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High-pt triggered dihadron correlations with vn background subtraction by STAR PDF

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High-p triggered dihadron correlations with v T n background subtraction by STAR Fuqiang Wang (for the STAR Collaboration) 2 Department of Physics, Purdue University, West Lafayette, Indiana 47907, USA 1 0 2 n a STARmeasurementsofdihadroncorrelationswithhigh-p triggerpart- √ T J cles in Au+Au collisions at s =200 GeV are presented with subtrac- NN 4 tion of v , v , and v backgrounds. The v azimuthal anisotropies were 2 3 4 n 2 measured by the two-particle cumulant method with η gap to reduce non- flow. Thedihadroncorrelationsrelativetothev2 aswellasthev3 harmonic ] x planes are also presented. Implications of the results are discussed. e - l 1. Introduction c u n Relativistic heavy ion collisions create a hot and dense medium ex- [ hibiting hydrodynamic properties. The particle azimuthal distributions are anisotropic resulting from hydrodynamic conversion of the initial spatial 1 v anisotropy. Hydrodynamics describe well the expansion and anisotropies of 6 particles at transverse momentum p < 2 GeV/c. Hard-scattering probes, T 0 on the other hand, interact with the medium and lose energy, resulting in 0 depletion of high-p hadrons in the final state. This jet-quenching phe- 5 T . nomenon provides an exclusive channel to study QCD interactions and de- 1 0 duce the properties of the QCD matter at high energy densities. 2 Dihadron correlations with high-p trigger particles have proven valu- T 1 able in jet-quenching studies. One of the difficulties in dihadron correlation : v measurements is the subtraction of combinatoric background. The back- Xi ground is not uniform but modulated by flow harmonics (correlation to the eventplane). Triggeredcorrelationshavebeenmeasuredwithonlyv andv r 2 4 a subtraction, assuming vanishing triangular flow (v ). Novel structures were 3 observed constituting a near-side long-range speudo-rapidity (∆η) correla- tion (‘ridge’) [1, 2] and a away-side double-peak azimuthal (∆φ) correlation (‘Mach-cone’) [1, 3, 4, 5]. Recent model studies suggest, however, that triangular and other odd harmonicsdonotvanishbecauseofinitialgeometryfluctuations[6]. Anon- zero v {2} from two-particle cumulant method has been measured [7, 8]; 3 (1) 2 √ v {2} = V , V ≡ (cid:104)cos(n∆φ)(cid:105) where ∆φ is the two-particle opening n n∆ n∆ azimuthal angle. While a non-zero v {2} itself is not a proof of finite hydro- 3 dynamictriangularflowbecausenonflowalsocontributes,thecentralityand p dependences of the measured v {2} do suggest that part of the v {2} is T 3 3 of hydrodynamic origin, and this part should be subtracted from dihadron correlations. Two questions arise: (1) How much does nonflow (correlation unrelated to the reaction plane) contribute to the measured v {2}? (2) n What are the effects of jet-medium interactions? This talk does not provide a complete answer to these questions, but makes progress towards that end. We report STAR measurements ofv and √ 2 v in Au+Au collisions at s = 200 GeV. We subtract v backgrounds 3 NN n and present the obtained dihadron correlations integrated over as well as relative to the v and v harmonic planes. We discuss possible implications 2 3 of our results. 2. Dihadron correlation with v subtraction n Figure 1 shows the v {2} and v {2} measurements by the two-particle 2 3 cumulant method [8]. The four-particle cumulant v {4} is also shown for 2 comparison. The v {2} has a weak centrality dependence, consistent with 3 its fluctuation origin. At large p in central collisions, v is comparable to T 3 v . An η-gap, |∆η| > 1, was applied in the analysis to reduce the nonflow 2 contributionsfromsmall-anglecorrelations,suchasjet-likecorrelations,res- onance decays, etc. Nonflow correlations beyond |∆η| > 1 still remain. One likely contribution comes from away-side jet-like correlations because the away-side jet partner is uncorrelated to the near-side jet in η. Fig.1. (Color online) Two- and four-particle anisotropy measurements v {2}, √ 2 v {4}, v {2} as a function of centrality in Au+Au collisions at s = 200 GeV 2 3 NN by STAR. The abscissa bins 0-6 stand for 10%-size centralities from 80% to 10%, and 7-8 for 5-10% and top 5% centralities. Three p ranges are shown, 0-2 GeV/c T (left), 1-2 GeV/c (middle), and 3-4 GeV/c (right). Two-particlecumulantv {2}measurestheneteffectofflow, flowfluctu- n ations, and nonflow. Except the nonflow contamination, v {2} is the most n truthful background to dihadron correlation. However, if v {2} is measured n 3 from the same pairs used in dihadron correlation analysis, then v {2} will n precisely describe the correlation function and the v {2}-subtracted signal n will by definition be zero. It is thus important to measure v {2} using pairs n farremovedinphase-spacefromthoseusedindihadroncorrelationanalysis. Dihadron correlations at low-to-intermediate p with ∆η gap in Pb+Pb T collisions at LHC were shown to be completely described by the sum of a few Fourier harmonics [7]. The particle anisotropies at a given p were T measured by the Fourier coefficients of their correlations to reference par- ticles from 0.2 < pref < 5 GeV/c with |∆η| > 1 in ALICE [7]: v (p ) = T n T (cid:113) V (p ,pref)/ V (pref,pref). The dihadron correlation result of Ref. [7], n∆ T T n∆ T T with trigger ptrig=2-3 GeV/c and associated passoc=1-2 GeV/c, thus indi- T T catesV (ptrig,pref)V (passoc,pref) ≈ V (ptrig,passoc)V (pref,pref),which n∆ T T n∆ T T n∆ T T n∆ T T is not surprising given the relatively small nonflow contributions (as gauged by the v {2} and v {4} measurements). Quantitatively how much nonflow 2 2 contributes to the measured V will require further studies. n∆ Fig.2. (Color online) v -subtracted dihadron correlations at |∆η| > 1 in Au+Au √ n collisions at s = 200 GeV by STAR. Three centrality ranges are shown: 50- NN 80%(left),20-50%(middle),andZDCtop12%(right). Thetriggerandassociated p ranges are 3-6 GeV/c and 2-3 GeV/c, respectively. The subtracted v {2} were T n measuredbythetwo-particlecumulantmethodwith|∆η|>1andreferenceparticle pref <2GeV/c. Thebackgroundisnormalizedsuchthattheaveragesignaliszero. T Figure 2 shows the dihadron correlation signals in Au+Au collisions at √ s = 200 GeV by STAR after v subtraction. The trigger and asso- NN n ciated p ranges are 3-6 GeV/c and 2-3 GeV/c, respectively. The v {2} T n were measured with reference particles from pref < 2 GeV/c, which is some- T what removed from the trigger and associated p regions. The blue data T points show the results with v , v , and v subtraction, while the black ones 2 3 4 show those with only v and v subtraction for comparison. In peripheral 2 4 collisions, no visible signal remains besides a negative dipole. This may suggest that the subtracted v contain nonflow contributions comparable n to the jet-like correlation between the trigger-associated pairs. In medium- central collisions, there seems finite correlation amplitude on the near side 4 which may indicate a ridge contribution. In other words, the previously observed ridge may not be completely explained by v . On the away side, a 3 broad correlation signal is still observed, however, the double-hump struc- ture is weaker. In the most central collisions, no away-side correlation is visible, consistent with the “disapparence” of away-side high-p hadrons. T The near-side correlation seems to indicate a finite peak consistent with remaining ridge contributions. 3. Dihadron correlation relative to the event plane Dihadron correlations as a function of the trigger particle azimuth rel- ative to the event plane, φ = φ − ψ , have been analyzed in 20-60% s t 2 Au+Au collisions by STAR [9]. The v and v backgrounds were sub- 2 4 tracted. The v was obtained from the average of two- and four-particle 2 cumulant methods [10]. The v was measured with respect to the v har- 4 2 monic event plane [10]. The effect of v background was estimated and 3 found to be insignificant [9]. In this talk we use for background subtrac- tion the measured v {2} (|∆η| > 0.7) and the parameterized v {ψ } = 2 4 2 1.15v {2}2 for v correlated to ψ . The resultant dihadron correlations at 2 4 2 |∆η| > 0.7 are shown in the black histograms in Fig. 3 and are consistent with the results in Ref. [9]. We further subtract the additional v {2} and 3 (cid:112) v {uncorr.} = v {2}2−v {ψ }2 backgrounds (both uncorrelated to ψ ): 4 4 4 2 2 2vtrig{2}vassoc{2}cos3∆φ+2vtrig{uncorr.}vassoc{uncorr.}cos4∆φ. The re- 3 3 4 4 sults are shown in Fig. 3 in the red histograms. The results again show that the effect of v is insignificant; however, the reduction in the near-side 3 correlation magnitude is noticeable. The event-plane dependent dihadron correlation analysis can be carried outwithrespecttothev harmonicplaneψ . Inreconstructingψ (andψ ), 3 3 3 2 particleswithin|∆η| < 0.5ofthetriggerparticleareexcluded. Analogousto correlationsrelativetoψ ,thev backgrounddependsonthetriggerparticle 2 3 azimuth φ = φ − ψ . The v and v backgrounds are independent of s,3 t 3 2 4 φ . Figure 4 shows in the right panels the dihadron correlation for trigger s,3 particles in-phase of ψ (|φ | < π/6) and out-of-phase (|φ −π/3| < π/6). 3 s,3 s,3 For comparison those for trigger particles in-plane of ψ (|φ | < π/4) and 2 s out-of-plane (|φ −π/2| < π/4) are shown in the left panels. The cartoon s inserts help visulize the geometry. The correlation results seem to indicate a near-side ridge for trigger particles both in-plane of ψ and in-phase of 2 ψ . For away side, the correlation is broader for triggers out-of-plane than 3 in-plane of ψ . To the contrary, the correlation is broader for triggers in- 2 phase than out-of-phase of ψ . These results seem to suggest path-length or 3 geometry effects on the away-side jet-like correlations. However, the exact nature of the effects need further investigations. 5 Fig.3. (Color online) v -subtracted dihadron correlations at |∆η|>0.7 in 20-60% √n Au+Aucollisionsat s =200GeVbySTAR.Thecorrelationsareshown,from NN upper left (in-plane) to lower right (out-of-plane) panel, in 15◦ steps in trigger particle azimuth relative to the event plane, φ . The trigger and associated p s T ranges are 3-4 GeV/c and 1-2 GeV/c, respectively. The subtracted v were mea- n sured by the two-particle cumulant method with |∆η|>0.7 and reference particle pref < 2 GeV/c. The subtracted v background (uncorrelated to the event plane) T 3 and the uncorrelated portion of v are shown in the green and pink histograms, 4 respectively. The background is normalized by the ZYAM prescription. 4. Summary We have presented dihadron correlations with trigger ptrig=3-6 GeV/c √T and associated passoc=2-3 GeV/c in Au+Au collisions at s = 200 GeV T NN by STAR, with v , v , and v background subtraction. The v anisotropy 2 3 4 n were measured by two-particle cumulant method with reference particles from 0.2 < pref < 2 GeV/c and with a relatively large η gap. A near- T side ‘ridge’ peak seems to remain in non-peripheral collisions. The away- side correlation, while strongly suppressed in central collisions, is broad in medium-central collisions. Wehavealsopresenteddihadroncorrelationsrelativetothev harmonic 2 event plane ψ as well as the v harmonic plane ψ , also with v , v , and 2 3 3 2 3 v background subtraction, in 20-60% Au+Au collisions. The effect of v 4 3 is small. A near-side ridge seems to be present in-plane of ψ (and in- 2 phase of ψ ), and disappear out-of-plane of ψ (and out-of-phase of ψ ). 3 2 3 The away-side correlation is single peaked for triggers in-plane of ψ and 2 broadens out-of-plane. This trend seems reversed relative to ψ –The away- 3 sidecorrelationissingle-peakedfortriggersout-of-phaseofψ andbroadens 3 6 Fig.4. (Color online) v -subtracted dihadron correlations at |∆η|>0.7 in 20-60% √n Au+Au collisions at s = 200 GeV by STAR. The correlations are shown for NN trigger particles in-plane (upper-left) and out-of-plane (lower-left) of the v event 2 plane(ψ ),andfortriggerparticlesin-phase(upper-right)andout-of-phase(lower- 2 right) of the v harmonic plane (ψ ). The trigger and associated p ranges are 3-4 3 3 T GeV/cand1-1.5GeV/c,respectively. Thesubtractedv weremeasuredbythetwo- n particle cumulant method with |∆η| > 0.7 and reference particle pref < 2 GeV/c. T The background is normalized such that the average signal is zero. in-phase. These results seem to indicate nontrivial path-length or geometry effects of the underlying physics. REFERENCES [1] J. Adams et al. (STAR Collaboration), Phys. Rev. Lett. 95 (2005) 152301. [2] B.I. Abelev et al. (STAR Collaboration), Phys. Rev. C 80 (2009) 064912. [3] S.S.Adleret al.(PHENIXCollaboration),Phys.Rev.Lett.97(2006)052301. [4] B.I.Abelevet al.(STARCollaboration),Phys.Rev.Lett.102(2009)052302. [5] M.M.Aggarwalet al. (STARCollaboration), Phys.Rev.C 82 (2010)024912. [6] B. Alver and G. Roland, Phys. Rev. C 81 (2010) 054905; Erratum, ibid Phys. Rev. C 82 (2010) 039903(E). [7] K.Aamodtetal.(ALICECollaboration),Phys.Rev.Lett.107(2011)032301. [8] P. Sorensen (for STAR Collaboration), arXiv:1110.0737 (2011). [9] H. Agakishiev et al. (STAR Collaboration), arXiv:1010.0690 [nucl-ex]. [10] J. Adams et al. (STAR Collaboration), Phys. Rev. C 72 (2005) 014904.

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