Present and future constraints on top EW couplings Present and future constraints on top EW couplings F. Richard June 20131 François Richard LAL/Orsay.

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Presentation transcript:

Present and future constraints on top EW couplings Present and future constraints on top EW couplings F. Richard June François Richard LAL/Orsay Workshop on Top physics at the LC 5-6 March 2014 LPNHE Paris

Introduction  In composite models which comprise e.g. extra-dimensions (RS), Little Higgs (LH), one expects a proeminent part for the top quarks  Predictions on possible deviations for top EW couplings span a large range from a few %, only visible with ILC, up more to several 10% observable at LHC  In this talk, I will indicate how LEP/Tevatron/ SLC constraints already tell us what one can realistically expect to observe F. Richard June 20132

A surprising plot F. Richard June A. Juste et al. hep-ph/

Origin of these constraints  Recall that if one modifies the fermion EW couplings the SM loops becomes UV divergent and this requires introducing a cutoff ~TeV to compute these contributions  Given this cutoff the top EW couplings anomalies are limited by LEP/SLD measurements F. Richard June 20134

Explicit formulae  If one assumes that charged currents are SM  CC =0 then at lowest order  1 ~  NC R  NC L ~axial term for Ztt F1AZ is tightly constrained F. Richard June A. Larios et al. hep-ph/

A not surprising plot F. Richard June 20136

Gauge invariance  Gauge invariance relates ZtLtL to WtLbL and ZbLbL  From LEP1 we know that ZbLbL has no anomaly meaning that    1 and   b only depend on neutral couplings ZbLbL and ZbRbR  Loop contributions therefore fully constrain ZtLtL and ZtRtR and the only freedom left comes from BSM compensating contributions to  1 and  b F. Richard June JA Aguilar et al. hep-ph/012037

Example of models F. Richard June 20138

Constraints  Take |  1 /  1 | and |  b /  b | <1.5 and =1 TeV  A wide range is allowed for dtR/tR while dtL/tL is restricted  Most models (after some ‘educated choices’) are consistent with these constraints  A few are at the edge meaning that they need a large BSM compensating loop contribution F. Richard June 20139

Close up F. Richard June

In detail F. Richard June ModeldtR/tR %dtL/tL %dtLbL/tLbL %db/bdb/b d  1/  1 d  Ztt/  Ztt % Carena Djouadi Gherghetta Grojean Hosotani Little Higgs Pomarol Wulzer Wulzer

Lessons  Loop constraints have allowed to trim most of the models (Djouadi and LH had a priori a wide range)  Most of the proposed models need large BSM contributions to compensate loop contributions meaning, e.g. for LH, that new particles like heavy vector quarks could be discovered at LHC14  While some of these models could be tested at LHC by measuring single top production or the Ztt production, it will take ILC for a conclusive test of the various scenarios  Disentangling of tL and tR is essential to separate models (difficult at LHC) F. Richard June

Comparisons F. Richard June Coupling errorsILCLHC 300 fb-1  ZtLtL/ZtLtL 0.6% -66% 15%  ZtRtR/ZtRtR 1.4%-100% 148%  tLtL/  tLtL 0.24%-7% 12%  tRtR/  tRtR 0.24%-7% 12%

Conclusions  Loop contributions + gauge invariance allows to put very useful restrictions on Wtb and Ztt coupling deviations  Some models require large compensating loops which implies light vector quarks  Single top and  Ztt from LHC still in infancy but in the future could indicate significant deviations  The same mechanisms operate for the Higgs sector  ILC will be a key instrument to fully elucidate the underlying top and Higgs physics and reach the highest sensitivity F. Richard June

BACK UPS F. Richard June

Higgs sector  The same mechanism is at work when Higgs couplings deviate from SM, compensating contributions are needed to satisfy the LEP/SLC constraints  Without these compensations hZZ coupling could not give significant deviations measurable at LHC or even at ILC  Quantatively one can write: with  v=1 for the SM case  A compensating term dT=0.2 allows to have  ²v=0.7 perfectly measurable at a LC F. Richard June

Higgs couplings F. Richard June

The RS solution for AFBb  Main formulas  Can be fully solved with ILC measurements  Determining Mkk requires running at 2 energies  F(ctR)/F(cbR)~30 close to mt/mb as one would expect in RS  Possibly additional terms due to quark mixing F. Richard June

CMS result on ttZ F. Richard June sig/SM= arXiv:

Single top experiment Vtb CDF D CMS ±0.04(th) ATLAS F. Richard June