Self-consistent analysis of hadron production in pp and AA collisions at mid-rapidity

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1 Self-consistent analysis of hadron production in pp and AA collisions at mid-rapidity G.I. Lykasov, A.I. Malakhov Joint Institute for Nuclear Research, Dubna 4980, Moscow region, Russia arxiv: v [hep-ph] 22 Jan 208 Abstract The self-consistent approach based on similarity of inclusive spectra of hadrons produced in pp and AA collisions is reviewed. This approach allows us to describe rather well the ratio of proton to anti-proton yields in AA collisions as a function of the initial energy at a wide range from a few GeV to a few TeV. We suggest its modification due to the quark-gluon dynamics to describe the inclusive spectra of hadrons produced in pp collision as a function of the transverse momentum p t at mid-rapidity. The extension of this approach to analyze the pion p t -spectra produced in AA collision at high and middle energies and mid-rapidity is given. The satisfactory description of experimental data on these spectra in pp and AA collisions within the offered approach is shown. Introduction The similarity principle, for example, in physics is well known. Its application to the particle production in hadron-hadron collision has been proposed several decades ago by E.Fermi [], I.Pomeranchuk [2], L.D.Landau [3] and R.Hagedorn [4]. It was noticed that the transverse momentum spectra of the particles produced in these collisions had a universal form like ρ h exp( m ht /T), at least, at not large values of m ht, where m ht is the transverse mass of the produced hadron h and T is a constant dependent only of the type of final hadrons. There are many statistical models applied successfully a similar form to describe hadronic yields produced in heavy-ion collisions (see, for example, [5]- [9] and references therein). Actually, the parameter T is nothing to do the average transverse mass m ht. However, according to many experimental data, the average transverse momentum p ht of the produced hadron or m ht = p 2 ht + m2 h depends on the initial energy s, especially at low s. Here s is the energy squared in the c.m.s. of colliding particles and m h is the mass of the produced hadron. Almost all theoretical approaches operate with the relativistic invariant Mandelstam variables s, t, u to analyze the hadron inclusive spectra in the mid-rapidity region. As usual, the

2 spectra are presented in the factorized forms of two functions dependent of t or p 2 t and s. However, there is another approach to analyze multiple hadron production in pp and AA collisions at high energies, which operates by using four velocities of the initial and final particles [0]. It is the so called the self-similarity approach, which demonstrates the similarity of inclusive spectra of hadrons produced in pp and AA collisions, as a function of similarity parameter Π. The approach of studying relativistic nuclear interactions in the four velocity space proved to be very fruitful []. In fact, this approach is valid not in the complete kinematical region. That will be discussed in our paper. The hadron inclusive spectra obtained within this approach are presented as a function of the relativistic invariant similarity parameter, which can be related to variables t and s, as it is shown in [2]. The general form of such spectrum is not factorized over t and s. In this paper we present further development of this approach and extend it to the hadron production in AA collisions at the center rapidity region. 2 The parameter or function of self-similarity Π. The description of multi particle states of the relativistic nuclear physics in terms of macroscopic variables such as temperature, pressure, density, entropy, contradicts to an important principle, which is emphasized by Heisenberg [3]: physical laws and the approval must be expressed only within the observed values. In the study of collisions of the relativistic nuclei most of these macroscopic variables have not been observed. In this work we have used the approach based on the law of similarity which is applied in relativistic nuclear physics but not based on Lagrange method. This allows one to design the solution based on the above principles. In hydraulics, as it is well known, methods of the theory of dimensionality and similarity are widely used. In fact, the invariant relations between the measured parameters of the problem are determined. In hydrodynamics the methods of similarity are widely applied they often are the only mean of the equation analysis. The versatility of the methods of similarity for the theory and experiment is not accidental. The fact is that similarity transformations define the invariant relationships which characterize the structure of all the laws of nature, including the laws of relativistic nuclear physics [4]. In analogy with the geometrical similarity for physical phenomena we have used invariant dimensionless combinations (similarity parameters), composed from the dimension values defining the task. For example, when planning large expensive hydraulic structures it is necessary to carry out physical modeling. Geometrically, the body of model is made similarly to the nature-body. For the steady motion of a viscous incompressible fluid flowing over the body, the directions of the velocities in the model and nature are the same. As the main parameters of the problem we have taken the following: l - the characteristic size of the body model, l 0 is the size of the nature body, l 0 /l is the coefficient of geometric similarity, and U is the velocity of the impinging flow, µ is the viscosity of the fluid, ρ is the fluid density. These parameters define the system of units: l - length, M - mass, T - time, and have the following dimensions: [l] = L, [U] = L T, [µ] = M L T, [ρ] = M L 3. From the defining parameters we can construct only one dynamic similarity parameter (a dimensionless combination, independent of the choice of measuring units): Π = ρul/µ =Re. This invariant is called the Reynolds number. To provide the similarity, it is required to have equality of this parameter for the model and nature. If the distance r is measured in units of l 2

3 and the velocity V is measured in units of U, the solutions of the hydrodynamic equations for the velocity distributions will have the following form: V/U = f(r/l, Re). From this expression it follows that the fields of the flow velocities around geometrically similar bodies are described by only one function, depending on r/l if the Reynolds numbers for these flows are the same. Within the self-similarity approach [0, ] the predictions on the ratios of the particles produced in AA collisions at high energies were given in [4, 5]. Let us briefly present here the main idea of this study. Consider, for example, the production of hadrons, 2, etc. in the collision of nucleus I with nucleus II: I + II () According to this assumption more than one nucleon in the nucleus I can participate in the interaction (). The value of N I is the effective number of nucleons inside the nucleus I, participating in the interaction which is called the cumulative number. Its values lie in the region of 0 N I A I (A I - atomic number of nucleus I). The cumulative area complies with N I >. Of course, the same situation will take place for the nucleus II, and it is possible to introduce the cumulative number of N II. For reaction () with the production of the inclusive particle we can write the conservation law of four-momentum in the following form: (N I P I + N II P II p ) 2 = (N I m 0 + N II m 0 + M) 2, (2) where N I and N II the number of nucleons involved in the interaction; P I, P II, p are four momenta of the nuclei I and II and particle, respectively; m 0 is the mass of the nucleon; M is the mass of the particle providing the conservation of the baryon number, strangeness, and other quantum numbers. In [4] the parameter of self-similarity is introduced, which allows one to describe the differential cross section of the yield of a large class of particles in relativistic nuclear collisions: Π = min[ 2 [(u IN I + u II N II ) 2 ] /2, (3) where u I and u II are four velocities of the nuclei I and II. The values N I and N II will be measurable, if we accept the hypothesis of minimum mass m 2 0 (u N + u 2 N 2 ) 2 and consider the conservation law of 4-momentum. Thus, the procedure to determine N I and N II, and, hence, Π, is the determination of the minimum of Π on the basis of the conservation law of energymomentum. Then, it was suggested [4, 5] that the inclusive spectrum of the produced particle in AA collision can be presented as the universal function dependent of the self-similarity parameter Π, which was chosen, for example, as the exponential function: Ed 3 σ/dp 3 = C A α(n I) I where α(n I ) = /3 + N I /3, α(n II ) = /3 + N II /3, C = mb GeV 2 c 3 st and C 2 = 0.25 ± A α(n II) II exp( Π/C 2 ), (4) 3

4 Equation (2) can be written as follows: N I N II Φ I N I Φ II N II = Φ M, (5) Where relativistic invariant dimensionless values have been introduced: Equation (5) can be written as follows: Φ I = [(m /m 0 ) (u I u ) + M/m 0 ]/[(u I u II ) ] Φ II = [(m /m 0 ) (u II u ) + M/m 0 ]/[(u I u II ) ] Φ M = (M 2 m 2 )/[2m2 0 ((u Iu II ) )]. [(N I /Φ II ) ] [(N II /Φ I ) ] = + [Φ M /(Φ I Φ II )]. (6) Minimum Φ is found from the following: Let us introduce the intermediate variables: dπ/dn I = 0, dπ/dn II = 0. (7) F I = [(N I /Φ II ) ], F II = [(N II /Φ I ) ]. From the above we obtain: F I F II = + Φ M /(Φ I Φ II ). Then (7) is also equal to 0 as From (3) we can obtain: dπ/df I = 0, dπ/df II = 0. 4Π 2 = N 2 I + N 2 II + 2N I N II (u I u II ), 4Π 2 = (F I + ) 2 Φ 2 II + (F II + ) 2 Φ 2 I + 2Φ I Φ II (F I + ) (F II + ) (u I u II ), F II = α/f I The condition of the minimum d(4π 2 )/df = 0 gives the equation for F I : FI 4 + F 3 I (Φ I/Φ II ) 2 (α 2 + αf I ) + (u I u II ) (Φ I /Φ II ) (F 3 I αf I) = 0 or FI 4 + F 3 I [ + (u Iu II )/z] (α/z) F I [(u I u II ) + (/z)] α 2 /z 2 = 0, where z = Φ II /Φ I. Changing I to II we should replace z (/z), F I (α/f II ). (α/f II ) 4 + (α/f II ) 3 [ + (u I u II )z] αz(α/f II )[(u I u II ) + z] α 2 z 2 = 0 or F 4 II + F 3 II [ + (u Iu II )z] zα F II [z + (u I u II )] α 2 z 2 = 0. Thus, at z = F I = F II, Φ I = Φ II = Φ. Since F I = F II, then (N I /Φ ) = (N II /Φ ) and N I = N II. F 2 = α and F I = F II = α /2 = [ + (Φ M /Φ 2 )] /2. 4

5 N I = N II = N = ( + F)Φ = { + [ + (Φ M /Φ 2 )] /2 }Φ. Π = /2[2N 2 + 2N 2 (u I u II )] /2 = N/ 2)[ + (u I u II )] = N ChY (u I u II ) = ch2y, (u I u ) = (m t /m ) ch( Y + y) = (m t /m ) ch(y y). (u II u ) = (m t /m ) ch(y y). Here m t is the transverse mass of the particle, m t = (m 2 + p2 t ) /2, Y - rapidity of interacting nuclei, y - particle rapidity. At y = 0 (in the central rapidity region) we obtain: (u I u ) = (u II u ) = (m t /m ) chy, m t = (m 2 + p2 t ) /2 Φ = (/m 0 ) (m t chy + M) [/(2sh 2 Y)] Φ M = (M 2 m 2 )/(4m 02sh 2 Y) N = [ + ((Φ M /Φ 2 ) + ) /2 ] [(m t /m 0 )chy + (M/m 0 )] [/(2sh 2 Y)] 2. Self-similarity function Π in the central rapidity region In the mid-rapidity region (y=0, y is the rapidity of particle ) the analytical form for Π was found in [5]. In this case N I and N II are equal to each other: N I = N II = N. N = [ + ( + Φ/Φ 2 ) /2 ]Φ, (8) where Φ = (m t chy + M)/(2m 0 sh 2 Y), (9) Φ = (M 2 m 2 )/(4m2 0 sh2 Y). (0) Here m t is the transverse mass of the particle, m t = (m 2 + p2 t ) /2, Y- rapidity of interacting nuclei. And then - Π = N chy. () This formula is obtained by searching for the minimum of the expression for Π by differentiation of the right-hand side of equation (3) on variables N I and N II taking into account the conservation law (2). For baryons we have the following: and for antibaryons - Π b = (m t chy m )chy/(m 0 sh 2 Y) (2) Π a = (m t chy + m )chy/(m 0 sh 2 Y). (3) The results of calculations for the ratio of the antiproton cross section to the proton one after integration of Eqs.(2,3) over dm t were presented in [2]. This ratio is compared to the experimental data including the latest data obtained at LHC [6 8]. Moreover, the satisfactory description of data at the wide energy range was shown [2]. The same calculations can be made for the ratio of yield of other antiparticles and particles. 5

6 2.2 Relation of self-similarity function Π to the Mandelstam variables s, t, u As it is mentioned above, the exponential form for the hadron inclusive spectrum given by Eq.(4) was chosen as an example and using it we can satisfactorily describe the ratio of total yields of antiprotons to the protons produced in heavy nucleus-nucleus collisions. Unfortunately, this simple form Eq.(4) contradicts to the LHC data on the inclusive spectra of hadrons produced in the central pp collisions, as shown in [9]. Therefore, we use the results of [9] to present the inclusive relativistic invariant hadron spectrum at the mid-rapidity region and at not large hadron transverse momenta p t in a more complicated form, which consists of two parts. The first one is due to the contribution of quarks, which was obtained within the QGSM [20,2] using the AGK (Abramovsky, Gribov, Kanchelli) cancellation [22] of n-pomeron exchanges for inclusive hadron spectra in the mid-rapidity region. It is written in the following form [9]: E(d 3 σ/d 3 p) q = φ q (y = 0, p t ) [nσ n (s)] = n= φ q (y = 0, p t )g(s/s 0 ), (4) where σ n (s) is the cross-section to produce the n-pomeron chain (or 2n quark-antiquark strings); g = 2 mb - constant, which is calculated within the quasi-eikonal approximation [23]; s 0 = GeV 2 ; = [α p (0) ] 0.2, where α p (0) is the sub critical Pomeron intercept [20, 2, 23]. The second part of the hadron inclusive spectrum at the mid-rapidity region was introduced in [9, 24] assuming the contribution of the nonperturbative gluons and calculating it as the one-pomeron exchange between two nonperturbative gluons in the collided protons [24]. This part was written in the following form [9]: E(d 3 σ/d 3 p) g = φ g (y = 0, p t ) φ g (y = 0, p t ) nσ n (s) n= (n )σ n (s) = n=2 σ n (s) = φ g(y = 0, p t ) [g(s/s 0 ) σ nd ], (5) n= where σ nd is the non diffractive pp cross section. Thus, taking into account the quark and gluon contributions we will get the following form for the inclusive hadron spectrum: E(d 3 σ/d 3 p) = [φ q (y = 0, p t ) + φ g (y = 0, p t ) ( σ nd /g((s/s 0 ) )] g(s/s 0 ) (6) The question arises, what is the relation of the similarity parameter Π to the relativistic invariant variables s, p 2 t? This relation can be found from Eqs.(8-) using ch(y) = s/(2m 0 ). Then, we have the following form for Π: { mt Π = 2m 0 δ + } sδ + + M2 m 2 δ (7) m 2 t where δ = 4m 2 0 /s; m t = p 2 t + m 2 is the transverse mass of the produced hadron h. At large initial energies s >> GeV the similarity parameter Π becomes as following: Π = m t 2m 0 ( 4m 2 0 /s) M2 m 2 ( 4m 2 m 2 0 /s) t (8)

7 For π-mesons m = µ π is the pion mass and M = 0; for K -mesons m = m K is the kaon mass and M = m K ; for K + -mesons m = m K and M = m Λ m 0, m Λ is the mass of the Λ-baryon. For π-mesons at p 2 t >> m 2 we have: m t Π m 0 ( 4m 2 0 /s) (9) One can see that in the general case the similarity parameter Π depends on p 2 t and s and asymptotically at large s >> 4m 2 0 it depends only on p2 tπ. Let us stress that the dependence of Π on s is crucial at low initial energies only. 2.3 Quark-gluon dynamics of soft NN interaction and self-similarity function Π The invariant inclusive spectrum can be also presented in the following equivalent form: ρ NN E h d 3 σ NN d 3 p h Taking into account (20) we can rewrite Eq.(6) in the form: = dσ π dp 2 t dy dσ π dm 2 t dy (20) dσ NN π dm 2 t dy = [φ q(y = 0, Π) + φ g (y = 0, Π) ( σ nd /g((s/s 0 ) )] g(s/s 0 ). (2) The first part of the inclusive spectrum (Soft QCD (quarks)) is related to the function φ q (y = 0, Π), which is fitted by the following form [9]: φ q (y = 0, Π) = A q exp( Π/C q ), (22) where A q = 3.68 (GeV/c) 2, C q = The function φ g (y = 0, Π) related to the second part (Soft QCD (gluons)) of the spectrum is fitted by the following form [9]: φ g (y = 0, Π) = A g mt exp( Π/C g ), (23) where A g =.7249 (GeV/c) 2, C g = Using (2) we can calculate the inclusive hadron spectrum as a function of the transverse mass. In Fig. the inclusive spectrum (/m t )dσ/dm t dy of π -mesons produced in pp collisions at the initial momenta P in = 3 GeV/c is presented versus their transverse mass m t. The similar satisfactory description of the NA6 data at P in = 58 GeV/c was obtained in our paper [2]. Using only the first part of the spectrum φ q (y = 0, m t ), which corresponds to the quark contribution, the conventional string model, let s call it the SOFT QCD (quarks), one can describe the NA6 data [25] rather satisfactorily at m t < GeV/c 2. This part of the inclusive spectrum corresponds to the dashed line in Fig.. The inclusion of the second part of spectrum due to the contribution of gluons (SOFT QCD (gluons)), the dotted line, allowed us to describe all the NA6 data up to m t.5 Gev/c, see the solid line in Fig. (Soft QCD(quarks+gluons)). Actually, at large s even at the NA6 energies Π m t /m 0 instead of (9). Generally the pion spectrum ρ NN (s, m t E h (d 3 σ/d 3 p h ) (ignoring the gluon part) can be presented in the following approximated form, which is valid for the NA6 energies and low transverse momenta p t < GeV/c: ρ NN (s, m t ) φ q (y = 0, Π)g(s/s 0 ) = g(s/s 0 ) A q exp( 7 m t (24) C q m 0 ( 4m 2 0 /s)) g(s/s 0 ) A q exp( m t T ),

8 (/m T )dn/dydm T, [GeV -2 c 4 ] P in =3 GeV/c Soft QCD (quarks + gluons) Soft QCD (quarks) Soft QCD (gluons) NA6 experimental data e m T, [GeV/c 2 ] Figure : Results of the calculations of the inclusive cross section of hadron production in pp collisions as a function of the transverse mass at the initial momenta P in = 3 GeV/c. They are compared to the NA6 experimental data [25]. where T = C q m 0 ( 4m 2 0 /s) (25) is the inverse slope parameter, which is called sometimes as the thermal freeze-out temperature. One can see from Eq.(25) that this thermal freeze-out temperature depends on the initial energy square s in the c.m.s. of collided protons. That is the direct consequence of the self-similarity approach, which uses the four-momentum velocity formalism. This s-dependence of T is significant at low initial energies and at s >> m 2 0 the slope parameter T becomes independent on s. To describe rather well the NA6 data at larger values of p t, the inclusive pion spectrum should be presented by Eq. (2), which has a more complicated form in comparison to the simple exponential form of Eq. (25). However, the main contribution to the inelastic total cross section comes from the first part of Eq.(2), which has the form given by Eq. (25).Eq. (25). We have calculated the inverse slope parameter T, as a function of the energy s given by Eq.(25) and presented in Fig. 2 (top ). There is a good agreement with the NA6 data [25] at 6 GeV < s <8 GeV and the JINR data [26, 27] at 2 GeV < s < 4 GeV. As, for example, in Fig. (2, bottom) we illustrate the satisfactory description of LHC data on inclusive spectrum of charged hadrons (mainly pions and kaons) at s = 7 TeV by using (6) and the perturbative QCD (PQCD) within the LO [9, 24]. This spectrum is the sum of inclusive spectra of pions and kaons, therefore it is presented as a function of the transverse momentum p t instead of functions of the transverse mass m t because the masses of a pion and kaon are different. In addition to the part of spectrum, which corresponds to (6), see the solid line in this figure, we also have included the PQCD calculations, see the dotted line. The PQCD calculations within the LO are divergent at low p t, therefore, the dotted line goes up, when p t 8

9 0.2 Our calculation NA6 data JINR,LHE data Inverse slope T, [GeV/c 2 ] s /2, [GeV] [/N ev ]dn/dydp t 2, y=0, [GeV -2 c 2 ] S /2 =7TeV SQCD(quarks+gluos) SQCD(quarks) SQCD(gluons) SQCD+PQCD Exp. data (ATLAS,CMS) e p t, [GeV/c] Figure 2: Top: the average pion transverse mass T = m t calculated using Eq. 25. The points at 6 GeV< s <8 Gev are the NA6 data [25], the points at 2 GeV < s < 4 GeV are the data extracted from [26,27]. Bottom: results of the calculations of the inclusive cross section of charge hadrons produced in pp collisions at the LHC energies as a function of their transverse momentum p t at s =7 TeV. The points are the LHC experimental data [28, 29]. decreases. The kinematical region about p t GeV/c 2 can be treated as the matching region of the nonpertubative QCD (soft QCD) and the pertubative QCD (PQCD). One can see from Fig. (2) that it is possible to describe rather well these inclusive spectrum in the wide region of p t at the LHC energies matching these two approaches. To describe rather well the LHC data on these inclusive p t -spectra at p t > 2-3 GeV/c, the PQCD calculation should be included, whose contribution has a shape similar to the power law p t -distribution [30]. 9

10 3 Nucleus-nucleus collisions in the central rapidity region The relativistic invariant inclusive spectrum of hadrons produced in AA collision in the central rapidity region and not large transverse momenta can be presented in the following form: Ed 3 σ AA /dp 3 = C A α(n I) I A α(n II) II ρ NN, (26) where ρ NN is the inclusive relativistic invariant pion spectrum in pp collision given by Eq. (2), α(n) = /3 + N/3, the s-dependent function N is calculated using Eqs. (8-0). The results of our calculations of p t -spectra of pions produced in AA collisions in the central rapidity region and different high and middle energies compared to different experimental data are presented in Figs. (3-5). One can see from Fig. (3) that our approach is able to get a satisfactory description of the data on pion production in AuAu and PbPb collisions at the STAR and LHC energies as well as in p p collisions, see Figs. (,2) at p t.2 GeV/c. In principle, there can be another theoretical interpretation of multiple hadron production in heavy-ion collisions at high energies based, for example, on the stationary thermal model [3,32]. At middle initial energies about GeV-8 GeV our calculations of pion p t -spectra in heavy ion collisions, namely AuAu, ArKCl, at the central rapidities result in a more or less satisfactory description of the data shape at low p t < GeV/c, as it also can be seen in Figs. (3-5). By calculation of all the pion p t -spectra in AA collisions at mid-rapidity we used the same form of ρ NN applied to the satisfactory description of the NA6 and LHC data on hadron production in pp collisions, see Figs. (3-5). The energy dependence of these spectra is given by the term g(s/s 0 ) for the quark contribution and the term (g(s/s 0 ) σ nd ) for the gluon contribution to ρ NN. The non diffractive cross section σ nd, as a difference between the total pp cross section σ tot and the elastic (σ el ) and the diffractive (σ di f ) cross sections at high energies is taken from the experimental data. At middle energies about several GeV there are very poor data on the diffractive cross section σ di f. Therefore, at s about a few GeV our calculations are not so precise, as at high energies. As one can see from Figs.(3-5) the p t -pion spectra in heavy ion collisions, as AuAu, PbPb, ArKCl, at the mid-rapidity are described rather satisfactorily within the proposed approach at p t < GeV/c. In Fig. (5, bottom) we present the prediction of pion m πt -spectrum in AuAu collision in the mid-rapidity region and centrality about (0-5)% for the HADES experiment at initial kinetic energy per nucleon about.25 GeV. A small deviation of our calculations from the HADES data can be seen in the p t -spectrum of the pions produced in C 2 C 2 collision at the initial kinetic energy E kin /nucl. = 2 GeV presented in Fig. 5. Similar deviation of the theory from the data is not seen in p t -spectra of the pions produced in heavy ion collisions, for example, AuAu, PbPb, ArKCl. It can be due to the difference between nuclear density ρ N (k) distribution in heavy nuclei and light nuclei. In the heavy nucleus ρ N (k) as function of the internal nucleon momentum k is more flat compared to the nucleon distribution in the light nucleus, therefore the pion production in heavy ion collision can be less sensitive to the nuclear structure compared to the same pion production in light nucleus-nucleus collisions. 4 Conclusion The inclusive hadron spectrum in the space of four-velocities is presented within the selfsimilarity approach as a function of the similarity parameter Π. The use of the self-similarity approach allows us to describe the ratio of the total yields of protons to the anti-protons produced in AA collisions as a function of the energy in the mid-rapidity region and a wide energy range from 0 GeV to a few TeV [2]. We have shown that the energy dependence of the similarity parameter Π included within this approach is very significant at low energies, namely at s < 6 GeV, and rather well repro- 0

11 (/m π,t ) 2 dn/dm π,t,[(/mevc 2 ) 3 ] x0 8 x0 7 x Total calculation for Au+Au->π +,- +X at E kin =200 GeV Quark contribution at E kin =200 GeV Gluon contribution at E kin =200 GeV Star data for Au+Au->π +,- at E kin =200 GeV Total calculation or Pb+Pb->π +,- +X at E kin =2760 GeV Quark contribution at E kin =2760 GeV Gluon contribution at E kin =2760 GeV ALICE data for Pb+Pb->π +,- +X at E kin =2760 GeV m π,t -m π, [GeV/c 2 ] /m π d 2 N/dm πt, [(/GeV/c 2 ) 2 ] Our calculation for Pb+Pb->π - + X at 40 GeV NA6 data on Pb+Pb->π - + X at 40 GeV Our calculation for Ar+Sc->π - + X at 40 GeV NA6 data on Ar+Sc->π - + X at 40 GeV Our calculation for Be+Be->π - + X at 40 GeV NA6 data on Be+Be->π - + X at 40 GeV Our calculation for p+p->π - + X at 40 GeV NA6 data on p+p->π - + X at 40 GeV m πt -m π, [GeV] Figure 3: Top: results of our calculations of pion p T -spectra in AuAu and PbPb collisions in the central rapidity region compared to the STAR [33] and ALICE [34] data. Bottom: Results of our calculations of pion m T -spectra in PbPb, ArS c, BeBe and pp collisions at the initial kinetic energy per nucleon E kin =40 GeV and the central rapidity region compared to the NA6 [35,36] data. duces the experimental data on the inverse slope or the thermal freeze-out temperature of the inclusive spectrum of the hadrons produced in pp collisions. The parameter Π increases and saturates when s grows. This is very significant for a theoretical interpretation of the future experimental data planned to get at FAIR, CBM (Darmstadt, Germany) and NICA (Dubna, Russia) projects. That is an advantage of the self-similarity approach compared to other theoretical models. However, we have also shown that the s dependence of Π is not enough to describe the inclu-

12 (/2π) d 2 N/d(m π,t ), [/(GeV/c 2 ) Theoretical calculation at E kin /nucleon=2 GeV AGS data at E kin /nucleon=2 GeV Theoretical calculation at E kin /nucleon=4 GeV AGS data at E kin /nucleon=4 GeV Theoretical calculation at E kin /nucleon=6 GeV AGS data at E kin /nucleon=6 GeV Theoretical calculation at E kin /nucleon=8 GeV AGS data at E kin /nucleon=8 GeV m π,t -m π, [GeV] 000 Total calculation Quark contribution Gluon contribution Hades data for Ar+Kcl->π + X at E kin/nucl =.75 Ge (/m πt ) 2 dn/dm πt, [(/MeV/c 2 ) 3 ] m πt -m π, [MeV/c 2 ] Figure 4: Top: our calculations of pion p T -spectra in AuAu collision in the central rapidity region and different initial energies compared to the AGS data [37]. Bottom: results of our calculations of pion p T -spectra in ArKcl collision in the central rapidity region and initial kinetic energy per nucleon about.75 GeV compared to the HADES data [38]. sive spectra of the hadrons produced in the mid-rapidity region, for example, in pp collisions in the wide region of initial energy, especially at the LHC energies. Therefore, we have modified the self-similarity approach using the quark-gluon string model (QGSM) [20, 2] and [9, 24] including the contribution of nonperturbative gluons, which are very significant to describe the experimental data on inclusive hadron spectra in the mid-rapidity region at the transverse momenta p t up to 2-3 GeV/c [9,24]. Moreover, the gluon density obtained in [24], whose parameters were found from the best description of the LHC data and also allowed us to describe the HERA data on the proton structure functions [40]. To describe the data in the mid-rapidity 2

13 (/m π,t ) 2 dn/dm π,t,[(/mevc 2 ) 3 ] x0-6 Total calculation at E kin = GeV Hades data for C+C->π - +X at E kin = GeV Total calculation at E kin =2 GeV Hades data for C+C->π - +X at E kin =2 GeV x m π,t -m π, [GeV/c 2 ] 000 Total calculation Quark contribution Gluon contribution /m πt dn/m πt, [(/MeV/c 2 ) 2 ] m πt -m π Figure 5: Top: results of our calculations of pion m πt -spectrum in C 2 C 2 collision in the central rapidity and initial kinetic energies about GeV and 2 GeV compared to the HADES data [39]. Bottom: our predictions of pion m πt -spectrum in AuAu collision in the central rapidity region and initial kinetic energy per nucleon about.25 GeV at the centrality about (0-5)%. region and values of p t up to 2-3 GeV/c, we have modified the simple exponential form of the spectrum, as a function of Π, and presented it in two parts due to the contribution of quarks and gluons, each of them has a different energy dependence. This energy dependence was obtained in [9] by using the Regge approach valid for soft hadron-nucleon processes. To extend the application of the offered approach to analyze these inclusive p t -spectra at large hadron transverse momenta, we have to take the PQCD calculations into account. This approach is applied to the analysis of pion production in pp, AA and pa collisions in 3

14 the mid-rapidity region. We have shown the self-consistent satisfactory description of the data on p t -spectra of the pions in these interactions in a wide region of initial energies and not large transverse momenta of pions. The approach suggested in this paper results in a more or less well description of these spectra for heavy-ion collisions. However, it can not be applied to the analysis of hadron production in light nucleus-nucleus collisions, especially, at middle energies because the production mechanism is very sensitive to the nuclear structure, which is different for heavy and light nuclei. Acknowledgements. We are very grateful to A.P. Jerusalimov, A.A. Baldin, A.V. Belayev, A.Yu. Troyan for giving us the experimental data obtained at the JINR. We thank M. Gumberidze, R. Holzmann, G. Kornakov, A. Rustamov, J. Stroth for extremely helpful discussions and very productive collaboration. We are also grateful to P. Braun-Munzenger, T. Galatyuk, V.P. Ladygin, M. Lorenz, V. Pechenov, B. Ramstein, P. Salabura for helpful discussions. References [] E.Fermi, Phys. Rev. 92 (953) 452. [2] I. Ya. Pomeranchuk, Izv. Dokl. Akad. Nauk Ser.Fiz. 78 (95) 889. [3] L.D. Landau, Izv. Akad. Nauk Ser. Fiz. 7 (953) 5. [4] R. Hagedorn, Supplemento al Nuovo Cimento Volume III, 47 (965); R. Hagedorn, Nuovo Cimento 35 (965) 395; R. Hagedorn, Thermodynamics of strong interactions,nuovo Cimento 56 A (968) 027 [5] J. Cleymans, H. Oeschler, K. Redlich and S. Wheaton, Phys. Rev. C73 (2006) ; arxiv:05094[hep-ph]. [6] A. Andronic, P. Braun-Munzinger, J. Stachel, Nucl. Phys. A 834 (200) 237C; arxiv: [nucl-th]. [7]. A. Andronic, P. Braun-Munzinger, J. Stachel, Nucl. Phys. A 772 (2006) 67; arxiv:0507 [nucl-th]. [8] F. Becattini, J. Manninen, and M. Gaździcki, Phys. Rev. C 73 (2006) ; arxiv:05092[hep-ph]. [9] S. V. Akkelin, P. Braun-Munzinger, Yu. M. Sinyukov, Nucl. Phys. A 70 (2002) 439; arxiv:0050 [hep-ph]. [0] A. M. Baldin, L. A. Didenko. Fortsch.Phys. 38 (990) []. M. Baldin, A. I. Malakhov, and A. N. Sissakian, Phys. Part. Nucl. 29 (Suppl. ) (200), [2] D.A. Artemenkov, G.I. Lykasov, A.I. Malakhov, Int.J.Mod.Phys.Conf.Ser. 39 (205) [3] W.Heisenberg. Physik und Philosophie, Frankfurt am Main, 959. [4] A.M.Baldin and A.A.Baldin. Physics of Particles and Nuclei 29(3), 998, [5] A. M. Baldin, A. I. Malakhov. JINR Rapid Communications, [87]-98 (998)

15 [6] A. Tawfik. Nuclear Physics A 859 (20) [7] [8] R. Klingenberg et al. Nuclear Physics A 60 (996) 306c-36c. [9] V. A. Bednyakov, A. A. Grinyuk, G. I. Lykasov, M. Pogosyan; Phys.Rev. D87 (203) [20] A. B. Kaidalov, Z.Phys. C2 (982) 63. [2] A. B. Kaidalov, Surveys High Energy Phys. 3 (999) 265. [22] V. Abramovsky, V. N. Gribov and O. Konchelli, Sov.J.Nucl.Phys. 8 (973) 308. [23] K. A. Ter-Martirosyan. Sov.J.Nucl.Phys., 44, 87 (986). [24] A. A. Grinyuk, G. I. Lykasov, A. V. Lipatov, N. P. Zotov. Phys.Rev. D87 (203) [25] A. A. Abgrall et al. Eur.Phys.J., C74 (204) [26] A.P.Jerusalimov et al. Eur.Phys.J. A5, 83 (205). [27] EPJ Web Conf. 38, 07008, (207). [28] V. Khachatryan, et al. (CMS Collaboration), Phys. Rev. Lett. 05, (200). [29] G. Aad, et al. (ATLAS Collaboration), New J. Phys. 3, (20). [30] J. Cleymans, G.I. Lykasov, A.S. Parvan, A.S. Sorin, O.V. Teryaev, Phys.Lett. B723 (203) 35; arxiv: [hep-ph]. [3] E.Schnedermann, U.Heinz, Phys.ReV. C47, 738 (993). [32] E.Schnedermann, J.Solfrank, U.Heinz, Phys.Rev. C48, 2462 (993). [33] B. I. Abelev et al. (STAR Collaboration), Phys. Rev. C 75, (2007); Phys.Rev.Lett., 97, 5230 (2006). [34] K. Aamodt, et al. (ALICE Collaboration), Eur. Phys. J. C (20); Phys. Lett. B693, 53 (200) ; Phys. Rev. D 82, (200); Phys. Rev. C88, (203). [35] E.Kaptur, PoS CPOD204, 053 (205). [36] M.Lewicki, arxiv: [hep-ex]. [37] J.L.Klay, et all.(ages Collaboration), Phys.Rev. C68, (2003). [38] P.Tlusty, et all.(hades Collaboration), arxiv: [nucl-ex]. [39] G.Agakishev, et all.(hades Collaboration), Eur.Phys.J., A40, 45 (2009). [40] A. V. Lipatov, G. I. Lykasov, N. P. Zotov, Phys.Rev. D89, 0400 (204) 5

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