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Higgs pair production at photon collider. ILC Physics WG general meeting 21. November 2009 Hiroshima University Nozomi Maeda. Introduction. Photon Linear Collider (PLC) is gamma-gamma collision option in ILC.
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Higgs pair production at photon collider ILC Physics WG general meeting 21.November 2009 HiroshimaUniversity Nozomi Maeda
Introduction Photon Linear Collider (PLC) is gamma-gamma collision option in ILC. We study feasibility of measurement of Higgs self-coupling constant l=lSM(1+dk) by gg->HH This process occurs at low energy(than e+e-). l contribution to cross section is different.
Energy optimization dk=+1 L:Luminosity(assume 1000fb-1) h:detection efficiency s:cross section hB:background suppression dk=-1 Higgs mass=120GeV
(+,+), (-,-) Background large background : gg->WW (sB~90pb) cf.) Signal:s = 0.044fb 0.044fb/90pb = 4.9×10-7 10-7background suppression is necessary.
Luminosity spectrum Simulation by CAIN. total luminosity of photon collision = 1.26×1035cm-2s-1 effective Xsec(Signal) = 0.013fb → 16event/year effective Xsec(BG) = 11,600fb → 1.467×107event/year hB<10-6 is required.
Analysis • gg->HH H -> bb or WW* or gg … Signal:HH->4b Background:WW->4quark H->bb mode has the largest Branching Ratio (when Higgs mass = 120GeV, B.R.=67.8%). reconstruct particles from jet pairs that has the smallest c2. M1,M2 = reconstructed particle mass M = MH or MW s2j = 2jets mass resolution
gg->WW rejuction • use Neural Net(JetNet) to separate gg->HH from gg->WW. • # of generated events : Signal = 5.00×104 BG = 7.50×107 • # of nodes : input = 9, hidden = 18, output = 1 • pre-Selection : # of loose b-tagged jets > 2 & # of tight b-tagged jets > 1 (loose : nsig=3.0, noffv=1 tight : nsig=3.0, noffv=2)
NN output • input parameters : c2H, c2W, # of tracks, momentum(transverse, longtidunal), Visible Energy, ycut, # of b-tagged jets(loose, tight) (loose : nsig=3.5, noffv=1 tight : nsig=3.5, noffv=2) black:BG blue:Signal NNout > 0.98 If PLC runs for 5years...Signal : 16×5×hSig ≒ 12.5 Background : 1.467×107×5×hBG ≒ 3.9 significance = 3.1s
gg->ZZ background gg->ZZ Xsec ≒ 50fb@300GeV photon helicity = (+1, +1) Integrate over 8deg<q<172deg (generated by Gounaris’s gamgamZZ code: hep-ph/0610085. offered by Tsumura-san.)
gg->ZZ background x=3.76 gg->ZZ effective Xsec ≒ 9.6fb→1.2×104events/year Integrate over 8deg<q<172deg (generated by Gounaris’s gamgamZZ code: hep-ph/0610085. offered by Tsumura-san.)
f Z g f f g Z f gamgamZZ code HELAS gg->ZZ->4fevent generator ZZ decay modes are ... q = light quark bbqq (12.9%), ccqq (10.3%), qqqq (18.3%), bbbb (2.28%), bbcc (3.62%), cccc (1.44%) bbbb……be background source. → simulate gg->ZZ event, and study how to reject gg->ZZ. → develop gg->ZZ->4fevent generator use gamgamZZ code and HELAS for calculating helicity amplitude.
g Z Z g (not includes Z decay mode and Luminosity) gg->ZZ event generator Xsec distribution total Xsec = 49.8fb (consistent with gamgamZZ code)
Summary • We study feasibility of measurement of Higgs self-coupling constant at PLC. • gg->WW background is 106 times larger than gg->HH signal. • Neural Net with b-tagging and kinematics can reject almost all gg->WW background. • gg->ZZ event generator developing in progress. • Next plan is including Z decay mode and Luminosity spectrum to gg->ZZ event generator.
gg->4b background b-tagging cannot reject gg->4b too. Xsec(not convolute gg luminosity) = 2.81fb@optimum gg energy + and other diagrams