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BSM and the Origin of Higgs Kobe Univ.  14 March 2012

Yutaka Hosotani

SO(5)xU(1)

Gauge-Higgs Unification

(2)

125 GeV,

but with non-SM couplings,

gauge-Higgs unification

2 not seen at LHC

as it is stable,

or

If the Englert-Brout-Higgs boson is

(3)

4D Higgs fields

H

extra-dim. component A

y

3

4-dim. components A

µ

4D gauge fields

γ , W , Z

EW symmetry breaking

Hosotani mechanism Aharonov-Bohm phase

Gauge-Higgs unification

A M in 5 dim.

(4)

e

iθˆH(x)

∼ P exp

� ig

C

dyA

y

Higgs boson as an AB phase in extra dim �

θ ˆ

H

(x) = θ

H

+ H (x) f

H

θ

H

= � Higgs �

f

H ■ 

masses for 

      quarks/leptons/W,Z

■ 

symmetry breaking

4

C y

θ H ∼ θ H + 2π differs from SM.

(5)

in Randall-Sundrum warped space SO (5) × U (1)

ds

2

= e

2k|y|

dx

µ

dx

µ

+ dy

2

0 ≤ | y | ≤ L = πR

Planck brane TeV brane

AdS Λ = − 6 k

2

SO (5) × U (1)

g

A

g

B

brane scalar

brane fermions quarks, leptons

YH, Oda, Ohnuma, Sakamura 2008 YH, Noda, Uekusa 2009

5

Agashe, Contino, Pomarol, 2005

� A

µ

A

y

(x, − y) = P

0

� A

µ

− A

y

(x, y)P

0

� A

µ

A

y

(x, πR − y ) = P

1

� A

µ

− A

y

(x, π R + y)P

1

Orbifold BC

y = 0 y = πR

(6)

P0 = P1 =

1

1

1

1

+1

4D gauge bosons and Higgs

φ1 φ2 φ3 φ4 Ay









Higgs

4D Higgs doublet

Aµ

 

 

W Z γ

θ

H

� = 0 → U (1)

EM

6

� = SU (2)

L

× U (1)

Y

SO(5) → SO (4) � SU (2)

L

× SU (2)

R

brane scalar SO(4) × U (1) → SU (2)

L

× U (1)

(7)

RS:

fermions

k , z

L

= e

kL

g

A

, g

B

One free parameter z L

parameters

quark/lepton masses

α

w

, sin

2

θ

W

m

Z

inputs

7

(8)

Warped space

Planck scale Weak scale

m W

8

TeV scale m KK

output ☺

m

KK

= πke

kL

∼ π √

kL m

W

kL = 30 ∼ 40 for zL = 1013 ∼ 1017

EW Symmetry breaking

output

input

input

(9)

Effective interactions

L eff ∼ − � 1 2 gf

H

sin ˆ θ

H

2

� W

µ

W

µ

+ 2 cos 1

2

θ

W

Z

µ

Z

µ

− y

f

f

H

sin ˆ θ

H

ψ

f

ψ

f

θ ˆ

H

= θ

H

+ H

f

H

f

H

= 2

√ kL

m

KK

π g

9

cos θ

H

WWH ×

Yukawa ZZH = SM

f

H

sin ˆ θ

H

→ v + H

in SM

θ

H

∼ θ

H

+ 2π

(10)

YH, Oda, Ohnuma, Sakamura 2008 YH, Noda, Uekusa 2009

Planck brane TeV brane

� T ˆ

R

B ˆ

R

� U ˆ

R

D ˆ

R

� X ˆ

R

Y ˆ

R

(

12

, 0)

SO(5) × U (1)

Leptons

 

 

ν

τ

τ L

1X

L

1Y

τ

 

 

1

 

 

L

2X

L

2Y

L

3X

L

3Y

ν

τ

 

 

0

Matter content

�Lˆ1XR1Y R

�Lˆ2XR2Y R

�Lˆ3XR3Y R

Quarks 

 

 

 U D X Y b

 

 

1 3

 

 

 T B

t b t

 

 

2 3

(

12

,

12

) ⊕ (0, 0)

vector rep

L

R

L L L

R

L L L L

R

L L L L

R

L L L L

Φ ˆ (0,

12

)

Brane scalar

� Φ ˆ � � = 0

Ψ(x, y) = P0γ5Ψ(x, y)

Ψ(x,πR y) = P1γ5Ψ(x,πR + y)

10

Anomaly

cancelation

(11)

11

m

H

= 135 GeV (z

L

= 10

15

)

θ

H

= π

2 SU (2) � L × U (1) � → U (1) EM

EW Symmetry breaking

Hosotani mechanism

z

L

= 10

15

0.5 1.0 1.5 2.0

0.5 U

-

0.5 0

-

1.

-

1.5

-

2.0

-

2.5

θ /π

H

gauge

total

fermions (top)

V

eff

H

)/m

4KK
(12)

H : −

all other SM particles : +

Stable Higgs

12

YH, Ko, Tanaka, 2009 YH, Tanaka, Uekusa, 2010

π

2 + H

f

H

− π

2 − H f

H

π

2 − H f

H

H parity  at   θ H = 1 2 π

mirror sym period π

(13)

Agashe, Contino, Da Rold, Pomarol 2006

T parameter Zb ¯ b

H parity 

13

{ T

α

} = { T

aL

, T

aR

, T

aˆ

, T

ˆ4

}

SO(5)/SO(4) SO(5) : SO(4) � SU (2)

L

× SU (2)

R

T

ˆ4

→ − T

ˆ4

P H : SU (2)

L

↔ SU (2)

R
(14)

SO (5) × U (1) X

Where is SU(2) x U(1) in SO(5) x U(1) ?

L Y

� = SU (2)

L

× U (1)

Y

→ SU (2)

L

× U (1)

Brane scalar

� Φ ˆ � � = 0

→ SO(4) × U (1)

X

� SU (2)

L

× SU (2)

R

× U (1)

X

B.C. 

→ U (1)

EM

θ

H

� = 0

14

(15)

YH, Sakamura 2007 Contino, Marzocca, Pappadopulo, Rattazzi 2011

Hatanaka, YH, Shimotani

SO(5) { T

La

, T

Ra

, T ˆ

a

, T ˆ

4

}

SU (2)

L

× SU (2)

R

{ I

La

, I

Ra

, I ˆ

a

, I ˆ

4

}

SU (2)

L

× SU (2)

R

� I

La

I

Ra

= 1 ± cos θ

H

2 T

La

+ 1 ∓ cos θ

H

2 T

Ra

∓ sin θ

H

√ 2 T ˆ

a

Note: T

La

+ T

Ra

= I

La

+ I

Ra

: custodial SU (2)

V

15

Q

EM

= I

L3

+ I

R3

+ Q

X

= T

L3

+ T

R3

+ Q

X

I

α

H

) = ΩT

α

1

Ω = e

iHT ˆ4

W

±

couples to I

L1

± iI

L2
(16)

YH, Sakamura 2007

Hatanaka, YH, Shimotani

W

±

I

L1

± iI

L2

Higgs I ˆ

4

= ˆ T

4

Z c

W

I

L3

− s

W

I

Y

I

Y

= s

φ

I

R3

+ c

φ

T

X

, s

φ

= t

W

γ s

W

I

L3

+ c

W

I

Y

I

α

H

) = ΩT

α

1

Ω = e

iHTˆ4

SU(2) rotates in SO(5). L

16

(17)

W

µ±

 Z

µ

γ

µ

Z ˜

µ

SU (2)

R

SU (2)

L

U (1)

X

� W

µ(n)

(x) �

C (z ; λ

(n)W

)I

L+

H

) − sin θ

H

√ 2 [ ˆ S (z ; λ

(n)W

) − C (z ; λ

(n)W

)] ˆ T

+

To be precise

All KK modes participate.

17

W

1

, W

2

W

3

B

µX

W

3

S, T : need reexamination.

SU(2) rotates in SO(5). L

(18)

Collider signatures

18

No single-Higgs production Higgs pair production

H parity 

Cheung, Song, 1004.2783, Alves, 1008.0016 YH, Tanaka, Uekusa, 1103.6076

Higgs = missing energy, momentum hard to confirm at LHC/ILC

Stable Higgs

(19)

sin

2

θ

W

χ

2

(AF B ) χ

2

(Z decay )

No. data

6 8

SM

0.2312 10.8 13.6

z

L

: 10

15

z

L

: 10

10

z

L

: 10

5

YH, Tanaka, Uekusa, 2011

Gauge couplings

precision measurements

◊   Z-decay branching fractions

◊   Forward-backward asymmetry in e

+

e

→ Z → � � ¯ , q q ¯

z

L

≥ 10

15

0.2309

6.3

0.2303 6.4

0.2284 7.1 16.5 37.7 184.5

19

(20)

Large widths

Strong couplings for right-handed quarks and lepton

KK Z (1) & γ (1)

m Γ z

L

in GeV

γ (1)

10

15

1144 1959 10

5

678 446 m

Γ z

L

in GeV

Z (1)

10

15

1130

422 10

5

653 104

20

Not seen at LHC, so far. ☹

(21)

W W Z W W Z

(1)

W W Z

(2)

W W Z

(3)

W W Z

(4)

W W Z

(5)

0.999 85

− 0.0343

2.07 × 10

5

− 1.25 × 10

3

− 1.38 × 10

5

− 2.04 × 10

4

g

W W Z(n)

/g

e

L

e

R

u

R

u

L

t

L

t

R

0.0311

− 0.0400

− 0.2058 2.516

− 1.656

− 1.467

Z (1) couplings

ν

eL

e

L

ν

µL

µ

L

u

L

d

L

t

L

b

L

u

R

d

R

t

R

b

R

1.0053 1.0053 1.0053 0.9816

− 5 × 10

12

− 0.0009

couplings

W

21

(22)

z

L

m

H

10

5

10

10

10

15

108 135

72 GeV

Stable Higgs Dark Matter

20 30 40 50 60 70 80 90 100

Higgs mass (GeV) 0

0.1 0.2

7 Hh2

semi-analytic micrOMEGAs WMAP

WMAP

Gauge-Higgs

m H

H

h

2

Relic abundance

WMAP data

m

H

= 70 ∼ 75 GeV

22

YH, Ko, Tanaka, 2009

(23)

Collider signatures  z

L

> 10

15

m

H

= 135 GeV Dark matter  m

H

= 70 ∼ 75 GeV z

L

∼ 10

5

23

SUSY exact  m

H

= 0

broken 70 ∼ 75 GeV

Hatanaka, YH, 1111.3756

� t

m

n

W, Z, Higgs

� m

n

t ˜

� m ˜

n

= �

m

2n

+ Λ

2stop

� W , ˜ Z, ˜ Higgs ˜

˜

m

n

= �

m

2n

+ Λ

2gh
(24)

24

0 500 1000 1500 2000 2500

0 200 400 600 800 1000

gh

� GeV �

stop

� GeV �

mh�120GeV

mh�75GeV

mh�70GeV Phase transition

No EWSB

zL = 1015 zL = 1017

m

h

= 120 GeV

m

h

= 75 GeV

m

h

= 70 GeV

Λ

stop

= 250 − 275 GeV Λ

gh

< 100 GeV

for m

h

= 70 ∼ 75 GeV

300 - 320 GeV stop

neutralino < 100 GeV

gluino > 1 TeV

(25)

25 125 GeV with non-SM couplings,

or

(extra dimensions).

gauge-Higgs

If the Englert-Brout-Higgs boson is

not seen at LHC (as it is stable),

Summary 

Referensi

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