Long-range collectivity in small collision systems with ...

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Long-range collectivity in small collision systems with two- and four-particle correlations at STAR Shengli Huang For STAR Collaboration Stony Brook University, Chemistry Department

Transcript of Long-range collectivity in small collision systems with ...

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Long-range collectivity in small collision systems with two- and four-particle

correlations at STAR

Shengli HuangFor STAR Collaboration

Stony Brook University, Chemistry Department

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Outline

qMotivation and Analysis MethodsqPhysics ResultsüThe v2 in different small systems at different collision energiesüThe c2{4} in d+Au collisions at different collision energiesqSummary

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What is the Origin of Ridge?

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q Ridge (a long-range near-side correlation) is observed in small systems at RHIC:Creation of a small QGP droplet or other mechanisms?

q If a small QGP droplet is indeed created:How does the system evolve in a small QGP droplet?How about the dependence of multiplicity and collision energy for the flow?

PHENIX:PRL115(2015)142301

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Initial Geometry and Final State Evolution

q Different initial geometry in small systems such as p/d/3He+Au

q Large eccentricity ≠ Large flow at low multiplicity: a large shear viscous correction

q The interplay between them can be explored by measuring the flow in different systems for events with same multiplicity

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0-5% p+Au

0-5% d+Au

0-5% He+Au

e2 0.23 0.54 0.50

e3 0.16 0.19 0.28

Glauber Model

J. L. Nagle PRL113(2014)112301

P. Liu arXiv:1804.04618

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Event Activity

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q Event classes with different activity are selected by using BBC east in the Au-going direction (-5.0<!<-3.3)

q Long-range two-particle correlationsare measured in TPC(|!|<0.9)

Sum

of A

DC fo

r Eas

t BBC

Raw Number of Tracks in TPC

d+Au 200 GeV

0-10%

90-100%

q Correlation between multiplicity at backward and mid-rapidity

q 10 event classes with different TPC <dN/d!> are selected by sum ADC of BBC east in d+Au collisions at 200 GeV

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Long-range Two-particle Correlations

q A near-side ridge is observed in the HM d+Au(<dN/d!>=17.8) and p+Au(<dN/d!>=10.1) collisions

q A Fourier function is employed to extract the Vn,n

d+Au 200 GeV

p+Au 200 GeV

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STAR Preliminary

High Multiplicity (HM) Low Multiplicity (LM)

"#/"Δϕ ~1 + ∑)*+, 2.),)×cos(nΔϕ))

Fourier Function

Integral vn = sqrt(Vn,n); vn(pT)= Vn,n(pT)/vn

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Two Jet Subtraction Methods

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1.Low multiplicity subtraction scaled by short-range (|Δ"|<0.5) near-side jet yield

#$,$&'()*+,-./,01) = #$,$

&' − #$,$5'×

7899:.5'

7899:.&' ×

<=>?,$>8@A9BC>&'

<=>?,$>8@A9BC>5'

ATLAS:PRC90(2014)044906CMS:PLB765(2017)193STAR: PLB743(2015)333

ü Assumption: short-range near-side jet modification = long-range away-side jet modification

ü A new developed method to subtract away-side jet contribution by ATLAS:

<?>DEF.(Δϕ) = F ×<5'(Δϕ) + <@BCH>(Δϕ)where<@BCH>(Δϕ) = G×(1 + 2×∑$MNO #$,$×cos(nΔϕ))

ATLAS:PRL(116)172301

STAR Preliminary

ü Assumption: away-side jet shape can be measured in LMevents and scaled by fit parameter “F” due to jet modification

2.Template Fit

Shengli HuangIt will cause a bias if assumptions are not correct

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v2 in HM d+Au (0-10%) at 200 GeV

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q v2 without subtraction is larger than that with subtraction for both methods. The subtraction of non-flow is crucial in small system!

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v2 in HM d+Au (0-10%) at 200 GeV

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q v2 without subtraction is larger than that with subtraction for both methods. The subtraction of non-flow is crucial in small system!

q At lower pT, the v2 from LM subtraction is around 35% lower than that from template fit, while they are quite similar at intermediate pT

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q v2 without subtraction is larger than that with subtraction for both methods. The subtraction of non-flow is crucial in small system!

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q At lower pT, the v2 from LM subtraction is around 35% lower than that from template fit. While they are quite similar at intermediate pT

q The subtracted v2 measured by STAR is similar to PHENIX measurement, which has at least 10% non-flow

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v2 in HM d+Au (0-10%) at 200 GeV

PRL114(2015)192301

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q Compared to d+Au results, v2 in p+Au without subtraction is much larger than that with subtraction for two methods

q In p+Au collision, the v2 from LM subtraction is much lower than that from template fit.

q v2 from template fit method is similar to PHENIX measurement at low pT

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v2 in HM p+Au (0-10%) at 200 GeV

PRC95(2017)034910

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p/d+Au v2 with same <dN/d!>

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q By LM subtraction method, v2 in d+Au is a little bit larger than that of p+Au collisions

q v2 between p+Au and d+Au collisions from template fit is similar, while the initial eccentricities are different by a factor of two

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q There is large difference between two methodsq LM subtraction leads to a negative V2,2 at low energy

ü Different kinematics between near- and away-side jet-like correlations?q V2,2 from template fit increases as a function of <dN/d!>

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Integral V2,2 vs. <dN/d!>

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Integral v2 from Template Fit

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q The unsubtracted integral v2 as a function of <dN/d!> is different in different systems at different collision energies

q The integral v2 from template fit shows a universal trend as a function of <dN/d!>

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Differential v2 from Template Fit in d+Au BES

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qThe differential v2 becomes negative at high pT in d+Au collisions at low energy

q The correlation from away-side jet is stronger at higher pT. This potentially can lead to large uncertainties in the non-flow subtraction

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c2{4} vs. <dN/d!>

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An indication that c2{4} is negative for high multiplicity d+Au collisions at 200 and 62.4 GeV, while the statistical uncertainties are large

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"# 4 = ⟪'()#(+,-+.(+/(+0)⟫−2⟪'()#(+,(+.)⟫3), 35 , 36, 37 are the azimuthal angles of four different particles in an event ;�� represents the average over all particles from all events within a given multiplicity range8# 4 = 9 −"#{4}

Four-Particle Cumulant

Efficiency Corrected TPC Multiplicity

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Summaryq Large difference between V2,2 from two methods has been observed at low

energyüThere are large uncertainties in the non-flow subtraction in small systems

qWe see similar v2 between p/d+Au collisions for same multiplicity.üv2 is not only driven by initial geometry

qThe integral v2 extracted by template fit shows a universal trend as a function of <dN/d!> for different small systems at different energies

üMultiplicity plays an important role for the flow in small systems!qc2{4} is negative at high multiplicity at 62.4 and 200 GeV, but the measurements

are limited by statistics.

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