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ACFA 7th Nov Taipei Taiwan

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Presentation on theme: "ACFA 7th Nov Taipei Taiwan"— Presentation transcript:

1 ACFA 7th Nov.9-12 2004 Taipei Taiwan
Towards Higgs Precision Measurement at ILC What we have done ? & What we have to do? JAPAN LC Physics study group Higgs subgroup and KEK Minamitateya Collaboration Yoshiaki Yasui (Tokyo Management Collage)

2 Why Precision Measurement?
What we can do after Higgs LHC? Higgs Precision Measurement EW SSB, mass generation Direct measurement of self coupling e+e- →hh X  luminosity upgraded LHC (SLHC)  (e+e- → hh X ) >> (e+e- → hhh X)   Diouadi et.al   SM New Physics!! Higgs coupling may be a probe of BSM

3 MSSM at ILC? But ..... Decoupling limit MH0 ≈ MH ≈ MA0 >> MZ hhh = (3gMZ/Cw)cos2sin()  3gMh02/2MW = hhhSM (MhSM=Mh0) hhhh = (3g2/Cw2)cos22   3g2Mh02/4MW2 =SMhhhh(MhSM=Mh0) Top Yukawa corrections are small Hollik et.al. Higgs self coupling = gauge coupling? We need more idea!!

4 Non SUSY THD at ILC? Higgs self coupling as a probe of THD
Kanemura et.al LCWS’04 Paris Baryogenesis  talk by Senaha-san

5 Radion(graviscalar)-Higgs mixing
Extra-dim at ILC? Radion(graviscalar)-Higgs mixing Ex:Warped Extra Dim model Randall Sundrum m > 2mh ⇒ hh bbbb m < mh, >> 1 ⇒ gg 0 Dominici et.al. Nucl.Phys. B671 (2003) zzh hhh =5GeV =5GeV radion mass mPlanck-warped scale

6 Towards Higgs Precision Measurement
Machine design parameters (CM energy, Luminosity,etc.) Detailed study of SM Higgs (Simulation, RC, etc.)   feedback this talk New Physics at ILC (SUSY,THD,LH,Extra-Dim,etc.)

7 What we have done? Priority ⇒ Higgs Physics at TeV LC
Higgs self coupling⇒ We started (from 2002) Top Yukawa Heavy Higgs, etc. etc..

8 @LCWS '02 Jeju Korea Assumption No bkg effects 100% signal efficiency
dominant for ECM > 1TeV by Yasui et.al.  LCWS’04 Paris France  Quick Simulation (includes bkg.) study!!

9 Our Strategy for simulation studies
Parton level Generator (tree level ⇔ GRACE-loop) LCGrace talk by Yasui, ACFA 6th India package for LC Higgs physics study: Mh ≤ 140 GeV e+e-  6f based on the GRACE System Bases ⇒ Monte Carlo integration ⇒ Cross section Spring ⇒ Events generator Hadronizer Pythia (interface from Spring to Pythia6) Simulator (Quick Simulation → Full Simulation) Analysis

10 Simulation Study Ecm = 1 TeV main mode  W-fusion
Higgs mass = 120 GeV      SM decay Br ISR/BSR included Signal & bkg event generator LCGrace (BASES+SPRING) Signal MC: X + hh /SM from 0.0 to 2.0 with 0.2 step Smearing simulation at parton level Jet energy resolution ~ 30%/√E (GeV) (detector R&D target value) ννhh quick analyses only for hh decaying to 4b Br(hh4b) ~ 47 % for 120 GeV SM Higgs Signal characteristics Large missing energy, missing Pt Only 4 b jets M1 jj ~ Mh M2 jj ~ Mh No isolated lepton

11 Signal and Background processes
By LCGrace Main bkg processes 4b + missing ννbbbb (~ ννZZ, ννZγ*) ννbbh (~ ννZh) Signal (for SM)

12 ννhh Analysis Flow bkg further reduction 2. Separate Zhh & fusion
Reconstructed ‘Higgs’ mass ννhh Analysis Flow ννbbbb = 1. Likelihood selection bkg further reduction 2. Separate Zhh & fusion different dependence (positive/negative interferences) 3. Combine with Zhh analyses for s-channel process 4. Check hh invariant mass 5. hhh measurements ννbbh =SM L = 1 ab-1 dep. of cross-section Zhh eehh /SM

13 ννhh ννhh selection Separate Zhh & fusion ννhh channel = =SM
L = 1 ab-1 ννbbbb = counts counts ννhh ‘fusion’ =SM ννbbh ‘Zhh’ Likelihood Missing mass [GeV] (~ OPAL Higgs scheme)

14 HH invariant mass distributions
‘Zhh-channel’ ‘fusion-channel’ counts counts =2  SM = Zhh ννhh =SM =SM hh invariant mass [GeV] hh invariant mass [GeV] (= visible mass)

15 hhh Measurement sensitivity
By Yamashita et.al. LCWS 2004 Mh=120 GeV Measured /SM True /SM 95%CL upper bound 95%CL lower bound 67%CL range Ilumi=1 ab-1 Pol beam= -80% @1TeV (SM Higgs Br) Use only hh4b (Br(hh4b)~47%) Eff.(4b) 80% Precise study  Radiative corrections are also important!!  Systematic study of the RC for Higgs physics at LC with GRACE

16 Radiative correction for e+e-ZHH
GRACE Phys.Lett.B576(2003)152 Zhang et al. Phys.Lett.B578(2004)349

17 Radiative correction for e+e-ee HH
=(O())/(tree)-1 Yasui et.al. ECFA2004 Durham UK W WG=W- 4r r=2.267% QED for Mh=120 GeV W for Mh=120GeV

18 Recent progress on the loop calculations
Single Higgs production e+e-ZH (full number of graphs = 341) e+e-H (1350) Phys.Lett. B559 (2003) A.Denner et.al. PLB 560(2003)196, NPB 660(2003)289 e+e-e+e- H (4470) Phys.Lett.B600(2004)65-76 top Yukawa e+e-t t H (2327) Phys.Lett. B571 (2003) Y.You et.al.PLB 571(2003) A.Denner et.al. PLB 575(2003)290, NPB 68(2004)85 Multi Higgs production e+e-ZHH (5417) Phys.Lett. B576 (2003) R.Zhang et.al.PLB(2004)349 e+e-ee HH (19638)  New results!! of 2 to 4 Weak corrections are sizable O(5-10)%

19 Summary What we have done? What we have to do?
A quick simulation study has been performed for Ecm=1 TeV For Mh=120 GeV: measurement sensitivity (only hhbbbb only) for =SM /SM= (1) (95%CL) /SM=  (1) (95%CL) /SM=  (1) (95%CL) What we have to do? Non-b decay of the Higgs  increase sensitivity Mh>140GeV  W-par decay of the Higgs ννhh 8f, 10f New version of Grace system Radiative corrections (systematic study have been done) sizable  include in the event generator New Physics study


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