In the present paper, some results on the correlations of the nucleus-nucleus interactions, at high energy, between different particle multiplicities are reported. The correlations between the multiplicities of the different charged particles emitted in the interactions of 22 Ne and 28 Si nuclei with emulsion at (4.1-4.5)A GeV/c have been studied. The correlations of the compound multiplicity nc, defined as the sum of both numbers of the shower particles ns and grey particles ng, have been investigated. The experimental data have been compared with the corresponding theoretical ones, calculated according to the modified cascade evaporation model (MCEM). An agreement has already been fairly obtained between the experimental values and the calculated ones. The dependence of the average compound multiplicity, on the numbers of shower, grey, black and heavy particles is obvious and the values of the slope have been found to be independent of the projectile nucleus. On the other hand, the variation of the average shower, grey, black and heavy particles is found to increase linearly with the compound particles. A strong correlation has been observed between the number of produced shower particles and the number of compound particles. Moreover, the value of the average compound multiplicity is found to increase with the increase of the projectile mass. Finally, an attempt has also been made to study the scaling of the compound multiplicity distribution showing that the compound multiplicity distribution is nearly consistent with the KNO scaling behavior.
PACSNumber(s): 25.75.−q, 25.75.Gz, 25.70.Pq, 25.70.Gh 1550048-1 Int. J. Mod. Phys. E 2015.24. Downloaded from www.worldscientific.com by MONASH UNIVERSITY on 08/25/15. For personal use only. 1550048-2 Int. J. Mod. Phys. E 2015.24. Downloaded from www.worldscientific.com by MONASH UNIVERSITY on 08/25/15. For personal use only. 1550048-4 Int. J. Mod. Phys. E 2015.24. Downloaded from www.worldscientific.com by MONASH UNIVERSITY on 08/25/15. For personal use only. 1550048-5 Int. J. Mod. Phys. E 2015.24. Downloaded from www.worldscientific.com by MONASH UNIVERSITY on 08/25/15. For personal use only.