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A Measurement of the Time-Dependence of Oscillations using Low- Electron-Muon Data


Abstract:

We present a measurement of the time-dependence of oscillations in collisions at using low- electron-muon data. The mass difference , between the heavy and light neutral mesons, is determined by fitting the fraction of like-sign leptons versus B proper- . From this we obtain , or .

1 Introduction

We use the low- electron-muon data collected by CDF during Run I in order to measure the mixing parameter . The strategy of the analysis is to form jets around the two leptons and reconstruct at least one B decay vertex in these jets. The flavour of the b quark in the vertexed jet, at the time of decay, is given by the charge of the associated lepton, while the quark type at production is given by the charge of the opposite lepton.

2 Sample Composition

The data sample used in the analysis was collected with an electron-muon trigger. The trigger selects events with an electron with transverse energy with respect to the beam direction ( ) greater than and a muon with transverse momentum ( ) greater than in Run IB ( in Run IA).

After the application of electron and muon quality cuts the sample consists of , and fake events. We define the relative fractions of events as:

The reason for this categorization of the events is that, since the sign of the lepton is used to determine the sign of the underlying quark, if the lepton is not real this sign correlation has been lost.

2.1 Fractions of Fake Leptons

The fraction of real electrons is measured to be from their ionization loss ( ) in the Central Tracking Chamber. For the real muon fraction we use the relative numbers of muon candidates observed in the inner and outer central muon detectors and the probabilities for muons and hadrons to penetrate the steel that is located in front of the outer detector. The real muon fraction is measured to be . Finally, the fraction of fake electrons in events with real muons is measured using similar techniques and is found to be negligible ( ). This implies that the fake electron events are fully contained in the fake muon events and we do not need to treat them separately.

2.2 Fits to the muon Distributions

The sample composition is determined by fitting the distribution of the muon. The variable is defined as the transverse momentum of the muon with respect to the direction of the highest track in a cone of radius 0.7 in space ( is the azimuthal angle with respect to the beam axis and is the pseudorapidity) around the muon direction. We use HERWIG Monte Carlo in order to obtain the distribution for and events and a fake data sample in order to obtain the fake distribution. The shapes for the various components of the data are shown in Figure 1. The data is fitted to these templates, with the following extra constraint: all templates are divided into like-sign (LS) and opposite-sign (OS), based on the lepton charges. The fit demands that events only contribute to the OS component, that the fakes are sign-symmetric, i.e. contribute equally to the OS and LS distributions, and that the events have a LS/OS ratio as given by the Monte Carlo. The LS/OS ratio implicitly contains information about the sequential decay fraction and the average mixing parameter, . These are varied in order to assign a systematic error to the values extracted from the fit. The results of the fits are shown in Figure 2 for OS and LS electron-muon events. In the full sample (LS+OS) the relative fractions are:

2.3 Fractions of Sequential Leptons

The fraction of sequential leptons (i.e. leptons coming from the b decay chain but not directly from the b-quark) is measured from the Monte Carlo which uses the latest CLEO decay tables. The fraction of sequentials is 20% (8%) on the muon (electron) side. After requiring a reconstructed secondary vertex in the event the fraction of sequentials increases by a relative 20% on the vertex side. Since these leptons are mostly coming from the process they have the wrong-sign with respect to the decaying b-quark and hence reduce significantly the statistical power of the analysis. We reduce the fraction of sequentials on the muon side by a cut on . The distribution for direct and sequential muons is shown in Figure 3. We demand:

The latter are events with no other track in a cone of 0.7 around the muon. This requirement is 75% efficient for direct muons and rejects 50% of the sequentials. This cut also changes the relative fractions of , and fake events. We use the sample composition before applying the cut and the efficiency of the cut for each of the three components of the data in order to extract the sample composition after the application of the cut. We also apply the relevant vertexing efficiencies to the fractions of events after the cut in order to estimate the sample composition after the cut and the vertexing requirement. The above procedure is done separately for the electron and muon-jets.

2.4 Measuring the Fake Fraction using Vertexing Efficiencies

We use the different vertexing efficiencies in , and fake events in order to measure the b-purity of the data:

where:

Solving the first of the above equations for gives:

which is a hyperbola in the space. In Figure 4 we plot the hyperbolas corresponding to the electron and muon-jet tag efficiencies as well as the double tag efficiencies. The measured fraction can be converted to the wanted fake fractions after vertexing using the following equation:

This result is insensitive to the amount of in the sample. We vary the fraction from ( ) in the estimate of the systematic error of the method.

2.5 Fits to the secondary vertex mass distributions

The fraction of events in the vertexed sample is also measured by fitting the mass of the tracks in the secondary vertex. The secondary vertex mass distributions are shown in Figure 5 for electron and muon-jets separately. This quantity discriminates well the component of the data from the fakes and . We fit these distributions for the fraction by fixing the fraction of fakes to what we measured by the method using the the vertexing efficiencies. The fit results and the relative contributions are shown in Figure 6.

We combine the fractions of events, measured using the various methods described above, in order to obtain the final sample composition after applying the vertexing requirement to either jet. This is summarized in Table 1 and is different for cases where the vertex is on the electron or the muon-jet.

3 Reconstruction of the B Hadron Proper Decay Time

The proper decay time (proper- ) of the B hadron is given by:

where is the B decay vertex in the transverse plane (with respect to the primary vertex) and , are the mass and transverse momentum of the B hadron, respectively. We reconstruct the B decay and the B hadron momentum from which the factor is derived.

3.1 Reconstruction of the B Hadron momentum

The B hadron momentum is reconstructed using a track clustering algorithm. Charged trajectories with are clustered to form jets in a cone of radius 0.7 in space. The performance of the method is studied using HERWIG Monte Carlo. The jet that contains the electron (muon) track is defined as the electron (muon)-jet. In Figure 7 we plot the ratio of the electron-jet divided by the original B hadron . The uncorrected distribution has a mean of 0.81 and a sigma of 21%. We apply a correction to , as a function of the jet mass, so that the mean of is . The jet mass is strongly correlated to the under/overestimate of because its difference from the B mass is a measure of how many of the B decay products we have missed or how many extra particles we have picked up. The dependence of is almost linear on the jet mass and is also shown in Figure 7. We use the inverse of the points of this histogram in order to correct the for the under/overestimate of . After the correction is applied the distribution is centered at 1 and the sigma is 21%. The same procedure is followed for the muon-jet. The results are shown in Figure 8. The final resolution on the muon-jet is 24%.

3.2 Reconstruction of the B Hadron Decay Vertex

The B decay vertex is reconstructed from tracks that are significantly displaced from the primary vertex along with the lepton tracks. All the tracks must be reconstructed in the silicon microstrip detector. The vertexing efficiency is measured from Monte Carlo to be about for jets with direct leptons and about for jets with sequential leptons. The efficiency is calculated with respect to jets that have at least two tracks reconstructed in the silicon microstrip detector. The resolution achieved, is shown for direct and sequential leptons in Figure 9.

The vertexing efficiency versus measured- is obtained from the Monte Carlo and is shown in Figure 10. The efficiency is small close to due to the selection of displaced tracks, but rises very fast and reaches the plateau in less than one b lifetime. The solid curve indicates the efficiency parametrization and the dashed lines the variations of the efficiency shapes that will be used in the estimate of the systematic errors.

4 Fitting Method and Results

The proper-time distribution of the decay in Like-Sign (LS) and Opposite-Sign (OS) events and the time-dependence of LS/TOT is predicted by building up the probability density of getting a wrong-sign (WS) and a right-sign (RS) lepton on the vertex side and the integrated probability of getting a WS and a RS lepton on the flavor-tag side. The following equations apply separately to electron and muon vertex tags, since the sample compositions are different in the two cases. Once the total LS and OS probabilities are constructed for the two samples, they are combined into one LS/TOT prediction which is used in forming the fit . In a event we can get Like-Sign leptons if one of the leptons is WS and the other is RS with respect to the decaying b-quark. Leptons from events contribute only to OS events, whereas leptons from fakes have a LS fraction which is measured to be (from several fake samples with a reconstructed secondary vertex).Then, the LS and OS probability densities are:

The right and wrong-sign probabilities on the vertex and flavor-tag side depend on the sample composition of the vertexed samples. The Like-Sign fraction, derived from the above equations is used to fit the LS/TOT fraction of leptons versus reconstructed .

The parameters used in the fit are:

Several fit parameters are highly correlated with , particularly anything which affects the overall LS/TOT normalization, e.g. . If only and are allowed to float in the fit, the correlation between them is -87%. This occurs because if changes, the entire LS/TOT curve shifts up or down. If is the only variable which can compensate, it is forced to change to fit the overall LS/TOT normalization rather than its shape. If several such parameters are allowed to float in the fit, they can take some of the normalization burden off , and allow it to fit the shape more effectively. The following parameters are allowed to float in the fit within their constraints:

We consider the measurements of those quantities to have true gaussian errors, and penalize the fit based on those errors. The fraction of sequential muons is not varying independently from the electron sequential fraction in the fit because the uncertainty in the fraction of sequential electrons and muons has a common origin. We constrain their ratio to be which is obtained from the Monte Carlo and allow only the fraction of sequential electrons to vary. We treat similarly the fake fractions in the samples with a secondary vertex on the muon and electron-jet ( and respectively) and fix the fraction to 47%. These ratios are varied in the evaluation of the systematic errors.

The fit to the Run I Electron-Muon data is shown in Figure 11. The final data sample consists of 10180 events. In about of these events there is a reconstructed vertex on both sides. The fit result is:

and the fit is 1.06 per degree of freedom. The error returned by the fit of has a statistical and a systematic component which is due to the other parameters that are floating in the fit. In Figure 12 we compare the measured distributions for all and Like-Sign events to the fit predictions.

4.1 Statistical and Systematic Errors

We generate multiple experiments with a toy Monte Carlo in order to verify that the fit result and error are within the expected range. The spread of the returned values gives an estimate of the statistical error. Figure 13 shows the results we get from 110 experiments, each generated with the same number of events that we have in the data (10180 events) and . The mean measured is . The shift of is under study and hence we do not correct the data result by it but instead we assign a systematic error of . From the distributions of errors and fit 's we see that the data fits give results within the expected range. Finally, the ratio of the expected minus the measured value over the error returned by the fit has a sigma of . The sigma would be 1 if the error returned by the fit was purely statistical. Hence, this is a measure of the statistical component of the fit error. The systematic error due to the parameters which are allowed to float in the fit is then times the error returned by the fit. This procedure is just splitting the error returned by the fit into a statistical and a systematic component. We also verify that the statistical error scales with by repeating 106 experiments with 4 times the data statistics. The RMS of the values returned by the fit is reduced by a factor of and the mean error on is reduced by a factor of . The systematic errors due to the other input parameters to the fit are summarized in Table 2 and are added in quadrature to the systematic component of the fit error in order to obtain the final systematic error in the measurement of .

5 Conclusion

We have measured the mixing parameter using the low- electron-muon data collected by CDF in Run I, by fitting the fraction of like-sign electron-muon events as a function of proper decay time. Parameters in the fit were allowed to float constrained to their errors. The result for the mass difference between the heavy and light meson is:

which translates to a measurement of the mixing parameter:



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