From unal@pngs02.hep.upenn.edu Sun Oct 3 15:02:44 1993 Received: from PNGS02.HEP.UPENN.EDU by cepheid.physics.utoronto.ca with SMTP id AA20293; Sun, 3 Oct 93 15:02:44 -0400 Received: by pngs02.hep.upenn.edu (AIX 3.2/UCB 5.64/4.03) id AA15955; Sun, 3 Oct 1993 15:02:35 -0400 From: unal@pngs02.hep.upenn.edu (unal) Message-Id: <9310031902.AA15955@pngs02.hep.upenn.edu> To: liss@fnald.fnal.gov, claudioc@fnald.fnal.gov, yagil@fnald.fnal.gov, dan@fnald.fnal.gov, bed@fnald.fnal.gov, hughes@fnald.fnal.gov, winer@fnald.fnal.gov, williams@williams.hep.upenn.edu, pekka@cepheid.physics.utoronto.ca Cc: unal@pngs02.hep.upenn.edu Subject: SVX/SLT background correlations Date: Sun, 03 Oct 93 15:02:34 -0500 Status: R Hi, I have been trying to investigate the background correlation between SVX and SLT in W+jets and its impact on the significance of the excess of events in a combined analysis. * The first ingredient needed is the amount of true heavy flavor tags and fake tags for each tagger.Here is what I have done to estimate these various contributions. Some of the numbers are not really more than educated guesses. I started from the mistag rate for SVX, defined from the -DL rate from jets => 0.73 +- 0.09 events in W+3,4 jets. To define the number of Wbbbar,Wccbar I took the average between the raw MC value and the value from the (+dl)-(-dl) rate from jets, with the difference as systematic error. Since to reproduce the +dl background estimate, one has to multiply by 2.8 the raw MC estimates of Wbbbar,ccbar, I used as central value 1.9*MC value with an error of +-0.9*MC value >From this, the number of Wbbbar before tagging is 2.63+-1.25 and the number of Wccbar before tagging is 4.29+-2.03 The number of Wc before tagging is 4.16+-1.24 For all these W+heavy flavor events, I assumed that the tagging efficiencies of SVX and SLT are uncorrelated, as indicated by top MC and used the following estimates eff (Wbbbar SVX)=0.20+-0.04 eff(Wbbbar SLT)=0.15+-0.05 (???) eff (Wccbar SVX)=0.04+-0.016 eff(Wccbar SLT)=0.052+-0.02 eff (Wc SVX)=0.035+-0.012 eff(Wc SLT)=0.020+-0.004 For the fake rate of SLT, I used the value from generic jets * 0.75+-0.15 (from the estimated purity of the tagger) Finally, I added the other background sources (0.13+-0.05 for SVX and 0.33+-0.12 for SLT assuming that they are uncorrelated). From the previous numbers, the total backgrounds are 1.70+-0.41 for SVX and 2.94+-0.51 for SLT. The W+b/c content is ~ 0.85 events for SVX and ~ 0.70 events for SLT The fact that I get a SLT background close to the direct estimate (3.0 events) is (if I used the correct efficiencies) a cross-check of the overall consistency of the SVX/SLT efficiencies, the heavy flavor purities and the overall background rates. * To compute the probability of a background fluctuation, I ran a small monte-carlo to simulate a large number of experiments with only background. This MC generates the total number of Wbbbar,Wccbar and Wc each with Poisson statistic. Each event is tagged by SVX, SLT of both according to the estimated efficiencies by generating random numbers. The number of fakes is computed in a similar way, starting from the total (52) number of W+3,4 jets. To account for the (small) fake correlation from the track multiplicity dependance of the fake rates, I assumed that the probability of the double fake is two times higher than the product of the individual probabilities (the factor 2 is the factor that I get in generic jet events). Finally, I accounted for the systematic uncertainties by smearing the various parameters with gaussian fluctuations. The Wbbbar and Wccbar errors are taken to be 100% correlated as well as the various SVX tagging efficiency errors. * From this MC, I get the following probabilities P (Number of SVX tags >=6) = 1.15 % P (Number of SLT tags >=7) = 3.57 % P (Number of SVX + SLT tags >=13)=0.29 % The average number of overlaps for all the experiments is 0.15 (3.3 % of the average total number of tags. Naively, one would have expected a little less than twice the jet by jet overlap in a jet sample which is 2 %). For the experiments with 13 tags or more, the average number of overlaps is ~ 1.0. Clearly, these background fluctuations are "dominated" by Wbbbar,ccbar fluctuations which produce at the same time a larger number of overlaps. Around 7% of these background experiments have 3 or more overlaps. Given the fact that 3 overlaps is already more than we expect from top, I dont think that we should put to much quantitative emphasis on this 7%. However this large number of overlaps is certainly a good indication that we are really seing an excess of Wbbbar event. * Adding the dilepton background (0.61+-0.13) and assuming that it is completely uncorrelated with the others, the probability to get 15 "tags" or more from all the background sources is 0.119 % Guillaume