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Measurement of the absolute branching fraction of D+ → K̅0 e+νe via 0π0π0*

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Article funded by SCOAP3 and published under licence by Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd
, , Citation M. Ablikim et al 2016 Chinese Phys. C 40 113001 DOI 10.1088/1674-1137/40/11/113001

1674-1137/40/11/113001

Abstract

By analyzing 2.93 fb−1 data collected at the center-of-mass energy with the BESIII detector, we measure the absolute branching fraction of the semileptonic decay D+ → K̅0 e+νe to be ℬ(D+ → K̅0 e+νe) = (8.59 ± 0.14 ± 0.21)% using , where the first uncertainty is statistical and the second systematic. Our result is consistent with previous measurements within uncertainties..

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1. Introduction

The study of semileptonic decays of D mesons can shed light on the strong and weak effects in charmed meson decays. The absolute branching fraction ℬ of the semileptonic decay D+ → K̅0e+νe can be used to extract the form factor of the hadronic weak current or the quark mixing matrix element |Vcs| [1], which are important to calibrate the lattice quantum chromodynamics calculation on and to test the unitarity of the quark mixing matrix. In addition, the measured ℬ(D+ → K̅0e+νe) can also be used to test isospin symmetry in the D+ → K̅0e+νe and D0→ Ke+νe decays [25]. Therefore, improving the measurement precision of ℬ(D+→ K̅0e+νe) will be helpful to better understand the D decay mechanisms.

Measurements of ℬ(D+ → K̅0e+νe) via have been performed by the MARKIII, BES, CLEO and BESIII Collaborations [26]. Recently, a measurement of has been carried out by the BESIII Collaboration [7]. However, no measurement of ℬ(D+ → K̅0e+νe) using has been reported so far. As a first step, we present in this paper a measurement of ℬ(D+ → K̅0e+νe) using , based on an analysis of 2.93 fb−1 of e+e collision data [8, 9] accumulated at the center-of-mass energy with the BESIII detector [10]. Since the measurement with the D0 → Ke+νe decay has achieved an accuracy of about 0.6% in our previous work [11], this analysis only aims to measure the absolute branching fraction for D+→K̅0e+νe.

2. BESIII detector and Monte Carlo

The BESIII detector is a cylindrical detector with solid-angle 93% of 4π that operates at the BEPCII collider. It consists of several main components. A 43-layer main drift chamber (MDC) surrounding the beam pipe performs precise determinations of charged particle trajectories and provides ionization energy loss (dE/dx) measurements that are used for charged particle identification (PID). An array of time-of-flight counters (TOF) is located radially outside the MDC and provides additional charged particle identification information. A CsI(Tl) electromagnetic calorimeter (EMC) surrounds the TOF and is used to measure the energies of photons and electrons. A solenoidal superconducting magnet located outside the EMC provides a 1 T magnetic field in the central tracking region of the detector. The iron flux return of the magnet is instrumented with about 1272 m2 of resistive plate muon counters (MUC) arranged in nine layers in the barrel and eight layers in the endcaps that are used to identify muons with momentum greater than 0.5 GeV/c. More details about the BESIII detector are described in Ref. [10].

A GEANT4-based [12] Monte Carlo (MC) simulation software, which includes the geometric description and a simulation of the response of the detector, is used to determine the detection efficiency and to estimate the potential backgrounds. An inclusive MC sample, which includes generic ψ(3770) decays, initial state radiation (ISR) production of ψ(3686) and J/ψ, QED (e+e → e+e, μ+ μ, τ+τ) and qq̅ (q = u,d,s) continuum processes, is produced at . The MC events of ψ(3770) decays are produced by a combination of the MC generators KKMC [13, 14] and PHOTOS [15], in which the effects of ISR [16] and Final State Radiation (FSR) are considered. The known decay modes of charmonium states are generated using EvtGen [17, 18] with the branching fractions taken from the Particle Data Group (PDG) [19], and the unknown decay modes are generated using LundCharm [20]. The D+ → K̅0e+νe signal is modeled by the modified pole model [21].

3. Measurement

3.1. Single tag D mesons

With a mass of 3.773 GeV just above the open charm threshold, the ψ(3770) resonance decays predominately into D00 or D+D meson pairs. In each event, if a D meson can be fully reconstructed via its decay into hadrons (in the following called the single tag (ST) D), there must be a recoiling D+ meson. Using a double tag technique which was first employed by the MARKIII Collaboration [22], we can measure the absolute branching fraction of the D+ → K̅0e+νe decay. Throughout the paper, charge conjugation is implied.

The ST D mesons are reconstructed using six hadronic decay modes: K+ππ, , K+πππ0, , and K+Kπ. The daughter particles and π0 are reconstructed via and π0γγ, respectively.

All charged tracks are required to be reconstructed within the good MDC acceptance |cosθ| < 0.93, where θ is the polar angle of the track with respect to the positron beam direction. All tracks except those from decays are required to originate from the interaction region defined as Vxy < 1.0 cm and |Vz| < 10.0 cm. Here, Vxy and |Vz| are the distances of closest approach to the Interaction Point (IP) of the reconstructed track in the plane transverse to and along the beam direction, respectively. For PID of charged particles [23], we combine the dE/dx and TOF information to calculate Confidence Levels for the pion and kaon hypotheses (CLπ and CLK). A charged track is taken as kaon (pion) if it has CLK > CLπ (CLπ > CLK).

The charged tracks from decays are required to satisfy |Vz| < 20.0 cm. The two oppositely charged tracks, which are assumed as π+π without PID, are constrained to originate from a common vertex. A π+π combination is considered as a candidate if its invariant mass lies in the mass window , where is the nominal mass [24]. The π+π combinations with L/σL > 2 are retained, where σL is the uncertainty of the reconstructed decay length L.

Photon candidates are selected by using the EMC information. The shower time is required to be within 700 ns of the event start time, which is the interval of the trigger start time to the real collision time [25]. The shower energy is required to be greater than 25 (50) MeV in the barrel (endcap) region. The opening angle between the candidate shower and the closest charged track is required to be greater than 10°. A γγ combination is considered as a π0 candidate if its invariant mass falls in (0.115, 0.150) GeV/c2. To obtain better mass resolution for the D candidates, the γγ invariant mass is constrained to the π0 nominal mass [24] via a kinematic fit.

To suppress combinatorial backgrounds, we define the variable ΔE = EmKnπEbeam, which is the difference between the measured energy of the mKnπ (m = 1, 2; n = 1, 2, 3) combination (EmKnπ) and the beam energy (Ebeam). For each ST mode, if there is more than one mKnπ combination satisfying the above selection criteria, only the one with the minimum |ΔE| is kept. The ΔE is required to be within (−25,+25) MeV for the K+ππ, , and K+Kπ combinations, and be within (−55,+40) MeV for the K+πππ0 and combinations.

To measure the yield of ST D mesons, we perform maximum likelihood fits to the spectra of the beam energy constrained masses of the accepted mKnπ combinations, as shown in Fig. 1. Here, is the measured momentum of the mKnπ combination. In the fits, the D signal is modeled by the MC simulated MBC distribution convolved with a double Gaussian function, and the combinatorial background is described by an ARGUS function [26]. The parameters of the double Gaussian function and the ARGUS function are float. The candidates in the ST D signal region defined as (1.863,1.877) GeV/c2 are kept for further analysis. Single-tag reconstruction efficiencies ST are estimated by analyzing the inclusive MC sample. The ST yields NST and the ST efficiencies are summarized in Table 1. The total ST yield is , where the uncertainty is the quadratic sum of the uncertainties from all the MBC fits.

Fig. 1.

Fig. 1. Fits to the MBC spectra of the (a) K+ππ, (b) , (c) K+πππ0, (d) , (e) and (f) K+Kπ combinations. The dots with error bars are data, the blue solid curves are the fit results, the red dashed curves are the fitted backgrounds and the pair of red arrows in each sub-figure denote the ST D signal region.

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Table 1. Summary of the ST yields , the ST and DT efficiencies ( and ), and the reconstruction efficiencies of . The efficiencies do not include the branching fractions for (used in the reconstruction of ST D mesons), K̅0π0π0 and π0γγ. The uncertainties are statistical only. The index i represents the ith ST mode.

ST mode i
D → K+ππ 782669±990 50.61±0.06 13.39±0.07 26.45±0.14
91345±320 50.41±0.17 13.81±0.22 27.40±0.44
D → K+πππ0 251008±1135 26.74±0.09 6.23±0.06 23.29±0.25
215364±1238 27.29±0.07 6.88±0.07 25.21±0.28
113054±889 28.31±0.12 6.74±0.10 23.79±0.37
D → K+Kπ 69034±460 40.83±0.24 10.54±0.20 25.81±0.50

3.2. Double tag events

In the system recoiling against the ST D mesons, the D+ → K̅0e+νe candidates, called the double tag (DT) events, are selected via . It is required that there be at least four good photons and only one good charged track that have not been used in the ST selection. The good charged track, photons and π0 mesons are selected using the same criteria as those used in the ST selection. If there are multiple π0π0 combinations satisfying these selection criteria, only the combination with the minimum value of is retained, where the and are the chi-squares of the mass constrained fits on π0γγ. A π0π0 combination is considered as a K̅0 candidate if its invariant mass falls in (0.45, 0.51) GeV/c2. For electron PID, we combine the dE/dx, TOF and EMC information to calculate Confidence Levels for the electron, pion and kaon hypotheses (CLe, CLπ and CLK), respectively. The electron candidate is required to have CLe > 0.001 and CLe/(CLe + CLπ + CLK) > 0.8, and to have a charge opposite to the ST D meson. To partially recover the effects of FSR and bremsstrahlung, the four-momenta of photon(s) within 5° of the initial electron direction are added to the electron four-momentum measured by the MDC. To suppress the backgrounds associated with fake photon(s), we require that the maximum energy of any of the extra photons, which have not been used in the DT selection, be less than 300 MeV.

In order to obtain the information of the missing neutrino, we define the kinematic quantity

Equation ((1))

where Emiss and are the total energy and momentum of the missing particle in the event, respectively. Emiss is calculated by

Equation ((2))

where E0 and Ee+ are the energies carried by K̅0 and e+, respectively. is calculated by

Equation ((3))

where , and are the momenta of D+, K̅0 and e+, respectively. To obtain better Umiss resolution, is constrained by

Equation ((4))

where is the momentum direction of the ST D meson and mD+ is the D+ nominal mass [24].

To determine the number of DT events, we perform a maximum likelihood fit to the Umiss distribution of the accepted DT candidates, as shown in Fig. 2. In the fit, the DT signal and the combinatorial background are modeled by the MC simulated Umiss shapes, respectively. From the fit, we obtain the DT yield in data as

Equation ((5))

where the uncertainty is from Umiss fit.

Fig. 2.

Fig. 2. Fit to the Umiss distribution of the D+→K̅0e+νe candidates. The dots with error bars are data, the blue solid curve is the fit result, the black dotted and the red dashed curves are the fitted signal and background.

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3.3. Branching fraction

The efficiency of reconstructing the DT events, called the DT efficiency epsilonDT, is determined by analyzing the signal MC events. The DT efficiencies obtained from MC simulations are corrected by the differences of π0 reconstruction efficiencies between data and MC simulations for the signal side. Dividing epsilonDT by epsilonST, we obtain the reconstruction efficiency for D+ → K̅0e+νe in each ST mode, epsilonD+ → K̅0e+νe, as summarized in Table 1. Weighting them by the ST yields observed in data, we obtain the averaged reconstruction efficiency of D+ → K̅0e+νe

Equation ((6))

which does not include the branching fractions of K̅0π0π0 and π0γγ.

The branching fraction of D+ → K̅0e+νe is determined by

Equation ((7))

where NDT is the DT yield, is the total ST yield, is the averaged reconstruction efficiency of D+ → K̅0e+νe, ℬ(K̅0π0π0) and ℬ(π0γγ) are the branching fractions of K̅0π0π0 and π0γγ [24], respectively. Here, we assume that constitutes half the decays of the neutral kaons.

Inserting the numbers of NDT, , , ℬ(K̅0π0π0) and ℬ(π0γγ) in Eq. (7), we obtain

where the uncertainty is statistical only.

3.4. Systematic uncertainty

In the measurement of the branching fraction, the systematic uncertainty arises from the uncertainties in the fits to the MBC spectra of the ST candidates, the ΔE, MBC and K̅0(π0π0) mass requirements, the π0 reconstruction, the e+ tracking, the e+ PID, the requirement, the Umiss fit, the selection method, the MC statistics, the quoted branching fractions and the MC generator.

The uncertainty in the fits to the MBC spectra of the ST candidates is estimated to be 0.5% by observing the relative change of the ST yields of data and MC when varying the fit range, the combinatorial background shape or the endpoint of the ARGUS function. To estimate the uncertainties in the ΔE, MBC and K̅0(π0π0) mass requirements, we examine the change in branching fractions when enlarging the ΔE selection window by 5 or 10 MeV; varying the MBC selection window by ±1 MeV/c2 and using alternative K̅0(π0π0) mass windows (0.460, 0.505), (0.470, 0.500), (0.480, 0.500) GeV/c2, respectively. The maximum changes in the branching fractions, 0.3%, 0.2%, and 0.9%, are assigned as the systematic uncertainties. The π0 reconstruction efficiency is examined by analyzing the DT hadronic decays D0 → Kπ+ and Kπ+π+π versus D̅0 → K+ππ0 and . The difference of the π0 reconstruction efficiencies between data and MC is found to be (−1.0±1.0)% per π0. The systematic uncertainty in π0 reconstruction is taken to be 1.0% for each π0 after correcting the MC efficiency of D+ → K̅0e+νe to data. The data-MC differences of the e+ tracking and PID efficiencies are estimated by analyzing e+eγe+eevents. To consider different kinematic distributions of e+, the data-MC differences are re-weighted by the momentum and cosθ distributions of e+ in the D+ → K̅0e+νe decays. The re-weighted data-MC difference 0.5% is quoted as the systematic uncertainties of the e+ tracking and PID efficiencies. The uncertainty in the requirement is estimated to be 0.1% by analyzing the DT hadronic DD̅ decays. The uncertainty in the Umiss fit is assigned to be 0.5%, which is obtained by comparing with the nominal value of the branching fraction measured with an alternative signal shape obtained with different requirements on the MC-truth matched signal shape, an alternative background shape after changing the relative ratios of the dominant backgrounds (doubling each of the simulated backgrounds for D00, D+D and qq̅ continuum processes), and alternative fit range (± 50 MeV). The difference of 0.3% in the π0π0 acceptance efficiencies of the minimum requirement between data and MC, which is estimated by the DT hadronic decays D0 → Kπ+π0 versus D̅0 → K+ππ0, is assigned as a systematic uncertainty due to the selection method. In this analysis, the mesons from the signal side are formed with photon candidates reconstructed under the assumption that they originate at the IP. We examine the DT efficiencies of the signal MC events in which the lifetimes of meson from the signal side are set to the nominal value and 0, respectively. The difference of these two DT efficiencies, which is less than 0.2%, is taken as the systematic uncertainty of the reconstruction. The uncertainties in the MC statistics and the ℬ(K̅0π0π0) are 0.5% and 0.2% [24], respectively. In our previous work, the uncertainty in the signal MC generator is estimated to be 0.1%, which is obtained by comparing the DT efficiencies before and after re-weighting the q2(=(pDpK)2) distribution of the signal MC events of D0 → Ke+νe to the distribution found in data [11], where the pD and pK are the four-momenta of the D and K mesons. The systematic uncertainties are summarized in Table 2. Adding all uncertainties in quadrature, we obtain the total systematic uncertainty to be 2.5%.

Table 2. Relative systematic uncertainties (in %) in the measurement of ℬ(D+ → K̅0e+νe).

source uncertainty
MBC fit 0.5
ΔE requirement 0.3
MBC∈(1.863,1.877) GeV/c2 0.2
Mπ0π0∈(0.45, 0.51) GeV/c2 0.9
π0 reconstruction 2.0
tracking for e+ 0.5
PID for e+ 0.5
0.1
Umiss fit 0.5
selection method 0.3
reconstruction 0.2
MC statistics 0.5
ℬ(K̅0π0π0) 0.2
MC generator 0.1
total 2.5

3.5. Validation

The analysis procedure is examined by an input and output check using an inclusive MC sample equivalent to a luminosity of 3.26 fb−1. Using the same selection criteria as those used in data analysis, we obtain the ST yield, the DT yield and the weighted reconstruction efficiency of D+ → K̅0e+νe to be 1683631±1768, 5802±85 and (26.07±0.11)%, where no efficiency correction has been performed. Based on these numbers, we determine the branching fraction ℬ(D+ → K̅0e+νe) = (8.82±0.13)%, where the uncertainty is statistical only. The measured branching fraction is in excellent agreement with the input value of 8.83%.

To validate the reliability of the MC simulation, we examine the cosθ and momentum distributions of K̅0 and e+ of the D+ → K̅0e+νe candidates, as shown in Fig. 3. We can see that the consistency between simulation and data is very good.

Fig. 3.

Fig. 3. Comparisons of the cosθ and momentum distributions of K̅0 ((a), (b)) and e+ ((c), (d)) of the D+ → K̅0e+νe candidates. The dots with error bars are data, the red histograms are the inclusive MC events, and the light black hatched histograms are the MC simulated backgrounds. These events satisfy a tight requirement of −0.06 GeV < Umiss < +0.06 GeV.

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4. Summary and discussion

Based on the analysis of 2.93 fb−1 data collected at with the BESIII detector, we measure the absolute branching fraction ℬ(D+ → K̅0e+νe) = (8.59 ± 0.14 ± 0.21)%, using . Figure 4 presents a comparison of ℬ(D+ → K̅0e+νe) measured in this work with the results obtained by other experiments. Our result is well consistent with the other measurements within uncertainties and has a precision comparable to the PDG value [24]. Our measurement will be helpful to improve the precision of the world average value of ℬ(D+ → K̅0e+νe).

Combining the PDG values for ℬ(D0 → Ke+νe), ℬ(D+ → K̅0e+νe) [24], and the lifetimes of D0 and D+ mesons (τD0 and τD+) [24] with the value of ℬ(D+ → K̅0e+νe) measured in this work, we determine

Equation ((8))

where is the uncertainty averaged branching fraction based on the PDG value and the one measured in this work. Combining with the branching fraction measured in this work, the precision of the test of the isospin symmetry is improved.

Fig. 4.

Fig. 4. Comparison of the ℬ(D+ → K̅0e+νe) measured in this work with those measured by other experiments, where the slash band is the world averaged branching fraction with uncertainty. For the BESIII measurement using , we take .

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Acknowledgments

The BESIII collaboration thanks the staff of BEPCII and the IHEP computing center for their strong support.

Footnotes

  • Supported by National Key Basic Research Program of China (2009CB825204, 2015CB856700), National Natural Science Foundation of China (NSFC) (10935007, 11125525, 11235011, 11305180, 11322544, 11335008, 11425524, 11475123), Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program, CAS Center for Excellence in Particle Physics (CCEPP), Collaborative Innovation Center for Particles and Interactions (CICPI), Joint Large-Scale Scientific Facility Funds of NSFC and CAS (11179007, U1232201, U1332201, U1532101), CAS (KJCX2-YW-N29, KJCX2-YW-N45), 100 Talents Program of CAS, National 1000 Talents Program of China, INPAC and Shanghai Key Laboratory for Particle Physics and Cosmology, German Research Foundation DFG (Collaborative Research Center CRC-1044), Istituto Nazionale di Fisica Nucleare, Italy, Koninklijke Nederlandse Akademie van Wetenschappen (KNAW) (530-4CDP03), Ministry of Development of Turkey (DPT2006K-120470), National Natural Science Foundation of China (NSFC) (11405046, U1332103), Russian Foundation for Basic Research (14-07-91152), Swedish Resarch Council, U. S. Department of Energy (DE-FG02-04ER41291, DE-FG02-05ER41374, DE-SC0012069, DESC0010118), U.S. National Science Foundation, University of Groningen (RuG) and Helmholtzzentrum fuer Schwerionenforschung GmbH (GSI), Darmstadt, WCU Program of National Research Foundation of Korea (R32-2008-000-10155-0).

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