2 The CDF Experiment at Fermilab Contents - Harvard University ...
2 The CDF Experiment at Fermilab Contents - Harvard University ...
2 The CDF Experiment at Fermilab Contents - Harvard University ...
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
46 Section 2: <strong>CDF</strong> Physics Analysis<br />
Indirect Lepton Veto<br />
Since all the Standard Model backgrounds contain in the nal st<strong>at</strong>e along with 6E T and<br />
jets also a lepton we dene an isol<strong>at</strong>ed track criterion to select the remaining standard model<br />
processes in the d<strong>at</strong>a. <strong>The</strong> composition of the complementary sample of events th<strong>at</strong> do not<br />
contain such an isol<strong>at</strong>ed charged track is expected to be QCD events with large 6E T arising<br />
from pure jet calorimeter resolution. Any excess of events in this sample will be the signal<br />
candid<strong>at</strong>es.<br />
We are modelling the QCD background using large monte carlo st<strong>at</strong>istics samples of<br />
inclusive 3 jet QCD events and by varying the jet resolution functions in order to get the<br />
shape vari<strong>at</strong>ion of the 6E T tails. This is a critical part into arriving to the result of the search<br />
for the supersymmetric signal. Completion of this part of the analysis and optimiz<strong>at</strong>ion of<br />
the requirements for identic<strong>at</strong>ion of signal candid<strong>at</strong>es will allow us to compare the d<strong>at</strong>a with<br />
the total background predictions. <strong>The</strong> QCD prediction of the low 6E T spectrum for events<br />
with <strong>at</strong> least three jets compared with the d<strong>at</strong>a is shown in gure 24. <strong>The</strong> comparison of<br />
the sample of events th<strong>at</strong> do contain an isol<strong>at</strong>ed track with Standard Model predictions for<br />
the backdrounds mentioned above (where we expect very low or none QCD contribution) is<br />
shown in g 25.<br />
We still need to study and estim<strong>at</strong>e the system<strong>at</strong>ic uncertainties for the Standard Model<br />
predictions. We expect a result of this search by the Fall of 1999.