35
Sanshiro Mizuno for the PHENIX collabora9on University of Tsukuba, RIKEN mail to : [email protected] Measurement Of Direct Photon Azimuthal Anisotropy In Au+Au √s NN =200GeV Collisions at RHICPHENIX experiment

MeasurementOf)DirectPhoton)Azimuthal)Anisotropy) In)Au+Au√ …€¦ · 2 PhotonanalysisinHeavyIonCollision Hadron ):)aer)freezeVout Photon) ):)any)stages)) Produconmechanism Inialhardscaering&

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Page 1: MeasurementOf)DirectPhoton)Azimuthal)Anisotropy) In)Au+Au√ …€¦ · 2 PhotonanalysisinHeavyIonCollision Hadron ):)aer)freezeVout Photon) ):)any)stages)) Produconmechanism Inialhardscaering&

Sanshiro  Mizuno  for  the  PHENIX  collabora9on  University  of  Tsukuba,  RIKEN  

 mail  to  :  [email protected]  

Measurement  Of  Direct  Photon  Azimuthal  Anisotropy  In  Au+Au  √sNN=200GeV  Collisions  

at  RHIC-­‐PHENIX  experiment

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2

Photon  analysis  in  Heavy  Ion  Collision

Hadron  :  aYer  freeze-­‐out  Photon    :  any  stages    Produc5on  mechanism  Ini5al  hard  sca7ering  parton  -­‐  medium  interac5on  Jet  fragmenta5on  Radia5on  from  QGP  and    Hadron  Gas  hadron  decay  

Hadron Photon

Photon  analysis  ü  Advantage  :  Penetra9ng  the  medium  

 Color-­‐less  and  charge-­‐less  Access  to  the  ini9al  stages  of  collision  

 ü  Disadvantage  :  Photons  from  different  stages    superimposed  

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photon  vn(M.Sanshiro) 3

What  is  direct  photon  ?

Direct  photons  are  all  photons  except  for  those  origina9ng  from    hadron  decays  (e.g.  π0-­‐>γ+γ).  Photon  sources  should  be  iden9fied.  (pT,  angular  dependence)  

Ini5al  hard  sca7ering

(thermal?)  radia5on  from  QGP (thermal?)  radia5on  from  HG

hard  parton  energy  loss

Jet  fragmenta5on

hadron  decay

p T(GeV

/c)

5me

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photon  vn(M.Sanshiro) 4

Direct  photon  pT  spectra

Photons  from  each  source  have  different  pT  distribu9on  pa`ern.  Photons  radiated  from  QGP  and  HG  are  dominant  in  low  pT  and  frac9on  of  photons  from  other  sources  increases  with  increasing  pT.  

P.R.L.  104,  132301(2010) P.R.C  84,  054906(2011)

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photon  vn(M.Sanshiro) 5

Medium  effect  (RAA)

RAA=1  not  modified  RAA≠1  medium  effect    Hadron  less  than  unity  -­‐>  medium  effect    

RAA

=(1/Nevt

AA

)d2NAA

/dpT

dy

< Ncoll

> /�inel

pp

⇥ d2�pp

/dpT

dy

photon  RAA=1  :  not  modified  

   -­‐>  Emi`ed  from  ini9al  hard  sca`ering  is  dominant.  RAA<<1  :  There  are  other  photon  sources  which  is  not  in  p+p  collisions  

   -­‐>  radiated  from  hot  medium??  

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6

The  pT  spectra  from  p+p  data  is  fi`ed    and  extrapolated  below  2  GeV/c.        The  excess  of  pT  spectra  are  fi`ed  and    effec9ve  temperature  is  extracted.      It  is  about  240  MeV.  (TFO≈100MeV)  Photons  are  emi7ed  from  very  hot    medium  at  early  5me  of  collisions.

a(1 + p2T /b)c

Ae�pT /Teff

arXiv:1405.3940v1

Radiated  from  very  hot  medium

photon  vn(M.Sanshiro)

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-3 -2 -1 0 1 2 3

9000

10000

11000

7

Azimuthal  anisotropy  (Ellip5c  flow)

photon  vn(M.Sanshiro)

v2  

dφ(φ-­‐ΨR.P.)

Reac5on  Plane dN

d(��

R.P

.)

N0[1 + 2v2cos{2(�� R.P.)}+ · · · ]charged  par9cle  dφ  distribu9on

•  anisotropic  pressure  gradient  in  par9cipant    (Ini9al  geometry)  

•  QGP  expansion  (viscosity  (η/s))  •  par9cles  emission  (coalescence)    It  relates  par5cipant  ini5al  geometry  and  η/s  of  QGP.  

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photon  vn(M.Sanshiro) 8

Photon  emi^ng  angle  dependence  w.r.t.  R.P.

Parton  Photon      Angular  dependence  of  emission    Ini9al  hard  sca`ering  :  v2≈0  Medium  induced  :  v2≤0  Jet  fragmenta9on  :  v2≥0  Radia9on  from  medium  :  v2>0

Photon  v2  measurement  is  a  powerful  probe  to  constrain  the  photon    source.  

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photon  vn(M.Sanshiro) 9

P.R.L.  109,  122302(2012)

It  is  consistent  with  hard  photons  produced  in  the  ini9al  hard  collision    at  high  pT.  (RAA≈1)    The  strength  of  photon  v2  at  low  pT  is  comparable  to  that  of  hadron  v2.  

Very  large  direct  photon  v2

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photon  vn(M.Sanshiro) 10

Direct  photon  puzzle

Ellip5c  flow:  It  is  needed  enough  9me  to  get  large  collec9ve  flow.  Hadrons  are  emi`ed  from  QGP  at  freeze-­‐out,  when  it  is  late  state.  Photons  from  QGP  and  HG  are  dominant  at  low  pT  and  they  have    large  v2.  

-­‐>  Photons  are  emi`ed  at  late  state??    pT  spectra:  radia9on  from  QGP  and  HG  are  dominant  at  low  pT  emi`ed  from  very  hot  medium  (Teff≈240MeV)  at  early  9me      There  is  discrepancy.  There  is  no  model  to  explain  simultaneously  the  both  observable.  

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Ψ3

Ψ2

Ψn  :  Par9cipant  Plane

Third  order  azimuthal  anisotropy  (v3)

photon  vn(M.Sanshiro)

vn =< cos{n(�� n)} >

dN

d(�� n)= N0[1 + 2

1X

n=1

vncos{n(�� n)}]

v3  is  originated  from  fluctua9on  of  par9cipants.  The  higher  order  is  expected  to  be  more  sensi9ve  to  ini9al  geometry    and  η/s  of  QGP.  Ψ3  and  Ψ2(R.P.)  should  be  independent.  

11

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photon  vn(M.Sanshiro) 12

Why  v3  is  measuremed?

B

Strong  photon  v2  has  not  yet  been  understood.    Radial  flow  effect  :  Effec9ve  temperature  is  affected  by    radial  flow.  v2>0  :  v3>0    Strong  magne5c  field  :  Direc9on  of  magne9c  field  and  Ψ2(R.P.)    are  related.  v2>0  :  v3≈0      v3  measurement  could  provide  addi9onal    constrain  photon  produc9on  mechanism.  

P.R.C  89,  044910  (2014)

Effec5v

e  Tempe

rature

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photon  vn(M.Sanshiro) 13

Azimuthal  anisotropy  measurement CNT  |η|  <0.35

1.0<  |η|  <2.8

Reac9on  Plane  detector  (RxNP)  is  used  for    measuring  Event  Plane.  Photons  and  π0  are  detected  by  EMCal  in  CNT.

vn =< cos{n(�� n)} >

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14

1.  π0,  γinc.  vn  measurement          2.  γdec.  vn  es5ma5on  from  π0  vn    Meson  spectra  are  assumed  by  mT  scaling.  Meson  vn  are  assumed  by  the  number  of    cons9tuent  quark  (NCQ)  scaling.        3. γdir.  vn  calcula5on  Rγ  is  measured  by  external    photon  conversion  method.

⌫dir.n =R�⌫inc.n � ⌫dec.n

R� � 1

R� = Ninc./Ndec.

Analysis  flow

arXiv:1405.3940

NCQ  scaling

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(GeV/c) Tp0 2 4

0

0.05

0.1

0.15

(GeV/c) Tp0 2 4

0

0.05

0.1

0.15

photon  vn(M.Sanshiro) 15

π0  and  inclusive  photon  vn  resuluts

π0  and  inclusive  photon  v2  and  v3  are  measured.  Mesons  vn  are  es9mated  by  the  NCQ  scaling  from  π0  vn  results.

π0  

γinc.

v2 v3 0-­‐60%  centrality  AuAu  200GeV  E.P.  :  RxN(I+O)

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(GeV/c) T

p0 5 10 15-110

10

310

510

710

910

1110

(GeV/c) T

p0 5 10 15-410

-110

210

510

810

1110

(GeV/c) T

p0 5 10 15-410

-310

-210

-110

1

(GeV/c) T

p0 5 10 150

0.05

0.1

0.15

0.2

(GeV/c) T

p0 5 10 150

0.05

0.1

0.15

0.2

photon  vn(M.Sanshiro) 16

Hadronic  decay  photon The  pT  spectra  and  vn  are  es9mated  from  π.  

pT  spectra  :  mT  scaling  vn  :  quark  number  scaling  

 

π η ω

meson  pT  spectra γdec.  pT  spectra contribu9on  ra9o  (Ri)

meson  v2 γdec.  v2

ρ η’  all  γdec.

vdec.n =X

i

Rivdec.in

p0

T

=q

p2T,⇡

0 +M2meson

�M2⇡

0

mT  scaling      decay  photon  vn  

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(GeV/c) Tp0 2 4

0

0.05

0.1

0.15

(GeV/c) Tp0 2 4

0

0.05

0.1

0.15

photon  vn(M.Sanshiro) 17

Inclusive  and  decay  photon  vn  comparison

γinc.  

γdec.

⌫dir.n =R�⌫inc.n � ⌫dec.n

R� � 1

Direct  photon  vn  are  extracted  from  the  devia9on  between    inclusive  and  decay  photon  via  below  func9on.  

v2 v3 0-­‐60%  centrality  AuAu  200GeV  E.P.  :  RxN(I+O)

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(GeV/c) T

p0 2 4

3v

0

0.05

0.1 0-60(%)3 v0π

3 vinc.γ

E.P.:RxN(I+O)Au+Au 200GeV

(GeV/c) T

p0 2 4

3v

0

0.05

0.13 vdir.γ

photon  vn(M.Sanshiro) 18

The  magnitude  of  γdir.  v3  is  similar  to  π0,  a  similar  trend  as  a  seen  in    case  of  v2.  Photon  azimuthal  anisotropies  may  be  affected  by  expansion  of  QGP.  

The  result  of  direct  photon  v3

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photon  vn(M.Sanshiro) 19

(GeV/c) T

p0 2 4

3v

-0.1

0

0.1

0.23 vdir.γ

E.P. : RxN(I+O)

(GeV/c) Tp0 2 4

3v

-0.1

0

0.1

0.2 Au+Au200GeV

(GeV/c) T

p0 2 4

3v

-0.1

0

0.1

0.20-20(%) 20-40(%) 40-60(%)

η  range  of  RxN(I+O)  is  from  1.0  to  2.8.  Non-­‐zero,  posi9ve  v3  is  observed  in  all  centrality  bins.  No  strong  centrality  dependence:  similar  tendency  as  for  charged    hadrons  (P.R.L.  107,  252301  (2011))  and  π0.  

Centrality  dependence  of  direct  photon  v3

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photon  vn(M.Sanshiro) 20

(GeV/c) T

p0 2 4

3v

-0.1

0

0.1

0.23 vdir.γ 3 v0π

E.P. : RxN(I+O)

(GeV/c) Tp0 2 4

3v

-0.1

0

0.1

0.2 Au+Au200GeV

(GeV/c) T

p0 2 4

3v

-0.1

0

0.1

0.20-20(%) 20-40(%) 40-60(%)

The  centrality  (in)dependence  of  γdir.  v3  is  also  observed  for  π0  v3.  

γdir.  and  π0  v3  show  similar  trend

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photon  vn(M.Sanshiro) 21

SoY  photons  have  provided  many  interes9ng  physics.  There  is  the  direct  photon  puzzle,  and  it  has  not  yet  been  understood.    Direct  photon  v3  is  measured  in  several  centrality  bins.  It  is  observed  that  

γdir.  v3  is  non-­‐zero  and  posi9ve  the  strength  of  γdir.  v3  is  comparable  to  hadron  v3  

They  are  similar  trend  to  γdir.  v2.  don’t  have  strong  centrality  dependence  

It  is  similar  tendency  to  hadron  v3.    The  results  of  direct  photon  v3  could  provide  important  keys  for    understanding  photon  produc9on  mechanism.  

Summary

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photon  vn(M.Sanshiro) 22

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photon  vn(M.Sanshiro) 23

Event  Plane  correla5on P.R.L.  107,  252301  (2011)

Ψ2  and  Ψ3  are  uncorrelated.

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photon  vn(M.Sanshiro) 24

0.0

0.1

0.2

0.3

v 2

gdirect (calorimeter)gdirect (conversions)

Au+AupsNN = 200GeV

RXP(I+O)

0 1 2 3 40.00

0.05

0.10

0.15

v 3

0-20%

0 1 2 3 4pT [GeV/c]

20-40%

0 1 2 3 4

40-60%

The  calorimeter  and  conversion  photon  measurements  are    consistent  within  systema9c  uncertainty.  

Comparison  of  γdir.  vn  with  the  two  methods

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photon  vn(M.Sanshiro)

MHBD:  Real  track  Mvtx    :  Measured  track

MHB

D[GeV

]

Mvtx[GeV] 25

Published  Real  photons  in  EMCal  :  1  -­‐  20  GeV/c  

large  errors  at  low  pT  (resolu9on,  contamina9on)  Virtual  photons  from  e+e-­‐  :  1  -­‐  4  GeV/c    New  method  Real  photons  are  measured  by  e+e-­‐  pair    from  external  photon  conversion      at  the  HBD  readout  plane.  ü  less  hadron  contamina9on  ü  good  momentum  resolu9on  pT  range  :  0.4  ~  5GeV/c  Extended  to  lower  pT  low  sta5s5cs  

Photons  by  external  conversion

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1)  real  photon  converts  to  e+e-­‐  in  HBD  backplane  2)  default  assump9on:  track  come  from  the  vertex  3)  momentum  of  the  conversion  tracks  will  be              mis-­‐measured  (see  black  tracks)  4)  apparent  pair-­‐mass  (about  12MeV)  will  be  measured              for  phtons  5)  assume  the  same  tracks  originate  in  the  HBD  backplane  6)  re-­‐calculate  momentum  and  pair  mass  with  this            “alternate  tracking  model”  7)  for  true  converted  photons  Matm  will  be  around  zero  

Real  track  es5mated  track

MHB

D[GeV

]

26 Mvtx[GeV] photon  vn(M.Sanshiro)

External  conversion  photon

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photon  vn(M.Sanshiro) 27

(GeV/c) T

p0 2 4

3v

0

0.05

0.1

0-60(%) (RxN(I+O))3 vdir.γ

Au+Au200GeV

(GeV/c) T

p0 2 4

3v

0

0.05

0.1

0-60(%) (RxN(In)+MPC)3 vdir.γ

Au+Au200GeV

RxN(I+O)  :  1.0  <|η|<  2.8  RxN(In)+MPC  :  1.5  <|η|<  3.8    The  magnitude  of  v3  is  comparable.

Comparison  γdir.  v3

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28

π±  and  π0  pT  spectra  are  fi`ed  and  its  func9on  is  used  for  es9ma9ng    the  other  meson  pT  spectra  by  mT  scaling.  They  are  used  as  a  input.  

p0

T

=q

p2T,⇡

0 +M2meson

�M2⇡

0

Input  decay  photon  :  pT  spectra

photon  vn(M.Sanshiro)

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29

The  ra9o  of  Each  meson  pT  spectra  to  π0  pT  spectra  is  known    to  be  constant  at  high  pT.  

Input  decay  photon  :  pT  spectra

photon  vn(M.Sanshiro)

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10�5

10�4

10�3

10�2

10�1

100

101

12p

p Td2 N

dpT

dy[(

GeV

/c)�

2 ]

0-20%

(a) Linnyk et al.vHees et al.Shen et al. (KLN)Shen et al. (MCGlb)direct g

20-40%

Au+AupsNN = 200GeV

(b)

0 1 2 3 4

10�5

10�4

10�3

10�2

10�1

100

101

40-60%

(c)

1 2 3 4 5pT [GeV/c]

60-92%

(d)

Linnyk  et  al.:  PHSD  transport  model;    Linnyk,  Cassing,  Bratkovskaya,    P.R.C  89,  034908(2014)    vHees  et  al.:  Fireball  model;  van  Hees,    Gale,  Rapp;  P.R.C  84,  054906(2011)    Shen  et  al.:  Ohio  hydro  for  two    different  ini9al  condi9ons;  Shen,  Heinz,  Paquet,  Gale;  P.R.C  84,  064903(2014)    The  yield  itself  is  s9ll  not  perfectly        described.  

arXiv:1405.3940

30

Yield  :  data  vs  theories

photon  vn(M.Sanshiro)

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photon  vn(M.Sanshiro) 31

0 1 2 3 40.00

0.05

0.10

0.15

0.20

0.25

0.30

0.35

v 2

gdirect (conversions)gdirect (calorimeter)

vHess et al. (b)vHess et al. (a)Linnyk et al.

0 1 2 3 4pT [GeV/c]

0 1 2 3 4

van  Hees  et  al:  P.R.C  84,  054906  (2011)  Linnyk  et  al.:  PHSD  model,  private  communica9on  

0-­‐20% 20-­‐40% 40-­‐60%

Comparison  γdir.  v2  with  theore5cal  calcula5ons

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photon  vn(M.Sanshiro) 32

Iden5fied  charged  par5cle  vn n

V

[GeV/c]T

p0 1 2 3 4

0

0.05

0.1

0.15

0.2x5.0}2Φ{4v

0 1 2 3 4

0

0.05

0.1

0.15

0.2x1.5}4Φ{4v

0 1 2 3 4

0

0.05

0.1

0.15

0.2

PHENIX Preliminaryx1.5}3Φ{3v

0 1 2 3 4

0

0.05

0.1

0.15

0.2 -π+π -K+ K

p p

±π correlated sys. of T

:p

200 GeV Au+Au 0-50%}2Φ{2v

�� ��������������

It  is  observed  that    all  harmonics  have  mass  ordering  there  are  meson  and  baryon  spliyng

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photon  vn(M.Sanshiro) 33

n/2

q/n n

V

[GeV]q/nTKE0 0.5 1 1.5 2-0.02

0

0.02

0.04

0.06

0.08

0.1 x154/2q/n}2Φ{4v

0 0.5 1 1.5 2-0.02

0

0.02

0.04

0.06

0.08

0.1 x4.04/2q/n}4Φ{4v

0 0.5 1 1.5 2-0.02

0

0.02

0.04

0.06

0.08

0.1PHENIX Preliminary

x2.53/2q/n}3Φ{3v

0 0.5 1 1.5 2-0.02

0

0.02

0.04

0.06

0.08

0.1-π+π

-K+ Kp p

±π correlated sys. of T:KE

200 GeV Au+Au 0-50%2/2q/n}2Φ{2v

�� ��������������

The  number  of  cons5tuent  quark  scaling  (NCQ  scale)

(a)  :  v2(KET)/nq  (b)  :  vn1/n  scaling  (a)+(b)  :  vn(KET)/nqn/2

All  par9cles  are  scaled  by  modified  NCQ    scaling.  

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photon  vn(M.Sanshiro) 34

π0  and  γdir.  v2  measurement  by  STAR

γdir.  v2  in  high  ET  region  are  consistent  with  0  within  systema9c    uncertainty,  while  π0  has  posi9ve  v2.  

Ahmed  M.  Hamed    shown  at  QM

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photon  vn(M.Sanshiro) 35

photon  vn  measurement  by  ALICE

v2

It  is  also  observed  that  γdir.  v2  is  posi9ve  in  low  pT  at  LHC-­‐ALICE.  v3  measurement  is  ongoing.

v3 γdec.  v3  γinc.  v3

arXiv:1212.3995v2 Friederike  shown  at  QM