radion flavor in warped extra
play

Radion flavor in Warped Extra Dimensions. a by Manuel Toharia - PowerPoint PPT Presentation

Radion flavor in Warped Extra Dimensions. a by Manuel Toharia (University of Maryland) at PHENO 2009, Madison, May 2009 a Based on arXiv:0812.2489 A.Azatov, M.T., L.Zhu Outline Introduction Flavor in RS The radion in RS radion


  1. Radion flavor in Warped Extra Dimensions. a by Manuel Toharia (University of Maryland) at PHENO 2009, Madison, May 2009 a Based on arXiv:0812.2489 A.Azatov, M.T., L.Zhu

  2. Outline • Introduction – Flavor in RS – The radion in RS • radion Flavor • Conclusions

  3. Introduction • Warped Extra Dimensions: One compact extra dimension with warped geometry. • Original setup: Two branes as boundaries and all SM fields on the TeV Brane → RS1. – Towers of KK gravitons – Radion graviscalar • More recent setups: Two branes, Higgs field on TeV brane, SM fields in the “bulk”. – Towers of KK gravitons – Towers of KK SM fields – Radion graviscalar

  4. Flavor anarchy: masses and mixings from fermion localization

  5. The Radion and its interactions In the RS1 model [ Randall,Sundrum, ( ′ 98)] the background metric g o AB is defined by R 2 e − 2 σ η µν dx µ dx ν + dy 2 η µν dx µ dx ν + dz 2 � ds 2 � = = z 2 with σ ( y ) = ky (and R = 1 /k ). Hierarchy created between the ( z = R and z = R ′ ). two boundaries at y = 0 and y = πr 0 The linear metric perturbations h AB ( x, y ) can be reduced to ds 2 = dx µ dx ν + e − 2 σ η µν + e − 2 σ h TT 1 + 2 e 2 σ r ( x ) � � �� � � dy 2 µν ( x, y ) − η µν r ( x ) (the graviscalar r ( x ) is massless. A stabilization mechanism pro- viding it with mass is assumed for example[ Golberger,W ise ( ′ 99)] )

  6. Ex. RS1 - Matter on the brane Higgs H 1 � dx 4 T µ S int ( r ) = µ φ 0 ( x ) Λ r Higgs-like couplings! �� � �� � α s φ 0 α s H G µν G µν v G µν G µν Gluon F 1 / 2 ( τ i ) / 2 − b 3 F 1 / 2 ( τ i ) / 2 8 π Λ r 8 π i i �� � �� � α φ 0 α H i N i F µν F µν e 2 i N i v F µν F µν γ c F i ( τ i ) − ( b 2 + b Y ) e 2 c F i ( τ i ) 8 π Λ r 8 π i i φ 0 H V V α V α M 2 V V α V α W , Z v M 2 Λ r H φ 0 m f ¯ v m f ¯ ff ff f Λ r

  7. Radion Production vs. Higgs production 2 10 1 10 0 10 −1 10 LHC σ (pb) −2 10 −3 10 −4 10 gg fusion −5 10 WW,ZZ fusion Tevatron W φ Run2 Z φ −6 10 − , gg −> tt − φ qq −7 10 200 400 600 800 1000 m φ (GeV) K.Cheung (’00)(Λ φ = 1 TeV) (CMS TDR)

  8. Radion Branchings vs. Higgs Branchings 1 WW gg ZZ 0.1 bb Br � Φ�� XX � 0.01 hh Ξ� 0 ΓΓ tt 0.001 � 4 10 BULK FIELDS RS1 � 5 10 100 200 300 400 500 600 m Φ Branchings of the radion vs. Branchings of Higgs vs. its its mass m φ mass (from CMS TDR)

  9. LHC REACH in ( m φ − Λ φ ) (with Nobu Okada)

  10. Radion couplings to 5D fermions • 1 family of bulk fermions and a Brane Higgs: [Csaki , Hubisz , Lee(07)] φ 0 ( c Q − c U ) m u ¯ uu Λ r Computation slightly involved, but a way to understand it is look at R ′ dependance in fermion mass term: m f ∼ Y v ( R/R ′ ) c Q − c U − 1 ∼ (1 /R ′ ) c Q − c U Radion can be understood as perturbation in the interbrane distance L , or in 1 /R ′ scale in the conformal frame. So we can 1 /R ′ → 1 /R ′ (1 + φ/ Λ r ) write Then include it in mass term and expand linearly in the radion ( c Q − c U ) φ/ Λ r (1 /R ′ ) c Q − c U ⇒ ( c Q − c U ) φ/ Λ r m f

  11. • We extend to 3 families and allow for bulk Higgs (localized towards IR brane) [ A . Azatov , M . T ., L . Zhu (arXiv:0812 . 2489)] φ 0 d ¯ Q − c j D ) m ij d iL d j ( c i R + h.c Λ r φ 0 ¯ d L ( c Q m d − m d c D ) d R Λ r where m d is not in the diagonal physical basis and c Q , D are diagonal matrices. c i Q,D are the fermion bulk parameters for UV fermions BUT | c i Q,D | = 1 / 2 for IR fermions (and c Q > 0 and c D < 0). ⇒ tree-level FCNC’s! Diagonalize fermion mass matrix means here φ 0 d phys ¯ d phys ( U † c Q U ) m d diag − m d diag ( W † c D W ) � � L R Λ r

  12. In the physical basis we obtain the estimate: L HFV = 1 � j φ 0 ¯ L d j a d d i m d i m d R + h.c. ij Λ r G ( c Q i ) λ 3 � �   m b m s ( c Q 1 − c D 1 ) ( c Q 1 − c Q 2 ) λ m d m d   � 2 ) λ 2 � m d m b a d ( c D 1 − c D 2 ) 1 ( c Q 2 − 1 ij ∼ ( c Q 2 − c D 2 )   λ m s m s     � � m d m s F ( c D i ) 1 ( c D 2 − c D 3 ) 1 ( 1 2 − c D 3 ) λ 3 λ 2 m b m b where we have taken c Q 3 = 1 2 (IR localized) and λ ∼ 0 . 22 . F and G are O ( . 1) functions of the c i ’s ⇒ a ds ∼ a sd ∼ 0 . 06

  13. Tree level RADION exchange will induce s L d R s R d L with coefficient 1 ⇒ K − ¯ C 4 = a ds a sd m d m s K mixing and ǫ K put tight bounds m 2 φ Λ 2 r 25000 25000 Radion interaction scale � r � GeV � a ds � 0.5 KKG � � M Pl � R � � GeV � 20000 20000 15000 15000 a ds � 0.12 10000 10000 M 1 5000 5000 a ds � 0.03 0 10 20 50 100 200 500 Radion mass m r � GeV � Figure 1: Bounds in m φ − Λ r plane from ǫ K . Here we have called � | a ds a ∗ a ds ≡ sd | . From [ A . Azatov , M . T ., L . Zhu (arXiv:0812 . 2489)]

  14. Outlook Maybe LHC discovers one or two neutral scalars, and that’s IT. Is it a Higgs? (or a 2 Higgs doublet model?) or is it an RS type scenario? (radion plus a Higgs?) The Radion is Higgs-like but has special signatures: • Very narrow width • Special production process and we have just seen that • Probing the size of FV couplings important. • Without flavor symmetry, m radion > ∼ 20 − 50 GeV • Flavor at LHC? ( r → t c ?) • Higgs-radion mixing?

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