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Study of a background reconstruction method for the measurement of D-meson azimuthal angular correlations

NUCLEAR PHYSICS AND INTERDISCIPLINARY RESEARCH

Study of a background reconstruction method for the measurement of D-meson azimuthal angular correlations

Long Ma
Xin Dong
Huan-Zhong Huang
Yu-Gang Ma
Nuclear Science and TechniquesVol.32, No.6Article number 61Published in print 01 Jun 2021Available online 14 Jun 2021
33400

We studied experimental background reconstruction methods for the measurement of the DD¯ correlation using PYTHIA simulation. The like-sign (LS) and side-band (SB) background methods, which are widely used in the experimental measurements of single D-meson production yields, were deployed for correlation study. It was found that the LS method, which describes the combinatorial background of single D0 meson yields, fails to reproduce the correlated background in the D0D0¯ correlation measurement, while the SB background method yields a good description of the background for both single D0 yields and the correlated background of the D0D0¯ correlation measurement. We further examined the validity of the correlation methods under different signal-to-background ratios, providing direct references for experimental measurements.

heavy flavorazimuthal correlationPYTHIA

1 Introduction

Quantum chromodynamics (QCD) is a theory that describes quarks, gluons, and the strong interaction between them. In QCD, heavy flavor quarks (c, b) are mostly produced through initial hard scattering in high-energy collisions of nucleons or nuclei. Because of their large masses, heavy quarks may offer a unique sensitivity for studying the cold and hot QCD medium created in these collisions [1-5]. In proton + proton (p+p) collisions, perturbative QCD (pQCD) calculations reproduce the inclusive heavy-flavor hadron-production cross-section data over a broad range of collision energies and rapidities [6-10]. The nuclear modification factor (RAA) for charmed hadrons in heavy-ion collisions is significantly modified compared to the p+p reference [11]. Several models with different energy-loss mechanisms can describe the experimental data [12, 13, 18, 19].

Recent research suggests that azimuthal correlations Δϕ between heavy quark pairs offer a new insight about charm-medium interaction dynamics, and therefore can help distinguish different energy-loss mechanisms in a hot QCD medium [14-17, 20]. The theoretical prediction indicates that pure radiative energy loss does not change the initial angular correlation function significantly, while pure collisional energy loss is more efficient at diluting the initial back-to-back charm pair correlation. Furthermore, the momentum broadening in the direction perpendicular to the initial quark momentum, which cannot be probed directly with traditional single-particle measurements (e.g., RAA and elliptic flow parameter v2), could be reflected in the azimuthal angle correlations [15, 21, 22].

In p+p collisions, charm-quark pairs are produced through initial back-to-back hard scattering in leading order. In next-to-leading order, the angular correlation between charm-quark pairs widens. In particular, it will show a near-side peak at Δϕ∼0 if the charm pairs are produced through gluon splitting. The measurement of DD¯ correlations in p + p collisions not only provides a baseline for measurements in heavy-ion collisions, but also offers a good constraint for pQCD calculations. D-mesons inherit most of the initial charm pair correlations, but weak decays smear the correlation significantly. Therefore, the measurement of DD¯ correlations should be the most sensitive probe for studying charm-quark pair correlations [23-25, 30].

The experimental reconstruction of the DD¯ azimuthal angular correlation is challenging. It requires the reconstruction of two charmed hadrons in a single event. Charmed hadrons must be reconstructed through their hadronic decay channels with small branching ratios. Furthermore, there is often a sizable background in each reconstructed charmed hadron. In single-charmed hadron yield measurements, for instance D0 mesons through the Kπ+ decay channel, several background methods, such as the like-sign (LS), side-band (SB), and mixed-event (ME) methods, were deployed by experimentalists [26, 27]. In the ME technique, background pairs are reconstructed using two daughter tracks from different events. Given that the tracks are produced in different events, the background reconstructed is uncorrelated with the foreground D0 candidates. By mixing multiple events, this method has the advantage of reproducing the combinatorial background with good statistics. In the LS technique, the background is generated by pairing the daughter tracks with the same charge sign. It contains the produced background correlated in pairs with opposite charge signs in the same event. In the SB technique, opposite sign pairs with invariant masses away from the D0 peak are used, two symmetric mass regions on both sides of the D0 peak are usually selected, and the average of these regions is chosen to represent the background underneath the D0 peak. Both LS and SB techniques can successfully reproduce the background in single D0 yield measurements with reasonable precision.

In this study, we investigated these background reconstruction methods for the experimental measurement of DD¯ correlations. The ME technique misses the background correlation in the same event and typically needs to be normalized to either LS or SB distributions. In this study, we focused on the comparison of the LS and SB background techniques.

2 PYTHIA study for DD¯ correlations

The Monte-Carlo event generator PYTHIA (version 8.168) was used in this study [28]. We focused on p+p collisions at s = 500 GeV. The parameters were adjusted so that PYTHIA could reproduce the experimental data on the inclusive cc¯ production cross-section in p+p collisions at 500 GeV, as measured by the STAR experiment at RHIC [29].

Figure 1 shows the cc¯ production cross-section as a function of the transverse momentum in PYTHIA in comparison with the STAR measurements. The modified PYTHIA parameters in this case were as follows: strong-interaction coupling constant (αs) of the final parton shower (TimeShower:alphaSvalue) set to 0.15; minimum invariant transverse-momentum (pT) threshold for hard QCD process (PhaseSpace:pTHatMin) set to 1.5 GeV/c. With this setting, PYTHIA properly describes both the magnitude and the pT spectrum. It was also found that changing these two parameters has a negligible effect on charm correlations.

Fig. 1.
(Color online) Charm-pair cross-section as a function of transverse momentum in p+p collisions at s = 500 GeV in PYTHIA (dashed line) compared with STAR measurements (solid circles).
pic

A sample of six-billion PYTHIA minimum bias events with this setting was generated for the D0D0¯ correlation study. D0 mesons can be directly accessed in the PYTHIA simulation based on their particle identification number. To emulate the experimental measurement, D0s were reconstructed by pairing the kaon and pion candidate pairs via the typical hadronic decay channel D0K- + π+ and its charge conjugate channel for D0¯. In a real experiment with a silicon vertex detector, many background tracks from the primary collisions can be eliminated, but considerable background remains, particularly in the low pT region.

In this study, we did not distinguish the secondary decay vertices in the D0 reconstruction. Instead, we combined all kaons and pions at mid-rapidity (|η| le; 1) in the final stage of the PYTHIA output. This allowed us to study the validity of the background reconstruction methods with different signal-to-background (S/B) ratios of the reconstructed D0 candidates. The invariant masses of the unlike-sign (US) and (LS) kaon and pion pairs in the same event were calculated. A finite momentum resolution effect was included so that the reconstructed D0 signal peak had the width observed in the experiment.

Figure 2 shows the D0(D0¯) signal and the combinatorial background from the LS and SB methods. The LS and SB background regions are denoted by the blue and red hatched areas, respectively. The invariant mass distribution of D0¯ is almost identical to D0 in both shape and magnitude. The background was found to be flat in PYTHIA within a relative wide invariant mass range. For simplicity, we denote D0(D0¯) candidates from K-π+(K+π-) pairs with unlike signs as ‘US’ candidates, and those from K-π- or K+π+ pairs with same charge sign as ‘LS’ background. The SB background is denoted as ‘SB’. Fig. 2 shows that both the LS and SB methods can reasonably reproduce the real background underneath the reconstructed D0 signals. For single-particle yield measurement, the D0 and D0¯ counts were calculated from Eqs. 1 and 2 for the LS and SB background methods, respectively.

Fig. 2
(Color online) Invariant mass distribution of all final-stage kaon and pion pairs with opposite signs in PYTHIA data at mid-rapidity (shown by solid red line, US). The LS method reproduces the combinatorial background shown by the blue solid line. The blue shaded region shows the LS background within a ±3σ window of the signal peak. The SB background regions are shaded in red.
pic

If the background methods work well for the D0D0¯ correlation measurement, the correlation signal between D0 and D0¯ can be derived using Eqs. 3 and 4. The asterisks (*) indicate the correlation functions between the pairs. We can also derive the D0D0¯ correlation signal from the PYTHIA simulation directly, and compare it to the reconstructed signals using these two background methods.

NLSD+D¯=US(Kπ+)+US(K+π)LS(Kπ)LS(K+π+) (1) NSBD+D¯=US(Kπ+)+US(K+π)SB(Kπ+)SB(K+π) (2) CLSDD¯=US(Kπ+)*US(K+π)LS(Kπ)*US(Kπ+)LS(K+π+)*US(K+π)+LS(Kπ)*LS(K+π+), (3) CSBDD¯=US(Kπ+)*US(K+π)SB(K+π)*US(Kπ+)SB(Kπ+)*US(K+π)+SB(Kπ+)*SB(K+π), (4)

The di-hadron correlation measurements are usually plotted as a function of the azimuthal angle difference, i.e., Δϕ=ϕD0ϕD0¯. The upper panel in Fig. 3 shows the correlations between US candidates and the LS backgrounds as a function of Δϕ. The pT > 1.0 GeV/c cut was set for both D0 and D0¯ mesons, and the mass-window cuts for US, LS, and SB pairs are shown as colored bands in Fig. 2. The plot shows that the correlation between LS and LS background pairs (LS*LS) tends to peak at Δϕ around 0 and that its magnitude is considerably larger than that between the LS background and US candidates (LS*US). The lower panel in Fig. 3 shows the results of the SB method with the same trigger pT and S/B ratio as the LS method. The correlation between the SB background and US candidates lies between the other two correlation terms. The correlation between two SB background pairs shows a trend similar to that between the SB background and US candidates.

Fig. 3.
(Color online) Upper Panel: cross-correlations of D0D0¯ from US candidates and LS backgrounds. The trigger and associated pT cuts were both set to 1 GeV/c with a S/B ratio of approximately 0.3. Lower panel: similar results from the SB method.
pic

Figure 4 shows the reconstructed D0D0¯ correlation signals with the LS and SB background methods in comparison with the real correlation signals from PYTHIA directly. Two sets of pT cuts were imposed for the triggered and associated D-mesons, as shown in the upper and lower panels, respectively. Panels in two different columns show the comparisons with two different mass-window cuts, which result in different S/B ratios of the reconstructed D0 candidates. The red data points represent the correlation signals from the reconstructed D0s, whereas the blue data points are the real D0 correlations directly obtained from PYTHIA with the same kinematic cuts applied. Similar results from the SB method are presented in Fig. 4.

Fig. 4.
(color online). D0D0¯ correlation as a function of the relative azimuthal angle Δϕ in p+p collisions at s = 500 GeV calculated using the LS method (upper panel) and SB method (lower panel) based on Eq. 3 in PYTHIA simulation. The transverse-momentum dependence is shown with pT cuts applied to the triggered and associated D mesons. Panels (a)–(d) show correlations of reconstructed D0 mesons under different S/B ratios in comparison with correlations of produced D0D0¯ pairs in PYTHIA.
pic

Note that the reconstructed correlations using the LS method are different from the real D0D0¯ signal from PYTHIA. In particular, the reconstruction correlations start to show an enhanced structure in the near-side region when the S/B ratio decreases. Reconstructed correlations using the SB method can reproduce the real D0D0¯ signal reasonably well in these kinematic and S/B ratio regions. In addition, the quality of the reproduction does not depend on the transverse-momentum cut. It depends on the S/B ratios of the D0 candidates.

ui=(1NtrigdNdΔϕi)reco,vi=(1NtrigdNdΔϕi)real (5) ΔP=1Ni=1k|uivivi|,ΔE=1Ni=1k|σui2+σvi2vi| (6)

To better illustrate the performance of these two background methods in measuring the angular correlations of the DD¯ pairs, we introduced two variables to quantify the goodness of fit for the reconstructed correlation signals with respect to the real D0D0¯ correlations from PYTHIA. ΔP and ΔE are defined in Eq. 6 to describe the relative differences between the data points and the statistical errors from this sample. Note that ui and vi are the values of the number of i data points of the reconstructed and real correlation signals in each Δϕ bin; N is the total number of data points in each correlation signal, assuming the same binning for the histograms. Fig. 5 shows the corresponding results from the LS and SB methods, respectively. Note that ΔP in the LS results shows a large deviation from ΔE when the S/B ratio decreases, indicating that the LS method fails to reproduce the real correlation at relatively low S/B ratios. The SB method exhibits good performance throughout the entire S/B ratio region investigated. The increase in both ΔP and ΔE in the low S/B region for the SB method is due to the reduced statistics. We also studied the performance of the two background methods by considering D0 from D* decay and non-prompt D0 from B-decay. The conclusions concerning the goodness of fit for both methods remain unchanged. Experimentally, as particle misidentification (Mis-PID) may affect the background reconstruction and cause double counting of the signals, we further evaluated such effects on the correlation reconstruction through a toy Monte-Carlo simulation based on the PID criteria for p+p collisions in STAR analysis [29]. We found that the mis-PID effect was significantly small (<1%) in this case.

Fig. 5.
(color online). Summary plots of the goodness of fit calculated using the LS method (upper panel) and SB method (lower panel) in the PYTHIA simulation. The estimator is shown as a function of the (S/B) ratio. The solid and dashed lines show ΔP and ΔE, respectively.
pic

In the LS method, when a K+π+ pair is selected, there is a higher probability of finding a K-π- pair than another K+π+ pair because of local and global charge conservation. The reconstructed correlation signal after LS background subtraction from Eq. 3 should contain all correlations between K+π- and K-π- pairs, including the D0D0¯ correlation of interest, as well as the correlation due to charge conservation. To further demonstrate that the additional correlation observed in the LS method is related to the underlying event instead of the D0D0¯ signal, we turned off the D0 hadronic decay process in the PYTHIA simulation and ran the same analysis.

Figure 6 shows the invariant mass distribution of pure pairs without D0 decay contribution. Cross-correlations between US/LS and LS/LS pairs are plotted in comparison with the US/US pair correlations in Fig. 7 with different cuts applied to the invariant mass region. Similarly, results from the SB method are shown in Fig. 8. There is a large difference between the LS*US and US*US pair correlations, while there is very a small difference between LS*LS and US*US. This is consistent with our understanding that there is an additional correlation that is not originated from the D0D0¯ pairs.

Fig. 6.
(Color online)Invariant mass distribution of pure pairs in PYTHIA. The D0-> hadronic decay process was turned off. Red line: US pairs. Blue hatched area: LS pairs within cut window. Red shaded area: SB pairs within cut window.
pic
Fig. 7.
(Color online) Cross-correlations of the pure LS and US pairs in the LS method.
pic
Fig. 8.
(Color online) Cross-correlations of SB and US pairs in the SB method.
pic

The SB method is not affected by charge conservation. Note that all cross-correlations fall in the same trend, and there is no remaining K+π--K-π+ correlation when the D0K+π- decay is turned off.

3 Conclusion

In summary, we studied background reconstruction methods for azimuthal correlations between D0 and D0¯ pairs using a PYTHIA simulation.

Both the LS and SB methods provide a good description of the background when reconstructing single D0 yields. However, when reconstructing the correlation signal, the LS method fails to reproduce the D0D0¯ correlation. The residual correlation after the LS background subtraction mainly comes from the underlying event activity, likely due to local or global charge conservation. We demonstrate that the SB method performs well in describing the correlation background and therefore reproduces the original D0D0¯ correlation in the S/B rate regions investigated. The upcoming sPHENIX experiment at RHIC will explore the charm correlation in p+p and Au+Au collisions by measuring the DD¯ azimuthal correlation with full reconstruction of D-mesons through their hadronic decay channels. Our study on correlation methods constitutes an important reference for future experimental measurements.

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