S 3 Symmetry as the Origin of CKM Matrix

Similar documents
Fermion Mixing Angles and the Connection to Non-Trivially Broken Flavor Symmetries

Yang-Hwan, Ahn (KIAS)

Maria Dimou In collaboration with: C. Hagedorn, S.F. King, C. Luhn. Tuesday group seminar 17/03/15 University of Liverpool

Standard Model & Beyond

Two-Higgs-Doublet Model

Leaving Plato s Cave: Beyond The Simplest Models of Dark Matter

Lepton Flavor Violation

Updated S 3 Model of Quarks

Introduction to the SM (5)

Electroweak-scale Right-handed Neutrino Model And 126 GeV Higgs-like Particle

arxiv: v1 [hep-ph] 16 Mar 2017

Electroweak and Higgs Physics

Problems for SM/Higgs (I)

generation Outline Outline Motivation Electroweak constraints Selected flavor constraints in B and D sector Conclusion Nejc Košnik

A model of the basic interactions between elementary particles is defined by the following three ingredients:

Neutrino Masses & Flavor Mixing 邢志忠. Zhi-zhong Xing. (IHEP, Winter School 2010, Styria, Austria. Lecture B

Adding families: GIM mechanism and CKM matrix

F. Börkeroth, F. J. de Anda, I. de Medeiros Varzielas, S. F. King. arxiv:

Yang-Hwan, Ahn (KIAS)

Spontaneous CP violation and Higgs spectra

Two models with extra Higgs doublets and Axions

Lecture III: Higgs Mechanism

Gauge-Higgs Unification on Flat Space Revised

Non-Abelian SU(2) H and Two-Higgs Doublets

A novel and economical explanation for SM fermion masses and mixings

Hidden two-higgs doublet model

+ µ 2 ) H (m 2 H 2

PARTICLE PHYSICS Major Option

Pati-Salam GUT-Flavour Models with Three Higgs Generations

The Standard Model and beyond

A Two Higgs Doublet Model for the Top Quark

SU(3)-Flavons and Pati-Salam-GUTs

Current knowledge tells us that matter is made of fundamental particle called fermions,

Can the Hbb coupling be equal in magnitude to its Standard Model value but opposite in sign? Howard E. Haber July 22, 2014

A Novel and Simple Discrete Symmetry for Non-zero θ 13

Antonio Pich. IFIC, CSIC Univ. Valencia.

Flavor Physics in the multi-higgs doublet models induced by the left-right symmetry

Search for new physics in rare D meson decays

Neutrino Models with Flavor Symmetry

Gauged Flavor Symmetries

The Higgs Boson and Electroweak Symmetry Breaking

Perspectives Flavor Physics beyond the Standard Model

SYMMETRY BEHIND FLAVOR PHYSICS: THE STRUCTURE OF MIXING MATRIX. Min-Seok Seo (Seoul National University)

Theoretical Particle Physics Yonsei Univ.

Simplified models in collider searches for dark matter. Stefan Vogl

Flavour and Higgs in Pati-Salam Models

Non Standard Neutrino Interactions

Foundations of Physics III Quantum and Particle Physics Lecture 13

Beyond Standard Model Effects in Flavour Physics: p.1

Extra-d geometry might also explain flavor

RG evolution of neutrino parameters

The Standard Model and Beyond

Beta and double beta decay

Flavour Physics Lecture 1

Low Scale Flavor Gauge Symmetries

Successful Leptogenesis in the Left-Right Symmetric Seesaw Mechanism

BINARY TETRAHEDRAL GROUP (T )

Lecture 03. The Standard Model of Particle Physics. Part II The Higgs Boson Properties of the SM

PHYSICS BEYOND SM AND LHC. (Corfu 2010)

Steve King, DCPIHEP, Colima

Introduction to Supersymmetry

SUSY models of neutrino masses and mixings: the left-right connection

E 6 Spectra at the TeV Scale

Dipole operator constraints on composite Higgs models

Mirror fermions, electroweak scale right-handed neutrinos and experimental implications

Symmetry Origin of Observable Nonunitary Neutrino Mixng Matrix in TeV Scale Seesaw Models

Introduction to particle physics Lecture 13: The Standard Model

Discrete dark matter mechanism

For Review Only. General Structure of Democratic Mass Matrix of Lepton Sector in E 6 Model. Canadian Journal of Physics

Phenomenology of the flavour messenger sector

Flavour and CP Violation Phenomenology in SUSY with an SU(3) Flavour Symmetry

Decoupling and Alignment in Light of the Higgs Data. Howard E. Haber Pi Day, 2014 Bay Area ParCcle Physics Seminar San Francisco State Univ.

Introduction to the Standard Model New Horizons in Lattice Field Theory IIP Natal, March 2013

Introduction to particle physics Lecture 6

Unified Dark Matter. SUSY2014 Stephen J. Lonsdale. The University of Melbourne. In collaboration with R.R. Volkas. arxiv:

perturbativity Pankaj Sharma Based on : arxiv: st September, 2012 Higgs-electroweak precision, vacuum stability and perturbativity

CP violation in charged Higgs production and decays in the Complex 2HDM

Triplet Higgs Scenarios

arxiv: v1 [hep-ph] 3 Aug 2016

Detection Prospects of Doubly Charged Higgs Bosons from the Higgs Triplet Model at the LHC

Quark flavour physics

DARK MATTER STABILITY FROM D ISCRETE FLA VOR SYMMETRIES

TeV-scale type-i+ii seesaw mechanism and its collider signatures at the LHC

The Higgs Mechanism and the Higgs Particle

Models of Neutrino Masses

The Higgs discovery - a portal to new physics

The standard model of electroweak interactions and QD has proven extremely successful. In the last decade no new elementary particles or interactions

Shahram Rahatlou University of Rome

The Standard Model. Antonio Pich. IFIC, CSIC Univ. Valencia

What multiple Higgs doublets can do for you

SO(10) SUSY GUTs with family symmetries: the test of FCNCs

New Physics from Vector-Like Technicolor: Roman Pasechnik Lund University, THEP group

Basics of Higgs Physics

Phenomenology of low-energy flavour models: rare processes and dark matter

Search for the exotic decays of the Higgs boson

Finding the Higgs boson

The Flavour Portal to Dark Matter

Lecture 3. A. Yu. Smirnov International Centre for Theoretical Physics, Trieste, Italy

Flavor, Higgs couplings and DM within September multi-higgs 5, 2016models1 / 48

Gauge U(1) Dark Symmetry and Radiative Light Fermion Masses

Transcription:

S 3 Symmetry as the Origin of CKM Matrix Ujjal Kumar Dey Physical Research Laboratory October 25, 2015 Based on: PRD 89, 095025 and arxiv:1507.06509 Collaborators: D. Das and P. B. Pal 1 / 25

Outline 1 2 3 4 5 6 2 / 25

Outline 1 2 3 4 5 6 3 / 25

Discrete symmetries in particle physics In SM fermions (both leptons and quarks) come in three generations There are inter-generational differences, in contrast to their uniformity in gauge interactions Two types of hierarchies in the flavor sector: Large hierarchy within the charged fermion sector and enormous hierarchy between charged fermion and neutrino masses Mixing information in quark and lepton sector Finite discrete symmetry groups (e.g., S 3, S 4, D 4, A 4 etc.) provide an effective way of explaining some of these flavor issues We will consider the case of S 3 symmetric model 4 / 25

Outline 1 2 3 4 5 6 5 / 25

S 3 is the permutation group of three objects The order of S 3 is 3! = 6 The six elements correspond to the following transformations e : (x 1, x 2, x 3) (x 1, x 2, x 3), a 1 : (x 1, x 2, x 3) (x 2, x 1, x 3), a 2 : (x 1, x 2, x 3) (x 3, x 2, x 1), a 3 : (x 1, x 2, x 3) (x 1, x 3, x 2), a 4 : (x 1, x 2, x 3) (x 3, x 1, x 2), a 5 : (x 1, x 2, x 3) (x 2, x 3, x 1). S 3 can also be thought of as the symmetry of an equilateral triangle with a 1 and a 1a 2 being the reflection and the 2π/3 rotation respectively 6 / 25

Outline 1 2 3 4 5 6 7 / 25

Scalar Potential The scalar sector consists of three SU(2) L scalar doublets φ i (i = 1, 2, 3) (φ 1, φ 2) T transform as an S 3 doublet and φ 3 is an S 3 singlet Most general S 3-symmetric scalar potential with these fields can be written as, V (φ i ) =µ 2 1(φ 1 φ1 + φ 2 φ2) + µ2 3φ 3 φ3 + λ1(φ 1 φ1 + φ 2 { φ2)2 + λ 2(φ 1 φ2 φ 2 φ1)2 + λ 3 (φ 1 φ2 + φ 2 φ1)2 + (φ 1 φ1 φ 2 φ2)2} { } + λ 4 (φ 3 φ1)(φ 1 φ2 + φ 2 φ1) + (φ 3 φ2)(φ 1 φ1 φ 2 φ2) + h.c. + λ 5(φ 3 φ3)(φ 1 φ1 + φ 2 φ2) + λ6 { (φ 3 φ1)(φ 1 φ3) + (φ 3 φ2)(φ 2 φ3) } + λ 7 { (φ 3 φ1)(φ 3 φ1) + (φ 3 φ2)(φ 3 φ2) + h.c. } + λ 8(φ 3 φ3)2 8 / 25

Scalar Potential The minimization conditions for the potential are: 2µ 2 1 = 2λ 1(v 2 1 + v 2 2 ) 2λ 3(v 2 1 + v 2 2 ) 6λ 4v 2v 3 (λ 5 + λ 6 + 2λ 7)v 2 3, 2µ 2 1 = 2λ 1(v 2 1 + v 2 2 ) 2λ 3(v 2 1 + v 2 2 ) 3v3 v 2 λ 4(v 2 1 v 2 2 ) (λ 5 + λ 6 + 2λ 7)v 2 3, 2µ 2 3 = λ 4 v 2 v 3 (v 2 2 3v 2 1 ) (λ 5 + λ 6 + 2λ 7)(v 2 1 + v 2 2 ) 2λ 8v 2 3. There exists three nontrivial conditions for consistency, λ 4= 0 a massless scalar v 2= 3v 1 and v 3 = 0 interesting for DM aspect (?) v 1= 3v 2 and v 3 arbitrary present case 9 / 25

For the case v 1 = 3v 2, even after spontaneous symmetry breaking, a Z 2 subgroup of S 3 remains preserved To be precise, the vacuum in the (φ 1, φ 2) T basis is ( 3, 1) T and ( ) 1 3 ( 3 ) ( ) ( ) 2 2 2 3 1 3 = with 2 2 = 1 2 1 1 3 2 1 2 3 2 1 2 This remnant Z 2 will be used to construct the realistic model for quarks 10 / 25

Physical Scalars After electroweak symmetry breaking from three SU(2) L doublet scalars we will have nine physical scalars Physical States Transformation under Z 2 h 0, H ± 1, A1 Odd h, H, H ± 2, A2 Even Here h will have the SM-like couplings in the alignment limit i.e., sin(β α) = 1 where β = tan 1 (2v 2/v 3) and α is the mixing angle in the h H sector 11 / 25

λs and Masses The quartic couplings and the physical scalar masses can be connected via the following relations: { 1 ( λ 1 = 2v 2 sin 2 m 2 h β cos2 α + m 2 ) ( H sin2 α + m 2 1+ m2 2+ cos2 β 1 )} 9 m2 h0, 1 { λ 2 = 2v 2 sin 2 (m 2 } 1+ β m2 A1 ) (m2 2+ m2 A2 ) cos2 β, ( ) 1 4 λ 3 = 2v 2 sin 2 β 9 m2 h0 + m2 2+ cos2 β m 2 1+, λ 4 = 2 mh0 2 1 9 v 2 sin β cos β, λ 5 = 1 { sin α cos α ( v 2 m 2 ) H sin β cos β m2 h + 2m 2 2+ + 1 m 2 } h0 9 cos 2, β λ 6 = 1 ( 1 m 2 ) h0 v 2 9 cos 2 β + m2 A2 2m2 2+, λ 7 = 1 ( 1 m 2 ) h0 2v 2 9 cos 2 β m2 A2 { 1 ( λ 8 = 2v 2 cos 2 m 2 h β sin2 α + m 2 ) H cos2 α 1 } 9 m2 h0 tan2 β. 12 / 25

Constraints from unitarity and stability log 10 (tan β) log 10 (tan β) Unitarity and stability demands that tan β [0.3, 17] and the physical scalars are below 1 TeV 13 / 25

Outline 1 2 3 4 5 6 14 / 25

Quark Sector In the gauge basis the S 3 transformation properties of the quarks, 1 : Q 3, u 3R, d 3R, ( ) ( ) Q1 u1r 2 :,, Q 2 u 2R ( d1r where Q i s are the usual left-handed SU(2) L quark doublets and u ir s (d ir s) are the right-handed up (down) type SU(2) L singlets The Yukawa Lagrangian is given by, L Yuk = L U Yuk + L D Yuk where ( L U Yuk = y1 u Q1 φ3u 1R + Q ) {( 2 φ3u 2R y2 u Q1 φ2 + Q ) 2 φ1 u 1R ( + Q1 φ1 Q } 2 φ2 )u 2R y3 u Q 3 φ3u 3R y4 u Q ( 3 φ1u 1R + φ ) 2u 2R ( ) y5 u Q 1 φ 1 + Q 2 φ 2 u 3R + h.c. L D Yuk =L U Yuk with (u ir d ir, y u i d 2R y d i, φ i φ i ) ) 15 / 25

Quark Mass Matrices The general form of the quark mass matrix (for brevity only up-type case is shown) is given by, y1 u v 3 + y2 u v 2 y2 u v 1 y5 u v 1 M u = y2 u v 1 y1 u v 3 y2 u v 2 y5 u v 2 y4 u v 1 y4 u v 2 y3 u v 3 This can be block-diagonalized by the unitary matrix, 1 3 0 2 2 X = 3 1 0 2 2 0 0 1 in the following way, y1 u v 3 2y2 u v 2 0 0 M block u = X M ux = 0 y1 u v 3 + 2y2 u v 2 2y5 u v 2 0 2y4 u v 2 y3 u v 3 Recall that the vacuum alignment v 1 = 3v 2 implies the breaking S 3 Z 2 16 / 25

The Z 2-odd combination of fermion will not mix with the Z 2-even counterparts in the fermion mass terms We can define the top quark as the Z 2-odd combination with mass m t = y u 1 v 3 2y u 2 v 2 = v y u 1 cos β y u 2 sin β The block-diagonal form of M block u implies that one can define the following intermediate basis in the up-sector separating the Z 2-odd and Z 2-even components, t c = X u u 1 u 2 u 3 Rotate further the 2 2 block to get the physical u and c quarks Similar treatment can be followed for down sector by identifying the b as the Z 2-odd combination 17 / 25

Getting the CKM Now one can get M diag u = U L Mblock u U R = diag(m t, m c, m u) where both U L and U R are block-diagonal One can take U L to be of the form 1 0 0 U L = 0 cos θ u sin θ u 0 sin θ u cos θ u Then M diag u = U L Mblock u U R = U L X M uxu R = U L MuU R (say); where U L,R = XU L,R Similarly in the down sector D L,R = XD L,R where 1 0 0 D L = 0 cos θ d sin θ d 0 sin θ d cos θ d 18 / 25

The CKM matrix is thus given by, V CKM = U L D L = U L D L = b s d t 1 0 0 c 0 cos θ C sin θ C where θ C = θ d θ u u 0 sin θ C cos θ C By choosing sin θ C = sin(θ d θ u) λ, one can reproduce the Cabibbo block of the CKM matrix The near block-diagonal structure of CKM matrix can be thought of as a direct consequence of the remnant Z 2 symmetry Only a mild breaking of this Z 2 can result in the exact structure of the CKM matrix 19 / 25

Mild Breaking of Z 2 Gives the Exact Form of CKM Matrix Introduce a soft S 3-breaking term (say, µ 2 13(φ 1 φ3 + φ 3 φ1)) This will slightly modify the VEV alignment, v 1 = 3v 2 + with v 1,2 Thus the mass matrix in the up sector (for example) will be, 0 y2 u y5 u 0 u M u = M u + y2 u 2 u 5 0 0 M u + u y4 u 2 0 0 0 0 u 4 0 0 Clearly, now we will have M diag u = U M L uu R where U L (and similarly U R ) can be defined as U L = U L U L and U L is close to unit matrix which takes care of the very small, 1 Aλ 2 Cλ 3 U L = Aλ 2 1 0 + O(λ 4 ) C λ 3 0 1 Note that D L can also be approximated as 1 3 20 / 25

Thus choosing the parameter C = A(ρ + iη), one can write, V CKM = U L U L D LD L b s d t 1 Aλ 2 Aλ 3 (1 ρ iη) = c Aλ 2 1 λ2 λ 2 + O(λ4 ) u Aλ 3 (ρ iη) λ 1 λ2 2 Even if we consider small departure of D L from 1 3 the general form of V CKM will not change 21 / 25

Outline 1 2 3 4 5 6 22 / 25

The Z 2-odd particles (e.g., h 0, A 1, H ± 1 ) will only have off-diagonal couplings with quarks involving 3rd generation physical quarks (t or b). But the mild breaking of Z 2 will lead to tiny diagonal couplings For example, if h 0 is light enough, it can be looked for in the channel t ch 0 followed by h 0 µτ or eτ. But for heavy h 0 ILC is the better option to produce h 0 via the coupling with SM-like Higgs h, (h 0 h 0 h) The precise measurement of the decay width h γγ can also put stringent constraints (see arxiv:1408.6133) Like most of the extended scalar sector models here also the FCNC related issues are to be dealt with much care 23 / 25

Outline 1 2 3 4 5 6 24 / 25

Starting from an S 3 symmetric theory and its spontaneous breaking to an approximate Z 2 answers the following puzzles Why the third generation of quarks are so different (massive) from the other two? As the third generation quarks are Z 2-odd Why the CKM matrix is nearly block-diagonal? Because of the misalignment of the mixing between the first two generations in the up and down sectors, both of which are Z 2-even The study of the lepton sector and a detailed exploration of the flavour constraints are yet to be done (future project) 25 / 25