Tsallis p ⊥ distribution from statistical clusters

It is shown that the transverse momentum distributions of particles emerging from the decay of statistical clusters, distributed according to a power law in their transverse energy, closely resemble those following from the Tsallis non-extensive statistical model. The experimental data are well reproduced with the cluster temperature T ≈ 160 MeV.

be interpreted as another confirmation of the standard statistical model rather than that of its non-extensive Tsallis version. 2 Indeed, the intriguing "unreasonable" success of the statistical model in description of multi-particle production in various processes and at various energies suggests that the final stage of the process of hadronization is dominated by the hadrons in the state of statistical equilibrium. It is also clear that the equilibrium cannot be global, as the observed spectra are far from isotropic. These observations lead naturally to the idea [19] that the transition from the early state of the process, dominated by interactions between the hadronic constituents, most likely proceeds through an intermediate stage of clusters emitting the final hadrons according to the rules of statistical physics.
If one admits that this process of cluster formation and thermal decay is a universal feature of hadronization, one is led to the conclusion that also the high transverse momentum jets hadronize in the same way (cf. [20]). It follows that the characteristic features of clustering should leave their imprints even in the region of hard physics. In the present paper we show that this picture, when combined with the power law distribution of the (transverse) Lorentz factor of the cluster, leads to transverse momentum distribution of the decay products which is very close to that of Tsallis (and thus also close to experiment).
In the next section the idea of the statistical cluster is formulated and the transverse momentum distribution of its decay products is derived. The relation to the Tsallis distribution is dis- cussed in Section 3. Summary and comments are given in the last section.

2.
Following the ideas explained above, the decay distribution of the statistical cluster at rest is taken in the form of the Boltzmann distribution which, for a cluster moving with the fourvelocity u μ becomes Consider a cluster at rapidity Y moving in the transverse direction with the velocity v ⊥ . We have (2) The distribution of particle momentum is then where φ is the angle between v and p ⊥ and where we have de- Integration over φ and y gives the distribution of the transverse momentum: To evaluate the distribution of transverse momenta of the cluster decay products, one needs the distribution of the cluster transverse velocity v ⊥ . In this paper we study a power law in the transverse Lorentz factor γ ⊥ (for a fixed cluster mass, this would correspond to a power law in its transverse energy). Thus we take Given simplicity of this assumption, it was rather surprising to find that it leads to the distribution which closely resembles that of  (5) and (6) where c is the normalization constant, q − 1 measures the deviation from the standard statistical model and T ts is the Tsallis temperature. 4 One sees that, except at very small p ⊥ , below ∼100 MeV, there is an excellent agreement between the two formulations and for all kinds of particles. One also sees that for p ⊥ ≥ 1 GeV it is difficult to distinguish between the two versions of the Tsallis distributions. For the distribution D 1 the Tsallis parameter T ts can be approximated by the simple relation T ts ≈ (q − 1)T . This is not true, however, for D 2 . In this case the relation between T ts and T is more complicated and, moreover, it depends substantially on the particle mass.
Recently, a new analysis of transverse momentum distribution of charged particles in terms of the Tsallis distribution has been published [6]. To compare these results with our approach, we have evaluated the distribution following from the decay of a cluster for pions, kaons and protons and constructed the distribution of charged particles, using the weights (1:1:2), as proposed in [6].
In Fig. 3 the results in the region from p ⊥ = 0 till p ⊥ = 5 GeV are compared with the Tsallis distribution from [6]. One sees that the agreement is very good, except at p ⊥ < 100 MeV. The parameters of the Tsallis distribution in this case are q − 1 = 0.150 and T ts = 76 MeV, in good agreement with [6]. The region p ⊥ ≥ 5 GeV is not shown because in this region one simply cannot distinguish between the two curves. Fig. 3. Transverse momentum distribution of charged particles from the statistical cluster decay (crosses), compared to the Tsallis distribution (dashed line) used in [6] (the first formula in (7)). 0 ≤ p ⊥ ≤ 5 GeV. T = 155 MeV, κ=6.5. Best fit from p ⊥ = 0 to p ⊥ = 50 GeV.

4.
In summary, we have discussed the transverse momentum distributions of particles emitted in the decay of a statistical cluster. It was shown that if the (transverse) Lorentz factor of the cluster follows a power law, the resulting distribution is very close to that derived from the Tsallis non-extensive statistics.
This result may be considered as a possible explanation of the surprising observation that the Tsallis formula works not only at small transverse momenta (where the ideas of statistical equilibrium may be applicable) but even at transverse momenta as large as ∼200 GeV.
Some comments are in order.
(i) It should be emphasized that the observed similarity between the Tsallis formula and that following from the statistical cluster decay, is only an approximation. Our results indicate, however, that it may be rather difficult to distinguish experimentally between these two approaches. Perhaps the measurements at larger transverse momenta may be helpful, as the two distributions start to deviate from each other at energies above 200 GeV. (ii) We have been discussing emission of a single statistical cluster. As it is rather unlikely that a high-energy jet may fragment into a single cluster, production of many clusters must also be considered. Since our discussion concerns only the single-particle distribution, however, the results are insensitive to the number of clusters produced in a given event, provided they are emitted independently. (iii) Clearly, the power law assumed in (6) is only a phenomenological guess and should be treated as such. Its main advantage is the extreme simplicity (for more elaborate calculations see, e.g., [14][15][16]). Needless to say, the parameter κ remains free at the present stage, and cannot be reliably evaluated from theory. (iv) It has been shown recently [27] that the distributions of transverse momenta at various energies follow a scaling law, suggested by the saturation property of the parton distributions. An interpretation of this observation in terms of the Tsallis approach was proposed in [16,28]. It would be thus interesting to investigate how this scaling property of the spectra translates into the results shown in the present paper.