Measurement of Heavy Quark cross-sections at CDF
نویسنده
چکیده
The measurement of heavy quark cross-sections provides important tests of the QCD theory. This paper reviews recent measurements of single b-quark and correlated b-quark cross-sections at CDF. Two new measurements of the single b-quark production at CDF agree with the first result from CDF Run II. This clarifies the experimental situation and confirms the recent agreement of theoretical prediction with data. A new measurement of the correlated bb̄ cross-section with dimuon events at CDF is presented. It agrees with theory and it does not confirm the anomalously large bb̄ cross-section seen in Run I by CDF and D 6O in dimuon events. 1. Single b-quark production at the Tevatron Historically the b-quark cross-sections measured at the Tevatron during Run I have been higher than expected from NLO QCD predictions. This fact fostered continuous efforts to improve both the measurements and the theoretical predictions. A first compatible calculation was delivered in 2002 [1] and updated in ref. [2]. Where the increase in predicted cross-section is mostly due to improved experimental inputs: PDF, αs, and especially fragmentation functions tuned for calculations with logarithms resummation at next-to-leading accuracy (NLL) [1]. These new results, while going in the right direction of a higher prediction, are almost compatible but still lower than the lastest CDF Run I result [3]. The first measurement of the b-quark cross-section with CDF Run II data uses pp̄ → J/ψ+X events [4]. This result is lower than the latest Run I result and in perfect agreement with the predictions [2]. This would be the end of the story, but the experimental picture is not fully clear as noted in ref. [5]. In fact, the experimental measurements are not fully consistent among themselves. Before claiming the solution of the long standing problem of b-quark production at the Tevatron, the experimental situation must be clarified. With this purpose CDF provided two additional measurements that use different decay modes. 2. Recent measurements of single b-quark cross-section at CDF The first result is a measurement of b-hadron (Hb) cross-section [6]. This measurement uses pp̄ → Hb + X → μ D + X events collected with the lepton plus displaced track trigger introduced in Run II. A signal of 3200 μD candidates with D → Kπ is reconstructed in a sample corresponding to a luminosity of 83pb. To obtain the cross-section, we first subtract the resonant background under the D peak, which is estimated to be 12.0% ± 3.2% with a combination of data measurement and MC simulations. Then we evaluate the acceptance with MC, while all the efficiencies are measured with data. Finally we unfold the pT (μD ) distribution using MC input to obtain the Hb differential cross-section shown in figure 1. The total cross-section is: σHb(pT > 9.0GeV/c, |y| < 0.6) = 1.34μb ± 0.08(stat.) +0.13 −0.14(syst.)± 0.07(BR) The second result is a measurement of B production cross-section with fully reconstructed pp̄ → B + X, B → J/ψK events [7]. It is based on a sample of 8200 signal events corresponding to a luminosity of 740pb. This analysis exploits the high-statistic available to simplify the selection and minimize the overall systematics. The total cross-section is: σB+(pT > 6.0GeV/c, |y| < 1) = 2.78 ± 0.24μb The two new CDF Run II measurements are compared to the previous CDF run II measurement and with the lastest theoretical prediction [2] in figure 1, where all results are scaled to σB+ . The agreement is quite good. It shows the result of several years of work to improve our understanding of bottom production. Figure 1. CDF Run II measurements of b-quark production compared to FONLL. (NLO) σ (Data)/ σ = 2b R 0 1 2 3 4 0 8 NLO calculation 0.15 ± 1.0 + X μ μ CDF II 0.2 ± 0.11 ± 1.2 > 6 GeV T p (errors are exp. and frag.) + X μ μ D0 I 0.76 ± 2.3 > 7 GeV T p (ratio to HVQJET) + X μ μ CDF I 0.48 ± 2.4 > 6.5 GeV T p + b-jet μ CDF I 0.15 ± 1.5 > 12 GeV T p jets b CDF I b 0.32 ± 1.0 > 20 GeV T p jets b CDF I b 0.30 ± 1.2 > 15 GeV T p Figure 2. Ratio of data/NLOtheory for correlated bb̄ cross-section measurements. 3. New measurement of correlated bb̄ cross-section at CDF The review of bb̄ cross-sections in ref. [5] shows that the five measurements from Run I are not consistent among themselves. This is represented by the first five points in figure 2. It seems that the data/theory ratio increases with the numbers of muons in the observed final state. A new measurement from CDF [8] addresses this anomalous effect. It uses dimuon events selected with pT > 3GeV/c, |η| < 0.7 and 5 < mμμ < 80GeV/c 2 . The invariant mass cut is used to reject events from sequential decays of a single b-quark and from the Z resonance. This dimuon sample includes events from different sources: • decays of heavy flavor quark pairs (bb̄, cc̄) • prompt Drell Yan processes, charmonium and bottomoium • K and π decays and misidentification In order to separate the different contributions and eventually count the number of dimuon events from heavy flavor quark pairs we fit the 2D distribution of the impact parameter of both muons. We first generate templates of the 1D impact parameter distributions. For prompt single muons we use data and for single muons from b-hadron and c-hadron decays we use a tuned Herwig simulation including full CDF II detector simulation. The three 1D templates obtained are combined into a six 2D templates for each possible dimuon source. Namely bb̄, cc̄, cb, promptprompt, prompt-b and prompt-c. The six templates are then used for a maximum likelihood fit of the measured 2D distribution. We find 54583 ± 678 dimuons from bb̄ and 24458 ± 1565 dimuons from cc̄ in our sample that corresponds to a luminosity of 740pb. The fraction of real muon pairs in our sample is estimated with both data and MC and it is found to be 0.96± 0.04 for bb̄ and 0.81 ± 0.09 for cc̄. The overall acceptance times efficiency is estimated with MC and corrected with scale factors measured on data. In table 1 we report our final results that are dimuon cross-sections from heavy flavor pairs instead of bb̄/cc̄ cross-sections. Where σb→μ,b̄→μ is defined as σbb̄ · BR(b → μ + X) 2 · A(pμT > 3GeV/c, |η| < 0.7, 5 < mμμ < 80GeV/c ). The σb→μ,b̄→μ error is dominated by luminosity uncertainty. The σc→μ,c̄→μ error is dominated by systematics from the impact parameter fit and the fake muon removal. In order to compare with theory, we calculate a prediction at dimuon level. We combine the MNR calculus with MRST98 PDF, Peterson fragmentation and we decay events with EvtGen as detailed in ref. [8]. Table 1 reports the results for two different fragmentation parameters (ǫ) in order to assess the uncertainty associated to fragmentation. Apart from fragmentation uncertainty, the theoretical error is 15% from mass and scales systematics plus a BR uncertainty of 3.7% and 6.7% respectively for bb̄ and cc̄. Table 1. Data/theory comparisons for dimuon cross-sections from heavy flavor.
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تاریخ انتشار 2007