1 24 th September 2007 C.P. Ward Sensitivity of ZZ→llνν to Anomalous Couplings Pat Ward University of Cambridge Neutral Triple Gauge Couplings Fit Procedure.

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Presentation transcript:

1 24 th September 2007 C.P. Ward Sensitivity of ZZ→llνν to Anomalous Couplings Pat Ward University of Cambridge Neutral Triple Gauge Couplings Fit Procedure Results Outlook

2 24 th September 2007 C.P. Ward Neutral Triple Gauge Couplings ZZZ and ZZγ vertices forbidden in SM Production of on-shell ZZ probes ZZZ and ZZγ anomalous couplings: f 4 Z, f 5 Z, f 4 γ, f 5 γ All = 0 in SM Forbidden in SM SM ZZ production diagrams

3 24 th September 2007 C.P. Ward Anomalous Couplings f 4 violate CP; helicity amplitudes do not interfere with SM; cross-sections depend on f 4 2 and sign cannot be determined f 5 violate P; contribute to SM at one-loop level: O(10 -4 ) Couplings increase with energy. Usual to introduce a form factor to avoid violation of unitarity: f i (s’) = f 0i / (1 + s’/Λ 2 ) n Studies below use n=3, Λ = 2 TeV Also assume couplings are real and only one non-zero: use f 4 Z as example, expect results for others to be similar

4 24 th September 2007 C.P. Ward Anomalous Coupling MC Use leading order MC of Baur + Rainwater Phys. Rev. D (2000) pp→ZZ→ffff No parton shower, underlying event, detector simulation CTEQ6L PDFs SM prediction l = e, μ p T (l) > 20 GeV |η(l)| < 2.5 p T (νν) > 50 GeV

5 24 th September 2007 C.P. Ward Signature of Anomalous Couplings Anomalous couplings increase cross-section at high p T Fit p T distribution to obtain limits on NTGC p T (l) > 20 GeV |η(l)| < 2.5 p T (νν) > 50 GeV

6 24 th September 2007 C.P. Ward Fits to p T Distribution Aim: estimate limits on anomalous couplings likely to be obtained from early ATLAS data from fit to Z(→ll) p T distribution in ZZ→llνν channel: Generate `fake data’ samples Binned max L fit to sum of signal + background Determine mean 95% C.L. Use results from full MC (CSC samples) for event selection efficiency and background to obtain realistic limits Also assess effect of varying background and systematic errors

7 24 th September 2007 C.P. Ward Full Simulation Results  = 3.2%  = 2.6% S/B =2.25 S/B =1.96 Events expected in 100fb -1 of data 100 fb -1 Tom Barber Diboson Meeting 13 th August 2007

8 24 th September 2007 C.P. Ward Calculation of Signal Distribution Use BR MC to calculate LO cross-section at several values of f 4 Z p T (l) > 20 GeV, |η(l)| 50 GeV Fit to quadratic in f 4 Z to obtain cross-section at arbitrary f 4 Z Correct for NLO effects using ratio / BR(SM ) Expected number of events = cross-section x efficiency x luminosity

9 24 th September 2007 C.P. Ward Signal Efficiency Efficiency from full MC using Tom’s event selection Drops with p T due to jet veto Fit results have some dependence on binning Reasonable variations change limits for 10 fb -1 by 10 – 15% Efficiency = events passing selection cuts divided by events generated with p T (l) > 20 GeV, |η(l)| 50 GeV

10 24 th September 2007 C.P. Ward Background Distribution Too few full MC events pass cuts to determine background shape Before cuts, background shape fairly similar to signal for p T > 100 GeV Assume background / SM signal flat: (error from MC stats) ● Background level has only small effect on limits

11 24 th September 2007 C.P. Ward `Fake Data’ Samples Construct from expected numbers of SM signal and background events Add Gaussian fluctuations for systematic errors: Signal: 7.2% correlated (6.5% lumi, 3% lepton ID) plus MC stat error on efficiency in each bin Background: 41% correlated (MC stats) Add Poisson fluctuation to total number of events

12 24 th September 2007 C.P. Ward Fits to p T Distribution One-parameter binned maximum likelihood fit to (f 4 Z ) 2 Likelihood for each bin is Poisson convolved with Gaussians for nuisance parameters representing systematic errors: L i = ∫ df s ∫ df b G(f s,σ s ) G(f b,σ b ) P(n;f s ν s +f b ν b ) n = number of `data’ events ν s, ν b = expected signal, background σ s, σ b = fractional systematic errors Minimize L = - ln(Π i L i ) 95% C.L. from L - L min = 1.92 Negative (f 4 Z ) 2 allows for downward fluctuations Lower bound to prevent negative predictions Depends on f 4 Z

13 24 th September 2007 C.P. Ward Example Fit

14 24 th September 2007 C.P. Ward Test Fit Make `fake data’ with various input values of (f 4 Z ) 2 to test fit Mean fitted parameter in excellent agreement with input parameter (but distribution distorted by lower bound on parameter at low luminosities for small f 4 Z ) 100 fb -1

15 24 th September 2007 C.P. Ward Test fit on 100 fb -1 Compare with Χ 2 fit using full correlation matrix (only suitable for high luminosity) Generate 1000 fake data samples for high luminosity and fit with both fits Good correlation between parameter values at minimum 95% C.L. limits tend to be higher for max likelihood fit – seems to result from treatment of systematic errors, but not understood

16 24 th September 2007 C.P. Ward Results from Max L Fit Lumi / fb -1 95% C.L Mean 95% C.L. on |f 4 Z | from 1000 fits Background level and systematic errors not important for early data No background: limits improve by 10% No sys errors: limits improve by 7% With as little as 1 fb -1 can improve LEP limits by order of magnitude LEP: |f 4 Z | < 0.3 no form factor

17 24 th September 2007 C.P. Ward Fit Variations Assess effect of varying background level and systematics on limits for 10 fb -1 Variation95% C.L.Change Default Bg / SM sig. = % No background % Δsys(bg) = 20% % Δsys(bg) = % Stat errors only %

18 24 th September 2007 C.P. Ward ZZ→llll Work has started to include ZZ→llll channel Branching ratio factor of 6 lower than ννll channel Efficiency much higher, background lower First indications are that sensitivity is similar to llνν channel Chara Petridou, Ilektra Christidi (Thessaloniki)

19 24 th September 2007 C.P. Ward Summary and Outlook Expect to achieve worthwhile limits with as little as 1 fb -1 of data (and maybe less) Much still to do for a `real’ analysis : Understand why max L fit gives higher limits Unbinned likelihood fit for lowest luminosities? How to determine background distribution from data? Set up framework for 2-D couplings Include 4-lepton channel – now in progress