a 2hdm from strong dynamics kei yagyu
play

A 2HDM from Strong Dynamics Kei Yagyu Seikei U arXiv: 1803.01865 - PowerPoint PPT Presentation

A 2HDM from Strong Dynamics Kei Yagyu Seikei U arXiv: 1803.01865 [hep-ph] Collaboration with Stefania De Curtis, Luigi Delle Rose, Stefano Moretti 2018, 12 th May, 22nd NHWG Meeting Introduction From LHC results At least 1 Higgs boson


  1. A 2HDM from Strong Dynamics Kei Yagyu Seikei U arXiv: 1803.01865 [hep-ph] Collaboration with Stefania De Curtis, Luigi Delle Rose, Stefano Moretti 2018, 12 th May, 22nd NHWG Meeting

  2. Introduction From LHC results  At least 1 Higgs boson exists.  It shows SU(2) L doublet nature.  Its mass is 125 GeV. But, Higgs is still mystery…. In fact, we do not know  The Nature of the Higgs boson.  The reason for the small Higgs mass with respect to a NP scale.  The true shape of the Higgs sector. 2 important paradigms (dynamics)  Supersymmetry (weak) and Compositeness (strong) Both scenarios can provide a 2HDM as a low energy EFT . Can we distinguish these scenarios from the 2HDM property? 1

  3. Plan of the talk  Introduction  Introduction to pNGB Higgs  Composite 2HDM (C2HDM)  Results  Summary

  4. Pion Physics ↔ Higgs Physics Georgi, Kaplan 80ʼs  From now on, let me say “ Composite Higgs ” as pNGB Higgs .  This scenario can be understood by analogy of the pion physics. Higgs Physics Pion Physics Fundamental QCD-like theory QCD Theory Spontaneous sym. SU(2) L ×SU(2) R → SU(2) V G → H breaking h ~ 125 GeV pNGB modes (π 0 , π ± ) ~ 135 MeV New spin 1 and ½ states Other resonances ρ ~ 770 MeV, … ~ Multi-TeV 2

  5. Basic Rules for Composite Higgs  Suppose there is a global symmetry G at scale above f (~TeV), which is spontaneously broken down into a subgroup H.  The structure of the Higgs sector is determined by the coset G/H.  H should contain the custodial SO(4) ≃ SU(2) L ×SU(2) R symmetry.  The number of NGBs (dimG-dimH) must be 4 or lager. G f H G sm v EM 3

  6. Basic Rules for Composite Higgs  Suppose there is a global symmetry G at scale above f (~TeV), which is spontaneously broken down into a subgroup H.  The structure of the Higgs sector is determined by the coset G/H.  H should contain the custodial SO(4) ≃ SU(2) L ×SU(2) R symmetry. G  The number of NGBs (dimG-dimH) should be 4 or lager. f H G sm v EM Table from Mrazek, Pomarol, Rattazi, Redi, Serra, Wulzer NPB 853 (2011) 1-48 4

  7. Basic Rules for Composite Higgs  Suppose there is a global symmetry G at scale above f (~TeV), which is spontaneously broken down into a subgroup H.  The structure of the Higgs sector is determined by the coset G/H.  H should contain the custodial SO(4) ≃ SU(2) L ×SU(2) R symmetry. G  The number of NGBs (dimG-dimH) should be 4 or lager. f Agashe, Contino, Pomarol (2005) H 1 Doublet: Minimal Composite Higgs Model G sm v EM Table from Mrazek, Pomarol, Rattazi, Redi, Serra, Wulzer NPB 853 (2011) 1-48 4

  8. Basic Rules for Composite Higgs  Suppose there is a global symmetry G at scale above f (~TeV), which is spontaneously broken down into a subgroup H.  The structure of the Higgs sector is determined by the coset G/H.  H should contain the custodial SO(4) ≃ SU(2) L ×SU(2) R symmetry. G  The number of NGBs (dimG-dimH) should be 4 or lager. f Gripaios, Pomarol, Riva, Serra (2009) H 1 Doublet + 1 Singlet Redi, Tesi (2012) G sm v EM Table from Mrazek, Pomarol, Rattazi, Redi, Serra, Wulzer NPB 853 (2011) 1-48 4

  9. Basic Rules for Composite Higgs  Suppose there is a global symmetry G at scale above f (~TeV), which is spontaneously broken down into a subgroup H.  The structure of the Higgs sector is determined by the coset G/H.  H should contain the custodial SO(4) ≃ SU(2) L ×SU(2) R symmetry. G  The number of NGBs (dimG-dimH) should be 4 or lager. f H 2 Doublets Mrazek, Pomarol, Rattazi, Redi, Serra, Wulzer (2011) G sm Bertuzzo, Ray, Sandes, Savoy (2013) v EM Table from Mrazek, Pomarol, Rattazi, Redi, Serra, Wulzer NPB 853 (2011) 1-48 4

  10. Basic Rules for Composite Higgs  Suppose there is a global symmetry G at scale above f (~TeV), which is spontaneously broken down into a subgroup H.  The structure of the Higgs sector is determined by the coset G/H.  H should contain the custodial SO(4) ≃ SU(2) L ×SU(2) R symmetry. G  The number of NGBs (dimG-dimH) should be 4 or lager. f H G sm v EM In this talk, I take SO(6)  SO(4)×SO(2). 4

  11. Construction of 2 pNGB Doublets  15 SO(6) generators: ^ (A=1-15, a=1-3, a=1-4) 6 SO(4) 1 SO(2) 8 Broken  pNGB matrix: U is transformed non-linearly under SO(6):  Linear rep. Σ(15): 15 = ( 6 , 1 ) ⊕ ( 4 , 2 ) ⊕ ( 1 , 1 ) under SO(4)×SO(2) Σ is transformed linearly under SO(6): Σ  g Σ g -1 and Σ 0  h Σ 0 h -1 5

  12. Higgs Potential  The potential becomes 0 because of the shift symmetry of the NGB.  the Higgs mass also becomes 0.  We need to introduce the explicit breaking of G.  NGB Higgs becomes p NGB with a finite mass. Kaplan, PLB365, 259 (1991)  Explicit breaking can be realized by partial compositeness Linear mixing a Particle in Particles in elementary sector strong sector 6

  13. Strategy SO(6) invariant Lagrangian Explicit Model with partial compositeness Integrating out heavy DOFs SU(2)×U(1) invariant Lag. Effective Lagrangian with form factors Coleman-Weinberg mechanism 2HDM potential with Effective Potential predicted parameters Higgs mass spectrum Phenomenology Higgs couplings, decays, etc… 7

  14. Explicit Model Based on the 4DCHM, De Curtis, Redi, Tesi, JHEP04 (2012) 042 Strong Sector Elementary Sector SO(6)×U(1) X Mixing SU(2) L ×U(1) Y → SO(4)× SO(2)×U(1) X Partial Compositeness 8

  15. Explicit Model Based on the 4DCHM, De Curtis, Redi, Tesi, JHEP04 (2012) 042 Strong Sector Elementary Sector SO(6)×U(1) X Mixing SU(2) L ×U(1) Y → SO(4)× SO(2)×U(1) X Partial Compositeness 8

  16. Explicit Model Based on the 4DCHM, De Curtis, Redi, Tesi, JHEP04 (2012) 042 Strong Sector Elementary Sector SO(6)×U(1) X Mixing SU(2) L ×U(1) Y → SO(4)× SO(2)×U(1) X Partial Compositeness + (Σ-ρ) interactions 8

  17. Explicit Model Based on the 4DCHM, De Curtis, Redi, Tesi, JHEP04 (2012) 042 C 2 symmetry (to avoid FCNCs) C 2 = diag(1,1,1,1,1,-1) Strong Sector Elementary Sector SO(6)×U(1) X Mixing SU(2) L ×U(1) Y → SO(4)× SO(2)×U(1) X Partial Compositeness + (Σ-ρ) interactions 8

  18. Explicit Model Based on the 4DCHM, De Curtis, Redi, Tesi, JHEP04 (2012) 042 Embeddings into SO(6) multiplets︓ Strong Sector Elementary Sector SO(6)×U(1) X Mixing SU(2) L ×U(1) Y → SO(4)× SO(2)×U(1) X Partial Compositeness 8

  19. Effective Lagrangian  All the strong sector information are encoded into the form factors:  We then calculate the 1-loop CW potential. K LL , K RR G LL , G RR K LR 9

  20. Effective Potential + O(Φ 6 ) 2 and λ i are given as All the potential parameters m i a function of strong parameters: 10

  21. Typical Prediction of Mass Spectrum E Ψ, ρ μ Y 1 : C 2 breaking term f H ± , H, A ★f  ∞ : All extra Higgses are decoupled  (elementary) SM limit h ~ 125 GeV ★To get M≠0, we need C 2 breaking (Yukawa alignment is required →A2HDM). 11

  22. f VS tanβ 12

  23. Correlation b/w f and m A 13

  24. Correlation b/w m A and κ V (= g hVV /g hVV SM ) 14

  25. Summary  Higgs as pNGB scenarios give natural explanation for a light Higgs and are well motivated by the analogy of pion physics .  Taking the SO(6)/SO(4)*SO(2) coset, we obtain C2HDMs as a low energy EFT , where 2HDM parameters can be predicted by the strong dynamics .  To get larger extra Higgs masses, we need to introduce the C 2 breaking term  Aligned 2HDM .  C2HDMs predict delayed decoupling as compared to the MSSM. 15

  26. Correlation b/w m A and κ V (= g hVV /g hVV SM )

  27. Correlation b/w f and M T

  28. Gauge Sector Lagrangian De Curtis, Redi, Tesi, JHEP04 (2012) 042 G 1 × G 2 × G 3 G i : Global SO(6) G V ʼ Σ 2 (8) U 1 (15=7+8) (gauged) mixed H [SO(4)×SO(2)] G V 8 + 8(Φ 1 , Φ 2 ) 7 + 8 NGBs are absorbed into the longitudinal components of gauge bosons of adj[SO(6)].

  29. Gauge Sector Lagrangian (in unitary gauge) De Curtis, Redi, Tesi, JHEP04 (2012) 042 Elementary Sector (g W , W μ ) Strong Sector (g ρ , ρ μ ) SO(6) SO(6) U 1 Σ 2 SO(4)×SO(2) SU(2) L ×U(1) Y

  30. Matching Conditions  We need to reproduce the top mass and the weak boson mass. g 2 V sm 2 ~ (246 GeV) 2 Y t

  31. Effective Lagrangian  Integrating out the heavy degrees of freedom (ρ A and ψ 6 ), we obtain the effective low energy Lagrangian ≔ K ≔ G

  32. Effective Lagrangian  Integrating out the heavy degrees of freedom (ρ A and ψ 6 ), we obtain the effective low energy Lagrangian ≔ K ≔ G These coefficients can be expanded as c 1 , c 2 , … are determined by strong parameters.

  33. Numerical Analysis Input parameters (to be scanned): Tadpole conditions: T 1 = T 2 = 0 165 GeV < m t < 175 GeV 120 GeV < m h < 130 GeV

  34. Yukawa Interactions  The structure of the Yukawa interaction is that in the Aligned 2HDM. t and tanβ can be predicted by strong dynamics,  All M 1 t , M 2 so the ζ t factor is also predicted. 33

  35. Yukawa Interactions

  36. Spurion Method  The Higgs potential is calculated only by using the spurion VEV Δ ψ and U. Merit: Quite General (but still we need to assume fermion rep. ) Demerit: Losing the correlation, O(1) uncertainties in pot. parameters. U T U 1

  37. Spurion Method Mrazek, Pomarol, Rattazi, Redi, Serra, Wulzer NPB 853 (2011) 1-48  Fermionic contribution assuming r = 6 -plet of SO(6).  Arbitral O(1) parameters appear in front of each operator. 36

Recommend


More recommend