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From RHIC to LHC: a relativistic diffusion approach

Abstract

We investigate stopping and particle production in heavy-ion collisions in a Relativistic Diffusion Model (RDM). Using three sources for particle production, the energy- and centrality dependence of rapidity distributions of net protons, and pseudorapidity distributions of charged hadrons in heavy systems at RHIC energies are precisely reproduced in the analytical model. The transport coefficients are then extrapolated from Au + Au at RHIC energies (<FONT FACE=Symbol>Ö</FONT>sNN=19.6 - 200 GeV) to Pb + Pb at LHC energies of <FONT FACE=Symbol>Ö</FONT>sNN= 5.52 TeV. Rapidity distributions for net protons, and pseudorapidity spectra for produced charged particles are obtained and discussed in a three-sources model at LHC energies.

Diffusion model


SOFT INTERACTIONS

From RHIC to LHC: a relativistic diffusion approach

Rolf Kuiper; Georg Wolschin

Institut für Theoretische Physik der Universität Heidelberg, Philosophenweg 16, D-69120 Heidelberg, Germany

ABSTRACT

We investigate stopping and particle production in heavy-ion collisions in a Relativistic Diffusion Model (RDM). Using three sources for particle production, the energy- and centrality dependence of rapidity distributions of net protons, and pseudorapidity distributions of charged hadrons in heavy systems at RHIC energies are precisely reproduced in the analytical model. The transport coefficients are then extrapolated from Au + Au at RHIC energies (ÖsNN=19.6 - 200 GeV) to Pb + Pb at LHC energies of ÖsNN= 5.52 TeV. Rapidity distributions for net protons, and pseudorapidity spectra for produced charged particles are obtained and discussed in a three-sources model at LHC energies.

Keywords: Diffusion model

I. INTRODUCTION

Stopping and particle production in relativistic heavy-ion collisions at the highest energies available at RHIC and LHC offer sensitive tools to test the nonequilibrium-statistical properties of these systems. Analytically soluble nonequilibrium-statistical models [1] not only allow to accurately describe a fairly large amount of phenomena, but also to predict results across the gap in center-of-mass energy from the highest RHIC energy in Au + Au collisions of =200 GeV [2, 3] to the LHC energy of = 5.52 TeV in Pb + Pb collisions.

Net-baryon (more precisely, net-proton) distributions have proven to be sensitive indicators for local equilibration, collective expansion, and deconfinement in heavy relativistic systems [4]. This is reconsidered in the analysis of SPS- and RHIC-results within the Relativistic Diffusion Model (RDM) for three sources in Sect. II. The dependence of the transport coefficients on the center-of-mass energy from AGS via SPS to RHIC is then used for predictions of net-baryon rapidity distributions at LHC.

It is of particular interest in relativistic collisions of heavy systems to determine the fraction of produced particles that attains - or comes very close to - local statistical equilibrium. In the three-sources RDM, these are the particles produced in the midrapidity source. Hence Au + Au and Cu + Cu pseudorapidity distributions of produced particles are analyzed at RHIC energies from =19.6 - 200 GeV, and the transport coefficients and numbers of produced particles as functions of the incident energies are determined in Sect. III.

For several reasonably motivated extrapolations of the transport coefficients a range of resulting distribution functions for produced charged hadrons in Pb + Pb collisions at LHC energies is discussed. The conclusions are drawn in Sect. IV.

II. NET-BARYON RAPIDITY SPECTRA

In the Relativistic Diffusion Model, the net-baryon rapidity distribution at RHIC energies emerges from a superposition of the beam-like nonequilibrium components that are broadened in rapidity space through diffusion due to soft (hadronic, low p^) collisions and particle creations, and a near-equilibrium (thermal) component at midrapidity that arises - among other processes - from hard (partonic, high p^) processes, and may indicate local quark-gluon plasma (QGP) formation.

The time evolution of the distribution functions is governed by a Fokker-Planck equation (FPE) in rapidity space [1, 4-7]

with the rapidity y = 0.5· ln((E+p)/(E-p)). The rapidity diffusion coefficient Dy that contains the microscopic physics accounts for the broadening of the rapidity distributions due to interactions and particle creations, and it is related to the drift term J(y) by means of a dissipation-fluctuation theorem (Einstein relation) which is used to actually calculate Dy in the weak-coupling limit [1]. The drift J(y) determines the shift of the mean rapidities towards the central value, and linear and nonlinear forms have been discussed.

Here we use µ = 1 (due to norm conservation) and q = 2- n =1 corresponding to the standard FPE, and a linear drift function

with the rapidity relaxation time ty, and the equilibrium value yeqof the rapidity [1,8]. This is the so-called Uhlenbeck-Ornstein process, applied to the relativistic invariant rapidity for the three components Rk(y,t) (k=1,2,3) of the distribution function [1, 4, 7].

Since the equation is linear, a superposition of the distribution functions [1, 4] emerging from R1,2(y,t = 0) = d (y yb) and R3(y,t = 0) = d (y-yeq) with mean values and variances obtained analytically from the moments equations yields the exact solution.

With an effective diffusion coefficient that includes not only the random behaviour of the particles, but also the effect of expansion, the available net-proton data for central Au+Au collisions at AGS, and Pb+Pb at SPS [9] can be reproduced precisely with only two sources in the RDM. The corresponding rapidity width coefficient is

Extending the model to RHIC energies of 200 GeV, one finds [4] that within the linear approach with q = 1 and two sources, it is impossible to reproduce the BRAHMS net-proton data [2] due to the high midrapidity yield.

It has therefore been proposed in [4] that an expanding midrapidity source emerges. With this conjecture, the RHIC data can be interpreted rather precisely in the linear q = 1 framework. A fraction of Zeq ~ 22 net protons (55 net baryons) near midrapidity reaches local statistical equilibrium in the longitudinal degrees of freedom, Fig. 2. The variance of the equilibrium distribution Req(y) at midrapidity is broadened as compared to the Boltzmann result due to collective (multiparticle) effects. This corresponds to a longitudinal expansion (longitudinal flow) velocity of the locally equilibrated subsystem as in hydrodynamical descriptions. Here we obtain the expansion velocity as proposed in [10].



The complete solution of (1) in the q = 1 case is a linear superposition of nonequilibrium and local equilibrium distributions. The net-baryon rapidity distribution becomes

with the interaction time tint (total integration time of the differential equation). The number of net baryons (here: net protons) in local equilibrium near midrapidity is Neq, and N1+N2+Neq is equal to the total number of net baryons. This yields a good representation of the BRAHMS data [2], as was already emphasized in [10]. Here the integration is stopped at the value of tint/ty that yields the best agreement with the data.

Based on the results for net protons from AGS to RHIC energies, the diffusion-model parameters have been extrapolated as functions of the center-of-mass energy to LHC energies of =5.52 TeV. This allows to obtain a first approximation of the net-proton distribution at LHC energies as shown in Fig. 1 together with the SPS- and RHIC-results. Here, the solid curve is for a midrapidity source with a particle content of 14% as at the highest RHIC energy, whereas the dashed curve corresponds to a particle content of only 7%.

Due to the small value of tint/ty = 0.14 that is obtained from the extrapolation [10], the distribution functions at LHC energies extend well beyond the initial beam rapidity shown by an arrow. Hence, this result will have to be corrected at large rapidities since it is likely to violate kinematic constrainsts.

III. PRODUCED CHARGED HADRONS IN THE RDM

The Relativistic Diffusion Model [1] in its linear form with explicit treatment of the collective expansion [4], or in its nonlinear version with implicit consideration of the collective effects, is also suitable for the description and prediction of rapidity distributions of produced charged hadrons.

If particle identification is not available, one has to convert the results to pseudorapidity space, h = -ln[tan(q / 2)] with the scattering angle q . The conversion from y- to h - space of the rapidity density is performed through the Jacobian

The average mass < m > of produced charged hadrons in the central region is approximated by the pion mass mp , and a mean transverse momentum < pT > = 0.4 GeV/c is used.

In the linear two-sources version, the RDM had been applied to pseudorapidity distributions of produced charged hadrons in Au+Au collisions at RHIC energies of 130 GeV and 200 GeV by Biyajima et al. [7]. However, it soon turned out from the above net-proton results [4], and from general considerations, that an additional midrapidity source is required [8, 12].

To allow for an extrapolation of our results for symmetric systems to LHC energies, RDM-calculations for Cu + Cu and Au + Au collisions at RHIC energies from 19.6 GeV via 62.4 GeV, 130 GeV to 200 GeV are performed as described in [11, 14].

The diffusion-model result at LHC energies with extrapolated transport parameters [11] and 50% particle content in the central source is shown in Fig. 2, curve [A]. The RHIC result for 200 GeV is also displayed.

Diffusion-model results using the extrapolations of the number of produced particles at midrapidity given by other authors have also been obtained. In particular, curve [C] uses a logarithmic extrapolation of the midrapidity value that yields dN/dh ~ 1100 [13], whereas the saturation model [13] predicts dN/dh ~ 1800 at midrapidity, with the resulting diffusion-model distribution [D]. The forthcoming LHC data are likely to be in between the cases [A] and [D] [11].

IV. CONCLUSION

Net-proton and charged-hadron distributions in collisions of heavy systems at SPS and RHIC energies have been described in a Relativistic Diffusion Model (RDM) for multiparticle interactions. Analytical results for the rapidity distribution of net protons in central collisions are found to be in good agreement with the available data. An extrapolation of the rapidity distributions for net protons to LHC energies has been performed. The precise number of particles in the midrapidity source remains uncertain at LHC energies and will have to be determined from experiment.

At RHIC - and most likely at LHC -, a significant fraction of the net protons (about 14 per cent at 200 GeV for Au + Au) reaches local statistical equilibrium in a fast and discontinuous transition which may indicate parton deconfinement.

In the three-sources RDM, pseudorapidity distributions of produced charged hadrons have been calculated [11] . The diffusion-model parameters have been optimized in a c2-minimization with respect to the available PHOBOS data in Au+Au and Cu+Cu at RHIC. Excellent results for the energy dependence of the distribution functions have been obtained.

In an extrapolation to LHC energies, the pseudorapidity distribution for produced charged hadrons has been calculated. Here the essential parameters relaxation time, diffusion coefficients or widths of the distribution functions of the three sources, and number of particles in the local equilibrium source will have to be adjusted once the ALICE data for Pb + Pb have become available in 2009.

[1] G. Wolschin, Eur. Phys. J. A 5, 85 (1999); Europhys. Lett. 47, 30 (1999); Phys. Rev. C 69, 024906 (2004).

[2] I.G. Bearden et al., BRAHMS Collaboration, Phys. Rev. Lett. 93, 102301 (2004).

[3] B.B.Back et al., PHOBOS Collaboration, Phys. Rev. Lett. 91, 052303 (2003).

[4] G. Wolschin, Phys. Lett. B 569, 67 (2003).

[5] W.M. Alberico, A. Lavagno, and P. Quarati, Eur. Phys. J. C 12, 499 (2000).

[6] M. Rybczynski, Z. Wlodarczyk, and G. Wilk, Nucl. Phys. B (Proc. Suppl.) 122, 325 (2003).

[7] M. Biyajima, M. Ide, T. Mizoguchi, and N. Suzuki, Prog. Theor. Phys. 108, 559 (2002).

[8] G. Wolschin, M. Biyajima, T. Mizoguchi, and N. Suzuki, Phys. Lett. B 633, 38 (2006); Annalen Phys. 15, 369 (2006).

[9] H. Appelshäuser et al., NA49 Collaboration, Phys. Rev. Lett. 82, 2471 (1999).

[10] G. Wolschin, Europhys. Lett. 74, 29 (2006).

[11] R. Kuiper and G. Wolschin, Annalen Phys. 16, 67 (2007).

[12] M. Biyajima, M. Ide, M. Kaneyama, T. Mizoguchi, and N. Suzuki, Prog. Theor. Phys. Suppl. 153, 344 (2004).

[13] N. Armesto, C. Salgado, and U. Wiedemann, Phys. Rev. Lett. 94, 022002 (2005).

[14] R. Kuiper, Diploma thesis, Universität Heidelberg (2006).

Received on 4 October, 2006; revised version received on 6 January, 2007

  • [1] G. Wolschin, Eur. Phys. J. A 5, 85 (1999);
  • Europhys. Lett. 47, 30 (1999);
  • Phys. Rev. C 69, 024906 (2004).
  • [2] I.G. Bearden et al., BRAHMS Collaboration, Phys. Rev. Lett. 93, 102301 (2004).
  • [3] B.B.Back et al., PHOBOS Collaboration, Phys. Rev. Lett. 91, 052303 (2003).
  • [4] G. Wolschin, Phys. Lett. B 569, 67 (2003).
  • [5] W.M. Alberico, A. Lavagno, and P. Quarati, Eur. Phys. J. C 12, 499 (2000).
  • [6] M. Rybczynski, Z. Wlodarczyk, and G. Wilk, Nucl. Phys. B (Proc. Suppl.) 122, 325 (2003).
  • [7] M. Biyajima, M. Ide, T. Mizoguchi, and N. Suzuki, Prog. Theor. Phys. 108, 559 (2002).
  • [8] G. Wolschin, M. Biyajima, T. Mizoguchi, and N. Suzuki, Phys. Lett. B 633, 38 (2006);
  • Annalen Phys. 15, 369 (2006).
  • [9] H. Appelshäuser et al., NA49 Collaboration, Phys. Rev. Lett. 82, 2471 (1999).
  • [10] G. Wolschin, Europhys. Lett. 74, 29 (2006).
  • [11] R. Kuiper and G. Wolschin, Annalen Phys. 16, 67 (2007).
  • [12] M. Biyajima, M. Ide, M. Kaneyama, T. Mizoguchi, and N. Suzuki, Prog. Theor. Phys. Suppl. 153, 344 (2004).
  • [13] N. Armesto, C. Salgado, and U. Wiedemann, Phys. Rev. Lett. 94, 022002 (2005).
  • [14] R. Kuiper, Diploma thesis, Universität Heidelberg (2006).

Publication Dates

  • Publication in this collection
    10 Aug 2007
  • Date of issue
    June 2007

History

  • Accepted
    06 Jan 2007
  • Received
    04 Oct 2006
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