radiative generation of the lepton mass

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Radiative Generation of the Lepton Mass Kei Yagyu (National Central U.) High1-2014, KIAS-NCTS Joint Workshop on Particle Physics, String Theory and Cosmology High1 Resort, Feb. 9-15, 2014 arXiv: 1311.4360 [hep-ph] Collaboration with Hiroshi Okada (KIAS)

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Radiative Generation of the Lepton Mass. Kei Yagyu (National Central U.). Collaboration with Hiroshi Okada (KIAS). arXiv : 1311.4360 [ hep-ph ]. High1-2014, KIAS-NCTS Joint Workshop on Particle Physics, String Theory and Cosmology High1 Resort, Feb. 9-15, 2014. Higgs Discovery. - PowerPoint PPT Presentation

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Page 1: Radiative Generation of the Lepton Mass

Radiative Generation of the Lepton Mass

Kei Yagyu (National Central U.)

High1-2014, KIAS-NCTS Joint Workshop on Particle Physics, String Theory and Cosmology

High1 Resort, Feb. 9-15, 2014

arXiv: 1311.4360 [hep-ph]

Collaboration with Hiroshi Okada (KIAS)

Page 2: Radiative Generation of the Lepton Mass

  Higgs Discovery A Higgs boson has been discovered with the mass of 126 GeV. Mass, CP and signal strengths are consistent with those of the SM Higgs boson within the error. So far, Higgs boson couplings are not measured so accurately.

κV

κ F

κV = ghVV (exp)/ghVV (SM)κF = ghFF (exp)/ghFF (SM)

In particular, Yukawa couplings have not been measured precisely (about ±50% error).

Scaling factors

2

SM

Page 3: Radiative Generation of the Lepton Mass

  Higgs Discovery A Higgs boson has been discovered with the mass of 126 GeV. Mass, CP and signal strengths are consistent with those of the SM Higgs boson within the error. So far, Higgs boson couplings are not measured so accurately.

κV

κ F

κV = ghVV (exp)/ghVV (SM)κF = ghFF (exp)/ghFF (SM)

In particular, Yukawa couplings have not been measured precisely (about ±50% error).

Scaling factors

3

SM

1

1.2

1.4

0.8

0.6Higgs discovery ≠ Yukawa interactions have been confirmed.

Page 4: Radiative Generation of the Lepton Mass

Yukawa Interaction in the SM

In the SM, the Yukawa Lagrangian and coupling are given by

Mass

Coup.

<Φ> (~ mt)

100 GeV

τ

1 GeV

μ

0.1 GeV

e

0.1 eV 0.001 GeV

νe, νμ, ντ

110-210-310-5

There is the one-to-one correspondence between mF and yF.

Neutrinos are massless

4

Page 5: Radiative Generation of the Lepton Mass

Yukawa Interaction in the SM

In the SM, the Yukawa Lagrangian and coupling are given by

Mass

Coup.

<Φ> (~ mt)

100 GeV

τ

1 GeV

μ

0.1 GeV

e

0.1 eV 0.001 GeV

νe, νμ, ντ

110-12

If we introduce νR and Dirac neutrino masses (L# cons.), then We need a too small Yukawa coupling.

10-210-310-5

5

Page 6: Radiative Generation of the Lepton Mass

Yukawa Interaction in the SM

In the SM, the Yukawa Lagrangian and coupling are given by

Mass

Coup.

<Φ> (~ mt)

100 GeV

τ

1 GeV

μ

0.1 GeV

e

0.1 eV 0.001 GeV

νe, νμ, ντ

1

We have already introduced tiny Yukawa couplings for c-leptons.

10-12 10-210-310-5

6

Page 7: Radiative Generation of the Lepton Mass

Yukawa Interaction in the SM

In the SM, the Yukawa Lagrangian and coupling are given by

Mass

Coup.

<Φ> (~ mt)

100 GeV

τ

1 GeV

μ

0.1 GeV

e

0.1 eV 0.001 GeV

νe, νμ, ντ

110-12 10-210-310-5

Why lepton masses are so small compared to the EW scale?

7

Page 8: Radiative Generation of the Lepton Mass

Yukawa Interaction in the SM

In the SM, the Yukawa Lagrangian and coupling are given by

Mass

Coup.

<Φ> (~ mt)

100 GeV

τ

1 GeV

μ

0.1 GeV

e

0.1 eV 0.001 GeV

νe, νμ, ντ

110-12 10-210-310-5

Why there is a large hierarchy between masses for neutrinos and charged

leptons?

8

Page 9: Radiative Generation of the Lepton Mass

Lepton Masses (Traditional Way)

Majorana neutrino mass

Dirac c-lepton mass

Tree level : Type-I, II and III seesawLoop level : Radiative seesaw models

9

Weinberg (1980)

Page 10: Radiative Generation of the Lepton Mass

Lepton Masses (Our Idea)

Majorana neutrino mass

Dirac c-lepton mass

Δ0,1 : SU(2) triplet Higgs fieldvΔ : Triplet VEV

10

Page 11: Radiative Generation of the Lepton Mass

Lepton Masses (Our Idea)

Majorana neutrino mass

Dirac c-lepton mass

Δi : SU(2) triplet Higgs fieldvΔ, vΔ

’ : Triplet VEV, vΔ << v

Loop

Loop

11

Page 12: Radiative Generation of the Lepton Mass

Lepton Masses (Our Idea)

Majorana neutrino mass

Dirac c-lepton mass

Δi : SU(2) triplet Higgs fieldvΔ : Triplet VEV, vΔ << v

Loop

Loop

12

Why lepton masses are so small compared to the EW scale?

Smallness is explained by the loop suppression factor and triplet VEVs.

Page 13: Radiative Generation of the Lepton Mass

Lepton Masses (Our Idea)

Majorana neutrino mass

Dirac c-lepton mass

Δi : SU(2) triplet Higgs fieldvΔ : Triplet VEV, vΔ << v

Loop

Loop

13

Why there is a large hierarchy between masses for neutrinos and charged

leptons?

Number of triplet VEV is different.

Page 14: Radiative Generation of the Lepton Mass

Model

Symmetry: SU(3)c×SU(2)L×U(1) Y×Z2(unbroken)×Z4

Particle Content (Z2-even, Z2-odd):

To forbid the tree level massesTo close the loop diagram + Stability of DM candidate

Φ Δ0 Δ1 Φ3/2 η S Li (eR, μR) τR Eα

SU(2)L

U(1)Y

2 3 3 2 2 1     2 1 1 1

1/2 0 1 3/2 1/2 0 -1/2 -1 -1 -1

Z4 -i -1 -1 1 1 -i 1 -i +i 1

Scalar bosons Leptons 14

Page 15: Radiative Generation of the Lepton Mass

Model

Particle Content (Z2-even, Z2-odd):Φ Δ0 Δ1 Φ3/2 η S Li (eR, μR) τR Eα

SU(2)L

U(1)Y

2 3 3 2 2 1     2 1 1 1

1/2 0 1 3/2 1/2 0 -1/2 -1 -1 -1

Z4 -i -1 -1 1 1 -i 1 -i +i 1

15

Page 16: Radiative Generation of the Lepton Mass

Model

Particle Content (Z2-even, Z2-odd):Φ Δ0 Δ1 Φ3/2 η S Li (eR, μR) τR Eα

SU(2)L

U(1)Y

2 3 3 2 2 1     2 1 1 1

1/2 0 1 3/2 1/2 0 -1/2 -1 -1 -1

Z4

e, μ

e, μ

Φ

-i -1 -1 1 1 -i 1 -i +i 1

16

Page 17: Radiative Generation of the Lepton Mass

Model

Particle Content (Z2-even, Z2-odd):Φ Δ0 Δ1 Φ3/2 η S Li (eR, μR) τR Eα

SU(2)L

U(1)Y

2 3 3 2 2 1     2 1 1 1

1/2 0 1 3/2 1/2 0 -1/2 -1 -1 -1

Z4

L

L

Δ1

-i -1 -1 1 1 -i 1 -i +i 1

17

Page 18: Radiative Generation of the Lepton Mass

Model

Particle Content (Z2-even, Z2-odd):Φ Δ0 Δ1 Φ3/2 η S Li (eR, μR) τR Eα

SU(2)L

U(1)Y

2 3 3 2 2 1     2 1 1 1

1/2 0 1 3/2 1/2 0 -1/2 -1 -1 -1

Z4

τ

Φ

-i -1 -1 1 1 -i 1 -i +i 1

18

Page 19: Radiative Generation of the Lepton Mass

Lagrangian

Masses for Eα Tauon mass

New Yukawa interactions

Scalar four point interactions

19

Page 20: Radiative Generation of the Lepton Mass

Charged Lepton (e, μ) Masses

Masses for Eα Tauon mass

20

α ≧ 2 is necessary.

Page 21: Radiative Generation of the Lepton Mass

Assumptions

21

We consider the case with α =3 and set the following assumptions.

with

Page 22: Radiative Generation of the Lepton Mass

Assumptions

22

We consider the case with α =3 and set the following assumptions.

Electron masswith

Page 23: Radiative Generation of the Lepton Mass

Assumptions

23

We consider the case with α =3 and set the following assumptions.

Muon masswith

Page 24: Radiative Generation of the Lepton Mass

Contours for M

24

~

10 GeV

Page 25: Radiative Generation of the Lepton Mass

Contours for M

25

~

~10

10 GeV

~0.05

Page 26: Radiative Generation of the Lepton Mass

Neutrino Masses

Masses for Eα Tauon mass

26

×L#

L# violating coupling

Page 27: Radiative Generation of the Lepton Mass

Neutrino Masses

Masses for Eα Tauon mass

27

×L#

L# violating coupling

O(10-4) O(10-4)

O(0.1) eV

~0.01 GeV

Page 28: Radiative Generation of the Lepton Mass

l → l γ Processes

28

Diagonal elements: a=b Muon g-2 (a=b=μ) Electron g-2 (a=b=e)

Off-diagonal elements : a≠b Lepton flavor violating process; i.e., μ → eγ

Same assumptions are taken as in the lepton masses

Δaab =

Δaab ∝ (Ml)ab = (Ml)aa

New physics contribution

Page 29: Radiative Generation of the Lepton Mass

l → l γ Processes

29

Δaab =

Same assumptions are taken as in the lepton masses

Diagonal elements: a=b Muon g-2 (a=b=μ) Electron g-2 (a=b=e)

Off-diagonal elements : a≠b Lepton flavor violating process; i.e., μ → eγ

Δaab ∝ (Ml)ab = (Ml)aa

New physics contribution

Page 30: Radiative Generation of the Lepton Mass

Muon g-2  

30

Bennett et al [Muon g-2 collaboration] Phys. Rev. D 73, (2006).

4.3 σ deviation

The current measured value at BNL is given by

The deviation in aμ from the SM prediction has been calculated by

Benayoun, David, Delbuono, Jegerlehner, Eur. Phys. J. C 72, (2012)..

Page 31: Radiative Generation of the Lepton Mass

Muon g-2

31

φ0 are the neutral Z2-odd scalar bosons.

Δaμ = Δaμμ ~

We have new contributions to g-2 from the Z2-odd particle loops.

∝ (Ml)μμ = mμ

O(10-8)

Page 32: Radiative Generation of the Lepton Mass

Muon g-2

32

Page 33: Radiative Generation of the Lepton Mass

Higgs Phenomenology

33

There are two pairs of doubly-charged Higgs bosons;

C.-W. Chiang, T. Nomura, K. Tsumura (2012); S. Kanemura, K.Y., H. Yokoya (2013).

Collider signatures from the doubly-charged Higgs bosons

W+

W+

Page 34: Radiative Generation of the Lepton Mass

Higgs Phenomenology

34

There are two pairs of doubly-charged Higgs bosons;

C.-W. Chiang, T. Nomura, K. Tsumura (2012); S. Kanemura, K.Y., H. Yokoya (2013).

Collider signatures from the doubly-charged Higgs bosons

W+

W+

Charged lepton mass matrix

Page 35: Radiative Generation of the Lepton Mass

We have proposed the new mechanism to naturally explain smallness of both masses for neutrinos and charged leptons and the hierarchy between them.

Smallness can be explained by the loop suppression and triplet VEVs. The mass hierarchy can be explained by the number of triplet VEV.

Discrepancy in the muon g-2 can be explained due to the O(1) muon Yukawa couplings which is required to reproduce mμ.

The lightest Z2-odd scalar boson can be a dark matter candidate.

Collider phenomenology can be rich. We have two pairs of the doubly-charged scalar bosons from Δ1 and Φ3/2.

Summary

35

Page 36: Radiative Generation of the Lepton Mass

36

Higgs coupling measurementsILC, TDRILC, Higgs White Paper, arXiv: 1310.0763

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