nuclear modification factor of d mesons in au+au collisions at snn = 200 gev · 2015. 11. 19. ·...

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1 Guannan Xie Nuclear Modification Factor of D 0 Mesons in Au+Au Collisions at s NN = 200 GeV Lawrence Berkeley National Laboratory University of Science and Technology of China October 28-31, 2015, Santa Fe, NM Guannan Xie (for the STAR Collaboration) 2015 Fall Meeting of the APS Division of Nuclear Physics

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Page 1: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

1 Guannan Xie

Nuclear Modification Factor of D0 Mesons in Au+Au Collisions at √sNN = 200 GeV

Lawrence Berkeley National Laboratory University of Science and Technology of China

October 28-31, 2015, Santa Fe, NM

Guannan Xie (for the STAR Collaboration)

2015 Fall Meeting of the APS Division of Nuclear Physics

Page 2: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

Motivation

2 Guannan Xie

Perturbative QCD calculations (FONLL) are consistent with experimental data.

STAR Preliminary

Charm quarks: mc >> ΛQCD, TQGP(RHIC/LHC) •  Produced early in collision at RHIC through hard scattering •  Experience the whole evolution of the system -> good probe for medium properties

STAR PreliminarySTAR: PRD 86 (2012) 072013, NPA 931 (2014) 520 CDF: PRL 91 (2003) 241804 ALICE: JHEP01 (2012) 128 FONLL: PRL 95 (2005) 122001

October 28-31, 2015, Santa Fe, NM

Page 3: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

binnumber of binary collisions N

1 10 210 310

b)µ (

y=0

/dy|

ccNN

σd

0

50

100

150

200

250

300

350

400

FONLL in p+p

FONLL err.

NLO err.

d+Au+e)0(D

)0Au+Au (Dp+p

+D*)0(D

= 200 GeVNNS

Sys. error

run9

run12

Motivation

3 Guannan Xie

Charm cross section follows number of binary collisions scaling => At RHIC, charm quarks are produced via initial hard scatterings.

STAR Preliminary

Perturbative QCD calculations (FONLL) are consistent with experimental data.

STAR: PRL 94 (2005) 62301, PRD 86 (2012) 072013, PRL 113 (2014) 142301 FONLL: PRL 95 (2005) 122001 NLO: Eur.Phys.J.ST 155 (2008) 213

October 28-31, 2015, Santa Fe, NM

Charm quarks: mc >> ΛQCD, TQGP(RHIC/LHC) •  Produced early in collision at RHIC through hard scattering •  Experience the whole evolution of the system -> good probe for medium properties

Page 4: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

Results Before the Heavy Flavor Tracker

4 Guannan Xie

•  Precision measurement is needed to further constrain models and to quantify medium properties.

•  New 2014 Au+Au results with HFT will be presented -- p+p and p+Au data with HFT are recorded (run 2015)

•  High pT: large suppression due to

energy loss, strong charm-medium interaction.

•  Enhancement at pT ~0.7-2 GeV/c, described by models with coalescence of charm and light quarks.

0 2 4 60

0.5

1

1.5

2

)A

AF

acto

r (R 40-80% (a)

0 2 4 6 8

10-40% (b)

(GeV/c)T

p0 2 4 6 80

0.5

1

1.5

2

Nu

clea

r M

od

ific

atio + X @ 200 GeV Central 0-10%0 D→STAR Au+Au

dataTAMUSUBATECHTorinoDuke w shad.Duke w/o shad.LANL

STAR: PRL 113 (2014) 142301

October 28-31, 2015, Santa Fe, NM

Page 5: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

STAR Detector

5 Guannan Xie

Time Projection Chamber: Tracking, PID (dE/dx)

Time Of Flight detector: PID (1/β)

Heavy Flavor Tracker

HFT: •  Silicon Strip Detector: r ~22 cm •  Intermediate Silicon Tracker: r ~14 cm •  PIXEL detector: r ~2.8 & 8 cm, MAPS, 20x20 µm2, 0.4%X0, air-cooled

October 28-31, 2015, Santa Fe, NM

Page 6: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

HFT Performance

Guannan Xie

DCA (Distance of Closest Approach) resolution •  ~ 30 µm at high pT

•  Kaon with p = 750 MeV/c, DCA resolution <50 µm

PIXEL detector DCA Resolution

Au+Au at √sNN = 200 GeV, with Heavy Flavor Tracker ~780M minimum bias events analyzed (out of total 1.2B recorded in 2014)

6

Run14 Au+Au @ 200 GeV

October 28-31, 2015, Santa Fe, NM

Page 7: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

D0 Meson Reconstruction

7 Guannan Xie

Direct topological reconstruction through hadronic channel:

With HFT: Greatly reduced combinatorial background

D0 w/o HFT with HFT

Year 2010 + 2011 2014

Significance per billion events

13 51

D0 (D0 )→ K ∓π ±(BR 3.89%)cτ ≈120µm

Topological cuts optimized by TMVA (Toolkit for Multi Variate Analysis)

October 28-31, 2015, Santa Fe, NM

Page 8: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

D0 Meson Signal

8 Guannan Xie

)2 (GeV/cπKM1.7 1.75 1.8 1.85 1.9 1.95 2 2.05 2.1

]310×

) [2C

ount

s/(1

0 M

eV/c

0

5

10

15

20

25

30

unlike, same evtlike, same evtunlike, mixed evt

Au+Au 200GeV, 0-80% MB < 2.0 GeV/c

T1.0 < p

360± = 8038 0#D=22.3S+BS/

)2 (GeV/cπKM1.7 1.75 1.8 1.85 1.9 1.95 2 2.05 2.1

)2C

ount

s/(1

0 M

eV/c

0

20

40

60

80

100

120

140

160

180

200

220

unlike, same evtlike, same evtunlike, mixed evt

Au+Au 200GeV, 0-80% MB < 8.0 GeV/c

T5.0 < p

29± = 417 0#D=14.4S+BS/

•  With the HFT, significantly enhanced D0 signal-to-background ratios in a broad range of transverse momentum

STAR Preliminary

STAR Preliminary

October 28-31, 2015, Santa Fe, NM

Page 9: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

Invariant yield

9 Guannan Xie

(GeV/c)T

p0 1 2 3 4 5 6 7 8

]-2

dy) [

(GeV

/c)

Tdp Tpπ

N/(2

2 d

8−10

7−10

6−10

5−10

4−10

3−10

2−10

1−10

Au+Au 0-10%

2014 [/20]0D

2010/11 [/20]0D

@ Au+Au 200 GeV0STAR D

+D*0p+p D

>bin

p+p Levy scaled by <N

•  [High pT] Consistent with published result, with improved statistical precision

STAR Preliminary

- Finalizing systematic uncertainties for pT< 2 GeV/c

PRL 113 (2014) 142301

October 28-31, 2015, Santa Fe, NM

Page 10: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

(GeV/c)T

p0 2 4 6 8

AAR

0

0.5

1

1.5

2

p+p uncert.

@ 200 GeV 0-10%0 D→Au+Au

20140D

2010/110D

Nuclear Modification Factor

10 Guannan Xie

•  High pT: significant suppression in central Au+Au collisions

•  New Au+Au results have improved statistical and systematic precision

•  p+p precision to be improved using 2015 data with HFT

PRL 113 (2014) 142301

STAR Preliminary

October 28-31, 2015, Santa Fe, NM

AuAu Ncoll uncertainty [left] pp normalization uncertainty [right]

Page 11: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

(GeV/c)T

p0 2 4 6 8

AAR

0

0.5

1

1.5

2

p+p uncert.

@ 200 GeV 0-10%0 D→Au+Au

20140D 2010/110D

0-12% STARπ

RAA : D0 vs. π

11 Guannan Xie

•  RAA(D) ~ RAA(π) at pT>4 GeV/c

STAR D0: PRL 113 (2014) 142301 STAR π : PLB 655 (2007) 104

STAR Preliminary

October 28-31, 2015, Santa Fe, NM

Page 12: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

(GeV/c)T

p0 2 4 6 8

AAR

0

0.5

1

1.5

2

p+p uncert.

@ 200 GeV 0-10%0 D→Au+Au

20140D 2010/110D

D 0-10% ALICE

RAA : RHIC vs. LHC

12 Guannan Xie

•  RAA@ RHIC ~ RAA@LHC

STAR D0: PRL 113 (2014) 142301 ALICE D: arXiv: 1509.06888

STAR Preliminary

October 28-31, 2015, Santa Fe, NM

Page 13: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

(GeV/c)T

p0 2 4 6 8

AAR

0

0.5

1

1.5

2

p+p uncert.

@ 200 GeV 0-10%0 D→Au+Au

20140D 2010/110D

DUKETAMUSUBATECH

RAA : Comparison to Models

13 Guannan Xie

•  DUKE: Langevin simulation, input parameter (2πT)D = 7 (tuned to the LHC data)

•  TAMU: non-perturb., Full T-matrix treatment, (2πT)D = 2-10

•  SUBATECH: perturb. +HTL +resummation, (2πT)D = 2-4

Data compatible with models which predict the value of diffusion coefficient in the range 2 < (2πT)D < 10, same models can also reproduce the measured D0 v2 [QM15,talk ID:493]

STAR Preliminary

STAR: PRL 113 (2014) 142301 DUKE: PRC 92 (2015) 024907 Theory: arXiv:1506.03981(2015) Theory curves: latest calculations from private communications

October 28-31, 2015, Santa Fe, NM

Page 14: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

Summary & Outlook

14 Guannan Xie

(GeV/c)T

p0 2 4 6 8

AAR

0

0.5

1

1.5

2

p+p uncert.

@ 200 GeV 0-10%0 D→Au+Au

20140D

2010/110D

STAR Preliminary

October 28-31, 2015, Santa Fe, NM

•  First measurement of D0 RAA using STAR HFT. –  Significant suppression at high pT in central Au+Au collisions –  Improved data precision, will further constrain models –  Extracted diffusion coefficient 2 < (2πT)D < 10 for central Au+Au collisions at RHIC,

consistent with what we learned from the charm hadron v2 measurements •  Near future outlook with HFT

–  Year 2014 full D0 spectra and RAA is coming soon –  Year 2015 p+p and p+Au data is on the way –  Year 2016 Au+Au 2 Billion minimum bias events, high statistics data will help to

reduce the uncertainty of the medium property (2πT)D

Page 15: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

Thank You

Page 16: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

Efficiency Correction

Embedding (~3% systematic uncertainty) –  Full STAR GEANT simulation + MC embedded in real raw data + data reconstruction chain

16 Guannan Xie

⊗D0 efficiency = TPC tracking eff HFT tracking eff topological cuts ⊗

Data-driven simulation (5-15% pT-dependent systematics) •  HFT matching and resolution smearing using distributions extracted

from data: –  HFT eff. × geometrical acceptance: (HFT matched tracks) / TPC tracks. –  Spatial resolution: DCA distributions of HFT matched tracks (XY-Z dependence).

Luminosity, centrality, azimuth and pseudo-rapidity dependence have been considered.

October 28-31, 2015, Santa Fe, NM

Page 17: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

Topology distribution comparison

17 Guannan Xie October 28-31, 2015, Santa Fe, NM

Page 18: Nuclear Modification Factor of D Mesons in Au+Au Collisions at sNN = 200 GeV · 2015. 11. 19. · Summary & Outlook Guannan Xie 14 (GeV/c) T p 02 4 6 8 AA R 0 0.5 1 1.5 2 p+p uncert

(GeV/c)T

Transverse Momentum p0 1 2 3 4 5 6 7

2v

0.05−

0

0.05

0.1

0.15

0.2

0.25

0.3

Non-flow est.Au+Au 200GeV, 0-80%

0DTAMU

DukeSUBATECH

V2 : Comparison to Models

18 Guannan Xie

Also good agreement between models and experiment for v2 Compatible with models predicting a value of diff. coefficient between 2 to ~10

STAR Preliminary

Theory curves: latest calculations from private communications

October 28-31, 2015, Santa Fe, NM