CMS-PAS-HIN-16-015 | ||
Measurement of ψ(2S) production in proton-lead and proton-proton collisions at √sNN= 5.02 TeV | ||
CMS Collaboration | ||
February 2017 | ||
Abstract: This note reports the measurement of prompt ψ(2S) production in proton-lead (pPb) and proton-proton (pp) collisions at √sNN= 5.02 TeV. The results are based on pPb and pp data samples collected by CMS at the LHC corresponding to an integrated luminosity of 34.6 nb−1 and 28.0 pb−1 respectively. The nuclear modification factor, RpPb, is calculated for prompt ψ(2S) in the kinematic interval 4 <pT< 30 GeV/c and −2.4<yCM<1.93, and compared to the RpPb of prompt J/ψ. The RpPb of the excited state is found to be smaller than the RpPb of the ground state, over the whole kinematic range studied. The suppression is more pronounced in the region of negative rapidity and pT< 10 GeV/c. | ||
Links:
CDS record (PDF) ;
inSPIRE record ;
CADI line (restricted) ;
These preliminary results are superseded in this paper, PLB 790 (2019) 509. The superseded preliminary plots can be found here. |
Figures | |
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Figure 1:
(Left) Fit of the dimuon mass distribution both to the J/ψ and ψ(2S) peaks of the pPb data in the kinematical bin −2.4<yCM<−1.93 and 4 <pT< 6.5 GeV/c. The signal is fitted with Crystal Ball and Gaussian functions and background is described with a Chebyshev polynomial of degree 3. (Right) Fit of the dimuon mass distribution both to the J/ψ and ψ(2S) peaks of the pPb data in the kinematical bin 0 <yCM< 0.9 and 10 <pT< 30 GeV/c. The signal is fitted with Crystal Ball and Gaussian functions and background is described with a Chebyshev polynomial of degree 3. |
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Figure 1-a:
Fit of the dimuon mass distribution both to the J/ψ and ψ(2S) peaks of the pPb data in the kinematical bin −2.4<yCM<−1.93 and 4 <pT< 6.5 GeV/c. The signal is fitted with Crystal Ball and Gaussian functions and background is described with a Chebyshev polynomial of degree 3. |
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Figure 1-b:
Fit of the dimuon mass distribution both to the J/ψ and ψ(2S) peaks of the pPb data in the kinematical bin 0 <yCM< 0.9 and 10 <pT< 30 GeV/c. The signal is fitted with Crystal Ball and Gaussian functions and background is described with a Chebyshev polynomial of degree 3. |
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Figure 2:
Rapidity dependence of RpPb for prompt ψ(2S) in three pT ranges. The error bars represent the statistical uncertainties, and the boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb= 1. |
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Figure 2-a:
Rapidity dependence of RpPb for prompt ψ(2S) in the 4 <pT< 6.5 GeV/c range. The error bars represent the statistical uncertainties, and the boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb= 1. |
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Figure 2-b:
Rapidity dependence of RpPb for prompt ψ(2S) in the 6.6 <pT< 10 GeV/c range. The error bars represent the statistical uncertainties, and the boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb= 1. |
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Figure 2-c:
Rapidity dependence of RpPb for prompt ψ(2S) in the 10 <pT< 30 GeV/c range. The error bars represent the statistical uncertainties, and the boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb= 1. |
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Figure 3:
Transverse momentum pT dependence of RpPb for prompt ψ(2S) in four rapidity ranges. The error bars represent the statistical uncertainties, and the shaded boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb = 1. |
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Figure 3-a:
Transverse momentum pT dependence of RpPb for prompt ψ(2S) in rapidity range −2.4<yCM<−1.93. The error bars represent the statistical uncertainties, and the shaded boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb = 1. |
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Figure 3-b:
Transverse momentum pT dependence of RpPb for prompt ψ(2S) in rapidity ranges −1.93<yCM<−1.5 and 1.5<yCM<1.93. The error bars represent the statistical uncertainties, and the shaded boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb = 1. |
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Figure 3-c:
Transverse momentum pT dependence of RpPb for prompt ψ(2S) in rapidity ranges −1.5<yCM<−0.9 and 0.9<yCM<1.5. The error bars represent the statistical uncertainties, and the shaded boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb = 1. |
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Figure 3-d:
Transverse momentum pT dependence of RpPb for prompt ψ(2S) in rapidity ranges −0.9<yCM<0 and 0<yCM<0.9. The error bars represent the statistical uncertainties, and the shaded boxes show the quadratic sum of systematic uncertainties. The fully correlated global uncertainty of 4.2% is displayed as a grey box arround RpPb = 1. |
Summary |
The pPb and pp collision data at √sNN= 5.02 TeV taken by the CMS detector are used to investigate the production of prompt ψ(2S). The results are based on pPb and pp data samples collected by CMS at the LHC corresponding to an integrated luminosity of 34.6 nb−1 and 28.0 pb−1 respectively. The nuclear modification factor of prompt ψ(2S) is determined in the kinematic interval 4 <pT< 30 GeV/c and −2.4<yCM< 1.93, and compared to the RpPb of prompt J/ψ. The suppression is more pronounced in the region of negative rapidity and at pT< 10 GeV/c. The RpPb of ψ(2S) is also found to be smaller to that of the J/ψ measured in Ref. [18], over the whole kinematic range studied. The different nuclear dependence of J/ψ and ψ(2S) reported here cannot be attributed to nPDF or coherent energy loss effects which predict a similar suppression in both channels. It may however be consistent with the picture of final state inelastic interaction of ψ(2S) mesons in the medium produced in pPb collisions at √sNN= 5 TeV. |
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Compact Muon Solenoid LHC, CERN |
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