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Measurement of KS0 and K*0 in p+p,d+Au, and Cu + Cu collisions at sNN=200 GeV

A. Adare et al. (PHENIX Collaboration)
Phys. Rev. C 90, 054905 – Published 7 November 2014

Abstract

The PHENIX experiment at the Relativistic Heavy Ion Collider has performed a systematic study of KS0 and K*0 meson production at midrapidity in p+p,d+Au, and Cu+Cu collisions at sNN=200 GeV. The KS0 and K*0 mesons are reconstructed via their KS0π0(γγ)π0(γγ) and K*0K±π decay modes, respectively. The measured transverse-momentum spectra are used to determine the nuclear modification factor of KS0 and K*0 mesons in d+Au and Cu+Cu collisions at different centralities. In the d+Au collisions, the nuclear modification factor of KS0 and K*0 mesons is almost constant as a function of transverse momentum and is consistent with unity, showing that cold-nuclear-matter effects do not play a significant role in the measured kinematic range. In Cu+Cu collisions, within the uncertainties no nuclear modification is registered in peripheral collisions. In central collisions, both mesons show suppression relative to the expectations from the p+p yield scaled by the number of binary nucleon-nucleon collisions in the Cu+Cu system. In the pT range 25 GeV/c, the strange mesons (KS0,K*0) similarly to the ϕ meson with hidden strangeness, show an intermediate suppression between the more suppressed light quark mesons (π0) and the nonsuppressed baryons (p,p¯). At higher transverse momentum, pT>5 GeV/c, production of all particles is similarly suppressed by a factor of 2.

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  • Received 23 May 2014

DOI:https://doi.org/10.1103/PhysRevC.90.054905

©2014 American Physical Society

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Vol. 90, Iss. 5 — November 2014

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Images

  • Figure 1
    Figure 1

    (a) Reconstructed mass and (b) 1σ Gaussian width of π0 as a function of the reconstructed pT for inclusive π0 mesons from data (open crosses), simulations (circles), and for π0 coming from KS0 decays (squares) in Cu+Cu collisions.

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  • Figure 2
    Figure 2

    The invariant mass distribution for π0π0 pairs measured in the MB d+Au collisions at 8<pT<9 GeV/c. The invariant mass reconstructed without any corrections is shown with red squares. The invariant mass reconstructed after corrections for the mass of reconstructed π0 to the PDG value is shown with blue open crosses. Same with additional correction accounting for the difference between inclusive π0 mesons and neutral pions produced in KS0 meson decay as described in the text is shown with black circles.

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  • Figure 3
    Figure 3

    The invariant mass reconstructed from two π0 mesons in the range 5<pT<6 GeV/c in (a) d+Au and (b) Cu+Cu collisions at sNN=200 GeV for the MB data. The distributions are approximated by a Gaussian plus a second-order polynomial shown by solid red and blue dashed curves, respectively.

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  • Figure 4
    Figure 4

    The invariant mass distributions of Kπ candidates, where K is identified in the TOF and π is matched in PC3, in the range 2.3<pT<2.6 GeV/c for (a) p+p, (b) d+Au, and (c) Cu+Cu collisions at sNN=200 GeV. The distributions are shown after subtraction of the mixed-event background and the correlated background from misidentified ϕK+K decays (see text for details). The distributions are fitted to the sum of the RBW function for the signal and a polynomial (second order in p+p and third elsewhere) for the background shown with a solid red curve. The residual background is also shown separately with a blue dashed curve. The ϕ contribution is shown by the magenta histogram.

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  • Figure 5
    Figure 5

    Reconstruction efficiency for (a) KS0 and (b) K*0 for d+Au collisions. The gray bands show the systematic uncertainty. Please refer to Table 3 for systematic uncertainties. Panel (b) shows the reconstruction efficiencies for the “unidentified,” “kaon identified,” and “fully identified” techniques for the K*0 analysis are shown by the dot-dashed blue curve, red solid curve, and black dashed curve, respectively.

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  • Figure 6
    Figure 6

    (a) Trigger efficiency for single photons as a function of cluster energy. (b) KS0 trigger efficiency as a function of pT. The bands show the systematic uncertainty. Results are presented for the Cu+Cu data recorded in 2005.

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  • Figure 7
    Figure 7

    (a) Cross section of K*0 meson production as a function of pT obtained with the “kaon identified,” “fully identified,” and “unidentified” analysis techniques in p+p collisions at s=200 GeV. The systematic uncertainties shown with boxes are mostly uncorrelated between analysis techniques. The solid blue line is the Tsallis function fit to the combined data points. The star symbols are the K*0 meson measurements from the STAR Collaboration [39]. (b) Ratio of the yields obtained with the three analysis techniques to the fit function. The scale uncertainty of 10% is not shown.

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  • Figure 8
    Figure 8

    KS0 meson invariant pT spectra (a) for d+Au and (b) for Cu+Cu collisions at sNN=200 GeV for different centrality bins. The systematic uncertainties are shown by the boxes. The solid curves are a fit of the KS0 p+p data by the Tsallis function [38]. The dashed curves are the fit function scaled by Ncoll. The global p+p uncertainty of 10% is not shown.

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  • Figure 9
    Figure 9

    K*0 meson invariant pT spectra (a) for d+Au and (b) for Cu+Cu collisions at sNN=200 GeV for different centrality bins. The systematic uncertainties are shown by the boxes. The solid curve is a fit of the K*0 p+p data by the Tsallis function [38]. The dashed curves are the fit function scaled by Ncoll. The global p+p uncertainty of 10% is not shown.

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  • Figure 10
    Figure 10

    KS0/π0 ratios for (a) d+Au and (b) Cu+Cu collisions at sNN=200 GeV for different centrality bins. The statistical uncertainties are shown by vertical bars and the systematic uncertainties are shown by the boxes.

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  • Figure 11
    Figure 11

    Nuclear modification factor as a function of pT for KS0 and K*0 for (a) most central and (b) most peripheral d+Au collisions at sNN=200 GeV. Results from π0 [59], ϕ [15], and protons [29] are also shown. The π0 results are shown from the data collected in 2003 and the results of the rest of the particles are obtained from 2008 data. The corresponding systematic uncertainties are shown by boxes. The global p+p uncertainty of 10% is not shown.

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  • Figure 12
    Figure 12

    The nuclear modification factor as a function of pT for KS0 and K*0 meson for centrality bins (a) 0%–20%, (b) 20%–40%, (c) 0%–94%, (d) 20%–60%, (e) 40%–60%, and (f) 60%–94% in Cu+Cu collisions at sNN=200 GeV. In all panels the statistical uncertainties are shown with vertical bars and the systematic uncertainties are shown with boxes. The global p+p uncertainty of 10% is not shown.

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  • Figure 13
    Figure 13

    Nuclear modification factor as a function of pT for KS0,K*0 for centralities (a) 0%–20%, (b) 0%–94% (MB), and (c) 60%–94% in Cu+Cu collisions at sNN=200 GeV. Results from π0 [8] and ϕ [15] are also shown. The statistical errors are shown by vertical bars. The systematic uncertainties are shown by boxes. The global p+p uncertainty of 10% is not shown.

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  • Figure 14
    Figure 14

    Comparison of the nuclear modification factor of π0 [8], ϕ [15], and K*0 in Cu+Cu collisions and proton [29] and kaon [29] in Au+Au collisions at sNN=200 GeV. The comparisons are made for (a) 40%–60% and (b) 60%–92% in Au+Au system and 0%–40% and 40%–94% in the Cu+Cu system corresponding to similar Npart values in the two systems. The statistical errors are shown by vertical bars. The systematic uncertainties are shown by boxes. The global p+p uncertainty of 10% is not shown.

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