Measurement of global spin alignment of K* and φ vector ...K*0 and φ Subhash Singha, QM 2019 5 •...
Transcript of Measurement of global spin alignment of K* and φ vector ...K*0 and φ Subhash Singha, QM 2019 5 •...
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Measurement of global spin alignment of K*0 and φ vector mesons using the STAR detector at RHIC
Subhash SinghaInstitute of Modern Physics Chinese Academy of Sciences, Lanzhou
and Kent State University, Ohio(For the STAR Collaboration)
This work in part supported by grant from DOE Office of Science
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Outline
•Motivation
•Analysis method
•Results:
Spin alignment of K*0 Comparison with φ meson (QM 2018) Comparison with ALICE results
•Summary and outlook
Subhash Singha, QM 2019
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Probe initial stages in HIC
• Initial large angular momentum (L) ~ 104 h
• Initial large magnetic field (B) ~ 1018 Gauss at RHIC
• Can polarize quarks in medium
F. Becattini, et. al., Phys Rev. C. 77, 024906 (2008) D. Kharzeev, Nucl Phys A803, 227 (2008)
Subhash Singha, QM 2019
Angular momentum Magnetic field
Nature 548, 62 (2017) (STAR Collaboration) Phys Rev C 98, 14910 (2018) (STAR Collaboration)Λ Polarization
• PH(Λ) & PH(Λ) > 0
• PH(Λ) > PH(Λ)
Positive vorticity
Hints of magnetic coupling
‣ First experimental access to study the vorticity of the medium
See talk by J. Adams 06/11, 2.00 pm
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Vector meson spin alignment (ρ00)
Subhash Singha, QM 2019
Z. Liang et. al., Phys. Lett. B629, 20 (2005) Y. Yang et. al., Phys. Rev. C 97, 034917 (2018)
dNd(cosθ*)
= N0 × [(1 − ρ00) + (3ρ00 − 1) cos2θ*)]
Observable
nRP
z
K*0
θ*
K+
π-
>
Reac
tion
Plan
e
‣ Deviation of ρ00 from (1/3) indicates spin alignment
K. Schiling et. al., Nucl. Phys. B 15 (1970) 397 Phys. Rev. C 77 (2008) 61902 (STAR Collaboration)
*θcos 1− 0.5− 0 0.5 1
(arb
uni
ts)
*θdc
osdN
0.5
0.6
0.7
Qualitative plot = 1/3
00ρ
= 0.2700ρ
Theoretical expectation of ρ00
Vorticity
Magnetic field
Hadronization
ρ00(ω) < 1/3
ρ00(B) > 1/3
ρ00(B) < 1/3
ρ00(rec) < 1/3
ρ00(frag) > 1/3
Electrically neutral vector mesonsElectrically charged vector mesons
Recombination
Fragmentation
Angular momentum and magnetic field can induce spin alignment of vector mesons
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K*0 and φ
5Subhash Singha, QM 2019
• Predominantly produced in primordial production• Negligible feed-down compared to Λ and Λ
• Λ spin polarization (PH): Required knowledge of orientation of the angular momentum vector, estimated by deflection of spectators (can use 1st-order event plane)
• Vector meson spin alignment (ρ00): Polarization direction not required. Not subject to local cancellation. (can use both 1st-order and 2nd-order event plane)
Characteristic of K*0 and φ:
Species K*0 φ
Quark content ds ss
Mass (MeV/c2) 896 1020Lifetime (fm/c) 4 45
Spin (JP) 1- 1-
Decays Kπ KK
Branching ratio 49% 66%
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The STAR detector and analysis details
6Subhash Singha, QM 2019
• Uniform acceptance, full azimuthal coverage• TPC: tracking, centrality and event plane• TPC+TOF: particle identification
collision system Au+Au
collision energy 54.4 and 200 GeV
# of good events 520 and 350 M
rapidity |y| < 0.5
background rotation of daughters
polarization axis perpendicular to TPC 2nd-order event plane
consistency check 3D-random event plane
Report K*0 ρ00 as function of transverse momentum and centrality
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)2 K (GeV/cπinvariant mass 0.75 0.8 0.85 0.9 0.95 1 1.05
Cou
nts
500
1000
1500
2000
310×
Au+Au 200 GeV, 10-60%DataBW functionResidual bkg function
2 0.2 MeV/c±mass = 891.0 2 0.7 MeV/c±width = 48.2
S/B = 0.0012
STAR Preliminary
* < 0.6θ < 2.0 GeV/c, 0.4 < cos T
1.5 < p
The STAR detector and signal reconstructionK*0 reconstruction:
7Subhash Singha, QM 2019
K*0 Kπ
•Rotational background subtraction•mass/width consistent with
published value• K* yield is the area under the Breit-
Wigner function
• Uniform acceptance, full azimuthal coverage• TPC: tracking, centrality and event plane• TPC+TOF: particle identification
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8Subhash Singha, QM 2019
Analysis method• Raw yield of K*0 is extracted from 5 cos θ* bins
nRP
z
K*0
θ*
K+
π-
>
Reac
tion
Plan
e
• Here polarization axis (nRP) is the direction perpendicular to the TPC 2nd-order event plane (Ψ2)
• θ* is the angle between the daughter (K+) momentum of K*0 in its rest frame and nRP
<
<
*θcos 0.0 0.2 0.4 0.6 0.8 1.0
*θd
cos ra
wdN
ev
ent
N1
31
32
33
34
35
3−10×
< 2.0 GeV/cT
Au+Au 200 GeV, 10-60%, 1.5 < p
Data
STAR Preliminary
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*θcos 0.0 0.2 0.4 0.6 0.8 1.0
*θd
cos co
rrdN
ev
ent
N1
55
60
65
3−10×
< 2.0 GeV/cT
Au+Au 200 GeV, 10-60%, 1.5 < pData
*)]θ(2 - 1) Cosobs00ρ) + (3 obs
00ρ[(1-
0p
STAR Preliminary
9Subhash Singha, QM 2019
Analysis method• Yield of K*0 is corrected for efficiency and acceptance
• Observed ρ00obs is calculated from fitting the yield with function:
• Observed ρ00obs is corrected for TPC event plane resolution (R)
ρ00 −13
=4
1 + 3R(ρobs
00 −13
)
A. Tang et. al., Phys Rev C 98, 044907 (2018)
dNd(cosθ*)
= N0 × [(1 − ρobs00 ) + (3ρobs
00 − 1) cos2θ*)]
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(GeV/c)T
p1 2 3 4 5
00ρ *0 K
0.25
0.30
0.35
0.40Au+Au 200 GeV, 10-60%STAR Preliminary
-sub event, TPC-EPηfull event, TPC-EP3D-random
(GeV/c)T
p1 2 3 4 5
00ρ *0 K
0.25
0.30
0.35
0.40Au+Au 54.4 GeV, 10-60%STAR Preliminary
-sub event, TPC-EPηfull event, TPC-EP3D-random
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K*0 ρ00 (pT)
• Significant deviation of ρ00 from 1/3 is observed at low pT for both 54.4 and 200 GeV• ρ00 from TPC η-sub and full event plane are consistent despite of different event
plane resolutions
Subhash Singha, QM 2019
• ρ00 results from 3D-random plane consistent with 1/3 as expected
For Au+Au 200 GeV, 10-60% centrality:TPC (Ψ2) resolution ~ 0.55 for η-sub event planeTPC (Ψ2) resolution ~ 0.77 for full event plane
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(GeV/c)T
p1 2 3 4 5
00ρ *0 K
0.25
0.30
0.35
0.40Au+Au, 10-60%
54.4 GeV200 GeV
STAR Preliminary
(GeV/c)T
p0 1 2 3 4 5
00ρ φ
0.25
0.30
0.35
0.40Au+Au 200 GeV, 20-60%
TPC EPZDC EP
STAR Preliminary
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ρ00 (pT): K*0 vs. φ
• Νοn-trivial and opposite pT dependence observed for K*0 and φ
Subhash Singha, QM 2019
Κ*0 φA
QM 2018
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(GeV/c)T
p1 2 3 4 5
00ρ *0 K
0.25
0.30
0.35
0.40Au+Au, 10-60%
54.4 GeV200 GeV
STAR Preliminary
(GeV/c)T
p0 1 2 3 4 5
00ρ φ
0.25
0.30
0.35
0.40Au+Au 200 GeV, 20-60%
TPC EPZDC EP
STAR Preliminary
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ρ00 (pT): K*0 vs. φ
• Trend for K*0 ρ00 is qualitatively consistent with the naive expectation from recombination/fragmentation of polarized quarks [1] but the magnitude is much larger
• φ ρ00 does not fit into naive recombination/fragmentation picture [1]• But it can be explained by the existence of coherent φ meson field [2]
Subhash Singha, QM 2019
[1] Z. Liang et. al., Phys. Lett. B629, 20 (2005) [2] X. Sheng et. al., arXiv:1910.13684 (2019)
QM 2018 Κ*0 φ
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〉 part N〈0 100 200 300
00ρ *0 K
0.25
0.30
0.35
0.40 < 1.5 GeV/c
TAu+Au, 1.0 < p 54.4 GeV
200 GeV
STAR Preliminary TPC-EP
13Subhash Singha, QM 2019
K*0 ρ00 (centrality)
• For peripheral collisions ρ00 ~ 1/3• For midcentral collisions ρ00 < 1/3 • For central collisions ρ00 close to 1/3
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〉 part N〈0 100 200 300
00ρ *0 K
0.25
0.30
0.35
0.40 < 1.5 GeV/c
TAu+Au, 1.0 < p 54.4 GeV
200 GeV
STAR Preliminary TPC-EP
14Subhash Singha, QM 2019
K*0 ρ00 (centrality)
• For peripheral collisions ρ00 ~ 1/3• For midcentral collisions ρ00 < 1/3 • For central collisions ρ00 close to 1/3• Trend similar to angular momentum vs. centrality
Angular momentum vs. impact parameter
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〉 part N〈0 100 200 300 400
00ρ φ
0.30
0.32
0.34
0.36
< 5.4 GeV/cT
Au+Au 200 GeV, 1.2 < pZDC EP
STAR Preliminary
〉 part N〈0 100 200 300
00ρ *0 K
0.25
0.30
0.35
0.40 < 1.5 GeV/c
TAu+Au, 1.0 < p 54.4 GeV
200 GeV
STAR Preliminary TPC-EP
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ρ00 (centrality): K*0 vs. φ
Subhash Singha, QM 2019
QM 2018 Κ*0 φ
Mesons
τ(fm/c)Φ 45K*0 4
• K*0 ρ00 < 1/3 • φ ρ00 > 1/3 • For midcentral collisions
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(GeV/c)T
p1 2 3 4 5
00ρ *0 K
0.15
0.20
0.25
0.30
0.35
0.40
ALICE, Pb+Pb, 10-50%
2.76 TeV
Au+Au, 10-60%54.4 GeV200 GeV
STAR Preliminary
〉 part N〈0 100 200 300 400
00ρ *0 K
0.1
0.2
0.3
0.4
< 1.2 GeV/cT
ALICE, 0.8 < pPb+Pb 2.76 TeV
< 1.5 GeV/cT
Au+Au, 1.0 < p54.4 GeV200 GeV
STAR Preliminary
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K*0 ρ00 : RHIC vs. LHC
•pT and centrality dependence of ρ00 at RHIC is similar to LHC energies but with much better precision
•At low pT and midcentral collisions hint that LHC measurements are lower than RHIC by 1-1.5σ
Subhash Singha, QM 2019 arXiv: 1910.14408 (2019) (ALICE Collaboration)
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Summary of ρ00/PH measurements from RHIC and LHC
Subhash Singha, QM 2019
Species Quark content JP ρ00/PH at top-RHIC ρ00/PH at LHC
K*0 ds 1- ρ00 < 1/3 (~4σ ) ρ00 < 1/3 (~3σ )
φ ss 1- ρ00 > 1/3 (~3σ ) ρ00 < 1/3 (~2σ )
Λ uds 1/2+ PH > 0 (~4σ ) PH ~ 0 (~1σ )
For midcentral collisions
• From current theoretical understanding PH Pq, while ρ00 Pq2• Given the small PH values observed at top RHIC and LHC energies, ρ00 expected to
be close to 1/3• Hence, the current ρ00 measurements are surprising!
• ρ00 can depend on hadronization, vorticity, electromagnetic and mesonic field• More theoretical input is needed to understand the data Z. Liang et. al., Phys. Lett. B629, 20 (2005)
Y. Yang et. al., Phys. Rev. C 97, 034917 (2018) X. Sheng et. al., arXiv:1910.13684 (2019)
∝ ∝ Pq: quark polarization
Nature 548, 62 (2017) (STAR Collaboration) Phys Rev C 98, 14910 (2018) (STAR Collaboration) arXiv: 1909.01281 (2019) (ALICE Collaboration) arXiv: 1910.14408 (2019) (ALICE Collaboration)
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•We presented pT and centrality dependence of ρ00 of neutral K* from 54.4 GeV and 200 GeV.
• K*0 ρ00 < 1/3 is observed for both 54.4 and 200 GeV
• Observation of K*0 spin alignment at RHIC energies
• pT and centrality dependence of ρ00 similar between RHIC and LHC
Summary
Subhash Singha, QM 2019
〉 part N〈0 50 100 150 200 250 300 350
00ρ *0 K
0.25
0.30
0.35
0.40 < 1.5 GeV/c
TAu+Au 54.4 GeV, 1.0 < p
54.4 GeV200 GeV
STAR Preliminary
• For midcentral collisions, ρ00 (K*0) < 1/3, while ρ00 (φ) > 1/3• Need quantitative estimation from models to better
understand the data
(GeV/c)T
p1 2 3 4 5
00ρ *0 K
0.25
0.30
0.35
0.40Au+Au, 10-60%
54.4 GeV200 GeV
STAR Preliminary
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OutlookFor Au+Au 200 GeV data:• STAR has collected more than 2 B events during 2014,
2016 and 2018. We expect to reach better statistical precision• Analysis of charged K* ρ00 with high statistics 200 GeV
data is underway
Subhash Singha, QM 2019
GeVNNs10 210
00ρ *0 K
0.1
0.2
0.3
0.4
< 5.0 GeV/c T
Au+Au, Centrality: 20-60 %, 1.2 < pSTAR Preliminary
Energy (GeV) # events (M)7.7 1009.1 16011.5 20014.5 32019.6 58027 500
(BES-II)
For lower energy Au+Au data (< 39 GeV):•High statistics and detector upgrades in 2nd phase of BES
will improve precision of vector meson ρ00 measurements
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20Subhash Singha, QM 2019
Thank you
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Backup slides
Subhash Singha, QM 2019
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)2 K (GeV/cπinvariant mass 0.75 0.8 0.85 0.9 0.95 1 1.05
Cou
nts
500
1000
1500
2000
310×
Au+Au 200 GeV, 10-60%DataBW functionResidual bkg function
2 0.2 MeV/c±mass = 891.0 2 0.7 MeV/c±width = 48.2
S/B = 0.0012
STAR Preliminary
* < 0.6θ < 2.0 GeV/c, 0.4 < cos T
1.5 < p
)2 K (GeV/cπinvariant mass 0.6 0.7 0.8 0.9 1.0 1.1 1.2 1.3 1.4 1.5
Cou
nts
0.05
0.10
0.15
0.20
910×
Au+Au 200 GeV, 10-60% K pairπSame event
K pairπRotated event
STAR Preliminary
* < 0.6θ < 2.0 GeV/c, 0.4 < cos T
1.5 < p
22
Invariant mass signal reconstruction
• K*0 signal is extracted by using rotational background subtraction method• Signal fitted with Breit Wigner function plus second order polynomial as residual
background• K*0 mass and width consistent with published values• K*0 yield is the area under the Breit Wigner function
Before background subtraction After background subtraction
Subhash Singha, QM 2019
Breit Wigner function
BW =1
2πAΓ
(m − m0)2 + (Γ/2)2 Κ*0 Κ*0
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Invariant mass signal reconstruction
•φ signal is extracted by using mixed event background subtraction method•Signal fitted with Breit Wigner function plus first order polynomial as residual
background• φ yield is the area under Breit Wigner function
Before background subtraction After background subtraction
Au+Au 200 GeV, centrality: 40-50%, pT: 1.2-1.8 GeV/c, cos θ*: 1/7- 2/7
φ meson
φ meson
Subhash Singha, QM 2019
BW =1
2πAΓ
(m − m0)2 + (Γ/2)2
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Centrality (%)0 10 20 30 40 50 60 70 80
-sub
EP
reso
lutio
nη
0
0.2
0.4
0.6
0.8
2ΨTPC event plane 54.4 GeV200 GeV
24
Event plane reconstruction
• Second order event plane (ψ2) is measured using TPC
Ψ2 =12
∑ wisin(nϕi)∑ wicos(nϕi)
Phys. Rev. C 58 (1998) 1671
Event plane from TPC:STAR Preliminary
Subhash Singha, QM 2019
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nRP
z
K*0
θ*
K+
π-
>
Reac
tion
Plan
e
Subhash Singha, QM 2019
Analysis method
• K*0 efficiency x acceptance (εrec) from embedding data
*θcos 0.0 0.2 0.4 0.6 0.8 1.0
)re
c∈
Acc
epta
nce
(×
Effic
ienc
y
0.2
0.4
0.6
0.8
< 2.0 GeV/cT
Au+Au 200 GeV, 10-60%, 1.5 < p
rec∈
STAR PreliminaryMC embedding
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〉 part N〈0 50 100 150 200 250 300 350
00ρ *0 K
0.15
0.20
0.25
0.30
0.35
0.40 < 1.5 GeV/c
TAu+Au 200 GeV, 1.0 < pSTAR Preliminary
-sub event, TPC-EPηfull event, TPC-EP3D-random
〉 part N〈0 50 100 150 200 250 300
00ρ *0 K
0.15
0.20
0.25
0.30
0.35
0.40 < 1.5 GeV/c
TAu+Au 54.4 GeV, 1.0 < pSTAR Preliminary
-sub event, TPC-EPηfull event, TPC-EP3D-random
26
K*0 ρ00 (centrality)
• Deviation of ρ00 from 1/3 is observed for mid-central collisions for both 54.4 and 200 GeV
• ρ00 results in peripheral collisions consistent with 1/3• ρ00 results from 3D random plane consistent with 1/3
Subhash Singha, QM 2019
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GeVNNs10 210
00ρ *0 K
0.1
0.2
0.3
0.4
< 5.0 GeV/c T
Au+Au, Centrality: 20-60 %, 1.2 < pSTAR Preliminary
27
Energy dependence of K*0 ρ00
• No beam energy dependence observed in ρ00 with current precision• High statistics data from STAR BES-II can improve precision in ρ00 measurements in lower
beam energiesSubhash Singha, QM 2019
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φ Κ*0
Results shown at QM 2018
• ρ00 (φ) > 1/3 for √sNN =39 and 200 GeV with >~ 3σ significance
• ρ00 (K*0) < 1/3 for √sNN = 11.5 - 39 GeV within ~ 1-2σ significance
High statistics data in 54.4 and 200 GeV allow precision measurement for centrality and transverse momentum dependence of ρ00 for K*0 and φ
Subhash Singha, QM 2019
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〉 part N〈0 100 200 300 400
00ρ *0 K
0.15
0.20
0.25
0.30
0.35
0.40
< 1.2 GeV/cT
ALICE Preliminary, 0.8 < pPb+Pb 2.76 TeV
< 1.5 GeV/cT
Au+Au, 1.0 < p54.4 GeV200 GeV
STAR Preliminary
(GeV/c)T
p0 1 2 3 4 5
00ρ *0 K
0.20
0.25
0.30
0.35
0.40
ALICE Preliminary, Pb+Pb, 10-50%2.76 TeV
Au+Au, 10-60%54.4 GeV200 GeV
STAR Preliminary
29
K*0 ρ00 (centrality): RHIC vs. LHC
Subhash Singha, QM 2019
In ALICE Preliminary results, EP resolution correction with “1/R” term as a correction
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〉 part N〈0 50 100 150 200 250 300 350
00ρ *0 K
0
0.1
0.2
0.3
0.4
0.5
0.6 < 1.5 GeV/c
TAu+Au, 1.0 < p
54.4 GeV200 GeV
STAR Preliminary
< 2.0 GeVT
Au+Au, p
200 GeV, PRC77
30
K*0 : comparison with published results
Subhash Singha, QM 2019
STAR(200 GeV) Published(Run-04) Preliminary(Run-11)
Event statistics 20 M 370 M
PID TPC only (poor S/B ratio) TPC+TOF
EP resolution correction
ρ00 −13
=4
1 + 3R (ρobs00 −
13 )1
R
• K*0 results are consistent with published results within 1-1.5σ considering systematic uncertainties
Phys. Rev. C 77 (2008) 61902 (STAR Collaboration)
A. Tang et. al., Phys. Rev. C 98 044907 (2018)
(GeV/c)T
p0 1 2 3 4 5
00ρ *0 K
0.1
0.2
0.3
0.4
0.5
0.6
0.7 Au+Au, 10-60%54.4 GeV200 GeV
STAR PreliminaryAu+Au, 20-60%200 GeV, PRC77