## Measurement of WW+WZ Production Cross Section in lvjj Channel in L=4.6 fb-1of CDF Run II Data Using a Matrix Element Technique

Barbara Alvarez3, Florencia Canelli1, Ricardo Eusebi4, Craig Group4, Martina Hurwitz1, Bruno Casal Larana2, Enrique Palencia4, Bernd Stelzer5

1University of Chicago
4Fermilab
5Institute for Particle Physics Canada, Simon Fraser University

• Abstract
• Event selection
• Analysis Method
• Validation of the method
• Systematic uncertainties
• Results

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## Abstract

We present a measurement of the WW+WZ production cross section in the channel with an identified electron or muon, large missing transverse energy, and two jets in 4.6 fb-1 of CDF II data. The analysis employs a matrix element technique which calculates event probability densities for signal and background hypotheses. We combine the probabilities to form a discriminant variable which is evaluated for signal and background Monte Carlo events. The resulting template distributions are fit to the data using a binned likelihood approach. We measure a cross section of 16.5+3.3-3.0 pb. The probability that the observed excess originated from a background fluctuation (p-value) is 2.9×10-8 (5.4σ).

## Event Selection

This analysis uses events from leptonic decay of one of the W bosons and hadronic decay of the other W or Z boson. We require a single, well-isolated lepton with high transverse energy, large missing transverse energy, and exactly two high-transverse-energy jets. Events with additional jets or leptons are vetoed to suppress Z+jets and top pair backgrounds. Cosmic ray and conversion events are also removed. The QCD multi-jet background is suppressed partially with the high missing transverse energy cut, and with additional cuts on the transverse mass of the leptonic W candidate and on the the direction of the missing energy.

Backgrounds need to have well-modeled shapes and normalizations. The largest background is due to W+jets events, which are modeled using the Alpgen fixed-order Monte Carlo generator and a Pythia parton shower. The normalization of the W+jets background is a free parameter in the final signal extraction. The QCD multi-jet background is much smaller; it is modeled using events from jet triggers where the lepton identification requirements have been loosened. The normalization of the QCD multi-jet background is determined by fitting the missing transverse energy spectrum in the data to a sum of expected contributions. Z+jets, top pair, and single top backgrounds are all relatively small backgrounds; both their shapes and normalizations are modeled using the Monte Carlo.

Fit to the missing transverse energy to determine the normalization of the QCD multi-jet background in four lepton categories.

 Process Expected number of events WW signal 1262 ± 114 WZ signal 196 ± 22 W+jets 35637 ± 686 Z+jets 1700 ± 223 QCD multijet 1514 ± 606 top pair 293 ± 39 single top 276 ± 41

Number of expected events for signal and background processes.

## Analysis Method

This analysis is based on a Matrix Element method applied to maximize the use of information in the events [2,3]. We calculate event probability densities under the signal and background hypotheses as follows. Given a set of measured variables of each event (the 4-vectors of the lepton and the two jets), we calculate the probability densities that these variables could result from a given underlying interaction (signal and background). The probability is constructed by integrating over the parton-level differential cross-section, which includes the matrix element for the process, the parton distribution functions, and the detector resolutions. This analysis calculates probabilities for several different underlying processes: WW, WZ, single top (s-channel and t-channel), Wbb-bar, Wcc-bar, Wc+jet, Wgj, and Wgg.

Transfer functions are used to include detector effects. Lepton quantities and jet angles are considered to be well measured. However, jet energies are not, and their resolution is parameterized from Monte Carlo simulation to create a jet resolution transfer function. We integrate over the quark energies and over the z-momentum of the neutrino to create a final probability density.

We use the probabilities to construct a discriminant variable for each event, referred to as the Event Probability Discriminant, or EPD. WW and WZ are combined to form a single signal probability. The EPD is defined as:

The templates of the EPD for background and signal processes (normalized to unit area) are shown below. The signal distribution falls less steeply than the background.

Templates of the EPD for signal and background processes, normalized to unit area.

The effectiveness of the discriminant in separating signal and background can also be shown by plotting the invariant mass of the two jets in bins of EPD. The majority of the background is in bins of low EPD, and quickly the discriminant isolates events with a mass close to the W mass, as expected for signal events. As the value of the EPD increases, the signal-to-background ratio is expected to improve.

Shape of the dijet invariant mass in bins of EPD

To quantify the WW+WZ content in the data, we perform a binned maximum likelihood fit. We fit a linear combination of signal and background shapes of the event probability discriminant to the data. The background normalizations (except for W+jets) are Gaussian constrained in the fit, with the width of the Gaussian determined by the uncertainties on the process cross section and the selection efficiency. The W+jets normalization is a free parameter. All sources of systematic uncertainty are included as nuisance parameters in the likelihood function. Sources of systematic uncertainties can affect the normalization and shape for a given process. Correlations between both are taken into account. The likelihood function is reduced through a standard Bayesian marginalization technique.

## Validation of the Method

We compare the distribution of many kinematic variables predicted by Monte Carlo simulation for signal and background to the data. In particular, we compare the distributions of the input variables to ensure the data matches the Monte Carlo prediction. We assign a shape uncertainty on the background if mismodeling is observed, using events with Mjj < 55 GeV and Mjj > 120 GeV.

ET and η of the two jets, ET of the lepton, missing transverse energy, dijet invariant mass, and Δ η between the two jets, shown as a stacked plot for the prediction with the data points superimposed. The hatched band corresponds to the uncertainty in the shape of the background.

Predicted and observed EPD for events with Mjj < 55 and Mjj > 120

## Systematic Uncertainties

Systematic uncertainties can affect both the normalization and the shape of background and signal processes. The normalization uncertainty includes changes to the event yield due to the systematic effect, and the shape uncertainty includes changes to the template histograms. Both of these effects are included in the likelihood function. A complete list of systematic uncertainties is given below.

• The jet energy scale systematic is obtained by changing the jet energy scale by 1 standard deviation (SD) and recalculating the event yield and the discriminant template histograms. We apply shape and normalization uncertainties to the signal template and background templates.
• We assign a shape uncertainty to the background templates associated with mismodeling in the pT of the dijet system and in the η of the second jet. The systematically changed template is derived from Monte Carlo events reweighted to agree with data in the region with Mjj < 55 and Mjj > 120.
• We vary the factorization and renormalization scele (Q2) in the Monte Carlo samples that have been created with the ALPGEN Monte Carlo program. An uncertainty on the shape of the W+jets background is applied.
• We increase or decrease the amount of initial state radiation in the Monte Carlo and recalculate the event yield for the signal.
• We increase or decrease the amount of final state radiation in the Monte Carlo and recalculate the event yield for the signal.
• We vary the eigenvectors in the CTEQ parton distribution function tables to determine the uncertainty from this effect. We also include the effect of using different versions of CTEQ and of using MRST with different values of ΛQCD. This results in a normalization uncertainty on the signal.
• We assign a small uncertainty to the signal acceptance associated with the jet energy resolution.
• We assign normalization uncertainties to background processes: for Z+jets, top pairs, and single top production the uncertainty in the production cross sections are used; for QCD multi-jets a 40% uncertainty is applied, and the W+jets normalization is a free parameter in the fit.
• We include an uncertainty on event detection efficiency due to the lepton ID scale factors that we apply to our Monte Carlo samples
• We include a 6% uncertainty on our measured luminosity.
We run pseudo-experiments to determine the expected effects of the systematic uncertainties. We find that the measurement is already nearly systematically limited, with an expected statistical uncertainty of 14% and expected systematic uncertainty of 16%. The most important systematic uncertainties are the jet energy scale uncertainty, contributing 8% to the total, the Q2 scale uncertainty, contributing 7%, and the luminosity uncertainty, contributing 6%. The total expected uncertainty is 21%.

## Results

 The likelihood fit of the sum of signal and background Event Probability Discriminant templates to data gave a cross section of $\sigma$WW+WZ = 16.5+3.3-3.0 pb. The significance of the signal is 5.4 σ.