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Violation in Mixing

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88 Ã Ë reconstruction and efficiency studies<br />

x 10 2<br />

1200<br />

1000<br />

800<br />

600<br />

400<br />

200<br />

0<br />

0.46 0.48 0.5 0.52 0.54<br />

Ks mass<br />

Figure 3-8. Invariant mass distribution of true Monte Carlo à Ë.<br />

3.3.4 Correction for the Monte Carlo efficiencies<br />

To evaluate the Ã Ë efficiency <strong>in</strong> data with respect to the Monte Carlo estimate, a set of corrections is<br />

produced with the <strong>in</strong>clusive analysis described above. The corrections are given <strong>in</strong> � b<strong>in</strong>s of the already<br />

def<strong>in</strong>ed -dimensional flight length: and they are simply the b<strong>in</strong>-by-b<strong>in</strong> ratios between the Ã Ë efficiency <strong>in</strong><br />

the on-resonance data over the Ã Ë efficiency <strong>in</strong> the MC samples. This ratio does not depend on lum<strong>in</strong>osity<br />

of the two samples. A correction ¦ is assigned <strong>in</strong> case there are no reconstructed Ã Ë <strong>in</strong> the �Ö b<strong>in</strong> <strong>in</strong><br />

data or <strong>in</strong> MC (i.e. high flight length values). They are also normalized to the first b<strong>in</strong>: that means that <strong>in</strong><br />

pr<strong>in</strong>ciple one could get the same correction values from the ratio between the number of reconstructed à Ë<br />

<strong>in</strong> the on-resonance data over the number of reconstructed Ã Ë <strong>in</strong> the MC samples. The normalization to the<br />

first b<strong>in</strong> is due to the fact that Ã Ë reconstruction has to be correlated to the track<strong>in</strong>g efficiency. S<strong>in</strong>ce the<br />

Ã Ë daughter candidates are selected from the list of all the charged tracks, the overall correction should take<br />

<strong>in</strong>to account also the differences of the charged track reconstruction <strong>in</strong> data and <strong>in</strong> Monte Carlo.<br />

This track<strong>in</strong>g correction is studied <strong>in</strong> different control samples and these analyses provide the correction<br />

value and the associated systematic error. For the ChargedTracks list (no selection cuts at all), it has been<br />

found that no correction is necessary but a systematic error of per track has to be <strong>in</strong>cluded <strong>in</strong>to the<br />

efficiency calculations. This leads to a systematic of per Ã Ë candidate.<br />

Thus, s<strong>in</strong>ce the normalization is done to the first b<strong>in</strong>, one should scale the pure Ã Ë correction for the track<strong>in</strong>g<br />

efficiency correction that has to be applied with<strong>in</strong> cm of flight length.<br />

The b<strong>in</strong>-by-b<strong>in</strong> number of reconstructed Ã Ë candidates is obta<strong>in</strong>ed with the usual double Gaussian fit<br />

with l<strong>in</strong>ear background to b<strong>in</strong>-by-b<strong>in</strong> <strong>in</strong>variant mass distributions: some examples of these fits are given<br />

<strong>in</strong> Fig. 3-13.<br />

Two sets of corrections are provided for each period (block 1 and block 2): the first set comes from ÃË reconstruction with no cuts except for the hadronic selection on the events, while the second set has an<br />

additional momentum cut (ÔÃË � ��Î� ). This method is used <strong>in</strong> order to provide corrections which are<br />

<strong>in</strong>dependent from the momentum range of the ÃË candidates taken <strong>in</strong>to account <strong>in</strong> the specific analyses.<br />

MARCELLA BONA

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