Photons at RHIC Yorito Yamaguchi CNS, University of Tokyo 1/14 - - PowerPoint PPT Presentation

photons at rhic
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Photons at RHIC Yorito Yamaguchi CNS, University of Tokyo 1/14 - - PowerPoint PPT Presentation

Photons at RHIC Yorito Yamaguchi CNS, University of Tokyo 1/14 Direct photons Sensitive and direct probe for all stages of a collision Generated in every stage of the collision Leave a medium without a strong interaction Provide


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Photons at RHIC

Yorito Yamaguchi CNS, University of Tokyo

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Direct photons

Sensitive and direct probe for all stages of a collision Generated in every stage of the collision Leave a medium without a strong interaction → Provide key inputs (Tinit & τ0) to describe evolution of the matter Their pT are characterized by their origin.

1/14

  • S. Turbide et al., PRL77,024909(2008)
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Direct photons

q q g γ

High pT : Initial hard scatterings

1/14

  • S. Turbide et al., PRL77,024909(2008)

Sensitive and direct probe for all stages of a collision Generated in every stage of the collision Leave a medium without a strong interaction → Provide key inputs (Tinit & τ0) to describe evolution of the matter Their pT are characterized by their origin.

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Direct photons

q q g γ

High pT : Initial hard scatterings Mid pT : Jet‐Medium interactions

Jet‐QGP photons

1/14

  • S. Turbide et al., PRL77,024909(2008)

Sensitive and direct probe for all stages of a collision Generated in every stage of the collision Leave a medium without a strong interaction → Provide key inputs (Tinit & τ0) to describe evolution of the matter Their pT are characterized by their origin.

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SLIDE 5

Direct photons

q q g γ

High pT : Initial hard scatterings Mid pT : Jet‐Medium interactions

Jet‐QGP photons

γ π ρ π

Low pT : Thermal radiations from QGP and Hadron Gas

Thermal photons

1/14

  • S. Turbide et al., PRL77,024909(2008)

Sensitive and direct probe for all stages of a collision Generated in every stage of the collision Leave a medium without a strong interaction → Provide key inputs (Tinit & τ0) to describe evolution of the matter Their pT are characterized by their origin.

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SLIDE 6

Direct photons

q q g γ

High pT : Initial hard scatterings Mid pT : Jet‐Medium interactions

Jet‐QGP photons

γ π ρ π

Low pT : Thermal radiations from QGP and Hadron Gas

Thermal photons

Elliptic flow, v2 of direct photons can disentangle their production processes.

1/14

  • S. Turbide et al., PRL77,024909(2008)

Sensitive and direct probe for all stages of a collision Generated in every stage of the collision Leave a medium without a strong interaction → Provide key inputs (Tinit & τ0) to describe evolution of the matter Their pT are characterized by their origin.

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SLIDE 7

Direct photons

q q g γ

High pT : Initial hard scatterings Mid pT : Jet‐Medium interactions

Jet‐QGP photons

γ π ρ π

Low pT : Thermal radiations from QGP and Hadron Gas

Thermal photons Hadron decay photons

Direct photon measurements are very challenging due to a large background from hadron decays. Elliptic flow, v2 of direct photons can disentangle their production processes.

1/14

  • S. Turbide et al., PRL77,024909(2008)

Sensitive and direct probe for all stages of a collision Generated in every stage of the collision Leave a medium without a strong interaction → Provide key inputs (Tinit & τ0) to describe evolution of the matter Their pT are characterized by their origin.

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Hard photon measurements

Statistical subtraction method by EMCals Firstly measure π0, η Strong suppression of high pT hadrons helps to measure direct γ for Au+Au → Identify remaining γ after subtraction of hadron decay γ as direct γ.

Hadronic All Direct

γ γ γ − =

p+p : Consistent with NLO pQCD calculation → Works for pQCD test d+Au : Also consistent with Ncoll‐scaled NLO pQCD → Little nuclear effects

d+Au d+Au p+p 2/14

B.I. Abelev et al., PRC81,064904(2010)

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Hard photons in Au+Au

Spectra : Also follows Ncoll‐scaled p+p for different centrality bins RAA : Suppression at high pT (pT>14GeV/c) due to isospin effect?

  • r due to initial state energy loss?

→ Experimentally challenging due to merging effect for decay photons.

3/14

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Different collision energy

Au+Au : 62.4GeV Pb+Pb : 2.76TeV 62.4GeV : Isospin effect would be at lower pT → Consistent NLO pQCD 2.76TeV : CMS measured isolated photons → No suppression → Inconsistent with 200GeV Au+Au, but efforts to finalize the 200GeV Au+Au result are ongoing.

4/14

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Process dependent factor

q

γ∗

g q e+ e-

How to measure low pT photons

Hard to measure by EMCals due to a finite energy resolution → Alternative method has been developed : “Virtual photon method” Virtual photon method Basic idea : Any source of γ can emit γ*, convert to low mass e+e‐ How to identify direct γ*→e+e‐ :

Relation between γ and associated γ*→e+e‐ emission rates

Direct γ* : If pT

2»mee 2, S(mee)~1

Dalitz decay : → Extraction of direct γ*→e+e‐ can be made by utilizing mee shape difference between direct γ* and hadrons.

5/14

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Determination of direct γ fraction

r : direct γ/inclusive γ

( ) ( ) ( ) ( )

ee dir ee c ee data

m f r m f r m f ⋅ + ⋅ − = 1

Hadrons Direct γ*

  • A. Adare et al., PRL104,132301(2010)

Determination of direct γ fractions in 0.1‐0.3GeV/c2 for pT>1GeV/c Negligible contribution of π0→γe+e‐ Satisfy an important assumption of pT

2»mee 2 → S(mee)~1

No contribution of π+π‐→e+e‐ Enhanced e+e‐ yield over known hadron contributions is clearly seen due to direct γ*→e+e‐. Extended fit result can also describe the data well in mee>0.3GeV/c2.

6/14

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Direct γ fractions

⎟ ⎟ ⎠ ⎞ ⎜ ⎜ ⎝ ⎛ +

T hadron T NLO T NLO

dp d dp d dp d

γ γ γ

σ σ σ

μ = 0.5pT μ = 1.0pT μ = 2.0pT

NLO pQCD expectations are calculated as : Direct γ fractions from virtual photon method plays an important role

  • n determination of direct photon v2 in low pT region.

7/14

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Low pT direct photon results

p+p vs d+Au : Consistent → Little nuclear effects p+p vs Au+Au : Observation of a clear excess in pT<3GeV/c → Exponential fit gives inverse slope of T = 221±19stat±19systMeV (Central).

p+p vs d+Au p+p vs Au+Au 8/14

  • A. Adare et al., PRL104,132301(2010)
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Tinit & τ0

TC from Lattice QCD ~ 170 MeV TAuAu(fit) ~ 220 MeV

Hydrodynamic models agree with the data within a factor of 2 Uncertainty on Tinit (300‐600MeV) is still large. Depending on thermalization time τ0 (0.1‐0.6fm/c) → Need sensitive observable to further constrain Tinit

9/14

  • A. Adare et al., PRC81,034911(2010)
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Further constraint of Tinit & τ0 by v2

10/14

  • R. Chatterjee & D. K. Srivastava, PRC 79, 021901 (2009)

Thermal radiation Fragmentation Bremsstrahlung Jet-Photon conversion

v2 > 0 v2 < 0 Hydro after τ0

Different direct photon production processes have different behavior of v2. Initial hard scattering → v2=0 Thermal radiation & Fragmentation → v2>0 Bremsstrahlung & JPC → v2<0 →Helps to disentangle compositions of direct photon spectrum Direct photon v2 is also sensitive to thermalization time τ0. Early thermalization → Small thermal photon v2 Late thermalization → Large thermal photon v2

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How to obtain direct photon v2

11/14

inclusive photon v2

Au+Au@200 GeV minimum bias

preliminary

1

2 2 2

− − =

γ γ

r v v r v

hadron inclusive direct

Statistical subtraction method

  • A. Adare et al., arXiv:1105.4126

1. Measure inclusive γ v2 using EMCals

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How to obtain direct photon v2

11/14

inclusive photon v2

Au+Au@200 GeV minimum bias

preliminary

1

2 2 2

− − =

γ γ

r v v r v

hadron inclusive direct

Statistical subtraction method

  • A. Adare et al., arXiv:1105.4126

1. Measure inclusive γ v2 using EMCals

  • Confirm NO charged hadron

contamination by external conversion method

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How to obtain direct photon v2

11/14

1

2 2 2

− − =

γ γ

r v v r v

hadron inclusive direct

Statistical subtraction method π0 v2

preliminary

inclusive photon v2

Au+Au@200 GeV minimum bias

  • A. Adare et al., arXiv:1105.4126

1. Measure inclusive γ v2 using EMCals

  • Confirm NO charged hadron

contamination by external conversion method 2. Measure π0 v2, and then evaluate

  • ther hadron v2 (η, ω, …) using

MC calculation

  • π0 v2 looks similar to inclusive γ v2
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How to obtain direct photon v2

11/14

1

2 2 2

− − =

γ γ

r v v r v

hadron inclusive direct

Statistical subtraction method π0 v2

preliminary

inclusive photon v2

Au+Au@200 GeV minimum bias

  • A. Adare et al., arXiv:1105.4126

1. Measure inclusive γ v2 using EMCals

  • Confirm NO charged hadron

contamination by external conversion method 2. Measure π0 v2, and then evaluate

  • ther hadron v2 (η, ω, …) using

MC calculation

  • π0 v2 looks similar to inclusive γ v2

3. Subtract hadron v2 from inclusive γ v2 with direct γ fractions from virtual photon method

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Direct photon v2

12/14

Surprisingly, a large direct photon v2 is observed in pT<3GeV/c Direct photon v2 →0 indicates prompt photons from initial hard scatterings are dominant in pT>5GeV/c

Au+Au@200 GeV minimum bias

Direct photon v2

preliminary

  • A. Adare et al., arXiv:1105.4126
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Comparison with model

13/14

Theory calculation: H. Holopainen et al., arXiv:1104.5371

Models predict a shape of direct photon v2, however they under‐predict a magnitude. Tinit = 580MeV, τ0 = 0.17fm/c → Need to understand observed direct photon v2 to further constrain Tinit & τ0

Au+Au@200 GeV 0‐20%

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Summary & Outlooks

14/14

Direct photons have been successfully measured in a wide‐ranging pT region for different collision systems at RHIC. High pT photons Statistical subtraction method (using EMCals) Possible suppression at pT>14GeV/c is observed in 200GeV Au+Au, but no suppression in different energy Au+Au (62.4GeV & 2.76TeV) Low pT photons Virtual photon method (γ*→e+e‐) Enhanced yield is observed in Au+Au Direct photon v2 has been also measured. Large v2 at low pT → Thermal photons? v2 = 0 at high pT → Photons from initial hard scatterings → Theoretical challenge to further constrain Tinit & τ0 Direct photons are still one of “hot” probes Low energy scan at RHIC & measurements at LHC → Systematic study in wide collision energy

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Backup

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π0 & η RAA