2013 version Ryuichiro Kitano (KEK, Sokendai) Univ., July 8, 2013
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1 2013 version Ryuichiro Kitano (KEK, Sokendai) Univ., July 8, 2013
2 126GeV
3
4 High scale GeV Higgs
5
6 elementary fermion elementary
7 K CP = elementary Λ~10,000TeV
8 v = 246 GeV TeV
9 TeV LEP [Ealer, Langacker 10]
10 Low scale TeV Higgs
11
12
13 Goldstone SUSY Yukawa? SUSY
14 SUSY vs 126GeV SUSY 126GeV MSSM
15 Low scale TeV Higgs elementary
16 QCD QCD
17 QCD
18 Quark Confinement Quarkonium mass spectrum and lattice simulations both support the Coulomb+linear potential model for the static quark anti-quark system. [JLQCD 08]
19 ? There is a pretty simple picture. Confinement is dual to Higgs mechanism, and in the dual picture, the quarks are magnetic monopoles. [Mandelstam 75, t Hooft 75] N S Coulomb like
20 ? There is a pretty simple picture. Confinement is dual to Higgs mechanism, and in the dual picture, the quarks are magnetic monopoles. [Mandelstam 75, t Hooft 75] N S
21 ? There is a pretty simple picture. Confinement is dual to Higgs mechanism, and in the dual picture, the quarks are magnetic monopoles. [Mandelstam 75, t Hooft 75] N S Linear potential
22 This mechanism provides us with a classical (Higgs) picture for the quark confinement. magnetic Coulomb force linear potential from flux tube
23 If there is such a classical picture, Where is the magnetic gauge boson in QCD? There are massive vector mesons ρ(770), ω(782).
24 If there is such a classical picture, Where is the magnetic Higgs boson in QCD? There are massive scalar mesons a0(980), f0(980).
25 Let s construct a model of ρ/ω/f0/a0 system as a Higgsed gauge theory (GL theory), and compute the quark potential. model: model parameters are determined by hadron masses and
26 Calculate the energy of the monopole-antimonopole system in the Higgsed vacuum. <H> 0 distance R Dirac monopoles with a unit charge. (static quarks)
27 We could reproduce the QCD potential. [RK, Nakamura, Yokoi 12] this line (monopole-antimonopole separation)
28 I think, it is not too crazy to say that, the low energy hadron physics is the magnetic picture of QCD! QCD
29
30 Scenario Standard Model in extra dim. (no Higgs) compactification + non-perturbative effects of SM gauge interactions Standard Model (with Higgs) Self-breaking [Dobrescu 98][Cheng, Dobrescu, Hill 99][Arkani-Hamed, Dimopoulos 98] [Arkani-Hamed, Cheng, Dobrescu, Hall 00]
31 large extra dim. no EWSB as making extra-dim. small Higgs phase?
32 Emergent Higgs Higgs may be in the emergent degrees of freedom. 0 mode+kk modes (elementary) emergent degrees of freedom? gv/n =1/R5 fermion+gauge 0 Standard Model Higgs from this sector? That would be an interesting unification.
33
34 SU(Nc) SU(Nc) SU(Nc) SU(Nc) SU(Nc) [Arkani-Hamed, Cohen, Georgi 01] [Hill, Pokorski, Wang 01][Cheng, Hill, Pokorski, Wang 01]
35 SU(Nc) SU(Nc) SU(Nc) SU(Nc) SU(Nc)
36 SU(Nc) SU(Nc) SU(Nc) SU(Nc) SU(Nc)
37 SU(Nc) SU(Nc) SU(Nc) SU(Nc) SU(Nc) N=2 SUSY version 6 (2,0) [Arkani-Hamed, Cohen, Kaplan, Karch, Motl 01]
38 extra dim + SUSY 126GeV
39 a toy model: 2-site model [RK, Nakai 12] UV free IR free top/bottom SU(3)1 Q SU(3)2 other quarks + top/bottom N=2 structure Topcolor model [Hill 91] [RK, Fukushima, Yamaguchi 10] ([Craig, Stolarski, Thaler 11][Csaki, Shirman, Terning 11][Cohen, Hook, Torroba 12][Evans, Ibe, Yanagida 12]...) gauged (Lagrange multiplier) (<Q>=v is fixed) KK modes no Higgs field
40 For (weak coupling) SU(3)1 x SU(3)2 SU(3)1+2 We get MSSM without Higgs as low energy theory. Below, we study the case with (strongly coupled region) we will see that magnetic degrees of freedom appear.
41 Seiberg duality [Seiberg 94] SU(3)1 factor gets strong weakly coupled magnetic picture (CFT) Higgs appeared. below the dynamical scale Λ1.
42 weakly coupled a-maximization gives [Intriligator, Wecht 03] (we assumed λb 4π by taking small vb) 1 (appearance of light degrees of freedom)
43 below Λ Partially composite Higgs [RK, Luty, Nakai 12] SU(2)1 factor confines (note: at this stage, λ s get renormalized by O(1) factors.) ( ) <H > = 0 gauged <S> 0 at SUSY level. S is not dynamical one can integrate them out.
44 arriving at the MSSM-like model μ-like terms obtained from kinetic terms for S and S. We consider SUSY breaking by turning on with
45 Higgs potential H CFT H H H Hd is the main Higgs direction H are heavy Partially composite Higgs [RK, Luty, Nakai 12]
46 H H CFT Higgs quartic term: H H not bad. tuning: required size of the Higgs quadratic terms typical size not bad. fixed point values:
47 q top mass H CFT t not bad. note: top obtains a mass from Hd fixed point values:
48 ~ t ~ CFT t stop/sbottom should be observed soon! (should have been observed?) fixed point values:
49 ~ h CFT ~ h Higgsino pretty light. fixed point values:
50 dynamical sector We can access to UV dynamics of QCD. We expect ρ-like resonances (W, Z ) very interesting.
51 Summary We studied a quiver model for EWSB. The Higgs fields emerge as magnetic degrees of freedom. By adding SUSY breaking terms, EWSB can occur while 126GeV Higgs boson is naturally explained.
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