Slow Particle Production in Nucleus-Nucleus Collisions at Relativistic Energies

In this paper an effort has been made to study the general characteristics of slow particles produced in the interactions of 32S-Em at 200 AGeV to extract the information about the mechanism of particle production. The results have been compared with the experimental results obtained by other workers. The multiplicity distributions of the slow target associated particles (black, grey and heavy tracks) produced by 32S-beam with different targets have been studied. Also several types of correlations among them have been investigated. The variation of the produced particles with projectile mass number and target size has been studied. Also the multiplicity distributions of slow particles with NBD fits are presented and scaling multiplicity distributions of slow particles produced have been studied in order to check the validity of KNO-scaling.


Introduction
The study of relativistic nucleus-nucleus (A-A) collisions has attained peculiar importance during the last few decades.In nucleus-nucleus collisions it is important to achieve complete information regarding the mechanism of particle production.When an energetic projectile collides with targets of nuclear emulsion, a number of charged and uncharged particles are produced.The emergence of these particles occurs in a very short time and after this the nucleus remains excited for quite a long time on nuclear scale.The nucleus then de-excites resulting in the emission of a large number of nucleons and other heavy fragments.Usually, the particles emitted through this process of evaporation appear as black tracks as well as low energy grey tracks in nuclear emulsion.So far, very little work has been carried out in the target fragmentation region.For the study of this region it is essential to have experimental data on low and medium energy particles produced due to the processes of rescattering and cascading.In this direction, the EMU01 and other experiments have made considerable effort to understand the role of slow target related particles in nucleus-nucleus collisions [1] [2].
The multiplicity of charged particles in high energy nucleus-nucleus interactions is an important parameter which indicates how many particles are produced in that interaction.The multiplicity distributions of produced particles or emitted particles help in learning the interaction mechanism.Generally, it is accepted that in high energy nucleus-nucleus collisions, the emission of slow target-associated particles (i.e.black tracks) and other heavier fragments takes place at a still latter stage with range L ≤ 3 mm, relative velocity β < 0.3 and energies less than 30 MeV.The emission of fast target associated particles mostly the knocked out protons known as grey particles, takes place at a relatively latter stage of the collision.These fast protons with range L ≥ 3 mm and relative velocity 0.3 ≤ β ≤ 0.7 lie in the energy range 30 to 400 MeV.Moreover, these target-associated particles are mostly slow and fast protons and grey particles are often assumed to be the measure of the number of encounters made by the incident hadron inside the target nucleus [3] and believed to be produced as a result of process of rescattering in the target spectator region.The black and grey tracks taken together are known as heavily ionizing tracks denoted by N h .
Our objective in this paper is to employ the interactions of 32 S in nuclear emulsion.The emulsion has the unique property of acting simultaneously as the target as well as the detector, for registering all the charged particles in 4π geometry with the highest spatial resolution as compared to the electronic detectors.We have reported some results based on the general characteristics of slow particles produced in the interactions of 32 S-Em 200 AGeV/c to extract the information about the mechanism of particle production.The multiplicity distributions of the slow target associated particles (black, grey and heavy tracks) produced by 32 S-beam with different targets have been studied.Also several types of correlations among them have been investigated.The variation of the produced particles with projectile mass number and target size has been studied.Some results have also been obtained on the angular distribution of black and grey tracks and values of F/B ratio for these distributions have also been presented.Also the multiplicity distributions of slow particles with NBD fits are presented and scaling multiplicity distributions of slow particles produced have been studied in order to check the validity of KNO-scaling.

Experimental Techniques
In the present experiment we have used two stacks of Ilford G5 nuclear emulsion plates exposed horizontally to a 32 S-beam at 200 AGeV from Supper Proton Synchrotron, SPS at CERN for data collection.The scanning of the plates is performed with the help of Leica DM2500M microscope with a 10X objective and 10× ocular lens provided with semi-automatic scanning stages.The method of line scanning was used to collect the inelastic 32 S-Em interactions.The interactions collected from line scanning were scrutinized under an optical microscope (Semi-Automatic Computerized, Leica DM6000M) with a total magnification of 10 * 100 using 10× eyepiece and 100× oil immersion objective.The measuring system associated with it has 1 μm resolution along X and Y axes and 0.5 μm resolution along the Z-axis.The detailed discussion about the present experiment can be found in our earlier publications [4]- [7].

Multiplicity Distributions
The analysis of the experimental data in terms of multiplicity distributions for different emitted secondaries (slow and fast protons) is one of the main sources of information about the mechanism of particle production.Figures 1(a)-(c) shows the multiplicity distributions of black, grey and heavily ionizing particles from 32 S-Emulsion interactions at 200 AGeV along with the distribution obtained from 28 Si-Em [8] and 16 O-Em [9] interactions at 14.6 AGeV and 200 AGeV respectively for comparison.It is observed from the figures that the peaks of the distributions appear in the lower values of N b , N g , and N h .These distributions seem to be independent of incident energy as well as projectile mass within statistical errors up to lower values of N b , N g , N h .This result is consistent with those obtained by other workers [8]- [13].It may also be noticed from the figures that the per- centage of events with large values of N b , N g , or N h increases with projectile mass.Finally, it may be concluded from the multiplicity distributions of slow and fast protons produced in nucleus-nucleus interactions that no significant differences are observed regarding the mechanism of their production with energy.AGeV [8] respectively are incorporated in the same figure for comparison.From the figures, it may be observed that the characteristics feature of the distribution is similar in shape for all targets, but the multiplicity range or decay tail increases with target size.It has also been found that the distributions for 32 S-AgBr are broader than those for 32 S-CNO interactions.This may reflect the effect of the target mass number on the number of collisions of 32 S beam with target nuclei.Experimental results obtained by other workers [8] [10] reproduce qualitatively similar results.

Scaling of Grey Particles
The possibility of scaling, i.e., similarity in the multiplicity distributions of grey tracks produced in hadron-nucleus and nucleus-nucleus interactions has also been examined.In the present analysis, the events with N g = 0 have been excluded because the coherent processes may also contribute to such events.Figure 4(a) shows the g g N N -distribution from 32 S-Em interactions at 200 AGeV.A straight line of the form: ( ) ( ) is found to represent the present data, N ev denotes the number of events in the given bin and A and B are constants.The best fit to the data is given as: For comparison the g g N N -distributions from 28 Si-Em at 14.6 AGeV and 4.5 AGeV and 12 C-Em at 4.5 AGeV [14] are also plotted in Figures 4(b)-(d).The values of the slopes for 28 Si-Em at 14.6 AGeV and 28 Si-Em and 12 C-Em interactions at 4.5 AGeV are found to be −0.88 ± 0.04, −0.89 ± 0.08 and −0.86 ± 0.06 respectively.The slope parameters are ~0.90, which are very much consistent with the value obtained for 32 S-Em at 200 AGeV.The constancy in the values of slopes for nucleus-nucleus collisions at different energies may be interpreted as existence of some kind of scaling for the production of grey tracks.

Mean Multiplicity of Secondary Particles
The mean multiplicity is the average number of charged particles produced in various types of high-energy heavy ion collisions.Multiplicity of different charged particles is helpful in understanding the mechanism of multiparticle production.The average values of number of black, grey and heavily ionizing particles produced in 32 S-Em interactions at 200 AGeV are displayed in  32 S-Em interactions at 200 AGeV by S. Dhamija et al. [2] and A. Dabrowska et al. [15] along with other results at different energies [8]- [10] [12] [13] [16]- [18] are also listed in Table 1 for the sake of comparison.It is for different interactions at different energies.(a) 32 S-Em at 200AGeV; (b) 32 Si-Em at 14.6 AGeV; (c) 32 Si-Em at 4.5 AGeV; (d) 32 C-Em at 200AGeV.because slow particles are produced due to evaporation of excited residual nucleus.We also study the dependence of the average multiplicities on projectile mass, A p , using the following power law: where i = b, g, h, and i N represents the mean multiplicity.The values of the slope (β) for black, grey, and heavy tracks obtained from the least -squares fits are given as (−0.0054 ± 0.009), (0.1407 ± 0.008) and (0.1125 ± 0.016) respectively.The dependence of indicates that the average excitation of the residual target nucleus has reached its saturation at present projectile energy.The strong dependence of the total charged secondary particles on the masses of colliding nucleus are due to the increase in the overlapping region of the two interacting nuclei.
Table 2 presents the mean multiplicities of black, grey and heavily ionizing particles for 32

Multiplicity Correlations
Multiplicity correlations among the heavily ionizing particles produced in nucleus-nucleus collisions have been widely studied which help to investigate the mechanism of particle production.In order to examine the behaviour of multiplicity correlations of secondary particles produced in nucleus-nucleus collisions, we have studied the correlations in the interactions of 32 S-Em at 200 AGeV.Generally, the experimental results have been analyzed by using linear fits of the type: where N i , N j = N g , N b and N h with i ≠ j.The values of inclination coefficients, a ij and intercepts, b ij are given in Table 4.The behaviour of multiplicity correlations of secondary particles produced in 32  A similar result was obtained by Otterlund [18] for proton-nucleus interactions over a wide range of energy.This means correlation does not depend upon mass of the projectiles and the contribution of the recoiling nucleons towards the excitation energy of the residual nucleus is approximately the same for P-nucleus and nucleus-nucleus interactions.
ii) Variation of  In order to see the dependence of the average multiplicities on the mass numbers of the target nuclei, the following relation has been used as: where "j" stands for black, grey and heavy particles respectively.The variation of average multiplicities on masses of the target nuclei is shown in Figure 7.The coefficients K and α, are determined from the least-square fit using the experimental data of the present study.The values of these coefficients are given in Table 5.The results depict that the multiplicities of black particles are nearly proportional to linear dimensions of target nuclei.The multiplicities of grey particles are characterized by extremely weak target size dependence.shows the normalized angular distributions for black and grey particles emitted in 32 S-Em collisions at 200 AGeV along with the results obtained by other workers [18] [21] for different projectiles and energies.It has been observed from the figure that the distributions are independent of projectile mass as well as the energy of the projectile.The production mechanism of the black particles, based on nuclear evaporation processes, are isotropically distributed in the rest frame of target nucleus and the distribution is influenced by a strong electromagnetic field of relativistic projectiles, which is almost symmetric about θ ≈ 90˚ in the laboratory system.Whereas the production mechanism of grey particles is based on inter-nuclear cascade processes and these particles are mainly emitted in forward direction.The forward and backward hemispheres are defined as the regions where emission angles are less than 90˚ (θ < 90˚) and greater than 90˚ (θ > 90˚) respectively.The forward (F) to backward (B) ratio for these distributions are calculated and presented in Table 6.

Angular Distribution of Slow Particles
It is clearly seen from the table that the F/B ratio shows the same behavior and its value for grey particles is more than black particles.Also the F/B ratio shows a weak dependence on the mass of projectile.The differences in the angular distributions of black and grey particles point to the fact that these particles originate in two different processes, the subsequent evaporation and the initial interaction of target nucleus.

KNO Scaling
Recently [24]- [26] the investigation of nuclear fragments produced in high energy nucleus-nucleus collisions shows that the multiplicity distributions of target fragments; black and grey particles can be described by Koba-Nielsen-Olesen scaling [27].Koba, Nielsen and Olesen have predicted that the multiplicity distributions of the produced particles in high-energy hadron-hadron collisions should obey a simple scaling law known as KNO scaling when expressed in terms of the scaling variable Z ( ) . If P n (s) represents the probability for the production of n charged particles in an inelastic hadron-hadron collision at a centre of mass energy √s, then the multiplicity distributions in high energy collision obey a scaling law: where σ n (s) is the partial cross-section for the production of n charged particles, σ inel is the total inelastic cross-section and N is the average number of charged particles produced.The KNO scaling thus implies that the multiplicity distribution is universal and ψ(z) is an energy independent function at sufficiently high energies when expressed in terms of scaling variable Z.It has been found by various workers the empirical expression for ψ(z) in hadron-hadron and hadronnucleus interactions obeys the semi-inclusive KNO scaling starting from few GeV.It is desirable to make similar studies in nucleus-nucleus collisions as it is expected that nucleus-nucleus collisions (A-A) at these energies can be visualized as superposition of nucleon-nucleon collisions.Several workers [24] [28]- [30] have reported that the validity of KNO scaling holds for the projectile helium particle and black tracks in heavy-ion interactions at Dubna, Bevatron, CERN and AGS energies.It has been shown [26] [31] that the multiplicity distributions of produced black and grey fragments obtained from the events of different projectiles over a wide range of energies in nucleus-nucleus collisions can be described by a KNO scaling law.These distributions can be represented by a universal function of the following form: where A and B are constants.
In the present work an attempt has been made to study the KNO scaling for the multiplicity distribution of slow and fast target associated particles produced in 32 S-emulsion collisions at 200 AGeV.A plot of ψ(z) as a function of the scaling variable Z ( ) for these medium energy target associated protons is shown in Figure 9(a) and Figure 9(b).The experimental points for 12 C and 28 Si at 4.5 AGeV [8], 28 Si at 14.6A GeV [8] and 16 O at 3.7 AGeV and 60 AGeV [9] respectively are also shown in the same figure.The solid curve in the figure is well represented by Equation ( 6).It is easily noticed from the figures that the multiplicity distributions of slow and fast target associated protons in nucleus-nucleus collisions at different energies are well described by Equation ( 6) for the different projectiles and seem to satisfy the scaling function.The best values of A and B used in Equation ( 6) are found to be 6.21 ± 0.85, 2.65 ± 0.10 and 5.26 ± 0.90, 2.89 ± 0.13 respectively for slow and fast target associated protons.The values of corresponding χ 2 /DOF are found to be 0.63 and 0.79 ± 0.04 respectively for slow and fast target associated protons which indicates that the fitting is good for different projectiles at different energies in case of slow protons but a small deviation from exact scaling can be seen for fast target associated protons in Figure 9(b).It is difficult to give any physical explanation of the multiplicity scaling for slow and fast protons and hence can be regarded as an empirical observation.

Negative Binomial Distribution of Black, Grey and Heavy Particles
The studies of multiplicity distribution in high energy heavy ion collisions have revealed some striking phenomenon which can be described by various models [27] [32]- [34].Among them, the most spectacular and well known is the negative binomial distribution (NBD) model [34].The NB law has been successful in describing the multiplicity results in recent high energy experiments.In Figures 10(a)-(c) the multiplicity distributions of black, grey and heavy particles in the interactions of 32 S-Em at 200 AGeV are shown with the corresponding best NB fits.The values of the free parameters of negative binomial distributions "k" and "n" and the χ 2 /DOF obtained using the CERN MINUIT curve fitting program are given in Table 7. From the table it can be concluded that the multiplicity distributions of secondary particles produced in 32 S-Em at 200 AGeV interactions can be fitted quite satisfactorily by the NBD having the form where n and n represent respectively the multiplicity and mean multiplicity, the value of k is determined from: ( )

Conclusions
The following conclusions may be drawn from the present study.i) It is observed that the peaks N b , N g , and N h of distributions appear in the lower values of N b , N g , and N h and all the distributions are essentially independent of incident energy and projectile masses.It is also clear that the target associated particles have a weak dependence on the projectile mass number A p .Further, the multiplicity distributions of slow and fast protons produced in nucleus-nucleus interactions give a clear indication that no significant differences are observed regarding the mechanism of their production with energy.
ii) It is found that mean multiplicity of slow particles increases with increase of centrality of collisions.A regular pattern in the values of the ratio iv) It may be noticed that as the impact parameter decreases (the degree of disintegration of the target nuclei increases), the ratio of the number of slow evaporated particles (N b ) to heavily ionizing particles (N h ) i.e. the v) The multiplicity correlations of secondary particles produced in nucleus-nucleus collisions are similar to hadron-nucleus collisions and could be represented by a linear dependence.
vi) It has been found that multiplicities of black particles are nearly proportional to linear dimensions of target nuclei whereas the multiplicities of grey particles are characterized by extremely weak target size dependence.
vii) The angular distributions of the black particles, based on nuclear evaporation processes, are isotropically distributed in the rest frame of target nucleus and the distribution is influenced by a strong electromagnetic field of relativistic projectiles, which is almost symmetric about θ ≈ 90˚ in the laboratory system.The angular distribution of grey particles and their production are based on inter-nuclear cascade processes.These fast protons are mainly emitted in forward direction.
viii) The multiplicity distributions of slow and fast target associated protons produced in 32 S-Em collisions at 200 AGeV along with other experimental data at various energy ranges exhibit a KNO scaling within experimental errors and a small scaling violations are found.ix) Also the multiplicity distributions of secondary particles produced in 32 S-Em at 200 AGeV interactions can be fitted quite satisfactorily by the NBD.

Figure 1 .
Figure 1.Multiplicity distributions of secondary charged particles produced in interactions of projectiles with emulsion for (a) black particles (b) grey particles and (c) heavily ionizing particles.

Figures 2 (
a)-(c) and Figures 3(a)-(c) show the N b , N g , and N h multiplicity distributions from 32 S-AgBr and 32 S-CNO interactions at 200 AGeV.The results obtained by other workers for 12 C and 28 Si at 4.5 and 14.6

Figure 2 .Figure 3 .
Figure 2. Multiplicity distributions of secondary charged particles produced in interactions of different projectiles with AgBr for (a) black particles (b) grey particles and (c) heavily ionizing particles.

Figure 4 .
Figure 4. Plot of ln(N ev ) vs g g N N mass number, A p , is shown in Figures 5(a)-(c).It has been reported that the values of β g for g N is slightly higher than the corresponding values in case of hadron-nucleus interactions [18] [19].The observation may indicate that the 32 S projectile at a given impact parameter are an extended object rather than a point object as in the case of a hadron beam.The variation of b N with A p is shown in Figure 5(a), which is almost independent of the projectile mass number and its energy.This constancy of b N Figure 5. Variation of S-Em interactions at 200 AGeV is shown in Figures6(a)-(c) along with their linear fits using least square method.From these plots following conclusions may be drawn.i) A clear saturation in the values of b N is observed in b N vs N g plot for values of N g beyond ~10.
g N with N b is similar to that of b N with N g .However, the saturations are not statistically significant.Also g N displays a linear dependence on N h in the whole range of N h .iii) The values of h N increases with the increase of N b and N g in the whole range of N b and N g in nucleusnucleus collisions.

Figure 6 .
Figure 6.Multiplicity correlations of various charged particles produced in the interactions of 32 S-Em at 200 AGeV.

Figure 7
Figure 7. Variation of

Figure 8 (
Figure 8(a) and Figure 8(b)shows the normalized angular distributions for black and grey particles emitted in32 S-Em collisions at 200 AGeV along with the results obtained by other workers[18] [21] for different projectiles and energies.It has been observed from the figure that the distributions are independent of projectile mass as well as the energy of the projectile.The production mechanism of the black particles, based on nuclear evaporation processes, are isotropically distributed in the rest frame of target nucleus and the distribution is influ-

Figure 8 .
Figure 8.The normalized angular distributions of (a) black and (b) grey particles in 32 S-Em interactions at 200 AGeV along with other results.

Figure 9 .
Figure 9. Multiplicity distribution of (a) slow target associated protons and (b) fast target associated protons in terms of KNO scaling in the interactions of 28 Si-Em at 4.5 and 14.6 AGeV, 12 C-Em at 4.5 AGeV and 16 O-Em at 3.7 and 60 AGeV with the present work of 32 S-Em at 200 AGeV.

Figure 10 .
Figure 10.The Multiplicity distributions of (a) black particles (b) grey particles and (c) heavily ionizing particles with NB fits in 32 S-Em interactions at 200 AGeV.
except for CNO (2 ≤ N h ≤ 7) events.iii)It can be observed that the value of g N depends weakly with increasing mass of the projectiles as well as energy of the projectiles.The values of b N do not exhibit any such trends.

Table 1 .
The values of b N , g N and h N measured in

Table 1 .
Mean obtained in 32 S-Em interactions at 200 AGeV are slightly larger than the values obtained by S. Dhamija et al. and A. Dabrowska et al.This discrepancy may be due to the different criteria of ionization chosen for black tracks by S. Dhamija and A. Dabrowska.The values of It can be observed from the results shown in the table that the value of multiplicities of various particles produced in heavy ion collisions at high energies.Energy/nucleon (A GeV) Collision Type b N g N h N Ref. b N b N

Table 2 .
Average values of in32S-Em interactions along with different N h intervals at 200 AGeV.
g N , b N , h N

Table 3 .
[20] the table it may be clearly noticed that as the impact parameter decreases (the degree of disintegration of the target nuclei increases), the ratio of the number of slow evaporated particles (N b ) to heavily ionizing particles (N h ) i.e. the This result contradicts the results obtained by Antonchilk et al.[20]for 7 ≤ N h ≤ 27 and N h ≥ 28 respectively.

Table 3 .
Values of D(N g ) and

Table 4 .
Values of inclination coefficients a ij and intercepts b ij in multiplicity correlation in32S-Em interactions at 200 AGeV.

Table 5 .
Values of coefficients K and α.

Table 6 .
The values of F/B ratio for the angular distribution of produced particles in nuclear collisions.

Table 7 .
Values of free parameters of NBD.