ESFA/DESY LC Workshop 1 Klaus Mönig and Jadranka Sekaric Klaus Mönig and Jadranka Sekaric DESY - Zeuthen MEASUREMENT OF TGC IN e COLLISIONS AT TESLA
ESFA/DESY LC Workshop 2 02/04/2003, Amsterdam INTRODUCTIONINTRODUCTION In order to predict the precision of measurement of trilinear gauge couplings (TGC) at a photon collider : (e W ) 1.signal to background separation study (e W ) for real and parasitic e -mode 2.observables sensitive to TGC (angular distributions, cross-sections …) and of measurement of and parameters, obtained by fit-minimizing the 2 value 3.estimated errors, and of measurement of and parameters, obtained by fit-minimizing the 2 value - effect of photon beam polarization on and measurement T E S L A
ESFA/DESY LC Workshop 3 EVENT SELECTION TOOLS: PYTHIA event generator SIMDET V3 detector simulation sample of 10 5 mixed signal and background events, generated with PYTHIA at E CM (e )= 450 GeV background for real and parasitic e -mode: e W qq T 37 pb e eZ 0 eqq T 3.5 pb qq T 137 pb WW l qq T 82 pb qq T 128 pb response of a detector simulated with SIMDET V3 Ws are reconstructed from hadronic final states 02/04/2003, Amsterdam T E S L A
ESFA/DESY LC Workshop 4 sufficientlyhigh W production cross-section allows us to efficiently separate signal from background sufficiently high W production cross-section allows us to efficiently separate signal from background Applied cuts: acceptance of detector - 7° acceptance of detector - 7° 02/04/2003, Amsterdam angular distributions for signal and bck. hadronic final states e W e eZ 0 qq W energy W energy ( ) Gev hadronic final states energy spectrum T E S L A
ESFA/DESY LC Workshop 5 High efficiency for hadronic channel, 84% with low background 02/04/2003, Amsterdam W mass W mass (60-100) Gev hadronic final states mass spectrum e W e eZ 0 qq final angular distributions after selection T E S L A
ESFA/DESY LC Workshop 6 Background for parasitic e mode : WW l qq same cuts as previous qq T E S L A e W WW qq angular distribution energy distribution 02/04/2003, Amsterdam W energy W energy ( ) Gev Applied cuts: acceptance of detector - 7° acceptance of detector - 7°
ESFA/DESY LC Workshop 7 T E S L A 02/04/2003, Amsterdam W mass W mass (60-100) Gev S/B WW ~ 9:1, purity ~ 90% angular distribution after selection mass distribution WWW qq
ESFA/DESY LC Workshop 8 OBSERVABLES SENSITIVE TO TGC analytic formula for total (differential) cross- section (A. Denner, A.Dittmaier, Nucl.Phys. B398 (1993)239 helicity amplitudes for different initial photon and final W states (E.Yehudai, Phys.Rev. D11(44)1991)) differential cross-section distribution over the decay angle (Bilenky at al.,Nuc.Phys. B(409) (1993)22 WHIZARD Monte Carlo tree–level generator (W.Kilian,University of Karlsruhe) total and differential cross-section 02/04/2003, Amsterdam T E S L A
ESFA/DESY LC Workshop 9 DCS in presence of anomalous coupling for J = ± 1 state normalized to its SM value DCS for J = ±1 state in SM 02/04/2003, Amsterdam T E S L A ANOMALOUS TGC can affect the total production cross-section and the shape of the differential cross-section
ESFA/DESY LC Workshop 10 02/04/2003, Amsterdam T E S L A Contribution of each helicity state of the W boson affects the distribution of their decay products
ESFA/DESY LC Workshop 11 WHIZARD Monte Carlo generator, 10 6 mixed pairs (du-bar and sc-bar) at E CM = 450 GeV, fixed photon-beam energy, polarized beams (P=100%), anomalous couplings for each event we observe 3 kinematic variables -W production angle with respect to the e- beam direction - cosθ -W polar decay angle - angle of the fermion with respect to the W flight direction measured in the W rest frame – cosθ 1 -azimuthal decay angle of the fermion with respect to a plane defined by W and the beam axis Monte Carlo SM events are reweighted with function R( ) ( and are free parameters) R( ) = 1 + A· + B· + C·( ) 2 + D·( ) 2 + E · 02/04/2003, Amsterdam T E S L A MONTE CARLO FIT
ESFA/DESY LC Workshop 12 2D (over cosθ, cosθ1and 3D(over cosθ, cosθ1, cross-section distributions are fitted 2D (over cosθ, cosθ1 ) and 3D (over cosθ, cosθ1, ) cross-section distributions are fitted L-error on the luminosity measurement norm-normalization constant 02/04/2003, Amsterdam T E S L A
ESFA/DESY LC Workshop 13 real mode/ parasitic mode E CM = 450 GeV, ∫L t = 110 fb -1 Monte Carlo 2D J = +1 LL1%0.1%accurate · /3.71.0/1.00.4/0.4 · / /2.1 Estimated errors of and for +1 photon polarization state (P=100%) – single parameter 2D and 3D fit Estimated errors of and for +1 photon polarization state (P=100%) – single parameter 2D and 3D fit real mode/ parasitic mode E CM = 450 GeV, ∫L t = 110 fb -1 Monte Carlo 3D J = +1 LL1%0.1%accurate · /3.11.0/1.00.4/0.4 · /2.9 02/04/2003, Amsterdam T E S L A
ESFA/DESY LC Workshop 14 - distribution slightly decreases error of ( L = 1%) and of for a factor 7 ! shape sensitivity in phi distribution phi distribution influences much more on 3D - Mean error on comes from L, not case for - Good agreement between 2 modes for and 02/04/2003, Amsterdam =1.01 =0.99 =0.01 =-0.01 T E S L A 2D3D 22
ESFA/DESY LC Workshop 15 02/04/2003, Amsterdam T E S L A Polarization influence on and - Polarization influence on and variation of laser polarization in the laser wave beam field influences the photon polarization sample with P =+0.9 polarized photons - sample with P =+0.9 polarized photons mixing the events with P =+1 and P =-1 in order to get preferred polarization (95:5) errors obtained from the fit are in a good agreement with previous ones sample with 1% different polarization - sample with 1% different polarization increased the N ev with P =-1 for 10% increase of N ev correspond to the P =+0.89 test-fit and … -we found : 1% changes in polarization -we found : 1% changes in polarization (accurate fit) within ~ 12 within ~ 1 Contribution from normalization and from polarization J
ESFA/DESY LC Workshop 16 02/04/2003, Amsterdam T E S L ASUMMARYSUMMARY -Efficient signal to background separation for both e modes - , ~ (error on luminosity measurement, L, is included) - Main contribution to the error of comes from L - Shape sensitivity for anomalous in phi distribution decreases error of - Variable polarization (1%) affects the measurement Future plans : - Variable photon-beam energy in WHIZARD - Resolution on reconstructed variables - Background influences on error predictions