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Doubly heavy baryons consisting of two heavy quarks (b or c) and one light quark (u, d, or s) are expected within the quark model [1, 2]. In proton-proton (
$ pp $ ) collisions at the Large Hadron Collider, a possible model for production of these states is through gluon-gluon fusion,$ g + g \to Q_1\overline{Q}_1 + Q_2\overline{Q}_2 $ (Q denotes a heavy quark), a process that can be computed using perturbative quantum chromodynamics (QCD) [3–5]. The doubly heavy baryon is then formed via hadronisation where the two heavy quarks form a diquark which binds with a light quark. Other models exist, including production at the scale of the hard process, or production via non-perturbative effects such as colour reconnection. The measurement of the properties of these doubly heavy baryons provides insight into both their production mechanism and internal structure.The observation and properties of the doubly heavy
$ \varXi_{cc}^{++} $ ($ ccu $ ) baryon have been firmly established by the LHCb collaboration [6–10], while the$ \varXi_{cc}^{+} $ ($ ccd $ ) and$ \varOmega_{cc}^+ $ ($ ccs $ ) baryons have been searched for [11–13], and only hints of a signal were seen. The LHCb collaboration has also carried out searches for the neutral doubly heavy baryons,$ \varXi_{b c}^{0}(b c d) $ [14] and$ \varOmega_{b c}^{0}(b c d) $ [15], but these states are yet to be observed.To date, no search has been performed for the
$ \varXi_{bc}^+ $ baryon, a bound state with quark content$ bcu $ . This baryon is expected to have a mass in the range of 6700–7029 MeV/$c^2$ [16–35], while its lifetime is predicted to be be-tween$ 240 $ and$ 607~{\rm{fs}} $ [21, 31, 36–38]. The$ \varXi_{bc}^+ $ production cross-section at a centre-of-mass energy of$\sqrt s $ =13 TeV is predicted to be about 16 nb [39] in the fiducial region$ {p_{\rm{T}}}>4\;{\rm{GeV}} /{c} $ and$ 1.9<\eta<4.9 $ , where$ {p_{\rm{T}}} $ is the momentum component transverse to the beam direction and η is the pseudorapidity.This article presents the first search for the
$ \varXi_{bc}^+ $ baryon through its decay via the$ J/\psi \varXi_c^+ $ channel, with$ J/\psi \to \mu^{+}\mu^{-} $ and$ \varXi_c^+ \to p K^{-}\pi^{+} $ final states, using$ pp $ collision data collected by the LHCb experiment at centre-of-mass energies of 7, 8, and 13 TeV, corresponding to integrated luminosities of 1, 2, and 6 fb−1, respectively.The search for this decay is advantageous over the previous
$ \varXi_{bc}^0 $ searches in several ways. First, the$ \varXi_{bc}^+ $ baryon is expected to have a larger lifetime than that of the$ \varXi_{bc}^0 $ baryon [21, 31, 36–38], which leads to a larger selection efficiency as the lifetime information is used to suppress background from primary$ pp $ interactions. Second, the mode studied here uses$J/\psi\to \mu^+ \mu^-$ decays, which typically have a selection efficiency three times larger than the fully hadronic modes used in the previous$ \varXi_{bc}^0 $ searches. Last, the modes used in the$ \varXi_{bc}^0 $ analyses involved suppressed$ b\to u $ or$ b\to s $ transitions, or W-exchange diagrams. Here the decay to the$ J/\psi \varXi_c^+ $ final state involves a colour-suppressed$ b\to c $ transition, with a decay amplitude that is less likely to be suppressed, as shown in Fig. 1.Figure 1. Example leading-order Feynman diagram for the
$ \varXi_{bc}^+ \to J/\psi \varXi_c^+ $ decay.To reduce systematic uncertainties, the
$\varXi_{bc}^+$ production cross-section times the$ \varXi_{bc}^+ \to J/\psi \varXi_c^+ $ branching fraction is measured relative to that of the normalisation mode$ B_{c}^{+} \to J/\psi D_{s}^{+} $ with$ J/\psi \to \mu^{+}\mu^{-} $ and$ D_{s}^{+} \to K^{+} K^{-}\pi^{+} $ decays. Specifically, the quantity$ {\cal{R}} $ is defined as$ \begin{equation} {\cal{R}}=\frac{\sigma(\varXi_{bc}^+ )\times{\cal{B}}(\varXi_{bc}^+ \to J/\psi \varXi_c^+)\times {\cal{B}}(\varXi_c^+ \to pK^-\pi^+)}{\sigma(B_c^+)\times{\cal{B}}(B_c^+ \to J/\psi D_s^+)\times {\cal{B}}(D_s^+ \to K^+K^-\pi^+)}, \end{equation} $
(1) where
$ \sigma(\varXi_{bc}^+) $ and$ \sigma(B_c^+) $ are the production cross-sections of$ \varXi_{bc}^+ $ and$ B_{c}^{+} $ hadrons, respectively, and${\cal{B}}$ is the branching fraction of the corresponding decay. The ratio$ {\cal{R}} $ is measured in the rapidity range$ 2.0 < y < 4.5 $ and in the${p_{\rm{T}}}$ region from 0 to 20$ {\rm{GeV}} /{c} $ . Measurements of$ {{\cal{R}}} $ are reported for the$\sqrt{s}=8 $ and 13 TeV data sets collected in 2012 and 2016–2018, corresponding to integrated luminosities of 2 and 5.4 fb−1, respectively. The 2011 data sample taken with a centre-of-mass energy of 7 TeV is small, and it is not used in the production rate measurement.The ratio
$ {\cal{R}} $ is evaluated as$ \begin{equation} {\cal{R}}=\frac{\varepsilon_{\rm norm}}{\varepsilon_{\rm sig}}\frac{N_{\rm sig}}{N_{\rm norm}}\equiv \alpha N_{\rm sig}, \end{equation} $
(2) where
$ \varepsilon_{\rm sig} $ and$ \varepsilon_{\rm norm} $ are the total efficiencies of the$ \varXi_{bc}^+ $ signal and$ B_{c}^{+} $ normalisation decay modes,$ N_{\rm sig} $ and$ N_{\rm norm} $ are the corresponding signal yields, and the derived quantity α is the single-event sensitivity.An estimate for
$ {\cal{R}} $ can be obtained by assuming that the ratio of production cross-sections$ \sigma(\varXi_{bc}^+)/\sigma(B_{c}^{+}) $ is about 0.4 [39–41],$ {\cal{B}}(\varXi_{bc}^+ \to J/\psi \varXi_c^+)\sim 1/3\cdot{\cal{B}}(B_{c}^{+} \to J/\psi D_{s}^{+}) $ due to colour suppression,${\cal{B}}(\varXi_c^+ \to pK^-\pi^+)= (0.62\pm 0.30)$ % [42, 43],${\cal{B}}(D_{s}^{+} \to K^+K^-\pi^+)=(5.39\pm 0.15)$ % [44], and assuming an efficiency ratio$ \varepsilon_{\rm sig}/\varepsilon_{\rm norm}\sim 1 $ . With these inputs, the value$ {\cal{R}}\sim0.015 $ is obtained. With 1100$ B_{c}^{+} \to J/\psi D_{s}^{+} $ candidates observed in the full data set collected by the LHCb experiment [45], approximately 15 reconstructed$ \varXi_{bc}^+ \to J/\psi \varXi_c^+ $ signal decays are expected in the LHCb detector acceptance. -
The invariant-mass distributions of selected
$ \varXi_{bc}^+ $ and$ B_{c}^{+} $ candidates in the full data sample are shown in Figs. 2 and 3, respectively. To improve the mass resolution of the$ \varXi_{bc}^+ \;(B_{c}^{+}) $ candidates, the$ J/\psi \varXi_c^+ \;(J/\psi D_{s}^{+}) $ invariant mass is calculated by constraining the$ J/\psi $ and$ \varXi_c^+\; (D_{s}^{+}) $ masses to their known values [44] and the$ \varXi_{bc}^+ \;(B_{c}^{+}) $ candidates to originate from their associated PV [64].Figure 2. (color online) Mass
$ m(J/\psi \varXi_c^+) $ distribution of selected$ \varXi_{bc}^+ $ candidates for the full data set. The fit (blue solid line) with the largest local significance at the mass of 6571 MeV/$c^2$ is superimposed.Figure 3. (color online) Mass
$ m(J/\psi D_{s}^{+}) $ distribution of selected$ B_{c}^{+} $ candidates for the full data set. The fit (blue solid line) is superimposed.The
$ \varXi_{bc}^+ $ signal yield is determined from an unbinned maximum-likelihood fit to the$ J/\psi \varXi_c^+ $ mass distribution. The signal is described by a double-sided Crystal Ball (DSCB) function [65] comprising a Gaussian core with power-law tails on both sides, where the tail parameters depend on the mass resolution, while the combinatorial background is described by an exponential function. The dependence of the mass resolution on the$ \varXi_{bc}^+ $ mass is determined from simulation. The mass resolution varies from about 4 MeV/$c^2$ at a$ \varXi_{bc}^+ $ mass of 6400 to 7 MeV/$c^2$ at 7100 MeV/$c^2$ . The mass region of interest from 6430 to 7120 MeV/$c^2$ is scanned in 3 MeV/$c^2$ steps, to search for any significant structures.The local significance of a signal peak is quantified with a p-value, which is calculated from the likelihood ratio between the background-plus-signal and the background-only hypotheses [66]. The local p-value is plotted in Fig. 4 as a function of
$ m(J/\psi \varXi_c^+) $ , showing a dip around 6571 MeV/$c^2$ , which has the largest local significance, expressed in number of standard deviations (σ), corresponding to$ 4.3\sigma $ . Another dip is seen around 6694 MeV/$c^2$ , with a local significance of$ 4.1\sigma $ . The fit results for the two mass peaks at 6571 and 6694 MeV/$c^2$ are shown in Figs. 2 and 5, and the signal yield is$ 75 \pm 19 $ and$ 58 \pm 16 $ , respectively. The global significance is evaluated using pseudoexperiments, by taking into account the look-elsewhere effect [67] in the mass range from 6430 to 7120 MeV/$c^2$ , and is estimated to be$ 2.8\sigma $ and$ 2.4\sigma $ for the two mass peaks at 6571 and 6694 MeV/$c^2$ , respectively. As no excess above$ 3\sigma $ is observed, upper limits on the production ratios are set for the data samples with centre-of-mass energies of$\sqrt s=8 $ and 13 TeV.Figure 5. (color online) Mass
$m(J / \psi \varXi_{c}^{+})$ distribution of selected$\varXi_{b c}^{+}$ candidates for the full data set. The fit (blue solid line) with the Second largest local significance at the mass of 6694$\mathrm{MeV} / c^{2}$ is superimposed.The
$ B_{c}^{+} $ signal yield is determined from an unbinned maximum-likelihood fit to the$ m(J/\psi D_{s}^{+}) $ distribution. The$ B_{c}^{+} $ signal is described by a DSCB function with the tail parameters depending on the mass resolution [45], while the combinatorial background is described by an exponential function. The fit to the full data set is shown in Fig. 3. A total of$ 706\pm38 ~ B_{c}^{+} \rightarrow J / \psi D_{s}^{+}$ signal decays are selected. The signal yields used in the measurement of$ {{\cal{R}}} $ are summarised in Table 1.$\;\;\;\;\;\;{\rm Data\; sample}$ $ \varepsilon_{\rm norm}/\varepsilon_{\rm sig} $ $ N_{\rm norm} $ α 2012 ( $ \sqrt s $ = 8 TeV)1.316 ± 0.013 75 ± 13 0.018 ± 0.003 2016 ( $ \sqrt s $ =13 TeV)1.207 ± 0.007 177 ± 20 0.0068 ± 0.0008 2017 ( $ \sqrt s $ =13 TeV)1.202 ± 0.006 193 ± 20 0.0062 ± 0.0006 2018 ( $ \sqrt s $ =13 TeV)1.222 ± 0.006 220 ± 21 0.0056 ± 0.0005 Table 1. Efficiency ratios
$ \varepsilon_{\rm norm}/\varepsilon_{\rm sig} $ between the normalisation and signal modes, signal yields of the normalisation mode$ N_{\rm norm} $ , and the single-event sensitivity α, for the default mass and lifetime of the$ \varXi_{bc}^+ $ baryon, 6900 MeV/$c^2 $ and 400 fs, respectively. Uncertainties are statistical only. -
The efficiency ratio between the
$ B_{c}^{+} $ and$ \varXi_{bc}^+ $ modes, defined as$ \varepsilon _{\rm norm}/\varepsilon _{\rm sig} $ , is determined from simulation, along with corrections to account for small residual differences between data and simulation. The signal efficiency depends upon the assumed mass and lifetime of the$ \varXi_{bc}^+ $ baryon. Simulated events are generated with a$ \varXi_{bc}^+ $ mass of 6900 MeV/$c^2$ and a lifetime$ \tau(\varXi_{bc}^+) = 400~{\rm{fs}} $ , labelled here as default. The tracking and PID efficiencies for both the signal and normalisation modes are corrected using calibration data samples [68–70]. The PID efficiency correction is applied by resampling the distributions of PID observables in simulation to match those in data for the variables used in the selection and in the BDT classifier before computing the efficiency. The efficiency ratio and the single-event sensitivity at the default$ \varXi_{bc}^+ $ mass and lifetime are summarised in Table 1 together with the signal yield of the normalisation mode, used in computing the single-event sensitivity.The efficiency ratio for other lifetime values are obtained by weighting the simulated events to reproduce lifetime hypotheses from 300 to 500
$ ~{\rm{fs}} $ in$ 50~{\rm{fs}} $ steps. An event-by-event weight is calculated as$ \begin{equation} w=\frac{(1/\tau)\cdot \exp{(-t/\tau)}}{(1/\tau_0)\cdot \exp{(-t/\tau_0)}}, \end{equation} $
(3) where t is the
$ \varXi_{bc}^+ $ decay time, τ is the new lifetime and$ \tau_0 $ is the default lifetime. The total efficiency is found to have a linear dependence on the$ \varXi_{bc}^+ $ lifetime. The value and uncertainty in the single-event sensitivity α are provided for each lifetime hypothesis and for each data-taking period (Table 2). The efficiency could also depend on the$ \varXi_{bc}^+ $ baryon mass hypothesis in the simulation, since it affects the kinematic distributions of the decay products. To assess this effect, large samples of simulated events are generated with alternative mass hypotheses in the range 6400–7050 MeV/$c^2 $ in 50 MeV/$c^2 $ steps. These samples are used to weight the${p_{\rm{T}}}$ distributions of the final-state particles in the fully simulated$ \varXi_{bc}^+ $ decay to match those of the other mass hypotheses, and the efficiency is then recalculated. A very small dependence on the$ \varXi_{bc}^+ $ mass, a 0.4% relative variation of the signal efficiency due to this weighting, is observed and considered as a systematic uncertainty.Data sample 300 $~{\rm{fs}}$ 350 $~{\rm{fs}}$ 400 $~{\rm{fs}}$ 450 $~{\rm{fs}}$ 500 $~{\rm{fs}}$ 2012 ( $ \sqrt s $ = 8 TeV)22 ± 4 20 ± 3 18 ± 3 16 ± 2 15 ± 2 2016 ( $ \sqrt s $ =13 TeV)8.4 ± 0.9 7.5 ± 0.8 6.8 ± 0.8 6.3 ± 0.7 5.9 ± 0.6 2017 ( $ \sqrt s $ =13 TeV)7.7 ± 0.7 6.8 ± 0.7 6.2 ± 0.6 5.7 ± 0.6 5.4 ± 0.5 2018 ( $ \sqrt s $ =13 TeV)6.9 ± 0.6 6.2 ± 0.6 5.6 ± 0.5 5.2 ± 0.5 4.9 ± 0.4 Table 2. Single-event sensitivity α in units of 10-3 for different lifetime hypotheses of the
$ \varXi_{bc}^+ $ baryon for different data taking periods. Uncertainties are due to the limited size of the simulated samples and the statistical uncertainties in the measured$ B_{c}^{+} $ yields. -
Systematic uncertainties affecting the measurement of
$ {{\cal{R}}} $ arise from the PID efficiency corrections, the track reconstruction efficiency, the difference in the$ \varXi_c^+ \to p K^{-}\pi^{+} $ Dalitz distribution between data and simulation, the variation of the efficiency with respect to the$ \varXi_{bc}^+ $ mass, the mass resolution used in the fit to the$ \varXi_{bc}^+ $ mass spectrum, and the fit model assumed to evaluate the normalisation yield. The total systematic uncertainty is calculated as the quadratic sum of each individual uncertainty presented in Table 3, assuming no correlation between the contributions.Source $ {\cal{R}} $ (%)PID 4.0 Tracking 0.8 $ \varXi_c^+ \to p K^{-}\pi^{+} $ Dalitz distribution0.5 $ \varXi_{bc}^+ $ mass0.4 Mass resolution 1.5 $ B_{c}^{+} $ signal shape0.2 Total systematic uncertainty 4.4 Table 3. Systematic uncertainties on the measurement of the production ratio,
$ {\cal{R}} $ .The largest systematic uncertainty is due to the PID efficiency correction. There are several sources of systematic uncertainty associated to this correction, mainly due to the limited size of the calibration samples, the assumption of no correlations between PID variables of each final state particle, and limitations in the method used to correct the PID variables. The largest contribution to the PID efficiency correction arises from the comparison between the efficiency obtained with the PID variables resampled assuming no correlations between the PID variables for each final state particle, and an alternative correction method that takes into account such correlations. This alternative method requires corrections in a higher number of dimensions of phase space, and can suffer from statistical fluctuations due to limited size of the calibration samples. This comparison gives a 3.6% contribution to the PID efficiency correction uncertainty. Summing all the contributions in quadrature, the total systematic uncertainty associated to the PID efficiency correction is 4%.
Two sources contribute to the systematic uncertainty associated to the tracking efficiency. The first uncertainty is statistical, arising from the limited size of the samples used to derive the efficiency correction. The second is due to hadronic interactions with the detector material [68]. Considering that two out of the three final-state hadrons in the signal and the normalisation modes are common, the effect cancels out in the ratio except for the proton coming from the
$ \varXi_c^+ $ decay and the positively charged kaon from the$ D_{s}^{+} $ decay. These two uncertainties are added in quadrature and the total systematic uncertainty due to the tracking efficiency is 0.8%.The uncertainty contribution due to the
$ \varXi_c^+ \to p K^- \pi^+ $ decay comes from an imperfect modelling of the Dalitz shape in the simulation. A new signal efficiency is obtained using a weighting technique to match the simulated Dalitz distribution with the one from data, and the resulting difference of 0.5% is taken as a systematic uncertainty.As described earlier, the
$ \varXi_{bc}^+ $ selection efficiency is found to depend on the$ \varXi_{bc}^+ $ mass at a level of 0.4%, which is neglected in the efficiency ratio, and is taken as a systematic uncertainty. The uncertainty coming from possible variations of the mass resolution, used in the$ m(J/\psi \varXi_c^+) $ fit, are obtained by varying the mass resolution by$ \pm $ 10%. The largest difference between the local significance from the p-value scan obtained with different mass resolutions, 1.5%, is taken as a systematic uncertainty. The signal yield of the normalisation mode is affected by the fit model. This is evaluated by considering a sum of two Gaussian functions with the same mean but different resolutions, rather than the default DSCB function. The difference between the two measured yields, 0.2%, is taken as a systematic uncertainty. The total systematic uncertainty on the measurement of the production ratio$ {\cal{R}} $ is 4.4%.
Search for the doubly heavy baryon ${\boldsymbol\varXi_{\boldsymbol {bc}}^{\bf +}}$ decaying to ${\boldsymbol J/\boldsymbol\psi \boldsymbol\varXi_{\boldsymbol c}^{\bf +}}$
- Received Date: 2022-04-19
- Available Online: 2023-09-15
Abstract: A first search for the