Flavour structure from the seesaw Michael A. Schmidt University of - - PowerPoint PPT Presentation

flavour structure from the seesaw
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Flavour structure from the seesaw Michael A. Schmidt University of - - PowerPoint PPT Presentation

Flavour structure from the seesaw Michael A. Schmidt University of Melbourne 28th Jun 2012 Alexei Smirnov Fest Whats nu? Invisibles 12 M. Lindner, MS, A. Y. .Smirnov, JHEP 0507 (2005) 048 C. Hagedorn, MS, A. Y. .Smirnov, Phys. Rev. D 79


slide-1
SLIDE 1

Flavour structure from the seesaw

Michael A. Schmidt

University of Melbourne

28th Jun 2012 Alexei Smirnov Fest What’s nu? – Invisibles 12

  • M. Lindner, MS, A. Y. .Smirnov, JHEP 0507 (2005) 048
  • C. Hagedorn, MS, A. Y. .Smirnov, Phys. Rev. D 79, 036002 (2009)

MS, A. Y. .Smirnov, Nucl.Phys. B857 (2012) 1-27

1

slide-2
SLIDE 2

Outline

1

Introduction

2

Implementations of Double Seesaw Structure

3

Stability with respect to Quantum Corrections

4

Conclusions

2

slide-3
SLIDE 3

Outline

1

Introduction

2

Implementations of Double Seesaw Structure

3

Stability with respect to Quantum Corrections

4

Conclusions

3

slide-4
SLIDE 4

Fermion Masses

✗1 ✗3 ✗2 ∆m2

31

∆m2

21

normal ordering ✗1 ✗2 ✗3 ∆m2

31

∆m2

21

inverted ordering

Huge hierarchy of charged fermions: mt : mc : mu ✘ 1 : 7 ✁ 103 : 105 mb : ms : md ✘ 1 : 2 ✁ 102 : 103 m✜ : m✖ : me ✘ 1 : 6 ✁ 102 : 3 ✁ 104 Neutral fermions have smaller masses and a weaker hierarchy ★ ★ ✒

✿ ✍ ✿

✒ ✒ ✒

✍ ✍

✿ ✍

✍ ✍

✿ ✍

4

slide-5
SLIDE 5

Fermion Masses

✗1 ✗3 ✗2 ∆m2

31

∆m2

21

normal ordering ✗1 ✗2 ✗3 ∆m2

31

∆m2

21

inverted ordering

Huge hierarchy of charged fermions: mt : mc : mu ✘ 1 : 7 ✁ 103 : 105 mb : ms : md ✘ 1 : 2 ✁ 102 : 103 m✜ : m✖ : me ✘ 1 : 6 ✁ 102 : 3 ✁ 104 Neutral fermions have smaller masses and a weaker hierarchy Small mixing angles in CKM matrix: ★12 ★23 ✒13 13✍ 2✿4✍ 0✿23✍ Large mixing angles in PMNS matrix: ✒12 ✒23 ✒13 34✍ 44✍ 9✿3✍

[Forero et. al (2012)]

34✍ 39✍ 9✿0✍

[Fogli et. al (2012)] 4

slide-6
SLIDE 6

Fermion Masses

✗1 ✗3 ✗2 ∆m2

31

∆m2

21

normal ordering ✗1 ✗2 ✗3 ∆m2

31

∆m2

21

inverted ordering

Huge hierarchy of charged fermions: mt : mc : mu ✘ 1 : 7 ✁ 103 : 105 mb : ms : md ✘ 1 : 2 ✁ 102 : 103 m✜ : m✖ : me ✘ 1 : 6 ✁ 102 : 3 ✁ 104 Neutral fermions have smaller masses and a weaker hierarchy Small mixing angles in CKM matrix: ★12 ★23 ✒13 13✍ 2✿4✍ 0✿23✍ Large mixing angles in PMNS matrix: ✒12 ✒23 ✒13 34✍ 44✍ 9✿3✍

[Forero et. al (2012)]

34✍ 39✍ 9✿0✍

[Fogli et. al (2012)]

Explanation of different structures? Compatibility with GUTs?

4

slide-7
SLIDE 7

Seesaw Mechanism

Standard Seesaw [Minkowski;Yanagida;Glashow;Gell-Mann,Ramond,Slansky;Mohapatra,Senjanovic]

Introduction of right-handed (RH) neutrinos N ▼ = ✒ mT

D

✁ MNN ✓ ✮

✗ ✙

  • ✘ ❖

❀ ✘ ❖

❁ ✮

❖ ✿

☛ ☞

❤ ✐ ❤ ✐

✮ ✘ ✮ ✮

5

slide-8
SLIDE 8

Seesaw Mechanism

Standard Seesaw [Minkowski;Yanagida;Glashow;Gell-Mann,Ramond,Slansky;Mohapatra,Senjanovic]

Introduction of right-handed (RH) neutrinos N ▼ = ✒ mT

D

✁ MNN ✓ ✮ m✗ ✙ mT

DM1 NNmD

mD ✘ ❖ (Λew) ❀ MNN ✘ ❖

  • 1014 GeV

✁ ❁ ΛGUT ✮ effective light neutrino mass: m✗ ❖ (0✿1 eV)

L☛ L☞ ❤H✐ ❤H✐ N

✮ ✘ ✮ ✮

5

slide-9
SLIDE 9

Seesaw Mechanism

Standard Seesaw [Minkowski;Yanagida;Glashow;Gell-Mann,Ramond,Slansky;Mohapatra,Senjanovic]

Introduction of right-handed (RH) neutrinos N ▼ = ✒ mT

D

✁ MNN ✓ ✮ m✗ ✙ mT

DM1 NNmD

mD ✘ ❖ (Λew) ❀ MNN ✘ ❖

  • 1014 GeV

✁ ❁ ΛGUT ✮ effective light neutrino mass: m✗ ❖ (0✿1 eV)

L☛ L☞ ❤H✐ ❤H✐ N

Different flavour structure possible ✮ ✘ ✮ ✮

5

slide-10
SLIDE 10

Seesaw Mechanism

Standard Seesaw [Minkowski;Yanagida;Glashow;Gell-Mann,Ramond,Slansky;Mohapatra,Senjanovic]

Introduction of right-handed (RH) neutrinos N ▼ = ✒ mT

D

✁ MNN ✓ ✮ m✗ ✙ mT

DM1 NNmD

mD ✘ ❖ (Λew) ❀ MNN ✘ ❖

  • 1014 GeV

✁ ❁ ΛGUT ✮ effective light neutrino mass: m✗ ❖ (0✿1 eV)

L☛ L☞ ❤H✐ ❤H✐ N

Different flavour structure possible If SO(10): RH neutrinos as well as all SM fermions in 16 ✮ mD ✘ mu ✮ Large (quadratic) hierarchy in neutrino masses ✮

5

slide-11
SLIDE 11

Seesaw Mechanism

Standard Seesaw [Minkowski;Yanagida;Glashow;Gell-Mann,Ramond,Slansky;Mohapatra,Senjanovic]

Introduction of right-handed (RH) neutrinos N ▼ = ✒ mT

D

✁ MNN ✓ ✮ m✗ ✙ mT

DM1 NNmD

mD ✘ ❖ (Λew) ❀ MNN ✘ ❖

  • 1014 GeV

✁ ❁ ΛGUT ✮ effective light neutrino mass: m✗ ❖ (0✿1 eV)

L☛ L☞ ❤H✐ ❤H✐ N

Different flavour structure possible If SO(10): RH neutrinos as well as all SM fermions in 16 ✮ mD ✘ mu ✮ Large (quadratic) hierarchy in neutrino masses ✮ Cancellation of hierarchies needed in neutrino mass matrix

5

slide-12
SLIDE 12

Seesaw Mechanism

Standard Seesaw [Minkowski;Yanagida;Glashow;Gell-Mann,Ramond,Slansky;Mohapatra,Senjanovic]

Introduction of right-handed (RH) neutrinos N ▼ = ✒ mT

D

✁ MNN ✓ ✮ m✗ ✙ mT

DM1 NNmD

mD ✘ ❖ (Λew) ❀ MNN ✘ ❖

  • 1014 GeV

✁ ❁ ΛGUT ✮ effective light neutrino mass: m✗ ❖ (0✿1 eV)

L☛ L☞ ❤H✐ ❤H✐ N

Different flavour structure possible If SO(10): RH neutrinos as well as all SM fermions in 16 ✮ mD ✘ mu ✮ Large (quadratic) hierarchy in neutrino masses ✮ Cancellation of hierarchies needed in neutrino mass matrix New scale below ΛGUT needed

5

slide-13
SLIDE 13

Solutions to Large Hierarchy from Seesaw

Forget about SO(10), use e.g. SU(5)

☛ ☞

❤ ✐ ❤ ✐

☛ ☞

❤ ✐ ❤ ✐

6

slide-14
SLIDE 14

Solutions to Large Hierarchy from Seesaw

Forget about SO(10), use e.g. SU(5) Use an alternative seesaw mechanism Alternative Seesaw Type II (scalar triplet) seesaw Type III (fermionic triplet) seesaw L☛ L☞ ❤H✐ ❤H✐ ∆ L☛ L☞ ❤H✐ ❤H✐ Σ

6

slide-15
SLIDE 15

Solutions to Large Hierarchy from Seesaw

Forget about SO(10), use e.g. SU(5) Use an alternative seesaw mechanism Cancel hierarchy through structure in RH Majorana mass matrix MNN . . . Alternative Seesaw Type II (scalar triplet) seesaw Type III (fermionic triplet) seesaw L☛ L☞ ❤H✐ ❤H✐ ∆ L☛ L☞ ❤H✐ ❤H✐ Σ

6

slide-16
SLIDE 16

Double Seesaw

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆

  • Mainly two different limits studied:

✢ ✢ ✮ ✘ ❖ ❀ ✘ ❖ ❀ ✘ ❖ ✿ ✢ ✢ ✮ ✘ ❖ ❀ ✘ ❖ ❀ ✘ ❖ ✘ ❂ ✘ ❂ ✘

7

slide-17
SLIDE 17

Double Seesaw

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆ ✮ m✗ = mT

DM1 SNMSSM1 T SN

mD Mainly two different limits studied: Inverse seesaw: MSN ✢ mD ✢ MSS ✮ e.g. mD ✘ ❖ (100 GeV) ❀ MSN ✘ ❖ (TeV) ❀ MSS ✘ ❖ (0✿01 keV) ✢ ✢ ✮ ✘ ❖ ❀ ✘ ❖ ❀ ✘ ❖ ✘ ❂ ✘ ❂ ✘

7

slide-18
SLIDE 18

Double Seesaw

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆ ✮ m✗ = mT

DM1 SNMSSM1 T SN

mD Mainly two different limits studied: Inverse seesaw: MSN ✢ mD ✢ MSS ✮ e.g. mD ✘ ❖ (100 GeV) ❀ MSN ✘ ❖ (TeV) ❀ MSS ✘ ❖ (0✿01 keV) Double seesaw: MSS ✢ MSN ✢ mD ✮ mD ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl) ✘ ❂ ✘ ❂ ✘

7

slide-19
SLIDE 19

Double Seesaw

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆ ✮ m✗ = mT

DM1 SNMSSM1 T SN

mD Mainly two different limits studied: Inverse seesaw: MSN ✢ mD ✢ MSS ✮ e.g. mD ✘ ❖ (100 GeV) ❀ MSN ✘ ❖ (TeV) ❀ MSS ✘ ❖ (0✿01 keV) Double seesaw: MSS ✢ MSN ✢ mD ✮ mD ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl) Naturally leads to correct scale of RH neutrinos MNN ✘ M2

SN❂MSS ✘ Λ2 GUT❂MPl ✘ 1013 GeV

7

slide-20
SLIDE 20

Double Seesaw

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❇ ❅

mT

D

mT

S✗

✿ MNN MT

SN

✿ ✿ MSS

✶ ❈ ❈ ❆ ✮ m✗ = mT

DM1 SNMSSM1 T SN

mD Mainly two different limits studied: Inverse seesaw: MSN ✢ mD ✢ MSS ✮ e.g. mD ✘ ❖ (100 GeV) ❀ MSN ✘ ❖ (TeV) ❀ MSS ✘ ❖ (0✿01 keV) Double seesaw: MSS ✢ MSN ✢ mD ✮ mD ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl) Naturally leads to correct scale of RH neutrinos MNN ✘ M2

SN❂MSS ✘ Λ2 GUT❂MPl ✘ 1013 GeV

7

slide-21
SLIDE 21

Double Seesaw

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❇ ❅

mT

D

mT

S✗

✿ MNN MT

SN

✿ ✿ MSS

✶ ❈ ❈ ❆ ✮ m✗ = mT

DM1 SNMSSM1 T SN

mD Mainly two different limits studied: Inverse seesaw: MSN ✢ mD ✢ MSS ✮ e.g. mD ✘ ❖ (100 GeV) ❀ MSN ✘ ❖ (TeV) ❀ MSS ✘ ❖ (0✿01 keV) Double seesaw: MSS ✢ MSN ✢ mD ✮ mD ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl) Naturally leads to correct scale of RH neutrinos MNN ✘ M2

SN❂MSS ✘ Λ2 GUT❂MPl ✘ 1013 GeV

If MSS singular, there are massless neutrinos.

7

slide-22
SLIDE 22

Cancellation of Hierarchy

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

mT

S✗

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆ ✮ m✗ = mDS

+ mLS

mD❀ mS✗ ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl)

Double seesaw (DS) contribution: mDS

✙ mT

DM1 SNMSSM1 T SN

mD

✿ ✿ ✿

✴ ✮

8

slide-23
SLIDE 23

Cancellation of Hierarchy

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

mT

S✗

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆ ✮ m✗ = mDS

+ mLS

mD❀ mS✗ ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl)

Double seesaw (DS) contribution: mDS

✙ mT

DM1 SNMSSM1 T SN

mD Linear seesaw (LS) contribution: mLS

mT

DM1 SNmS✗ + (✿ ✿ ✿ )T ✐

generally smaller ✑

✴ ✮

8

slide-24
SLIDE 24

Cancellation of Hierarchy

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

mT

S✗

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆ ✮ m✗ = mDS

+ mLS

mD❀ mS✗ ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl)

Double seesaw (DS) contribution: mDS

✙ F TMSSF Linear seesaw (LS) contribution: mLS

F TmS✗ + (✿ ✿ ✿ )T ✐ generally smaller Cancellation [Smirnov (1993,2004)] F ✑ M1 T

SN

mD non hierarchical ✮ weak hierarchy in m✗ ✴ ✮

8

slide-25
SLIDE 25

Cancellation of Hierarchy

Double Seesaw [Mohapatra,Valle;Barr] Introduce additional singlets S ▼ =

✵ ❇ ❅

mT

D

mT

S✗

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆ ✮ m✗ = mDS

+ mLS

mD❀ mS✗ ✘ ❖ (Λew) ❀ MSN ✘ ❖ (ΛGUT) ❀ MSS ✘ ❖ (MPl)

Double seesaw (DS) contribution: mDS

✙ F TMSSF Linear seesaw (LS) contribution: mLS

F TmS✗ + (✿ ✿ ✿ )T ✐ generally smaller Cancellation [Smirnov (1993,2004)] F ✑ M1 T

SN

mD non hierarchical ✮ weak hierarchy in m✗ F ✴ 1 (Dirac screening ✮ Dirac flavour structure is cancelled)

8

slide-26
SLIDE 26

Outline

1

Introduction

2

Implementations of Double Seesaw Structure

3

Stability with respect to Quantum Corrections

4

Conclusions

9

slide-27
SLIDE 27

How can this structure be obtained? – no SO(10)

Abelian Symmetry – L number With the charges L(✗L) = L(N) = 1, L(S) = 0 ✣

  • MSSSS

✗ ✣

✛ in basis (✗❀ N❀ S)T L(▼) =

✵ ❇ ❅

2 2 1 ✿ 2 1 ✿ ✿

✶ ❈ ❆

✮ ▼

✵ ❇ ❅

✗ ❤✣✐

✿ ❤✛✐ ✿ ✿

✶ ❈ ❆

✂ ✂

✵ ❇ ❅

❀ ❀ ❀ ✿ ❀ ❀ ✿ ✿ ❀

✶ ❈ ❆

10

slide-28
SLIDE 28

How can this structure be obtained? – no SO(10)

Abelian Symmetry – L number With the charges L(✗L) = L(N) = 1, L(S) = 0, L(✣) = 2 and L(✛) = 1 MSSSS + Y✗L✣N + YSNSN✛ in basis (✗❀ N❀ S)T L(▼) =

✵ ❇ ❅

2 2 1 ✿ 2 1 ✿ ✿

✶ ❈ ❆ ✮ ▼ = ✵ ❇ ❅

Y✗ ❤✣✐ ✿ YSN ❤✛✐ ✿ ✿ MSS

✶ ❈ ❆

✂ ✂

✵ ❇ ❅

❀ ❀ ❀ ✿ ❀ ❀ ✿ ✿ ❀

✶ ❈ ❆

10

slide-29
SLIDE 29

How can this structure be obtained? – no SO(10)

Abelian Symmetry – L number With the charges L(✗L) = L(N) = 1, L(S) = 0, L(✣) = 2 and L(✛) = 1 MSSSS + Y✗L✣N + YSNSN✛ in basis (✗❀ N❀ S)T L(▼) =

✵ ❇ ❅

2 2 1 ✿ 2 1 ✿ ✿

✶ ❈ ❆ ✮ ▼ = ✵ ❇ ❅

Y✗ ❤✣✐ ✿ YSN ❤✛✐ ✿ ✿ MSS

✶ ❈ ❆

Minimal LR symmetry SU(2)L ✂ SU(2)R ✂ U(1)BL G(▼) =

✵ ❇ ❅

[3❀ 1] [2❀ 2] [2❀ 1] ✿ [1❀ 3] [1❀ 2] ✿ ✿ [1❀ 1]

✶ ❈ ❆

10

slide-30
SLIDE 30

Setup within SO(10)

Lagrangian ☛ij 16i 16j H + ☞ij Si 16j ∆ + (MSS)ij SiSj 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 ▼ =

✵ ❇ ❅

mT

D

mT

S✗

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆

mD = ☛ ❤H✐ ❀ MSN = ☞ ❤∆✐N ❀ mS✗ = ☞ ❤∆✐✗ ✮ ☛ ☞ ✦

11

slide-31
SLIDE 31

Setup within SO(10)

Lagrangian ☛ij 16i 16j H + ☞ij Si 16j ∆ + (MSS)ij SiSj 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 ▼ =

✵ ❇ ❅

mT

D

mT

S✗

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆

mD = ☛ ❤H✐ ❀ MSN = ☞ ❤∆✐N ❀ mS✗ = ☞ ❤∆✐✗ ✮ correlation between ☛ and ☞ needed. ✦

11

slide-32
SLIDE 32

Setup within SO(10)

Lagrangian ☛ij 16i 16j H + ☞ij Si 16j ∆ + (MSS)ij SiSj 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 ▼ =

✵ ❇ ❅

mT

D

mT

S✗

✿ MT

SN

✿ ✿ MSS

✶ ❈ ❆

mD = ☛ ❤H✐ ❀ MSN = ☞ ❤∆✐N ❀ mS✗ = ☞ ❤∆✐✗ ✮ correlation between ☛ and ☞ needed. Cancellation Mechanism e.g. Frogatt Nielsen mechanism ✦ Hierarchy cancelled, anarchical spectrum

[Hall, Murayama, Weiner (1999); de Gouvêa, Murayama (2012)] 11

slide-33
SLIDE 33

Realisation with Extended Gauge Symmetry I

SO(10) ✚ E6 27 ✦ 16 ✟ 10 ✟ 1 ✮ Singlets are in the same representation ✏

❢ ❣ ❢ ❣

✑ ✂ ✂ ✵ ❇ ❅

✗ ✶ ❈ ❆ ✘

  • ❀ ❀

✘ ❀ ❀ ✁ ✘ ❀ ❀ ✁

❀ ✁ ✚ ✚

❀ ✁

❀ ✁ ✚ ✚

❀ ✁

❀ ✁ ❀ ❀ ✚

12

slide-34
SLIDE 34

Realisation with Extended Gauge Symmetry I

SO(10) ✚ E6 27 ✦ 16 ✟ 10 ✟ 1 ✮ Singlets are in the same representation 27i 27j ✏ Y ❢ij❣

27

27 + Y ❢ij❣

351S 351S + Y [ij] 351A 351A

✑ ✂ ✂ ✵ ❇ ❅

✗ ✶ ❈ ❆ ✘

  • ❀ ❀

✘ ❀ ❀ ✁ ✘ ❀ ❀ ✁

❀ ✁ ✚ ✚

❀ ✁

❀ ✁ ✚ ✚

❀ ✁

❀ ✁ ❀ ❀ ✚

12

slide-35
SLIDE 35

Realisation with Extended Gauge Symmetry I

SO(10) ✚ E6 27 ✦ 16 ✟ 10 ✟ 1 ✮ Singlets are in the same representation 27i 27j ✏ Y ❢ij❣

27

27 + Y ❢ij❣

351S 351S + Y [ij] 351A 351A

✑ In terms of SU(3)L ✂ SU(3)R ✂ SU(3)C Leptons L = ✵ ❇ ❅ L

˙ 1 1

E e E + L

˙ 2 2

✗ e+ ✗ L

˙ 3 3

✶ ❈ ❆ ✘

  • 3❀ 3❀ 1

[QL ✘ 3❀ 1❀ 3✁ , QR ✘ 1❀ 3❀ 3✁ ]

❀ ✁ ✚ ✚

❀ ✁

❀ ✁ ✚ ✚

❀ ✁

❀ ✁ ❀ ❀ ✚

12

slide-36
SLIDE 36

Realisation with Extended Gauge Symmetry I

SO(10) ✚ E6 27 ✦ 16 ✟ 10 ✟ 1 ✮ Singlets are in the same representation 27i 27j ✏ Y ❢ij❣

27

27 + Y ❢ij❣

351S 351S + Y [ij] 351A 351A

✑ In terms of SU(3)L ✂ SU(3)R ✂ SU(3)C Leptons L = ✵ ❇ ❅ L

˙ 1 1

E e E + L

˙ 2 2

✗ e+ ✗ L

˙ 3 3

✶ ❈ ❆ ✘

  • 3❀ 3❀ 1

[QL ✘ 3❀ 1❀ 3✁ , QR ✘ 1❀ 3❀ 3✁ ]

Relevant Higgs multiplets H ✚

  • 3❀ 3❀ 1

✁ ✚ 27 HS ✚

  • 3❀ 3❀ 1

✁ +

  • 6❀ 6❀ 1

✁ ✚ 351S HA ✚

  • 3❀ 3❀ 1

✁ +

  • 3❀ 6❀ 1

✁ + (6❀ 3❀ 1) ✚ 351A

12

slide-37
SLIDE 37

Realisation with Extended Gauge Symmetry II

Dirac Screening structure obtained from ❉ (HA)

˙ 1 1

❊ ✬ ❖ (SU(2)L breaking scale) ❉ (HA)❢33❣

1

❊ ✬ ❖ (SU(2)R breaking scale) ❉ (HS)❢33❣

❢˙ 3˙ 3❣

❊ ✬ ❉ (HA)

˙ 3 3

❊ ✬ ❖ (SU(3)L ✂ SU(3)R breaking scale) in basis ✏ ✗ ✘ L

˙ 2 3❀ N ✘ L ˙ 3 2❀ S ✘ L ˙ 3 3❀ S✵ ✘ L ˙ 1 1❀ S✵✵ ✘ L ˙ 2 2

✑ ✵ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❅ Y351A ❉ (HA)

˙ 1 1

❊ ✿ Y351A ❉ (HA)❢33❣

1

❊ ✿ ✿ Y351S ❉ (HS)❢33❣

❢˙ 3˙ 3❣

❊ Y351A ❉ (HA)

˙ 1 1

❊ ✿ ✿ ✿ Y351A ❉ (HA)

˙ 3 3

❊ ✿ ✿ ✿ ✿ ✶ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❆ ✮

13

slide-38
SLIDE 38

Realisation with Extended Gauge Symmetry II

Dirac Screening structure obtained from ❉ (HA)

˙ 1 1

❊ ✬ ❖ (SU(2)L breaking scale) ❉ (HA)❢33❣

1

❊ ✬ ❖ (SU(2)R breaking scale) ❉ (HS)❢33❣

❢˙ 3˙ 3❣

❊ ✬ ❉ (HA)

˙ 3 3

❊ ✬ ❖ (SU(3)L ✂ SU(3)R breaking scale) in basis ✏ ✗ ✘ L

˙ 2 3❀ N ✘ L ˙ 3 2❀ S ✘ L ˙ 3 3❀ S✵ ✘ L ˙ 1 1❀ S✵✵ ✘ L ˙ 2 2

✑ ✵ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❅ Y351A ❉ (HA)

˙ 1 1

❊ ✿ Y351A ❉ (HA)❢33❣

1

❊ ✿ ✿ Y351S ❉ (HS)❢33❣

❢˙ 3˙ 3❣

❊ Y351A ❉ (HA)

˙ 1 1

❊ ✿ ✿ ✿ Y351A ❉ (HA)

˙ 3 3

❊ ✿ ✿ ✿ ✿ ✶ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❆ ✮

13

slide-39
SLIDE 39

Realisation with Extended Gauge Symmetry II

Dirac Screening structure obtained from ❉ (HA)

˙ 1 1

❊ ✬ ❖ (SU(2)L breaking scale) ❉ (HA)❢33❣

1

❊ ✬ ❖ (SU(2)R breaking scale) ❉ (HS)❢33❣

❢˙ 3˙ 3❣

❊ ✬ ❉ (HA)

˙ 3 3

❊ ✬ ❖ (SU(3)L ✂ SU(3)R breaking scale) in basis ✏ ✗ ✘ L

˙ 2 3❀ N ✘ L ˙ 3 2❀ S ✘ L ˙ 3 3❀ S✵ ✘ L ˙ 1 1❀ S✵✵ ✘ L ˙ 2 2

✑ ✵ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❇ ❅ Y351A ❉ (HA)

˙ 1 1

❊ ✿ Y351A ❉ (HA)❢33❣

1

❊ ✿ ✿ Y351S ❉ (HS)❢33❣

❢˙ 3˙ 3❣

❊ Y351A ❉ (HA)

˙ 1 1

❊ ✿ ✿ ✿ Y351A ❉ (HA)

˙ 3 3

❊ ✿ ✿ ✿ ✿ ✶ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❈ ❆ ✮ Construction of viable Higgs Potential important

13

slide-40
SLIDE 40

Realisation with Flavour Symmetry within SO(10)

Explain number of generations: 16i ✘ 3 ✂ ✮ ✤

✛ ☛ ✤ ☞ ✤ ❀

Particle Content 16i Si H ∆ ✤i SO(10) 16 1 10 16 1

14

slide-41
SLIDE 41

Realisation with Flavour Symmetry within SO(10)

Explain number of generations: 16i ✘ 3 Complex representation 3, otherwise 3 ✂ 3 contains singlet ✮ A4 not possible, but: T7[Luhn,Nasri,Ramond], Σ(81)[Ma], . . . ✤

✛ ☛ ✤ ☞ ✤ ❀

Particle Content 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 T7 3 1i 11 11 3❄

14

slide-42
SLIDE 42

Realisation with Flavour Symmetry within SO(10)

Explain number of generations: 16i ✘ 3 Complex representation 3, otherwise 3 ✂ 3 contains singlet ✮ A4 not possible, but: T7[Luhn,Nasri,Ramond], Σ(81)[Ma], . . . Explain difference in CKM and MNS matrix (in lowest order) ✤

✛ ☛ ✤ ☞ ✤ ❀

Particle Content 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 T7 3 1i 11 11 3❄

14

slide-43
SLIDE 43

Realisation with Flavour Symmetry within SO(10)

Explain number of generations: 16i ✘ 3 Complex representation 3, otherwise 3 ✂ 3 contains singlet ✮ A4 not possible, but: T7[Luhn,Nasri,Ramond], Σ(81)[Ma], . . . Explain difference in CKM and MNS matrix (in lowest order) Flavons (gauge group singlets charged with respect to GF) ✤

W ✛ ☛ij Λ 16i 16j H✤ + ☞ij Λ Si 16j ∆✤ + (MSS)ij SiSj ❀

Particle Content 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 T7 3 1i 11 11 3❄

14

slide-44
SLIDE 44

T7: Realisation

Field 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 T7 3 1i 11 11 3❄ Superpotential W ✛ ☛ H (163 163 ✤1 + 161 161 ✤2 + 162 162 ✤3)❂Λ + ☞1 ∆ S1 (161 ✤1 + 162 ✤2 + 163 ✤3)❂Λ + ☞2 ∆ S2 (161 ✤1 + ✦ 162 ✤2 + ✦2 163 ✤3)❂Λ + ☞3 ∆ S3 (161 ✤1 + ✦2 162 ✤2 + ✦ 163 ✤3)❂Λ + A S1 S1 + B (S2 S3 + S3 S2) + h✿c✿ with ✦ = e2✙ i ❂3

15

slide-45
SLIDE 45

T7: Lowest Order

mD = ☛ ❤H✐ Λ ✵ ❅ ❤✤2✐ ❤✤3✐ ❤✤1✐ ✶ ❆ ❤ ✐ ✵ ❅ ☞ ☞ ☞ ✶ ❆ ✵ ❅ ✦ ✦ ✦ ✦ ✶ ❆ ✵ ❅ ❤✤ ✐ ❤✤ ✐ ❤✤ ✐ ✶ ❆ ✵ ❅ ✁ ✁ ✁ ✶ ❆

✗ ✙

✒☛ ❤ ✐ ❤ ✐ ✓ ✵ ❅

✁ ✶ ❆

✑ ☞ ❀ ✑ ☞ ☞ ❀

✤ ✑

✏ ❤✤ ✐

❤✤ ✐ ❀ ❤✤ ✐ ❤✤ ✐ ❀ ❤✤ ✐ ❤✤ ✐

16

slide-46
SLIDE 46

T7: Lowest Order

mD = ☛ ❤H✐ Λ ✵ ❅ ❤✤2✐ ❤✤3✐ ❤✤1✐ ✶ ❆ MSN = ❤∆✐N Λ ✵ ❅ ☞1 ☞2 ☞3 ✶ ❆ ✵ ❅ 1 1 1 1 ✦ ✦2 1 ✦2 ✦ ✶ ❆ ✵ ❅ ❤✤1✐ ❤✤2✐ ❤✤3✐ ✶ ❆ ✵ ❅ ✁ ✁ ✁ ✶ ❆

✗ ✙

✒☛ ❤ ✐ ❤ ✐ ✓ ✵ ❅

✁ ✶ ❆

✑ ☞ ❀ ✑ ☞ ☞ ❀

✤ ✑

✏ ❤✤ ✐

❤✤ ✐ ❀ ❤✤ ✐ ❤✤ ✐ ❀ ❤✤ ✐ ❤✤ ✐

16

slide-47
SLIDE 47

T7: Lowest Order

mD = ☛ ❤H✐ Λ ✵ ❅ ❤✤2✐ ❤✤3✐ ❤✤1✐ ✶ ❆ MSN = ❤∆✐N Λ ✵ ❅ ☞1 ☞2 ☞3 ✶ ❆ ✵ ❅ 1 1 1 1 ✦ ✦2 1 ✦2 ✦ ✶ ❆ ✵ ❅ ❤✤1✐ ❤✤2✐ ❤✤3✐ ✶ ❆ MSS = ✵ ❅ A ✁ B ✁ ✁ ✶ ❆

✗ ✙

✒☛ ❤ ✐ ❤ ✐ ✓ ✵ ❅

✁ ✶ ❆

✑ ☞ ❀ ✑ ☞ ☞ ❀

✤ ✑

✏ ❤✤ ✐

❤✤ ✐ ❀ ❤✤ ✐ ❤✤ ✐ ❀ ❤✤ ✐ ❤✤ ✐

16

slide-48
SLIDE 48

T7: Lowest Order

mD = ☛ ❤H✐ Λ ✵ ❅ ❤✤2✐ ❤✤3✐ ❤✤1✐ ✶ ❆ MSN = ❤∆✐N Λ ✵ ❅ ☞1 ☞2 ☞3 ✶ ❆ ✵ ❅ 1 1 1 1 ✦ ✦2 1 ✦2 ✦ ✶ ❆ ✵ ❅ ❤✤1✐ ❤✤2✐ ❤✤3✐ ✶ ❆ MSS = ✵ ❅ A ✁ B ✁ ✁ ✶ ❆ m✗ ✙ ✒☛ ❤H✐ ❤∆✐N ✓2 D✤ ✵ ❅ ˜ A + 2˜ B ˜ A ˜ B ˜ A ˜ B ✁ ˜ A + 2˜ B ˜ A ˜ B ✁ ✁ ˜ A + 2˜ B ✶ ❆ D✤

˜ A ✑ A 9☞2

1

❀ ˜ B ✑ B 9☞2☞3 ❀ D✤ ✑ diag

✏❤✤2✐

❤✤1✐ ❀ ❤✤3✐ ❤✤2✐ ❀ ❤✤1✐ ❤✤3✐

16

slide-49
SLIDE 49

T7: Lowest Order

mD = ☛ ❤H✐ ❤✤1✐ Λ ✵ ❅ ✎2 ✎ 1 ✶ ❆ MSN = ❤∆✐N ❤✤1✐ Λ ✵ ❅ ☞1 ☞2 ☞3 ✶ ❆ ✵ ❅ 1 1 1 1 ✦ ✦2 1 ✦2 ✦ ✶ ❆ ✵ ❅ 1 ✎2 ✎ ✶ ❆ MSS = ✵ ❅ A ✁ B ✁ ✁ ✶ ❆ m✗ ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 ✵ ❅ (˜ A + 2˜ B)✎6 (˜ A ˜ B)✎3 (˜ A ˜ B)✎3 ✁ ˜ A + 2˜ B ˜ A ˜ B ✁ ✁ ˜ A + 2˜ B ✶ ❆

˜ A ✑ A 9☞2

1

❀ ˜ B ✑ B 9☞2☞3 ❀ D✤ ✑ diag

✏❤✤2✐

❤✤1✐ ❀ ❤✤3✐ ❤✤2✐ ❀ ❤✤1✐ ❤✤3✐

= diag ✎❀ ✎2❀ ✎2✁

16

slide-50
SLIDE 50

T7: Solar Mixing Angle

mLS

mT

D M1 SN mS✗ + (✿ ✿ ✿ )T ✐

mS✗ originates from Si 16j ∆ ✤ ✮ mLS

diagonal ✮

✵✐✗

✵ ❅ ☞✵ ☞✵ ☞✵ ✶ ❆ ✵ ❅ ✦ ✦ ✦ ✦ ✶ ❆ ✵ ❅ ❤✤ ✐ ❤✤ ✐ ❤✤ ✐ ✶ ❆

✗ ✙

✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ✵ ❇ ❇ ❇ ❅

☞ ✎

☞ ✦

☞ ✦ ✿

✿ ✶ ❈ ❈ ❈ ❆ ❤ ✐ ❤

✵✐✗ ❤✤ ✐ ✎

☛ ❤ ✐ ✮ ❤ ✐ ✎ ✘ ❀ ❀ ☞ ☞✵❂☞

17

slide-51
SLIDE 51

T7: Solar Mixing Angle

mLS

mT

D M1 SN mS✗ + (✿ ✿ ✿ )T ✐

mS✗ originates from Si 16j ∆ ✤ ✮ mLS

diagonal ✮ introduce ∆✵:

mS✗ = ❤∆✵✐✗ Λ ✵ ❅ ☞✵

1

☞✵

2

☞✵

3

✶ ❆ ✵ ❅ 1 1 1 1 ✦ ✦2 1 ✦2 ✦ ✶ ❆ ✵ ❅ ❤✤1✐ ❤✤2✐ ❤✤3✐ ✶ ❆

✗ ✙

✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ✵ ❇ ❇ ❇ ❅

☞ ✎

☞ ✦

☞ ✦ ✿

✿ ✶ ❈ ❈ ❈ ❆ ❤ ✐ ❤

✵✐✗ ❤✤ ✐ ✎

☛ ❤ ✐ ✮ ❤ ✐ ✎ ✘ ❀ ❀ ☞ ☞✵❂☞

17

slide-52
SLIDE 52

T7: Solar Mixing Angle

mLS

mT

D M1 SN mS✗ + (✿ ✿ ✿ )T ✐

mS✗ originates from Si 16j ∆ ✤ ✮ mLS

diagonal ✮ introduce ∆✵:

mS✗ = ❤∆✵✐✗ Λ ✵ ❅ ☞✵

1

☞✵

2

☞✵

3

✶ ❆ ✵ ❅ 1 1 1 1 ✦ ✦2 1 ✦2 ✦ ✶ ❆ ✵ ❅ ❤✤1✐ ❤✤2✐ ❤✤3✐ ✶ ❆

Leading order

m✗ ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 ✵ ❇ ❇ ❇ ❅ 2 X

3

i=1

˜ ☞i ✎3 X

3

i=1

˜ ☞i ✦1i X

3

i=1

˜ ☞i ✦i1 ✿ ˜ A + 2˜ B ˜ A ˜ B ✿ ✿ ˜ A + 2˜ B ✶ ❈ ❈ ❈ ❆ X = ❤∆✐N ❤∆✵✐✗ ❤✤1✐ ✎ 3 ☛ ❤H✐ Λ ✮ ❤∆✐N ✎ ✘ ˜ A❀ ˜ B ❀ ˜ ☞i = ☞✵

i❂☞i

17

slide-53
SLIDE 53

T7: Phenomenology

Dominant 2-3 block in neutrino mass matrix preserved, ✒12, ✒13 can be fitted: tan ✒12 ✙ X ❥ ˜ ☞2 ˜ ☞3❥ ♣ 6 ❥˜ B❥ ❀ sin ✒13 ✙ X ❥2 ˜ ☞1 ˜ ☞2 ˜ ☞3❥ ♣ 2 ❥2˜ A + ˜ B❥ ❀ ✒23 ✙ ✙ 4 ✙ ✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ☞ ☞ ☞ ❥ ❥ ✒ ❥ ❥ ✒ ☞ ☞ ☞ ✙ ✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ❥ ❥ ☞ ☞ ✒ ☞ ☞ ✙ ✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ❥ ❥ ☞ ☞ ✒ ☞ ☞ ✙ ✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ❥ ❥

✙ ✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ✏ ❥ ❥ ❥ ❥

✁ ✑

18

slide-54
SLIDE 54

T7: Phenomenology

Dominant 2-3 block in neutrino mass matrix preserved, ✒12, ✒13 can be fitted: tan ✒12 ✙ X ❥ ˜ ☞2 ˜ ☞3❥ ♣ 6 ❥˜ B❥ ❀ sin ✒13 ✙ X ❥2 ˜ ☞1 ˜ ☞2 ˜ ☞3❥ ♣ 2 ❥2˜ A + ˜ B❥ ❀ ✒23 ✙ ✙ 4 m1 and m2 especially changed: m1 ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 ☞ ☞ ☞3 ❥˜ B❥ tan2 ✒12 ❥2˜ A + ˜ B❥ sin2 ✒13 ☞ ☞ ☞ m2 ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 3 ❥˜ B❥ ☞ ☞1 tan2 ✒12 ☞ ☞ m3 ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 ❥2˜ A + ˜ B❥ ☞ ☞1 + sin2 ✒13 ☞ ☞ ✙ ✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ❥ ❥

✙ ✒ ☛ ❤ ✐ ❤ ✐ ✎ ✓ ✏ ❥ ❥ ❥ ❥

✁ ✑

18

slide-55
SLIDE 55

T7: Phenomenology

Dominant 2-3 block in neutrino mass matrix preserved, ✒12, ✒13 can be fitted: tan ✒12 ✙ X ❥ ˜ ☞2 ˜ ☞3❥ ♣ 6 ❥˜ B❥ ❀ sin ✒13 ✙ X ❥2 ˜ ☞1 ˜ ☞2 ˜ ☞3❥ ♣ 2 ❥2˜ A + ˜ B❥ ❀ ✒23 ✙ ✙ 4 m1 and m2 especially changed: m1 ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 ☞ ☞ ☞3 ❥˜ B❥ tan2 ✒12 ❥2˜ A + ˜ B❥ sin2 ✒13 ☞ ☞ ☞ m2 ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 3 ❥˜ B❥ ☞ ☞1 tan2 ✒12 ☞ ☞ m3 ✙ ✒ ☛ ❤H✐ ❤∆✐N ✎ ✓2 ❥2˜ A + ˜ B❥ ☞ ☞1 + sin2 ✒13 ☞ ☞ ∆m2

21 ✙

✒ ☛ ❤H✐ ❤∆✐N ✎ ✓4 9 ❥˜ B❥2(1 2 tan2 ✒12) ∆m2

32 ✙

✒ ☛ ❤H✐ ❤∆✐N ✎ ✓4 ✏ ❥2˜ A + ˜ B❥29❥˜ B❥2 1 tan2 ✒12 ✁2✑

18

slide-56
SLIDE 56

Outline

1

Introduction

2

Implementations of Double Seesaw Structure

3

Stability with respect to Quantum Corrections

4

Conclusions

19

slide-57
SLIDE 57

Stability with respect to RG

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

m✗ = mT

DM1 SNMSSM1 T SN

mD stable with respect to RG?

☛ ☞

☞ ☛ ☞

20

slide-58
SLIDE 58

Stability with respect to RG

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

m✗ = mT

DM1 SNMSSM1 T SN

mD stable with respect to RG? Two contributions to m✗ from

Active N: Y T

✗ M1Y✗

Effective D5 operator: ✔

☛ ☞

☞ ☛ ☞

20

slide-59
SLIDE 59

Stability with respect to RG

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

m✗ = mT

DM1 SNMSSM1 T SN

mD stable with respect to RG? Two contributions to m✗ from

Active N: Y T

✗ M1Y✗

Effective D5 operator: ✔

MSSM (T7) ✦ same RG equations (non–renormalization theorem)

☛ ☞

☞ ☛ ☞

20

slide-60
SLIDE 60

Stability with respect to RG

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

m✗ = mT

DM1 SNMSSM1 T SN

mD stable with respect to RG? Two contributions to m✗ from

Active N: Y T

✗ M1Y✗

Effective D5 operator: ✔

MSSM (T7) ✦ same RG equations (non–renormalization theorem) SM: additional vertex corrections

L☛ L☞ N H H

L☛ ✔ L☞ H H L☛ L☞ N H H H H

L☛ ✔ L☞ H H H H

[Antusch, Kersten, Lindner, Ratz (2002)] 20

slide-61
SLIDE 61

Running between Mass Thresholds

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

☞ ☛

RG transformation

(n)

Y✗

RG

(n)

ZN

T (n)

Y✗

(n)

Zext

(n)

MNN

RG

(n)

ZN

T (n)

MNN

(n)

ZN

(n)

RG

(n)

Zext

T (n)

(n)

Zext

(n)

Z✔

✔ ✑

✔❀

  • ✔ ❀

✙ ✒ ✕ ✓ ❤✣✐

✗ ✙ ❤ ✐

✗ ✔

21

slide-62
SLIDE 62

Running between Mass Thresholds

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3) L☛ ✔ L☞ H H L☛ ✔ L☞ H H H H

RG transformation

(n)

Y✗

RG

(n)

ZN

T (n)

Y✗

(n)

Zext

(n)

MNN

RG

(n)

ZN

T (n)

MNN

(n)

ZN

(n)

RG

(n)

Zext

T (n)

(n)

Zext

(n)

Z✔

✔ ✑

✔❀

  • ✔ ❀

✙ ✒ ✕ ✓ ❤✣✐

✗ ✙ ❤ ✐

✗ ✔

21

slide-63
SLIDE 63

Running between Mass Thresholds

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3) L☛ ✔ L☞ H H L☛ ✔ L☞ H H H H

RG transformation

(n)

Y✗

RG

(n)

ZN

T (n)

Y✗

(n)

Zext

(n)

MNN

RG

(n)

ZN

T (n)

MNN

(n)

ZN

(n)

RG

(n)

Zext

T (n)

(n)

Zext

(n)

Z✔

Z✔ ✑ diag ✥

(0)

Z✔❀

(01)

Z✔ ❀

(02)

Z✔ ✦

(0n)

Z✔ = 1 + 1 16✙2 ✒ ✕ + 9 10g 2

1 + 3

2g 2

2

✓ ln ❤✣✐ Mn+1 MNN = MT

SNM1 SS MSN

V T

N MNNVN = DN ✑ (Mi)

Leading Order Correction to Neutrino Mass

Rescaling of RH neutrino masses Mi: m✗ ✙ ❤H✐2 Z T

ext

✂ Y T

✗ VNZ✔D1 N V T N Y✗

✄ Zext

21

slide-64
SLIDE 64

Two Loop Contribution to RH Neutrino Masses

Renormalization of RH neutrinos Ni Nj H H L Nk L ∆Mij = 2 (16✙2)2

k

(Y ②

✗ Y✗)ik

Y ②

✗ Y✗

jk Mk

1 ✎ + 1 2 + ln ✖2 M2

k

✦ The finite Higgs mass has been neglected. There are ❖

  • ✖2

H❂M2 k

✁ corrections.

Assuming y3 ✢ y2 ✢ y1 and not all UR❀i3 vanish: ∆Mi ✘ y4

3

(8✙2)2

k

U✄

R❀k3UR❀i3

✐2 Mk ln ✏

Λ2❂M2

k

[Aparici, Herrero-Garcia, Rius, Santamaria (2011); MS, Smirnov (2011)] 22

slide-65
SLIDE 65

Fourth Generation

100 103 106 109 1012 1015 1010 109 108 107 106 105 104 103 102 101 100 M GeV Ξ U e4, Τ4

2

U Μ4

2

. 1 5 e V 1

  • 2

e V 1

  • 3

e V 1

  • 4

e V 0.15eV 10 2 eV 10 3 eV 10 4 eV 0.15eV 102 eV 103 eV 104 eV

mD = me = 511 keV, ✘ = (UL)☛4(UR)i4

✵ ❇ ❅

fL m ✿✿✿ mE4 f T

R

✿✿✿ ✿✿✿ M4 ✿✿✿ ✿✿✿ ✿✿✿ M

✶ ❈ ❆

mtree

☛☞ ✬ mE4

k

m☛k Mk ✂ ✂(UL)☞4(UR)k4+(☛ ✩ ☞)

να νβ W W eα eβ ν4 [Petcov, Toshev (1984); Babu,Ma (1988)] 23

slide-66
SLIDE 66

Outline

1

Introduction

2

Implementations of Double Seesaw Structure

3

Stability with respect to Quantum Corrections

4

Conclusions

24

slide-67
SLIDE 67

Summary & Conclusions

Double Seesaw structure can accomodate different hierarchies in charged and neutral fermion masses A complete cancellation of the Dirac structure can be obtained Standard (Fermionic singlet) seesaw within SO(10) ✂ Gf possible ✮

25

slide-68
SLIDE 68

Summary & Conclusions

Double Seesaw structure can accomodate different hierarchies in charged and neutral fermion masses A complete cancellation of the Dirac structure can be obtained Standard (Fermionic singlet) seesaw within SO(10) ✂ Gf possible Study of RG stability of double seesaw structure Within MSSM, double seesaw structure is stable Threshold corrections in non-SUSY dominantly lead to a rescaling of RH neutrino masses ✮ Structure of formula in cancellation mechanism modified

25

slide-69
SLIDE 69

Thank you, Alexei! For the collaboration and for everything, what I learned from you!

slide-70
SLIDE 70

Thank you, Alexei! For the collaboration and for everything, what I learned from you! All the best for the next 60 years!

slide-71
SLIDE 71

T7: Group Theory

T7 ✘ = Z7 ⋊ Z3 ✚ SU(3), also called Frobenius group Smallest group with complex 3: order 21 Irreducible representations: 11, 12, 13 ✘ = 1✄

2 and 3, 3❄

1i like in Z3: 11 and 12 ✡ 13 are invariant Generators of 3:

A =

✵ ❅

e2✙ i ❂7 e4✙ i ❂7 e8✙ i ❂7

✶ ❆ ❀

B =

✥ 0

1 1 1

❢3 ✡ 3❣ = 3 ✟ 3✄: (a1❀ a2❀ a3)T ✘ 3: (a3 a3❀ a1 a1❀ a2 a2)T ✘ 3, (a❢2 a3❣❀ a❢3 a1❣❀ a❢1 a2❣)T ✘ 3✄ 3 ✡ 1i = 3: (a1❀ a2❀ a3)T ✘ 3, c ✘ 1i: (a1 c❀ ✦i1 a2 c❀ ✦1i a3 c) with ✦ = ei 2✙❂3

27

slide-72
SLIDE 72

Higher-Dimensional Operators and Mass Scales

Higher-dimensional operators up to mu ☛ ✘ ✎4✑, ✑ = ❤✤1✐ Λ ✘ 0✿48 ✤n

1 A

  • ✦ e 2 ✙ i

7

n ✤n 1 ✘ ❖ (1)

✤n1

1

✤3

A

  • ✦ e 2 ✙ i

7

(n+3) ✤n1 1

✤3 ✘ ❖

✎2✑ ✮ Introduction of Z7 Problem: MSS ✘ ❖

✎4MPl

, but contributions like MSS ✘ SS ❤✤✐n ❂Λn1 Solution: forbid tree-level and generate MSS at higher order Observe: only one covariant SS✤3❂Λ2 ✘ (a S1S1 + b (S2S3 + S3S2)) ✤1✤2✤3❂Λ2 Field 16i Si H ∆ ✤i T7 3 1i 11 11 3✄ Z7 3 2 1 1

28

slide-73
SLIDE 73

T7: Higher-Dimensional Operators

Consider operators up to order mu ☛ ✘ ✎2✑ = ✑17, ✑ = ❤✤1✐ Λ ✘ 0✿48 Additional Z7 to forbid operators

Field 16i Si H ∆ ✤i T7 3 1i 11 11 3✄ Z7 3 3 1 ✦ All higher-dimensional operators suppressed by ✑7 compared to LO. ✦ Vanishing entries are filled.

Structure of covariants periodic in 7 due to subgroup Z7 of T7

Structure Transformation Properties Order in ✎ under Generator A ✤n

1

e 2 ✙ i

7

n ✤n 1

❖ (1) ✤n1

1

✤2 e 2 ✙ i

7

(n+1) ✤n1 1

✤2 ❖

  • ✎2✁

✤n1

1

✤3 e 2 ✙ i

7

(n+3) ✤n1 1

✤3 ❖ (✎) ✤n2

1

✤2

3

e 2 ✙ i

7

(n+6) ✤n2 1

✤2

3

  • ✎2✁

29

slide-74
SLIDE 74

T7: Cabibbo Angle and Charged Lepton Masses

Cabibbo Angle By introduction of 16H❀ 16✵

H ✘ (1T7❀ 6Z7)

1 M

16i 16j 16H 16✵

H

✑ ✒✤

Λ

✓3

contributes to down type and charged lepton mass matrix mdown ✙ ❤16H✐✗

✒❤16✵

H✐N

M

✓ ✵ ❇ ❅

❖(✎4✑3) ❖(✑3) ❖(✎6✑3) ✿ ❖(✎4✑3) ❖(✎2✑3) ✿ ✿

✶ ❈ ❆

Charged Lepton Mass Matrix The introduction of 45H ✘ (1T7❀ 4Z7) 1 M✵

16i 16j H 45H

✑ ✒✤

Λ

✓4

can generate needed Georgi-Jarlskog factor.

30

slide-75
SLIDE 75

T7: Flavon Potential

T7 W = ✔ ✤1 ✤2 ✤3 F-terms: F✤1 = ❅W ❅✤1 = ✔ ✤2 ✤3 and cyclic ✮ ❤✤2❀3✐ = 0, ❤✤1✐ ✻= 0 T7 ✂ Z7 Renormalizable part forbidden Introduce U(1)R: superpotential: +2, matter: +1, Higgs/flavons: 0 and driving field ✣ ✘ (3✄❀ 5)+2 ✮ superpotential linear in ✣ W = ✔ ✣ ✤2 = ✔ ✣1 ✤2 ✤3 + cyclic F✣1 = ✔ ✤2 ✤3 and cyclic ✮ ❤✤2❀3✐ = 0, ❤✤1✐ ✻= 0 Leading order can be obtained, Further investigation needed to generate viable flavon potential

31

slide-76
SLIDE 76

Σ(81): Group Theory

Σ(81) ✚ U(3): order 81 Irreducible representations: 1i, i = 1❀ ✿ ✿ ✿ ❀ 9 and 3i, i = 1❀ ✿ ✿ ✿ ❀ 8 Rep. 14 15 16 33 35 37 Rep✿❄ 17 18 19 34 36 38 Kronecker products:

1i ✡ 1j = 1i+j mod 3 ❀ i❀ j = 1❀ 2❀ 3 3i ✡ 1j = 3i ❀ i = 1❀ 2 ; j = 1❀ 2❀ 3: (a1❀ a2❀ a3)T ✘ 3i, c ✘ 1j: (a1 c❀ ✦i1 a2 c❀ ✦1i a3 c) ❢31 ✡ 31❣ = 32 ✟ 34: (a1❀ a2❀ a3)T ✘ 31: (a1 a1❀ a2 a2❀ a3 a3)T ✘ 32 with ✦ = ei 2✙❂3 31 ✡ 32 = 11 ✟ 12 ✟ 13 ✟ 37 ✟ 38: (a1❀ a2❀ a3)T ✘ 31, (b1❀ b2❀ b3)T ✘ 32: (a1 b1❀ a2 b2❀ a3 b3)T ✘ 11

32

slide-77
SLIDE 77

Σ(81): Group Theory

Σ(81) ✚ U(3): order 81 Irreducible representations: 1i, i = 1❀ ✿ ✿ ✿ ❀ 9 and 3i, i = 1❀ ✿ ✿ ✿ ❀ 8 Rep. 11 12 14 15 16 31 33 35 37 Rep✿❄ 11 13 17 18 19 32 34 36 38 Kronecker products:

1i ✡ 1j = 1i+j mod 3 ❀ i❀ j = 1❀ 2❀ 3 3i ✡ 1j = 3i ❀ i = 1❀ 2 ; j = 1❀ 2❀ 3: (a1❀ a2❀ a3)T ✘ 3i, c ✘ 1j: (a1 c❀ ✦i1 a2 c❀ ✦1i a3 c) ❢31 ✡ 31❣ = 32 ✟ 34: (a1❀ a2❀ a3)T ✘ 31: (a1 a1❀ a2 a2❀ a3 a3)T ✘ 32 with ✦ = ei 2✙❂3 31 ✡ 32 = 11 ✟ 12 ✟ 13 ✟ 37 ✟ 38: (a1❀ a2❀ a3)T ✘ 31, (b1❀ b2❀ b3)T ✘ 32: (a1 b1❀ a2 b2❀ a3 b3)T ✘ 11

32

slide-78
SLIDE 78

Σ(81): Group Theory

Σ(81) ✚ U(3): order 81 Irreducible representations: 1i, i = 1❀ ✿ ✿ ✿ ❀ 9 and 3i, i = 1❀ ✿ ✿ ✿ ❀ 8 Rep. 11 12 14 15 16 31 33 35 37 Rep✿❄ 11 13 17 18 19 32 34 36 38 Kronecker products:

1i ✡ 1j = 1i+j mod 3 ❀ i❀ j = 1❀ 2❀ 3 3i ✡ 1j = 3i ❀ i = 1❀ 2 ; j = 1❀ 2❀ 3: (a1❀ a2❀ a3)T ✘ 3i, c ✘ 1j: (a1 c❀ ✦i1 a2 c❀ ✦1i a3 c) ❢31 ✡ 31❣ = 32 ✟ 34: (a1❀ a2❀ a3)T ✘ 31: (a1 a1❀ a2 a2❀ a3 a3)T ✘ 32 with ✦ = ei 2✙❂3 31 ✡ 32 = 11 ✟ 12 ✟ 13 ✟ 37 ✟ 38: (a1❀ a2❀ a3)T ✘ 31, (b1❀ b2❀ b3)T ✘ 32: (a1 b1❀ a2 b2❀ a3 b3)T ✘ 11

32

slide-79
SLIDE 79

Σ(81): Realisation

Particle Content Field 16i Si H ∆ ✤i SO(10) 16 1 10 16 1 Σ(81) 31 1i 11 11 32 ✘ = 3❄

1

Lagrangian L ✛ ☛ H (163 163 ✤✄

1 + 161 161 ✤✄ 2 + 162 162 ✤✄ 3)❂Λ

+ ☞1 ∆ S1 (161 ✤1 + 162 ✤2 + 163 ✤3)❂Λ + ☞2 ∆ S2 (161 ✤1 + ✦ 162 ✤2 + ✦2 163 ✤3)❂Λ + ☞3 ∆ S3 (161 ✤1 + ✦2 162 ✤2 + ✦ 163 ✤3)❂Λ + A S1 S1 + B (S2 S3 + S3 S2) + h✿c✿

33

slide-80
SLIDE 80

Σ(81): Lowest Order

mD = ☛ ❤H✐ Λ ✵ ❅ ❤✤1✐✄ ❤✤2✐✄ ❤✤3✐✄ ✶ ❆ MSN = ❤∆✐N Λ ✵ ❅ ☞1 ☞2 ☞3 ✶ ❆ ✵ ❅ 1 1 1 1 ✦ ✦2 1 ✦2 ✦ ✶ ❆ ✵ ❅ ❤✤1✐ ❤✤2✐ ❤✤3✐ ✶ ❆ MSS = ✵ ❅ A ✁ B ✁ ✁ ✶ ❆

m✗ ✙

☛ ❤H✐ ❤∆✐N

✦2 ✵ ❇ ❅

˜ A + 2˜ B ˜ A ˜ B ˜ A ˜ B ✁ ˜ A + 2˜ B ˜ A ˜ B ✁ ✁ ˜ A + 2˜ B

✶ ❈ ❆

˜ A ✑ A 9☞2

1

❀ ˜ B ✑ B 9☞2☞3

34

slide-81
SLIDE 81

Σ(81): Phenomenology

Charged Fermions Quark mass hierarchy ❤✤1✐✄ : ❤✤2✐✄ : ❤✤3✐✄ = ✎2 : ✎ : 1, ✎ ✘ 3 ✁ 103 Zero mixing in quark sector mt ✮ ❤✤3✐✄ ✘ Λ ✮ higher-dimensional operators are relevant Neutrinos Dirac mass hierarchy exactly drops out m✗ ✙

☛ ❤H✐ ❤∆✐N

✦2 ✵ ❇ ❅ ✏˜

A + 2˜ B

✑ ✏˜

A ˜ B

✑ ✏˜

A ˜ B

✁ ˜ A + 2˜ B ˜ A ˜ B ✁ ✁ ˜ A + 2˜ B

✶ ❈ ❆

Neutrino mass matrix diagonalized by tri-bimaximal mixing matrix m2 = 3

☞ ☞ ☞ ☞ ☞

☛ ❤H✐ ❤∆✐N

☞ ☞ ☞ ☞ ☞

2 ☞

☞ ☞˜

A

☞ ☞ ☞ ❀ m1❀3 = 3 ☞ ☞ ☞ ☞ ☞

☛ ❤H✐ ❤∆✐N

☞ ☞ ☞ ☞ ☞

2 ☞

☞ ☞˜

B

☞ ☞ ☞

35

slide-82
SLIDE 82

Σ(81): Higher-Dimensional Operators (General)

Order in ✎ Structure Representation ❖ (1) ✤m

3 (✤❄ 3)nm

11❀2❀3 for (2 m n) mod 3 = 0 (m = 0❀ ✿✿✿❀ n) 3rd comp. of 31 for (2 m n) mod 3 = 1 3rd comp. of 32 for (2 m n) mod 3 = 2 ❖ (✎) . . . . . .

Structure of operators calculable to arbitrary order All higher-dimensional operators suppressed compared to LO. Vanishing entries are filled. Additional Zn symmetry can be introduced to suppress higher-dimensional operators, e.g. Z3 ✮ Numerical Example to show the possibility to fit the data

36

slide-83
SLIDE 83

Σ(81): Higher-Dimensional Operators (Numerical)

mD =

1✿1589 ✁ 106 8✿6454 ✁ 107 ✿ 1✿0051 ✁ 103 3✿4268 ✁ 104 ✿ ✿ 0✿63863

❤H✐ ❀ MSN =

7✿4031 ✁ 106 4✿6288 ✁ 106 3✿2038 ✁ 106 3✿0486 ✁ 103 1✿9009 ✁ 103 ✦ 1✿4336 ✁ 103 ✦2 1✿2503 0✿91423 ✦2 0✿71852 ✦

❤∆✐N ❀ MSS =

1 1✿7689 ✁ 102 ✦2 3✿8688 ✁ 102 ✦ ✿ 1✿1516 ✁ 102 ✦ 0✿7475 ✿ ✿ 2✿3890 ✁ 102 ✦2

MPl

m✗ ✙ ✵ ❅ 1✿1809 ✁ ei 0✿019 1✿7675 ✁ ei 3✿12 1✿5297 ✁ e i 3✿08 ✿ 2✿5403 ✁ e i 0✿031 3✿4549 ✁ ei 3✿11 ✿ ✿ 1✿8254 ✶ ❆ ✁ 102 eV ∆m2

21 = 7✿9 105 eV2 ❀

∆m2

32 = 2✿5 103 eV2 ❀

✒12 = 33✿0✍ ❀ ✒13 = 4✿5✍ ❀ ✒23 = 49✿5✍ ❀ ✍ = 137✍ ❀ ✬1 = 313✍ ❀ ✬2 = 162✍

37

slide-84
SLIDE 84

Σ(81): Flavon Potential

In polar coordinates ✤i = Xiei ✘i V✤(Xj❀ ✘j) = M2 ❳

i

X 2

i + ✕1

i

X 4

i + ✕2

i✻=k

X 2

i X 2 k + 2✔

i

X 3

i cos (☛ + 3✘i)

Minimisation: ❅V✤ ❅X1 = 2X1

  • M2 + 2✕1X 2

1 + ✕2X 2 2 + ✕2X 2 3 + 3✔X1 cos (☛ + 3✘1)

✁ ! = 0 ❅V✤ ❅✘1 = 6✔X 3

1 sin (☛ + 3✘1) !

= 0 and cyclic Minimum ❤X1✐ = ❤X2✐ = 0 ❀ ❤X3✐ = 3✔ + ♣ 9✔2 8M2✕1 4✕1 ❀ ❤✘3✐ = ☛ ✝ ✙ 3 possible in a certain region of parameter space (M2❀ ✕1❀ ✕2❀ ✔❀ ☛).

38

slide-85
SLIDE 85

RG Evolution EFT by EFT

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

Neutrino mass operator

(3)

OM (Λ) = ✵ ❇ ❅ 0

(3)

Y T

✗ H

(3)

MNN ✶ ❈ ❆ ✵ ❇ ❅

✿ ✶ ❈ ❆ ✥ ✦

✗ ❀

✑ ✵ ❅

✶ ❆

slide-86
SLIDE 86

RG Evolution EFT by EFT

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

Neutrino mass operator

(3)

OM (Λ) = ✵ ❇ ❅ 0

(3)

Y T

✗ H

(3)

MNN ✶ ❈ ❆

RG transformation

Y✗

RG

  • ✦ Z T

N Y✗ Zext

MNN

RG

  • ✦ Z T

N MNN ZN

RG

  • ✦ Z T

ext ✔ Zext Z✔

✵ ❇ ❅

✿ ✶ ❈ ❆ ✥ ✦

✗ ❀

✑ ✵ ❅

✶ ❆

slide-87
SLIDE 87

RG Evolution EFT by EFT

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

Neutrino mass operator

(3)

OM (Λ) = ✵ ❇ ❅ 0

(3)

Y T

✗ H

(3)

MNN ✶ ❈ ❆

RG Evolution

(3)

OM (M3) = ✵ ❇ ❅ 0

(3)

Z T

ext (3)

Y T

H

(3)

ZN ✿

(3)

Z T

N (3)

MNN

(3)

ZN ✶ ❈ ❆ ✥ ✦

✗ ❀

✑ ✵ ❅

✶ ❆

slide-88
SLIDE 88

RG Evolution EFT by EFT

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

Neutrino mass operator

(3)

OM (Λ) = ✵ ❇ ❅ 0

(3)

Y T

✗ H

(3)

MNN ✶ ❈ ❆

RG Evolution

(3)

OM (M3) = ✵ ❇ ❅ 0

(3)

Z T

ext (3)

Y T

H

(3)

ZN ✿

(3)

Z T

N (3)

MNN

(3)

ZN ✶ ❈ ❆

Diagonalization

(3)

UT

N (3)

Z T

N (3)

MNN

(3)

ZN

(3)

UN=

(2)

MNN M3

(3)

Z T

ext (3)

Y T

✗ (3)

ZN

(3)

UN✑

(2)

Y T

✗ ❀

y T

3

✑ ✵ ❅

✶ ❆

slide-89
SLIDE 89

RG Evolution EFT by EFT

❤H✐ M1 M2 M3 Λ ✖ (0) (1) (2) (3)

Neutrino mass operator

(3)

OM (Λ) = ✵ ❇ ❅ 0

(3)

Y T

✗ H

(3)

MNN ✶ ❈ ❆

RG Evolution

(3)

OM (M3) = ✵ ❇ ❅ 0

(3)

Z T

ext (3)

Y T

H

(3)

ZN ✿

(3)

Z T

N (3)

MNN

(3)

ZN ✶ ❈ ❆

Diagonalization

(3)

UT

N (3)

Z T

N (3)

MNN

(3)

ZN

(3)

UN=

(2)

MNN M3

(3)

Z T

ext (3)

Y T

✗ (3)

ZN

(3)

UN✑

(2)

Y T

✗ ❀

y T

3

Integrate Out

(2)

OM (M3) =

✵ ❅ y T

3 M1 3

y3 H2

(2)

Y T

H ✿

(2)

MNN

✶ ❆

slide-90
SLIDE 90

RG corrections to Neutrino Mass – Technical details

m✗ = 1 2Z T

ext

✷ ✹

(3)

mT

D

✵ ❅XN

(3)

M1

NN + (3)

M1

NN X T N

✶ ❆ (3)

mD

✸ ✺ Zext

XN ✑

(3)

ZN

(3)

UN

(2)

Z ✵

N (2)

U✵

N Z✔ (2)

U

✵②

N (2)

Z

✵1

N (3)

U②

N (3)

Z 1

N (2)

Z ✵

N✑

✵ ❅

(2)

ZN 1

✶ ❆ ❀

(2)

U✵

N✑

✵ ❅

(2)

UN 1

✶ ❆ ❀

Z✔ ✑ diag

(0)

Z✔❀

(01)

Z✔ ❀

(02)

Z✔

Approximation

V T

N (3)

MNN VN = DN ✑ diag(M1❀ M2❀ M3) ✮ XN ✙ VNZ✔V ②

N

m✗ ✙ ❤H✐2 Z T

ext

✧ (3) Y T

✗ VNZ✔D1 N V T N (3)

Y✗ ★ Zext

✮ Dominantly rescaling of right-handed neutrino masses

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