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Dissipation and fragmentation of low-Q^2 scattered partons in Au-Au collisions at RHIC PDF

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Preview Dissipation and fragmentation of low-Q^2 scattered partons in Au-Au collisions at RHIC

Preprint submitted to HEAVY ION Acta Phys.Hung.A 22/1 (2005) 000–000 PHYSICS Dissipation and fragmentation of low-Q2 scattered partons in Au-Au collisions at RHIC 6 0 0 R. L. Ray and M. Daugherity, STAR Collaboration 2 n Department of Physics, The University of Texas at Austin, a J Austin, Texas 78712, USA 0 2 Received 1 January 2005 2 v 5 Abstract. Two-particlecorrelationsandevent-wisefluctuationsintransverse 7 momentum pt are reported for Au-Au collisions at √sNN = 62 and 200 GeV 0 on pseudorapidity η and azimuth φ. Distributions of all pairs of particles 0 (no leading trigger particle) reveal jet-like correlations, or peaks at pair-wise 1 5 openinganglesoforder1radianorless. Thewidthofthissame-sidecorrelation 0 peak increases dramatically on pseudorapidity and decreases on azimuth for / increasing collision centrality. Evolution of the same-side peak with centrality x e suggestsdissipationoflow-Q2partonsviastrongcouplingtoanexpandingbulk - medium. p correlations, which provide access to temperature and/or velocity l t c distributions in the colliding system, are also presented. u n Keywords: correlations,fluctuations, Au-Au collisions, minijets : v PACS: 24.60.Ky, 25.75.Gz i X r a 1. Introduction Theoreticaldescriptionsofrelativisticheavy-ioncollisionspredictabundantlow-Q2 gluonproductionintheearlystagesofthecollisionwithrapidpartonthermalization driving the formation of a colored medium [ 1, 2, 3]. Remnants of these semi-hard processesmaysurvivetothefinal,decouplingstageowingtothefinite sizeandlife- time of the collision volume. If so, there should be contributions to nonstatistical event-wise fluctuations of mean-p p and two-particle correlations. Large non- t t h i statistical p fluctuations have been reported for Au-Au collisions at 130 GeV [ t h i 4] and 200 GeV [ 5] which are much larger than was observed at the SPS [ 6, 7]. Studyofthe relatedtwo-particlecorrelationsfacilitatesinterpretationofevent-wise fluctuations in terms of underlying dynamics. In this paper we report preliminary two-particle correlations for Au-Au collisions at 62 GeV on (η,φ) and p fluctua- t h i 2 R. Ray and M. Daugherity tions and p correlationsfor Au-Au at 200 GeV [ 8] from the STAR Collaboration. t 2 Low-Q partons are emphasized in order to probe nonperturbative QCD medium effects. These data complement the two-particle correlations for Au-Au collisions at 130 GeV reported in [ 9, 10]. DataforthepresentanalysiswereobtainedwiththeSTARdetector[11]where charged particles were accepted in η 1.3, 2π azimuth, and p 0.15 GeV/c. t | | ≤ ≥ Corrections were made for two-track inefficiencies and charge-sign dependent cuts were applied to minimize quantum and Coulomb correlation contributions. These cuts do not significantly affect the correlation structures shown here. Cuts based on dE/dx in the STAR Time Projection Chamber tracking detector were applied to reduce photon conversion e± contamination. See Ref. [ 10] for discussion of the various cuts. 2. Autocorrelations In conventional jet analysis event-wise concentrations of transverse momentum or energy localized on angle variables (η,φ) are identified. In heavy ion collisions, where such identification is impractical, jet studies are based on a high-p ‘leading t particle’ which may estimate a parton momentum direction and some fraction of 2 its magnitude. However, for low-Q partons identification of a ‘leading particle’ is not possible. Furthermore the number of correlated hadrons from each low-Q2 partonisexpectedtoberelativelysmallwhilethenumberofsuchpartonsperevent is large (of order tens). Observation of these relatively soft correlated hadrons is accessed via autocorrelations which are well-known in signal processing disciplines to enable weak but repetitive signals, which cannot be detected individually, to be accurately measured in aggregate. An autocorrelation is a projection by averaging from subspace (x1,x2) onto difference variable x∆ x1 x2. The autocorrelations ≡ − reportedin[9, 10]andheredonotrequirealeading-ortrigger-particle,butinstead use all particle pairs within the acceptance. The two-particle correlationdensity per final state particle is defined by ∆ρ/√ρmix [ρsib(p~1,~p2) ρmix(p~1,p~2)]/√ρmix, (1) ≡ − where ρsib(p~1,p~2) is the object distribution comprised of particle pairs from single events (sibling pairs) and the reference distribution, ρmix(p~1,p~2), consists of pairs formed by sampling each particle of the pair from two different but similar events (mixed-event pairs). Studies of measured two-particle correlation projections onto subspaces (pt1 vs pt2), (η1 vs η2) and (φ1 vs φ2) indicate that the principle depen- dences for Au-Au collision data are on (pt1+pt2), (pt1 pt2), and the differences − η∆ η1 η2 and φ∆ φ1 φ2. For the latter two the correlation distributions ≡ − ≡ − are simultaneously projected onto difference variables φ∆ and η∆; the projectionis then referred to as a joint autocorrelation. Dissipation of low-Q2 partons 3 3. Charge-Independent Joint Autocorrelations on (η∆,φ∆) Plotted in Fig. 1 are perspective views of preliminary charge-independent joint autocorrelations∆ρ/√ρmix ondifferencevariables(η∆,φ∆)forthreecentralitybins (approximately 80-90%, 50-60% and 10-20%) for Au-Au collisions at 62 GeV. The distributionsaredominatedby1)acos(2φ∆)componentattributedtoelliptic flow; 2) a cos(φ∆) component associated with transverse momentum conservation, and 3) a 2D same-side (φ∆ < π/2) peak, which is the principal object of interest | | 2 here, and assumed to be associated with low-Q scattered parton fragmentation. In addition, for the most-peripheral data, a φ∆ independent gaussian distribution on η∆ is observed similar to that seen in correlation studies of p-p collision data [ 12] and assumed to be due to charge-ordering associated with longitudinal string fragmentation. This feature vanishes quickly with centrality. The same-side peak STAR Preliminary 0.03 0.004 0.001 0.02 0.002 0.01 0 0 0 -0.01 4 4 4 3 3 3 fD2 10-1 -2-1.5-1-0.50 0.51 1.52 2 10-1 -2-1.5-1-0.500.5 11.5 2 2 10-1 -2-1.5-1-0.50 0.5h1 D1.5 2 Fig. 1. ∆ρ/√ρref for Au-Au collisions at √sNN = 62 GeV on (η∆,φ∆) for centralities 80-90%,50-60% and 10-20% fraction of Au-Au total cross section. ∼ in Fig. 1 varies strongly with centrality, transitioning from nearly symmetric on (η∆,φ∆)forperipheralcollisionstodramaticallybroadenedalongη∆ andnarrowed on φ∆ for the more central collisions. Resonance (e.g. ρ0,ω) decays contribute about 3% of the peaks at (0,0) [ 10]. Electron conversion pairs which remain after the dE/dx cuts add to the bin at (0,0) producing the narrow spike there. Mean-p fluctuation measure ∆σ2 (δη,δφ) [ 4] obtained for particles within a t pt:n two-dimensionalbinofsize(δη,δφ),isequivalenttoanintegralofp autocorrelation t ∆ρ(pt :n;η∆,φ∆)/√ρmix overdifferencevariablesfrom(0,0)to(δη,δφ)[8]. Inver- sion of this integral equation yields p autocorrelations. The latter provide access t to temperatureand/orvelocitydistributions inthe collidingsystemindependentof that afforded by number of pair correlations [ 8]. Fig. 2 shows ∆σ2 (δη,δφ) (left pt:n panel), the resultingp autocorrelation(middle panel), andp autocorrelationwith t t cos(2φ∆) and cos(φ∆) subtracted [ 8] (right panel). The same-side peak structure broadens dramatically with centrality (not shown) on η∆ as in Fig. 1 but remains narrower than the corresponding number of pair correlations. 4 R. Ray and M. Daugherity STAR preliminary STAR preliminary STAR preliminary 22 (GeV/c)pt:n000000000.....00000....000001234123455555 22 (GeV/c)ref-000000....0000..0001200125555 12 2 (GeV/c)ref000000....000000..000011..0001272712555555 12 Ds 0 1.5 √r -0.01 0 √r 0 0 Fig. 2.df6(δη4,δφ)2 sca00le0-.5d1edhpenDr / dent pfD4 flu2ctua0tion-,2-p1hDauDrt / ocorreflaD4tion2, and0 p -2a-1uhtDo- t t t h i correlation with cos(2φ∆) and cos(φ∆) terms subtracted for mid-central (20-30%) Au-Au collisions at 200 GeV. ρ is the same as ρ in the text. ref mix 4. Conclusions In STAR we arestudying howthe same-side autocorrelationstructures evolvewith centrality in Au-Au collisions at √sNN = 62, 130 and 200 GeV. Same-side charge- averagepair number and p autocorrelationsstrongly elongate on η and narrow on t φ. The STAR experimentresults reportedhereandelsewhere[8, 9, 10]areconsis- tent with a picture in which (1) semi-hard parton scattering transfers momentum (p ) to the bulk medium, inducing temperature/velocity fluctuations in the soft t p range whose correlation amplitudes scale with the number of binary collisions t per participant, and (2) particles correlated with semi-hard scattered partons in the early stages of the collision interact with the longitudinally expanding medium resulting in larger average η∆ . The reduced width on φ is not understood. | | References 1. K.Kajantie,P.V.LandshoffandJ.Lindfors,Phys. Rev. Lett.59(1987)2527. 2. A. H. Mueller, Nucl. Phys. B 572 (2000) 227. 3. G. C. Nayak, A. Dumitru, L. D. McLerran and W. Greiner, Nucl. Phys. A 687 (2001) 457. 4. J.Adamsetal.(STARCollaboration), Phys. Rev. C 71 (2005) 064906. 5. S.S.Adleret al.(PHENIXCollaboration),Phys. Rev. Lett.93(2004)092301. 6. D. Adamov´a et al. (CERES Collaboration), Nucl. Phys. A 727 (2003) 97. 7. T. Anticic et al. (NA49 Collaboration), Phys. Rev. C 70 (2004) 034902. 8. J. Adams et al. (STAR Collaboration), eprint nucl-ex/0509030, submitted to Phys. Lett. B; T. Trainor, R. Porter and D. Prindle, J. Phys. G: Nucl. Part. Phys. 31 (2005) 809. 9. J. Adams et al. (STAR Collaboration), eprint nucl-ex/0408012. 10. J. Adams et al. (STAR Collaboration), eprint nucl-ex/0411003. 11. K. H. Ackermann et al., Nucl. Instrum. Meth. A 499 (2003) 624; see other STAR papers in volume A499. 12. R.J. Porter and T.A. Trainor (STAR Collaboration), eprint hep-ph/0406330.

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