non resonant collider signatures of a singlet driven
play

Non-resonant Collider Signatures of a Singlet-Driven Electroweak - PowerPoint PPT Presentation

Non-resonant Collider Signatures of a Singlet-Driven Electroweak Phase Transition Chien-Yi Chen University of Victoria / Perimeter Institute C.-Y. C, J. Kozaczuk and I. M. Lewis, 1704.0xxxx ACFI Workshop: Making EWPT


  1. Non-resonant Collider Signatures of a Singlet-Driven Electroweak Phase Transition Chien-Yi Chen University of Victoria / Perimeter Institute C.-Y. C, J. Kozaczuk and I. M. Lewis, 1704.0xxxx ACFI Workshop: Making EWPT a April 7, 2017

  2. Holy grails [Quigg lecture at the 2004 SLAC Summer Institute. ]

  3. Holy grails [Quigg lecture at the 2004 SLAC Summer Institute. ]

  4. Holy grails Strong indication of new physics [Quigg lecture at the 2004 SLAC Summer Institute. ]

  5. Baryogenesis v Evidence from cosmology: v Sakharov’s 3 conditions (1967), for baryogenesis v Baryon number violation v Out of equilibrium v C and CP violation v EW baryogenesis is one of the potential solutions v Need new physics because in SM: EW phase transition is a crossover, instead of 1 st order 1) CP violation is too small 2)

  6. Testability v LHC is running! v What’s the sensitivity of HL-LHC, 100 TeV pp colliders, and future e+ e- colliders to the region of parameter space where SFOPT is allowed? v Gravitational waves: Bubble collisions

  7. Model: SM+singlet

  8. SM + Singlet v SM Higgs doublet H mixes with an additional singlet S. The singlet doesn’t couple to SM fermions and gauge bosons.

  9. SM + Singlet v SM Higgs doublet H mixes with an additional singlet S. The singlet doesn’t couple to SM fermions and gauge bosons.

  10. SM + Singlet v SM Higgs doublet H mixes with an additional singlet S. The singlet doesn’t couple to SM fermions and gauge bosons.

  11. SM + Singlet v SM Higgs doublet H mixes with an additional singlet S. The singlet doesn’t couple to SM fermions and gauge bosons.

  12. SM + Singlet v SM Higgs doublet H mixes with an additional singlet S. The singlet doesn’t couple to SM fermions and gauge bosons. If apply Z 2 symmetry: S-> -S

  13. SM + Singlet v SM Higgs doublet H mixes with an additional singlet S. The singlet doesn’t couple to SM fermions and gauge bosons. v After spontaneous symmetry breaking: ✓ ◆ 1 0 H → , in unitary gauge √ h + v 2 S → S + x

  14. SM + Singlet v Mass eigenstates and mixing angle: S h 2 h 1 θ h h 1 = h cos θ + S sin θ h 2 = − h sin θ + S cos θ Mass eigenstates Gauge eigenstates : the Higgs we observed; its couplings to fermions and gauge v h 1 bosons are universally suppressed by a factor of . cos θ : Heavy Higgs; its couplings to fermions and gauge bosons are v h 2 universally suppressed by a factor of . sin θ f f

  15. SM + Singlet v Cubic terms: ∼ λ 221 v Quartic terms are not very relevant for EWBG

  16. Effective potential V e ff ( φ h , φ s , T ) = V 0 ( φ h , φ s ) + V CW ( φ h , φ s ) 1 + V T ( φ h , φ s , T ) + V ring ( φ h , φ s , T ) T v breakdown + : bosons − : fermions φ i : background fields n j : degrees of freedom m 2 j ( φ h , φ s ) : field dependent [Profumo, Ramsey-Musolf, Shaughnessy (2007)] mass squared [Espinosa et al. NPB 854(2012)]

  17. Double Higgs Production

  18. Double Higgs Production through Gluon Fusion v Important because it can be used to measure the Higgs self-couplings Observed Higgs In SM: h 1 h 1 h 1 h 1 h 1 λ 111

  19. Double Higgs Production through Gluon Fusion v Important because it can be used to measure the Higgs self-couplings Observed Higgs In SM: h 1 h 1 h 1 h 1 h 1 λ 111 BSM: h 2 h 1 h 1 λ 211 v Production cross section of di-Higgs can be enhanced due to the decay of heavy resonances if m 2 > 2 m 1

  20. Double Higgs Production through Gluon Fusion v Resonant production in the singlet model and its implication for EWBG [1] J. M. No and M. Ramsey-Musolf, Phys. Rev. D 89, no. 9, 095031 (2014) [2] K. Assamagan et al., arXiv:1604.05324 [hep-ph]. [3] A. V. Kotwal, M. J. Ramsey-Musolf, J. M. No and P. Winslow, arXiv:1605.06123 [hep-ph]. [4] T. Huang, J. M. No, L. Pernié, M. Ramsey-Musolf, A. Safonov, M. Spannowsky and P. Winslow, arXiv:1701.04442 [hep-ph]. [5] R. Contino et al., arXiv:1606.09408 [hep-ph]. …

  21. Double Higgs Production through Gluon Fusion v What if is small and ? sin θ m 2 < 2 m 1 v Non-resonant production dominates BSM: σ ( h 2 h 2 ) and σ ( h 1 h 2 )

  22. Parameter space v Small angle regions are mostly dominated by σ ( h 2 h 2 ) v Plot for 100 TeV is similar

  23. Constraints on scalar potential v Vacuum stability: no vacuum exit at T=0 that is deeper than EW vaccum with v=246 GeV and v s = 0 GeV v Perturbativity: all dimensionless couplings < 4 pi at the EW scale v Perturbative unitarity: [Lee et al. PRD 16(1977)] v Number of free parameter (once fix and ) sin θ m 2 a 2 , b 3 and b 4 v

  24. Parameter space v Shaded region: satisfy all constraints v Blue regions show strongly first-order phase transition (SFOPT) allowed region

  25. Collider signatures: trilepton channel v Signal: v f v Background: v Jets fakes leptons: dominant background, t tbar v 3 prompt leptons: v WZ (W ) γ ∗ v WWW v ttW v ttZ or tt γ ∗ v tt

  26. Collider signatures: variables v Transverse mass : m T a q ( E a T + E b p a p b m T ( a, b ) ≡ T ) 2 − ( ~ T + ~ T ) 2 b T ) 2 = ( p a T ) 2 + m 2 ( E a a : can be a particle or a group of particles a , b : useful in rejecting backgrounds with non-prompt v leptons. V. Khachatryan et al. [CMS Collaboration], Eur. Phys. J. C 76, no. 8, 439 (2016)

  27. Collider signatures: variables j j ν W − h 2 p W + ν W + p ¯ h 2 ν W − : reconstruct mass of the mother particle ( ) when final v h 2 m T 2 states involves missing energy. v Two possibilities: 1) m 1 � ⇥ m T ( jj ` 1 , E miss T 1 ) , m T ( ` 2 ` 0 , E miss ⇤ T 2 =Min Max T 2 ) E miss + E miss = E miss E miss E miss T 1 T 2 T T 1 T 2 2) m 2 T 2 = m 1 T 2 ( ` 1 ↔ ` 2 ) 0

  28. Collider signatures: variables v Total invariant mass of visible particles:

  29. Collider signatures: benchmark points v LHC 14 TeV at 3/ab:

  30. Collider signatures: benchmark points v LHC 14 TeV at 3/ab:

  31. Collider signatures: benchmark points v LHC 14 TeV at 3/ab: v LHC 100 TeV at 30/ab:

  32. Collider signatures v m min T

  33. Additional probes CEPC and ILC v Presence of an addition scalar, alters the Zh 1 production cross section due to contributions to the wave-function renormalization of h 1 [Craig et al. PRL 111(2013), Curtin et al. JHEP1411 (2014), Huang et al. PRD.94 (2016) ] v Sensitivity of lepton colliders: δ Zh 1 > 1% [Dawson, et al. 1310.8361)] Higgs self-coupling measurement at pp collider for HL-LHC for 100 TeV pp collider [Dawson, et al. 1310.8361)] [Curtin et al. JHEP 1411(2014)]

  34. HL-LHC λ 111 Higgs self- coupling measurement (to the right) Excluded by HL-LHC ILC or CEPC (to the right)

  35. 100 TeV collider v Muon Higgs self- v Leptonic dipole moments: coupling measurement (solid, to the right) ILC or CEPC (dashed, to the right) v Green region: 5 sigma discovery using trilepton channel at 100 TeV with 30/ab v Yellow region: excluded by 2 sigma using trilepton channel at 100 TeV wth 30/ab

  36. Take Home Message v Direct probe of EWPT in non-resonantscalar pair production channels at both 14 TeV LHC and 100 TeV collider v At 14 TeV LHC, measurement of the h 1 self-coupling as well as that from lepton colliders will provide better coverage v At a 100 TeV collider, non-resonant production with m 2 ~170 GeV is sensitive to most of the parameter space with SFOPT.

  37. Take Home Message Prospect: channel σ ( h 1 h 2 ) v : displaced decay of h 2 m 2 < m 1 v

  38. THANK YOU!

  39. BACKUP

  40. Constraints on Mixing Angle v Light Higgs coupling measurements: ≡ sin 2 θ < 0 . 12 v combine v Independent of branching ratios of new decay channels v Independent of m 2 ATLAS-CONF-2014-010 v Heavy Higgs searches: v Depend on branching ratios of new decay channels v E.g. take B new =0, for sin 2 θ < 0 . 2 200 < m 2 < 600 GeV arXiv: 1504.00936, CMS 40

  41. Parameter space v Purple: satisfy all requirement at both tree and 1-loop level v circled: satisfy all requirement when 1-loop correction is added

  42. 14 TeV 100 TeV

  43. Collider signatures v m T 2

  44. Collider signatures v m vis

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend