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CMS-PAS-HIN-21-006
Two-particle femtoscopic correlation measurements of K0S and Λ(¯Λ) particles in PbPb collisions at sNN= 5.02 TeV
Abstract: Two-particle correlations as a function of relative momentum are presented for K0S, Λ, and ¯Λ strange hadrons produced in lead-lead collisions at sNN= 5.02 TeV. The data were obtained using the CMS detector at the LHC. Such correlations are sensitive to quantum statistics and to possible final-state interactions between the particles. Source radii extracted from K0SK0S correlations in different centrality regions are found to decrease in going from central to peripheral collisions. Strong-interaction scattering parameters (i.e., scattering length and effective range) are determined from ΛK0S¯ΛK0S and ΛΛ¯Λ¯Λ correlations using the Lednicky-Lyuboshits model and compared to other experimental and theoretical results.
Figures & Tables Summary References CMS Publications
Figures

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Figure 1:
The invariant mass of K0S (left) and Λ+¯Λ (right), and their corresponding fits in the 0-80% centrality range. The circles are the data, and the fit is shown with a solid curve for the total fit, a dashed-dotted curve for the signal component, and a dashed curve for the background component. The vertical lines indicate the ±2σ peak region.

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Figure 1-a:
The invariant mass of K0S (left) and Λ+¯Λ (right), and their corresponding fits in the 0-80% centrality range. The circles are the data, and the fit is shown with a solid curve for the total fit, a dashed-dotted curve for the signal component, and a dashed curve for the background component. The vertical lines indicate the ±2σ peak region.

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Figure 1-b:
The invariant mass of K0S (left) and Λ+¯Λ (right), and their corresponding fits in the 0-80% centrality range. The circles are the data, and the fit is shown with a solid curve for the total fit, a dashed-dotted curve for the signal component, and a dashed curve for the background component. The vertical lines indicate the ±2σ peak region.

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Figure 2:
The correlation distributions and fits for the K0SK0S pair for the 20-30% centrality range (left), and the ΛK0S¯ΛK0S (right) and ΛΛ¯Λ¯Λ (bottom) pairs with 0-80% centrality. In these plots, red circles are the experimental results, the blue solid line is the fit using Eq. (7), and the green dotted line is the nonfemtoscopic background from Eq. (6).

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Figure 2-a:
The correlation distributions and fits for the K0SK0S pair for the 20-30% centrality range (left), and the ΛK0S¯ΛK0S (right) and ΛΛ¯Λ¯Λ (bottom) pairs with 0-80% centrality. In these plots, red circles are the experimental results, the blue solid line is the fit using Eq. (7), and the green dotted line is the nonfemtoscopic background from Eq. (6).

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Figure 2-b:
The correlation distributions and fits for the K0SK0S pair for the 20-30% centrality range (left), and the ΛK0S¯ΛK0S (right) and ΛΛ¯Λ¯Λ (bottom) pairs with 0-80% centrality. In these plots, red circles are the experimental results, the blue solid line is the fit using Eq. (7), and the green dotted line is the nonfemtoscopic background from Eq. (6).

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Figure 2-c:
The correlation distributions and fits for the K0SK0S pair for the 20-30% centrality range (left), and the ΛK0S¯ΛK0S (right) and ΛΛ¯Λ¯Λ (bottom) pairs with 0-80% centrality. In these plots, red circles are the experimental results, the blue solid line is the fit using Eq. (7), and the green dotted line is the nonfemtoscopic background from Eq. (6).

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Figure 3:
Left: Rinv as a function of centrality by considering only the QS (blue circle), and both the QS and FSI effects (red circles). Right: Rinv as a function of mT (dark markers) and compared with ALICE data (light markers) for PbPb collisions at sNN= 2.76 TeV [27] in 0-10, 10-30, and 30-50% centrality classes. For each data point, the line and shaded area indicate the statistical and systematic uncertainty, respectively.

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Figure 3-a:
Left: Rinv as a function of centrality by considering only the QS (blue circle), and both the QS and FSI effects (red circles). Right: Rinv as a function of mT (dark markers) and compared with ALICE data (light markers) for PbPb collisions at sNN= 2.76 TeV [27] in 0-10, 10-30, and 30-50% centrality classes. For each data point, the line and shaded area indicate the statistical and systematic uncertainty, respectively.

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Figure 3-b:
Left: Rinv as a function of centrality by considering only the QS (blue circle), and both the QS and FSI effects (red circles). Right: Rinv as a function of mT (dark markers) and compared with ALICE data (light markers) for PbPb collisions at sNN= 2.76 TeV [27] in 0-10, 10-30, and 30-50% centrality classes. For each data point, the line and shaded area indicate the statistical and systematic uncertainty, respectively.

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Figure 4:
The λ parameter as a function of centrality by considering only the QS (blue circles) and both the QS and FSI effects (red circles). For each data point, the line and shaded area indicate the statistical and systematic uncertainty, respectively.

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Figure 5:
The values of d0 and f0 (left) and the values of f0 and f0 (right). In the left plot, the blue triangles and square markers are for ΛK0S¯ΛK0S and ΛΛ¯Λ¯Λ correlations, respectively, and are compared with the ΛΛ¯Λ¯Λ result from the STAR experiment [28] and ΛK0S¯ΛK0S results from ALICE experiment [27]. A reanalysis of STAR data for ΛΛ¯Λ¯Λ correlations is shown in the shaded area [32]. Theory calculations of the ΛΛ interaction parameters are shown as black triangles [33,34]. The blue dotted lines correspond to the relation d0=|f0|/2. In the right plot, the triangle is for ΛK0S¯ΛK0S correlations, and is compared with the ALICE ΛK0S¯ΛK0S result [27]. For each data point, the two lines and the box indicate the (one-dimensional) statistical and systematic uncertainties, respectively.

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Figure 5-a:
The values of d0 and f0 (left) and the values of f0 and f0 (right). In the left plot, the blue triangles and square markers are for ΛK0S¯ΛK0S and ΛΛ¯Λ¯Λ correlations, respectively, and are compared with the ΛΛ¯Λ¯Λ result from the STAR experiment [28] and ΛK0S¯ΛK0S results from ALICE experiment [27]. A reanalysis of STAR data for ΛΛ¯Λ¯Λ correlations is shown in the shaded area [32]. Theory calculations of the ΛΛ interaction parameters are shown as black triangles [33,34]. The blue dotted lines correspond to the relation d0=|f0|/2. In the right plot, the triangle is for ΛK0S¯ΛK0S correlations, and is compared with the ALICE ΛK0S¯ΛK0S result [27]. For each data point, the two lines and the box indicate the (one-dimensional) statistical and systematic uncertainties, respectively.

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Figure 5-b:
The values of d0 and f0 (left) and the values of f0 and f0 (right). In the left plot, the blue triangles and square markers are for ΛK0S¯ΛK0S and ΛΛ¯Λ¯Λ correlations, respectively, and are compared with the ΛΛ¯Λ¯Λ result from the STAR experiment [28] and ΛK0S¯ΛK0S results from ALICE experiment [27]. A reanalysis of STAR data for ΛΛ¯Λ¯Λ correlations is shown in the shaded area [32]. Theory calculations of the ΛΛ interaction parameters are shown as black triangles [33,34]. The blue dotted lines correspond to the relation d0=|f0|/2. In the right plot, the triangle is for ΛK0S¯ΛK0S correlations, and is compared with the ALICE ΛK0S¯ΛK0S result [27]. For each data point, the two lines and the box indicate the (one-dimensional) statistical and systematic uncertainties, respectively.
Tables

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Table 1:
Summary of systematic uncertainties in K0SK0S correlations in different centrality bins

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Table 2:
Summary of systematic uncertainties in ΛK0S¯ΛK0S correlations in 0-80% centrality

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Table 3:
Summary of systematic uncertainties in ΛΛ¯Λ¯Λ correlations in 0-80% centrality

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Table 4:
Extracted values of the Rinv, f0, f0, d0, and λ from ΛK0S¯ΛK0S and ΛΛ¯Λ¯Λ correlations in the 0-80% centrality.
Summary
The K0SK0S, ΛK0S¯ΛK0S, and ΛK0S¯ΛK0S femtoscopic correlations are extracted from data collected in PbPb collisions at a center-of-mass energy per nucleon pair of sNN= 5.02 TeV. This is the first report of ΛK0S¯ΛK0S correlations in PbPb collisions. The source size Rinv is extracted for K0SK0S correlations in six equal width centrality bins covering the 0-60% centrality range and is found to decrease going towards more peripheral collisions. The extraction of Rinv as a function of mT is also presented for K0SK0S correlations and is compared with ALICE results at sNN= 2.76 TeV. Measured values for Rinv, based on ΛK0S¯ΛK0S, and ΛK0S¯ΛK0S correlations, are also presented for the 0-80% centrality range. The Lednicky-Lyuboshits model fits to the correlation data indicate that the ΛK0S¯ΛK0S interaction is repulsive and ΛK0S¯ΛK0S interaction is attractive with no evidence for a bound H-dibaryon.
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