Search for the Contribution of H->WW*
to the cross section for high transverse
momentum dileptons in 1fb-1 of Run II data

Authors : D. Benjamin, P.Bussey,S.Chuang, T.Davies, D. Hidas, M. Kruse, A.Robson, R. St. Denis, A.S.Thompson : for the CDF Collaboration


Abstract

We study the sources of dileptons in p pbar collisions in 1 fb$^{-1}$of CDF Run II data, looking for evidence of a contribution of Higgs production from gg fusion and semileptonic decay to WW pairs where final state leptons are electrons and muons. We first measure the cross section times branching ratio for ppbar -> Z0 -> e+ e- and ppbar -> Z0 -> mu+ mu-



Introduction

Searches for evidence of the contribution of the Higgs to events observed at the Tevatron are intensifying as the data sample is increasing. A previous analysis of dileptons [6] put limits on the cross section at about a factor of 14 higher than the standard model prediction at $M_h=160$GeV/c$^2$. With improvements in NNLO computations [2] this became a factor of 10. Results for the direct search of a Standard Model Higgs presented in summer of 2006 for CDF alone as well as with CDF and D0 combined are shown in Figure 1. The limit on the cross section limit for production of a standard model higgs having $M_h=160$GeV/c$^2$ comes to within a factor of 4 of the Standard Model Prediction. CDF improvements and increased data volume for the low mass values of the Higgs have resulted in signficant improvements such that all values are now a within a factor of 20 of the Standard Model cross section in the range $114 < M_{h} < 200$ GeV/c$^2$.

Figure 2: Summer 2006 Electoweak working group fits to the Standard Model Higgs.
\begin{figure}\vspace*{-0.1cm}
\begin{center}
\mbox{\epsfig{file=v230/img/s06_blueband.eps,width=0.65\textwidth}}
\end{center}\end{figure}

The latest Electroweak working group fits [4] shown in Figure 2 place the preferred value at $M_h= 85 ^{+39}_{-28} $GeV/c$^2$, at 68% confidence level. Precision electroweak measurements indicate that that $M_h<$166 GeV/c$^2$ at 95% confidence. Direct searches indicate that $M_h>$114.4 GeV/c$^2$ at 95% confidence [1] [5]. Combining this with the precision electroweak measurements gives a limit of $M_h<$199 GeV/c$^2$ at 95% confidence.

At the Tevatron the dominant SM Higgs boson production mechanism is gluon-gluon fusion, gg$\rightarrow $H (Figure 3). A second Higgs production mechanism, vector boson fusion, produces the same final state plus two forward, hard jets, and contributes an extra 7% to the WW final state. A third Higgs production mechanism, quark-quark fusion, which produces a Higgs in association with a W boson, is about 2 orders of magnitude smaller. The branching ratios of the Higgs to W pairs dips to 15% at 120GeV/c$^2$ and rises to 90% at 160GeV/c$^2$, contributing to the search over the full range from 110 GeV/c$^2$ to 200 GeV/$c^2$. This is the range considered in this analysis.

Figure 3: SM Higgs production versus the mass of the Higgs boson.
\begin{figure}\vspace*{-0.1cm}
\begin{center}
\mbox{\epsfig{file=v230/old/HWWxsection.eps,width=0.65\textwidth}}
\end{center}\end{figure}

Figure 4: Feynman diagram for the dominant production mechanism and for a secondary contribution to the same final state of both final state W's decaying leptonically.
\begin{figure}\vspace*{-0.1cm}
\begin{center}
\begin{tabular}{c}
\epsfig{file=...
...ile=v230/img/Vbf, width=0.65\textwidth}\\
\end{tabular}\end{center}\end{figure}


Table 1: The SM Higgs production cross section and branching ratios of H$\rightarrow $WW are presented. The NNLO computations [3] are given in the columns $gg\rightarrow H^0$ and Vbf. These are multiplied by the branching ratios /citethwg in the column BR(WW) to obtian the values in the columns $gg\rightarrow H^0 \rightarrow WW$ and Vbf $\rightarrow H^0 \rightarrow WW$. Since the leptons can be e, $\mu $ or $\tau $, the values must be multiplied by 9 $\times \rm{BR}(W^-\rightarrow e^- \bar{\nu}_e)=
9\times 0.1054 $. This results in the values in the columns marked gg $\rightarrow H^0 \rightarrow WW \rightarrow llvv$ and Vbf $\rightarrow H^0 \rightarrow WW \rightarrow llvv$. These columsn are summed to give the final column labelled ``Tot''. This is the number of events produced in 1 $fb^{-1}$.
$M_h$ $gg\rightarrow H^0$ Vbf Br(WW) $gg\rightarrow H^0$ Vbf $\rightarrow H^0$ gg $\rightarrow H^0$ Vbf $\rightarrow H^0$ Tot
$\rightarrow WW$ $\rightarrow WW$ $\rightarrow WW$ $\rightarrow WW$
$\rightarrow llvv$ $\rightarrow llvv$
GeV/c$^2$ fb fb fb fb fb fb fb
100 1657 99.5 0.1000 165.7 9.95 17.46 1.05 18.51
110 1281 0.0440 56.36 9.71 5.94 1.02 6.96
120 1006 71.7 0.1320 132.79 9.46 13.99 1 14.99
130 801 0.2869 229.81 17.32 24.21 1.83 26.04
140 646 52.1 0.4833 312.21 25.18 32.9 2.65 35.55
150 525 0.6817 357.89 29.8 37.71 3.14 40.85
160 431 38.2 0.9011 388.37 34.42 40.92 3.63 44.55
170 357 0.9653 344.61 30.43 36.31 3.21 39.52
180 297 28.3 0.9345 277.55 26.45 29.24 2.79 32.03
190 249 0.7761 193.25 20.94 20.36 2.21 22.57
200 211 21 0.7347 155.02 15.43 16.33 1.63 17.96




In this analysis the data sample has been tripled and more sophisticated multidimensional techniques attempt to use the dilepton events more efficiently. The standard model prediction of signal cross-sections and branching ratios, and the expected number of events in 1 $fb^{-1}$ are shown in Table 1, for different Higgs masses for the gluon as well as vector boson fusion processes1 The detector acceptances needs to be taken into account. The dilepton acceptance is of order 12% at $M_h=160$ GeV/c$^2$.



Apparatus

an 
isometric view of the CDF II detector This analysis is carried out in Fermilab, where the TeVatron collides proton and antiproton beams at center-of-mass energy of 1.96 TeV in Run II.

This analysis is carried out using the data collected from May 02 to September 03 at CDF, one of the two collision points at which a delicate detector is constructed and well-maintained to get data. Shown to the right is an isometric view of the CDF II detector. Counting outwards from the beampipe central line, the detector is comprised of a silicon vertex detector (SVX II), a multiwire drift chamber (COT) for particle tracking, lead-scintillator electromagnetic calorimeters ({C/P}E{M/S}), iron-scintillator hadronic calorimeters ({C/W/P}HA) and drift-tube chambers and scintillators (C{M/S}{U/P/X}) for muon detection. Radiation hazards are dissolved with concrete shielding.



Event Selection

Events with two high pt leptons are chosen. Cuts are applied to

This is achieved as follows.

High Pt Leptons Event selection consists first of finding dilepton candidates which consist of

Elimination of b's: A Drell-Yan Sample We then proceed to study the dominant sources of dilepton events; however we do not try to compute and compare the b sources of events so in order to eliminate the b's, we require that the leptons:

The isolation cut is defined for calorimeter as the ratio of the calorimeteter energy, excluding the electron EM energy, in a cone of 0.4 around the electron, to the electron tower energy.

The isolation cut for the tracking is the sum of all transvers momenta of all tracks in a cone of 0.4 around the lepton, excluding the lepton track to the pt of the lepton.

Drell-Yan Removal: A WW sample This yields a sample of dilepton events that are dominated by Drell-Yan production. Drell-Yan production is characterized by the lack of missing energy because they tend to an angle between the leptons of 180 degrees and a balance of energy between the leptons. Hence we require that there be missing energy in the event. Since we are ultimately trying to isolate the contribution of Higgs decays, we are mindful of the Higgs masses and place a series of missing energy cuts on the dilepton samples as we work towards enhancing the contribution of the Higgs to the dileptons. Therefore the missing energy cut is placed at

Practically speaking, this cut ranges from 27.5 to 40 GeV for 110 < MH < 200 GeV/c2.

The remaining events are dominated by WW production and some top. The top contribution is reduced by applying jet cuts:

This results in a sample of WW dominated dileptons.

Higgs Discrimination To enhance the contribution of the Higgs decays to WW, the following cuts are applied to the events.

The angular correlations of the dileptons in the WW final states are different when mediated by the spin-0 Higgs than when produced by other electroweak interactions. We therefore fit the predicted angular distribution for a contribution from the spin-0 and continuum production in order to determine the sensitivity of the analysis to a contribution from Higgs production.


Plots

Legend for Plots Legend for plots gif eps


Jets

jet Et spectrum of 1-jet
        events jet Et spectrum of 1-jet plot gif eps residuals gif eps and 2-jet plot gif eps residuals gif eps

Number of jets Number of Jets before cuts plot gif eps residualsgif eps


Leptons

Leading lepton pt spectrum
        at initial level leading lepton pt spectrum after b rejection cuts, in Drell-Yan dominated dilepton sample: plot gif eps residuals gif eps

Break down into ee, emu and mumu

ee plot gif eps ee residuals gif eps

emu plot gif eps emu residuals gif eps

mumu plot gif eps mumu residuals gif eps


Leading lepton pt spectrum
        at final level Leading Lepton Et at final level: plot gif eps residuals gif eps

Break down into ee, emu and mumu

ee plot gif eps ee residuals gif eps

emu plot gif eps emu residuals gif eps

mumu plot gif eps mumu residuals gif eps


subleading lepton pt spectrum
        at initial level Subleading lepton pt spectrum after b rejection cuts, in Drell-Yan dominated dilepton sample

plot gif eps residuals gif eps


Break down into ee, emu and mumu


ee plot gif eps ee residuals gif eps

emu plot gif eps emu residuals gif eps

mumu plot gif eps mumu residuals gif eps



Subleading lepton pt spectrum after Higgs selection Subleading Lepton Et in WW dominated sample after Higgs selection plot gif eps residuals gif eps

Break down into ee, emu and mumu

ee plot gif eps ee residuals gif eps

emu plot gif eps emu residuals gif eps

mumu plot gif eps mumu residuals


R separation between leptons
        at initial level R separation between leptons after b rejection cuts, in Drell-Yan dominated dilepton sample

plot gif eps residuals gif eps

Break down into ee, emu and mumu

ee plot gif eps ee residuals gif eps

emu plot gif eps emu residuals gif eps

mumu plot gif eps mumu residuals gif eps


subleading lepton pt spectrum
        at initial level R separation between leptons in WW dominated sample after Higgs selection plot gif eps residuals gif eps

Break down into ee, emu and mumu

ee plot gif eps ee residuals gif eps

emu plot gif eps emu residuals gif eps

mumu plot gif eps mumu residuals


Z Cross Section

Z
        Cross Section for Various Dilepton types Z Cross Section for Various Dilepton types gif eps


DrellYan/WW/Higgs Selection

missing Et distribution at initial level missing Et distribution in Drell-Yan dominated sample after jet cuts for MH=160: plots gif eps residuals gif eps

by ee, emu, mumu

ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 120 plots gif eps residuals gif eps

for 200 plots gif eps residuals gif eps


Mll distribution at initial level Mll distribution after Missing Et cut, in WW-dominated sample for MH=160: plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 120 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 140 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 180 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 200 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps


Mll distribution at initial level Sum of lepton pt + missing Et distribution after Mll cut in WW dominated sample for MH=160: plots gif eps residuals gif eps

by ee, emu, mumu

ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 120 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 140 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 180 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps

for 200 plots gif eps residuals gif eps

by ee, emu, mumu ee plots gif eps ee residuals gif eps emu plots gif eps emu residuals gif eps mumu plots gif eps mumu residuals gif eps


Results

Dileptona and gg->H->WW->lvlv acceptance Dilepton and gg->H->WW->lvlv signal acceptance gif eps
signal cut efficiencies cut efficiences on signal MH = 160 GeV(ps)
Common uncertainties, same for ee, emu, mumu Common uncertainties(ps) and differing in ee, emu, and mumu Common uncertainties dependent on dilepton combination(ps)

Shape uncertainties Shape uncertainties(ps) grand summary table per 5 masses
grand summary table for 110-150 GeV110-150(ps)   grand summary table for 160-200 GeV160-200(ps)
summary table for each mass
summary table for 110 GeV110(ps)   summary table for 120 GeV120(ps)   summary table for 130 GeV130(ps)   summary table for 140 GeV140(ps)   summary table for 150 GeV150(ps) 
summary table for 160 GeV160(ps)   summary table for 170 GeV170(ps)   summary table for 180 GeV180(ps)   summary table for 190 GeV190(ps)   summary table for 200 GeV200(ps)  

dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level
dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level

dilepton azimuthal angle distribution at final level for 110<= Mh <=200 GeV/c2 for all leptons

dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level
dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level

dilepton azimuthal angle distribution at final level for 110<= Mh <=200 GeV/c2 for ee events

dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level
dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level

dilepton azimuthal angle distribution at final level for 110<= Mh <=200 GeV/c2 for emu events

dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level
dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level dilepton azimuthal angle distribution at final level

dilepton azimuthal angle distribution at final level for 110<= Mh <=200 GeV/c2 for mumu events

SM gg -> H -> WW production limits SM gg -> H -> WW production limits