CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures...

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CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings? Horizontal symmetry to solve SUSY flavor problem 3. Prediction of GUT on FCNC 4. Spontaneous CP violation 5. Summary with M. Bando, T. Yamashita with S. Kim, A. Matsuzaki, K. Sakurai, T. Yoshikawa M. Ishiduki New New

Transcript of CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures...

Page 1: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.)

1. SUSY GUT and Yukawa structures2. Unification for Matter sector Why are larger neutrino mixings? Horizontal symmetry to solve SUSY flavor problem3. Prediction of GUT on FCNC4. Spontaneous CP violation 5. Summary

with M. Bando, T. Yamashitawith S. Kim, A. Matsuzaki, K. Sakurai, T.   Yoshikawa     M. Ishiduki

NewNew

Page 2: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Quark&Lepton Masses & Mixings

SU(5) GUT with an assumption can explain these hierarchies

It may result in large FCNC in SUSY models

Page 3: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Masses & Mixings and GUT

020

4060

80100

120140

160180

up down chargedlepton

neutrino

1st2nd3rd

- 12

-10

-8

-6

-4

-2

0

2

4

Log[M

f/G

eV

]

updowncharged leptonneutrino

u, c, t Strongest

Neutrinos Weakest e, μ , τ    Middled, s, b Middle

CKM small mixings

MNS large mixings

These can be naturally realized in SU(5) GUT!!

Page 4: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

SU(5) SUSY GUT

Quark mixings(CKM) Lepton mixing(MNS)

have stronger hierarchy than

Stronger hierarchy leads to smaller mixings

Albright-BarrSato-Yanagida…

Page 5: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Mass hierarchy and mixings

Stronger hierarchy leads to smaller mixings

Stronger hierarchy Smaller mixings

Page 6: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

SU(5) SUSY GUT

Quark mixings(CKM) Lepton mixing(MNS)

have stronger hierarchy than

Stronger hierarchy leads to smaller mixings

Good agreement with masses & mixings

Page 7: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Large mixings and FCNC Even if universal sfermion masses at cutoff,

radiative correction induces non-universality.

Large mixings for SO(10) GUT relation

Large

Large FCNC are expected.

Borzumati-Masiero 85

Moroi 00 (SU(5))

Hisano-Moroi-Tobe-Yamaguchi-Yanagida Barbieri-Hall-Strumia 95

Chang-Masiero-Murayama 02 (SO(10))

Page 8: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Lepton Flavor Violation SO(10)

Masiero,Vempati,Vives 02

Page 9: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Constraints to EDM of Hg (neutron)

Bs mixing

Hisano-Shimizu 03

CDF 06

Page 10: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

1st Summary & Questions SU(5) GUT is in good agreement with the

hierarchies of quark & lepton masses and mixings.

has stronger hierarchy than Suppressed FCNC & EDM

SO(10) GUT relation looks bad. More unification of quark and lepton ? Origin of the assumption? Origin of various Yukawa hierarchies ?

Page 11: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

E6 GUT can answer these questions !

Page 12: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

E6 GUT answers these questions

More unification of quark and lepton ? Yes

E6 SO(10) Origin of the assumption ? Origin of various Yukawa hierarchies ?

Various Yukawa hierarchies can be induced from one Yukawa hierarchy in E6 GUT.

Page 13: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Unification

Three of six become superheavy after the breaking

Once we fix , three light modes of six are determined.

Guisey-Ramond-Sikivie,Aichiman-Stech, Shafi,Barbieri-Nanopoulos,Bando-Kugo,…

We assume all Yukawa matrices

Page 14: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Milder hierarchy for

fields from become superheavy.

Light modes have smaller Yukawa

couplings and milder hierarchy than

Superheavy

•Larger mixings in lepton sector than in quark sector.•Small•Small neutrino Dirac masses Suppressed radiative LFV

unless

Bando-N.M. 01N.M, T. Yamashita 02

Page 15: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

How to obtain various Yukawas?

Page 16: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

2nd Summary unification explains why the lepton sector has

larger mixings than the quark sector. Suppressed radiative LFV

A basic Yukawa hierarchy

The other Yukawa hierarchies

Hierarchy of is stronger than that of

Three come from the first 2 generation of

Page 17: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

SUSY flavor problem

E6+horizontal (family) symmetry More structures for suppressing FCNC.

Page 18: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Horizontal Symmetry

The 1st 2 generation have universal sfermion masses. Large top Yukawa coupling

Not sufficient to suppress FCNC

Dine-Kagan-LeighPomarol-TommasiniBarbieri-Hall…

•Origin of Yukawa hierarchy•Universal sfermion masses to suppress FCNC

Page 19: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Large neutrino mixings and FCNC

The universal sfermion masses only for the 1st 2 generation do not suppress FCNC sufficiently

if          .

Universality for all three generations is required!

Page 20: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

In E6 various Yukawa hierarchies are produced from one basic hierarchy from U(2) breaking.

Unification of generations by (or ) realizes the universality of sfermion masses.

A prediction for sfermion mass spectrum

This shift makes this model consisitent with the present experiments.(Universal masses for )

The 3rd generation FCNC can be large.(Testable)

+horizontal symmetry

Different

Universal mass Universal mass

N.M. 02,04N.M, T. Yamashita 04

Page 21: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Structures suppressing FCNC for

Small Yukawa couplings Small Universal sfermion masses for can increase without destabilizing the weak

scale. (Effective SUSY)

Page 22: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

How does FCNC processes take place in this model?

10: 5:

flavor violating No source of flavor violation

Since 10 contains Q, the form of unitary matrix V is CKM-like. We can parametrize it with Cabibbo angle λ.

For example, for the right-handed charged slepton sector,

Page 23: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Predictions of E6 GUT+horizontal symmetry

must be around the weak scale,because of the stability of the weak scale,while can be taken larger.

10: 5:

Kim-N.M.-Matsuzaki-Sakurai-Yoshikawa

Page 24: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

By picking up the 3-2 element, the size of τ→μ transition rate is order .

For μ→eγ, there are two passes to change the flavor μ→e. Both they are order .

If we raise overall SUSY scale m …

Propagator suppression from 1 or 2 generation becomes stronger, but mass difference

increase. As a result, both transition rate remain finite, and don’t decouple!

Non decoupling feature of this model (in lepton flavor violation)

Page 25: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Can we discover the LFVat the future experiments?

11100.1 (exclude)

9100.7

(exclude)

8100.7

14100.1

MEG experiment

τ→μγ

μ→eγ Detectable unless <400GeV

(super-)KEKB

Detectable, when tanβ is large and    <250GeV

Page 26: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

This model says thatfinal state lepton tends to be right-handed.

ie jep

ppq

p

Final state lepton has different chirality from initial one.

Intermediate state must be right-handed to pick up the .

Right-handed

e

e

Left-handed

spin

spin

How can we see this feature experimentally?

It is possible to check this feature experimentally by measuring the angular distribution of final state lepton.

Opposite fromMSSM+

Page 27: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Predictions (Quark sector)

The maginitudes are

the same order as of

the RGE effects in the universal mass case. New CP phases!!

The CP violation in B meson system may be detectable.

Page 28: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

CP violation in B meson

SM E6

O(0.04) O(0.006)

<0.15

0.006 <0.01

very small

very small

For

Page 29: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Bd φKs,η’Ks

O(0.1) deviation in B factory may be confirmedin SuperB factory.

is possible.

Gluino contribution is decoupled.Chargino contribution is not decoupled. in the limit

Page 30: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Summary table of E6 predictions

SM E6

O(0.04) O(0.006)

  <0.15

0.006 <0.01

very small

Page 31: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Strictly speaking,

when e.g.

This can be consistent with the experiments,

but the predictions can be changed.

If we take , this model dependent parts can be neglected.

No weak scale unstability!!

Discussions

Page 32: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

SUSY CP problem

Spontaneous CP violation by the VEV of F.

The severe constraints from CEDM are also satisfied because of real up-Yukawa couplings.

Page 33: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

SUSY CP problem EDM constraints from 1 loop

CEDM from Hg(neutron) even if Hisano-Shimizu ‘04

Contributions through stop loop are not decoupled.Complex Yukawa couplings induce them generically.

Page 34: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Difficulties in CEDM constraints

We usually assume complex Yukawa couplings to induce KM phase.

Complex Yukawa couplings induce the

complex generically.

Then CEDM constraints become severe.

Page 35: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Spontaneos CP violation in E6 +

Idea:

1,If the Higgs which breaks horizontal symmetry has complex phase, we can obtain complex Yukawa couplings, and KM phase.

2, Naively the suppression can be expected for the phase of SUSY parameters.

Ishiduki-Kim-N.M.-Sakurai

Page 36: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Anomalous GUT

To suppress the relative CP phase between and , non-trivial discrete charge must be imposed to .

N.M. 01, Bando-N.M. 01N.M.-Yamashita 02

Generic Interactions (Higher Dim. Op.)with O(1) Coefficients

The symmetry define the theory      Doublet-triplet splitting Suppressed Proton decay (dim. 5) Mass spectrum of Superheavy fields GUT scales and the other VEV scales Natural gauge coupling unification (miraculous cancellation!) Realistic quark&lepton masses and mixings (bi-large neutrino mixings) mu problem is solved

Page 37: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

A model with a discrete symmetry

Real up-type Yukawa couplings real

CEDM constraints can be satisfied. Complex down-type Yukawa couplings

KM phase can be induced. The point

: real,

: complex

Bonus 1

Page 38: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

A model with a discrete symmetry Bonus 2: small up quark mass is realized.

Usually, to obtain the CKM matrix

Too large good value!

Page 39: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

A model with a discrete symmetry

Bonus 3?: # of O(1) parameters =10 13 physical parameters

One of the relations

Page 40: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

A model with a discrete symmetry

The discrete symmetry is consistent with the E6 Higgs sector which realizes doublet-triplet splitting and

mixing is required to avoid massless electron in this model.

Page 41: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Summary In GUT, one basic hierarchy for Yukawa couplings

results in various hierarchical structures for quarks and leptons including larger neutrino mixings.

Horizontal symmetry can easily reproduce the basic hierarchy, and suppress FCNC naturally in GUT. (not in SO(10) GUT)

Spontaneous CP violation solves SUSY CP problem(CEDM)

The simpler unification of quarks and leptons explains the more questions.

larger neutrino mixings

SUSY Flavor ProblemSUSY CP Problem

Page 42: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Summary Peculiar sfermion spectrum can be tested.

without unstability of weak scale. FCNC of 3rd generation becomes larger.

LFV ( ) and CP violation in B ( etc) may be detectable in future.

Polarization of final lepton can test the GUT scenario.      

Different

Universal mass Universal mass

Page 43: CP & SUSY breaking and GUT Nobuhiro Maekawa (Nagoya Univ.) 1. SUSY GUT and Yukawa structures 2. Unification for Matter sector Why are larger neutrino mixings?

Future work

What is the signature in LHC? CP violation in neutrino oscillation? The origin of SUSY breaking? The mediation me

chanism of SUSY breaking? Can the D term contribution be sufficiently smal

l?

Decoupling feature mildens the constraints

Non-Abelian discrete symmetry? Cosmology? ….