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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
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
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
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)
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??
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)
-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.
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.
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
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.
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
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
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)} >
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
(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)
(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
(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)
(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
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
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
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
photon vn(M.Sanshiro) 22
photon vn(M.Sanshiro) 23
Event Plane correla5on P.R.L. 107, 252301 (2011)
Ψ2 and Ψ3 are uncorrelated.
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
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
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
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
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)
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)
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)
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
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
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.
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
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