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核子あたり重心系衝突エネルギー 5.02 TeVでの陽子鉛衝突におけるJ /ψ生成

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論文の内容の要旨

J/ψ production in p-Pb collisions at√sN N = 5.02 TeV

(核子あたり重心系衝突エネルギー5.02 TeVでの陽子鉛衝突におけるJ/ψ生成)

氏 名  林 真一

Quantum Chromodynamics predicts quark deconfinement and the transition to strongly interacting matter, quark-gluon plasma (QGP), at extremely high temperature and density. Relativistic heavy ion collisions are an unique tool to study the properties of QGP. Since the yield of J/ψ is expected to decrease in QGP due to Debye screening of color charges, J/ψ suppression is one of the strong signatures of QGP formation [1]. PHENIX experiment at the Relativistic Heavy Ion Collider (RHIC) in the Brookhaven National Laboratory (BNL) observed strong suppression of J/ψ production in Au–Au collisions at √sN N = 200 GeV [2]. The J/ψ yields measured by the ALICE experiment at the Large Hadron Collider (LHC) in the European Organization for Nuclear Research (CERN) were also suppressed in Pb–Pb collisions at√sN N = 2.76 TeV. In addition, non-negligible suppression of the J/ψ yield was observed in d–Au collisions at√sN N = 200 GeV at RHIC. Suppression in d–Au collisions is thought as normal nuclear matter effects such as gluon shadowing and nuclear absorption. The understanding of normal nuclear matter effects in heavy ion collisions is essential in the discussion of the QGP effects.

This thesis presents the measurement of inclusive J/ψ production in minimum bias p–Pb collisions at

s

N N = 5.02 TeV at mid-rapidity (−1.37 < y < 0.43) with the ALICE central barrel detectors. The main aim of this analysis is the investigation of normal nuclear matter effects in relativistic heavy ion collisions.

J/ψ is detected via dielectron decay channels by calculating their invariant mass. In the ALICE central

barrel, electrons are reconstructed using the Inner Tracking System (ITS) and the Time Projection Chamber (TPC) in |η| < 0.9. Figure 1 shows the pT-integrated invariant mass spectra of unlike-sign,

expected background, and background subtracted pairs. Since the main source of the background is combinatorial pairs, event mixing technique is used to estimate the shapes of the background.

The measured production cross section of inclusive J/ψ in p–Pb collisions at √sN N = 5.02 TeV at mid-rapidity (−1.37 < y < 0.43) is determined by

dσJ/ψ

dy = 930 ± 83 (stat) ± 74 (syst) µb. (1)

In order to investigate nuclear matter effects in p-Pb collisions, the nuclear modification factor (RpPb)

is introduced. It is defined as RpPb= YpPb ⟨Ncoll⟩Ypp , (2) 1

CORE Metadata, citation and similar papers at core.ac.uk

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) 2 c (GeV/ ee m 2.2 2.4 2.6 2.8 3 3.2 3.4 3.6 3.8 4 2 c

Counts per 40 MeV/

0 50 100 150 200 250 300 ULS pairs Mix BG pairs BG subtracted pairs Signal shape fit (MC)

/NDF: 38.5/48 2 χ =5.02 TeV NN s p-Pb at This Work

Fig.1 Invariant mass distribution of unlike-sign, mixing background, and background subtracted

pairs in p-Pb collisions. The solid red line shows the result of the fitting to the subtracted signal.

where YpPb, Ypp are the invariant yield of J/ψ in pp and p–Pb collisions, respectively. ⟨Ncoll⟩ is the average number of binary nucleon-nucleon collisions in p–Pb collisions. In this analysis, the J/ψ yield in pp collisions at√s = 5.02 TeV is estimated by interpolation from the measured pp spectra [6]. RpPb of

inclusive J/ψ production at mid-rapidity (-1.37 < y < 0.43) is extracted as

RpPb= 0.74 ± 0.07 (stat) ± 0.13 (syst). (3)

Compared with RpPb at forward rapidity via the dimuon decay measurements, the magnitude of RpPb

at mid-rapidity is compatible within the uncertainties.

CMS y -4 -3 -2 -1 0 1 2 3 4 pPb R 0.4 0.6 0.8 1 1.2 1.4 -1 b µ = 53 int L < 0.43, CMS : -1.37 < y -e + e → ψ J/ , -1 = 5.8 n b int L < -2.96, CMS : -4.46 < y + µ → ψ J/ -1 = 5.0 n b int L < 3, CMS : 2.03 < y + µ → ψ J/ This Work =5.02 TeV NN s p-Pb at Grobal Uncertainty: 3.4%

EPS09 NLO + CEM (Vogt) EPS09 LO (Ferreiro) = 1.5 mb (Ferreiro) abs σ EPS09 LO + = 2.8 mb (Ferreiro) abs σ EPS09 LO + CMS y -4 -3 -2 -1 0 1 2 3 4 pPb R 0.4 0.6 0.8 1 1.2 1.4 -1 b µ = 53 int L < 0.43, CMS : -1.37 < y -e + e → ψ J/ , -1 = 5.8 n b int L < -2.96, CMS : -4.46 < y + µ → ψ J/ -1 = 5.0 n b int L < 3, CMS : 2.03 < y + µ → ψ J/ This Work =5.02 TeV NN s p-Pb at Grobal Uncertainty: 3.4% /fm (Arleo et al) 2 =0.075 GeV 0 ELoss, q /fm (Arleo et al) 2 =0.055 GeV 0 EPS09 NLO + ELoss, q

Fig.2 Comparison of the rapidity y dependence of the data to the gluon shadowing models (Left)

and the coherent energy loss model (Right) in p–Pb collisions at√sN N = 5.02 TeV [8, 9].

The left panel of Fig. 2 shows the comparison of the y dependence of RpPb with the shadowing model

calculations [8–10]. At mid-rapidity, both EPS09 NLO and LO calculations are consistent with the experimental results within the uncertainties. The right panel of Fig. 2 shows the comparison of the y dependence of RpPb with the coherent energy loss model calculation [10]. Coherent energy loss model

with typical transport coefficient ˆq shows a reasonable description of the y dependence of the measured

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RpPb. Figure 3 shows the comparison of the pTdependence between the measured RpPb and the model

calculations [10, 11]. The coherent energy loss model shows the reasonable description of both y and pT

dependence of the data. However, the uncertainties of data and model calculations are still large. The further reduction of the uncertainties is needed to obtain the conclusive explanation of normal nuclear matter effects in heavy ion collisions at LHC.

(GeV/c) T p 0 1 2 3 4 5 6 7 8 9 10 pPb R 0 0.2 0.4 0.6 0.8 1 1.2 1.4 =5.02 TeV NN s p-Pb at -1 b µ = 53 int L < 0.43, CMS : -1.37 < y -e + e → ψ J/

Gluon Saturation (Fujii, Watanabe) /fm (Arbelt et.al.) 2 =0.055 GeV q EPS09+ELoss with /fm (Arbelt et.al.) 2 =0.075 GeV q ELoss with This Work

Fig.3 Comparison of the pT dependence between the measured RpPb and the model calculations

in p–Pb collisions at √sN N = 5.02 TeV. The violet, green, and magenta bands show the

calcu-lation based on gluon saturation with CGC framework, coherent energy loss with EPS09 nPDF parametrization, and coherent energy loss with the proton PDF parametrization [10, 11].

(GeV/c) T p 0 1 2 3 4 5 6 7 8 9 10 AA , R 2) pPb (R 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 =5.02 TeV, MB, -1.37 < y < 0.43 NN s , p-Pb pPb ALICE R =2.76 TeV, 0-50%, |y| < 0.8 NN s , Pb-Pb AA ALICE R =2.76 TeV, 0-100%, |y| < 2.4 NN s , Pb-Pb AA CMS R This Work (GeV/c) T p 0 1 2 3 4 5 6 7 8 9 10 AA S 0 0.5 1 1.5 2 2.5 : 0-50%, |y| < 0.8 AA S ALICE : 0-100%, |y| < 2.4 AA S CMS This Work )) 2 pPb R /( AA R ( AA S =2.76 TeV, NN s Pb-Pb

Fig.4 Comparison of RAA and (RpPb)2 in ALICE and CMS (Left) and surviving fraction (SAA)

(Right) of J/ψ production in Pb–Pb collision.

Under the assumption that the shadowing effect is dominant compared to other normal nuclear matter effects, normal nuclear matter effects in RAA is approximated by the convolution of RpPb [7]. Figure 4

shows the inclusive J/ψ RAA in Pb-Pb collisions at √sN N =2.76 TeV in 0–50% centrality and the product of inclusive J/ψ RpPb and surviving fraction (SAA) defined as

SAA=

RAA

RpA(−y) × RpA(y)

. (4)

Compared between (RpPb)2 at√sN N = 5.02 TeV and RAA in Pb–Pb collisions at√sN N = 2.76 TeV, the suppression is seen at high pT above 4.5 GeV/c. This suppression is qualitatively consistent with

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the color screening pictures. On the other hand, the enhancement of the J/ψ yield is observed at lower

pT, which is due to the regeneration of J/ψ in Pb–Pb collisions [12].

参考文献

[1] T. Matsui and H. Satz, Phys. Lett. B 178 416 (1986). [2] A. Adare et al, Phys. Rev. Lett. 98 232301 (2007). [3] A. Andronic, arXiv:1409.5778 (2015).

[4] A. Adare et al, Phys. Rev. Lett. 107 142301 (2011).

[5] N. Brambilla et al, Eur. Phys. J. C 71 1534, arXiv:1010.5827 (2011). [6] F.Bossu et al, arXiv:1103.2394 (2011).

[7] E.Ferreiro, et al, Phys. Lett. B680 50-55, arXiv:0809.4684 (2009), T. Gunji, Phys. Rev. C 76 051901 (2007).

[8] R. Vogt, Phys. Rev. C 81 044903 (2010).

[9] E. Ferreiro et al, Phys. Rev., C 88 4 047901 (2013).

[10] F. Arleo et.al, JHEP03 122, JHEP05 155, arXiv:1212.0434 (2013).

[11] H. Fujii and K. Watanabe, J. Nucl. Phys. A. 2013 06 011, arXiv:1304.2221 (2013). [12] Zhou et al, Phys. Rev. C 89 054911 (2014)

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