kinematic energy distribution. Therefore, a natural question is which energy range of pion does invert the sensitivity of ratio to symmetry energy from central to peripheral collisions. To this end, we show in Figure 4 the kinematic energy distribution of ratio with different impact parameter. In general, it is similar to above observation that the sensitivity of ratio to symmetry energy is decreasing at lower kinematic energy as increasing the impact parameter especially from midcentral to peripheral collisions and even shows an opposite sensitivity in very peripheral collisions. However, for the pion ratio at larger kinematic energy, its value with the softer symmetry energy is also larger even in very peripheral collisions albeit with a larger error bar. This naturally gets us to look at the impact parameter dependence of ratio formed by less energetic pions and more energetic pions, separately. For this purpose, we take empirically a kinematic energy cut of 250 MeV and classify pions into less energetic and more energetic groups. Shown in Figures 5(a) and 5(b) is the impact parameter dependence of ratio formed by less energetic pions and more energetic pions, respectively. It is seen that the transition of sensitivity of ratio to symmetry energy is mainly from less energetic pions; that is, the softer symmetry energy gets the less energetic pions to form a smaller ratio in peripheral collisions while these pions generate a larger ratio in central collisions. Certainly, the softer symmetry energy also leads more energetic pions to form a larger ratio in peripheral collisions. Nevertheless, due to the fact that most of pions are less energetic at this beam energy as shown in Figure 5(d), thus the behaviour of ratio formed by all pions without any kinematic energy cut is almost similar to those formed by less energetic pions as shown in Figure 5(c).

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Now let us show the reason for pion ratio transition in probing the symmetry energy from central to peripheral collisions. To this end, we show the average density of participating region over the whole reaction time in Figure 6(a) from central to peripheral collisions. It can be found that almost all the pions are produced at supersaturation density at central heavy-ion collisions but subsaturation density at peripheral collisions. On the other hand, from the symmetry potential in Figure 6(b) and symmetry energy in Figure 1, it can be found that the stiffer symmetry energy with parameter generates a larger symmetry energy and a larger symmetry potential when the density of participating region is higher than the normal density, thereby generating stronger repulsive effects for neutrons but attractive effects for protons and thus leading to a smaller ratio in central collisions. On the contrary, when the density of participating region is lower than the normal density, the stiffer symmetry energy with parameter corresponds to a smaller symmetry energy and a smaller symmetry potential compared to the case of the softer symmetry energy with parameter , then naturally generating a larger ratio in peripheral collisions. This implies the ratio as a probe of high-density symmetry energy effective only in central at most to midcentral collisions, thereby avoiding the possible information of low-density symmetry energy carried in ratio from peripheral collisions.

**(a)**

**(b)**

In summary, we have carried out an investigation about the impact parameter dependence of ratio in probing the nuclear symmetry energy using heavy-ion collision. Within an isospin-dependent transport model, the Pb + Pb collisions are performed with different impact parameter at a beam energy of 400 MeV/nucleon. It is shown that the sensitivity of ratio on symmetry energy has a transition from central to peripheral collisions due to the fact that the less energetic pions measure the high-density symmetry energy in central collisions but the low-density symmetry energy in peripheral collisions. Therefore, we suggest the signature as a high-density symmetry probe effective only in central at most to midcentral collisions. Certainly, other effects such as pion production threshold and energy conservation and pion potential, which are not considered in the present study, can also influence significantly the sensitivity of ratio to symmetry energy as shown in others [32–34].

#### Conflict of Interests

The authors declare that there is no conflict of interests regarding the publication of this paper.

#### Acknowledgments

This work is supported by the National Natural Science Foundation of China under Grant no. 11405128 and Xi’an Science and Technology Planning Project no. CXY1352WL29.

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#### Copyright

Copyright © 2016 Gao-Feng Wei et al. 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. The publication of this article was funded by SCOAP^{3}.