a light composite higgs and its heavy vector partners

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A Light Composite Higgs and its Heavy Vector Partners Kenneth Lane, with Lukas Pritchett Boston University

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A Light Composite Higgs and its Heavy Vector Partners

Kenneth Lane, with Lukas Pritchett Boston University

A Light Composite Higgs and its Heavy Vector Partners

Kenneth Lane, with Lukas Pritchett Boston University

The data

The light composite Higgs model

Tests for Run 2

⇢H , aH ! V V, V H cross sections

⇢H , aH ! V V, V H decays

1.5 2 2.5 3 3.5

Even

ts /

100

GeV

1−10

1

10

210

310

410DataBackground model1.5 TeV EGM W', c = 12.0 TeV EGM W', c = 12.5 TeV EGM W', c = 1Significance (stat)Significance (stat + syst)

ATLAS-1 = 8 TeV, 20.3 fbs

WZ Selection

[TeV]jjm1.5 2 2.5 3 3.5

Sign

ifica

nce

2−1−0123

Run 1

ATLAS “WZ” nonleptonic

[TeV]W' m1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3

WZ)

[fb]

→ B

R(W

' ×

W')

→(p

p σ

1−10

1

10

210

310

410 Observed 95% CL

Expected 95% CL

uncertaintyσ 1±

unceirtaintyσ 2±

EGM W', c = 1

ATLAS-1 = 8 TeV, 20.3 fbs

Run 1

ATLAS “WZ” nonleptonic

[GeV]GM1000 1500 2000 2500

ZZ)

[pb]

→ bu

lk B

R(G

× 95

-310

-210

-110

1

600

observedS

Frequentist CL

σ 1± expected S

Frequentist CL

σ 2± expected S

Frequentist CL

= 0.5PlM/k ZZ), → bulk

x BR(GTHσ

= 0.2PlM/k ZZ), → bulk

x BR(GTHσ

CMS = 8 TeVs at -1L = 19.7 fb

Run 1

CMS “ZZ” semileptonic

[GeV]GM1000 1500 2000 2500

) [pb

]bu

lk G

→ (p

p 95

-310

-210

-110

1 observedS

Frequentist CL

σ 1± expected S

Frequentist CL

σ 2± expected S

Frequentist CL

= 0.5PlM/k), bulk G→ (pp THσ

I II III

CMS = 8 TeVs at -1L = 19.7 fb

600

Run 1

CMS “WW” semileptonic

(GeV)W'M1000 1500 2000

WH

) (pb

)→

*BR

(W'

95%

σ

-310

-210

-110

1

10

800

ObservedSFull CLσ 1± Expected SFull CLσ 2± Expected SFull CL

WH)→ * BR(W' W'

HVT B(gv=3):xsec WH)→ * BR(W' W'LH model:xsec

(8 TeV)-119.7 fbCMS combinedµPreliminary e+

Run 1

CMS “WH” semileptonic

Run 2

ATLAS “WH” semileptonic

Mass[TeV]1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3

Sigm

a

2−

1−

0

1

2

3

4

5ATLAS Dijet

ATLAS All-Hadronic WZ

ATLAS Dilepton plus Jet(s)

ATLAS Lepton plus Jet(s) WZ

CMS Dijet

CMS All-Hadronic WZ

CMS Dilepton plus Jet(s)

CMS Lepton plus Jet(s)

CMS WR

“WZ” resonance significances

Run 1

Mass[TeV]1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3

Sigm

a

2−

1−

0

1

2

3

4

5 ATLAS DijetATLAS DileptonATLAS All-Hadronic WWATLAS All-Hadronic ZZATLAS Dilepton plus Jet(s)ATLAS Lepton plus Jet(s) WWCMS DijetCMS DileptonCMS All-Hadronic WWCMS All-Hadronic ZZCMS Dilepton plus Jet(s)CMS Lepton plus Jet(s)

“WW,ZZ” resonance significances

Run 1

Mass[TeV]1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3

Sigm

a

2−

1−

0

1

2

3

4

5ATLAS Dilepton bb

ATLAS Lepton, MET bb

CMS Ditau Jet(s)

CMS All-Hadronic WH

CMS All-Hadronic ZH

CMS Lepton, MET bb

WH resonance significances

Run 1

• ALL models for H(125) are finely-tuned:

-> The SM (of course) -> SUSY -> even composite Higgs models! They require top, W-partners — none have been found. (see, e.g., Guidice 1307.7879 Bellazzini, Csaki, Serra 1401.2457, Barnard, et al. 1409.7391)

A new composite Higgs model

models for H(125) are finely-tuned:

-> The SM (of course) -> SUSY -> even composite Higgs models! They require top, W-partners — none have been found. (see, e.g., Guidice 1307.7879 Bellazzini, Csaki, Serra 1401.2457, Barnard, et al. 1409.7391)

Do we need top, W partners?

ALL•

A new composite Higgs model

TC models (Yamawaki, et al., Sannino, et al.)

No plausible explanation why H(125) is so light (dilaton??)

No plausible explanation why H(125) is so much lighter than other technihadrons — where is ⇢T ??

A new composite Higgs model

(KL, PRD 90, (2014) 9, 09525; arXiv:1407:2270; KL + Luke Pritchett, in preparation; see also Chivukula, Cohen, KL NPB 343 (1990) 554)

(inspired by BHL PRD41, 1647 (1989))

A new composite Higgs model

A fine-tuned solution

NJL applied to strong ETC:

Strong ETC, not TC, drives EWSB!•

(KL, PRD 90, (2014) 9, 09525; arXiv:1407:2270; see also Chivukula, Cohen, KL NPB 343 (1990) 554)

(BHL PRD41, 1647 (1989))

A new composite Higgs model

A fine-tuned solution

NJL applied to strong ETC:

Strong ETC, not TC, drives EWSB!•

• ETC coupling is fine-tuned to be near the critical value for EWSB.

(KL, PRD 90, (2014) 9, 09525; arXiv:1407:2270; see also Chivukula, Cohen, KL NPB 343 (1990) 554)

A new composite Higgs model

A fine-tuned solution

NJL applied to strong ETC:

Strong ETC, not TC, drives EWSB!

The fine tuning: in the large-N approximation,

(BHL PRD41, 1647 (1989))

ETC coupling is fine-tuned to be near the critical value for EWSB.

(a physical cut-off)mf ,MH ' 2mf ⌧ ⇤ETC = ⇤

A new composite Higgs model

• WEAK TC binds T-fermions to make technihadrons with

M⇢H ,MaH , · · · = O(⇤TC) = 1 � 2TeV � MH , but ⌧ ⇤

⇢H , aH , . . .

A new composite Higgs model

• WEAK TC binds T-fermions to make technihadrons with

M⇢H ,MaH , · · · = O(⇤TC) = 1 � 2TeV � MH , but ⌧ ⇤

⇢H , aH , . . .

(this slide is too small to hold the argument)

A new composite Higgs model

• WEAK TC binds T-fermions to make technihadrons with

M⇢H ,MaH , · · · = O(⇤TC) = 1 � 2TeV � MH , but ⌧ ⇤

⇢H , aH , . . .

The Higgs is much lighter than • ⇢H , aH , . . .

A new composite Higgs model

• WEAK TC binds T-fermions to make technihadrons with

M⇢H ,MaH , · · · = O(⇤TC) = 1 � 2TeV � MH , but ⌧ ⇤

⇢H , aH , . . .

The Higgs is much lighter than • ⇢H , aH , . . .

and there are no top, W-partners!•

a simplest TC-ETC model:

LETC = G1 qiaL tRa tbR qLib + G3 T

i↵L UR↵ U�

R TLi�

+G2

�qiaL tRa U↵

R TLi↵ + h.c.�

consider this model in the limit of large-N and weak-TC

qL = (t, b)L 2 (2, 16, 3C , 1TC), tR 2 (1, 2

3, 3C , 1TC), bR 2 (1,�1

3, 3C , 1TC)

TL = (U,D)L 2 (2, 0, 1C , dTC), UR 2 (1, 12, 1C , dTC), DR 2 (1,�1

2, 1C , dTC)

In the limit of large N and weak TC:

A magic relation that makes everything else work— including disappearance of -divergence!

mt =G1NCmt

8⇡2

⇣⇤2 � m2

t ln⇤2

m2t

+G2dTCmU

8⇡2

⇣⇤2 � m2

U ln ⇤2

m2U

mU = G2NCmt

8⇡2

⇣⇤2 � m2

t ln⇤2

m2t

+G3dTCmU

8⇡2

⇣⇤2 � m2

U ln ⇤2

m2U

⇤2

Independence of NC and dTC = dim(dTC)

) G2 = (mU/mt)G1 = (mt/mU)G3

This has a pole at

##2mU2mt

mt(⇤) = 118GeV,mU(⇤) = 126GeVat ⇤ = 500TeVNC = 3, NTC = 15) MH = 250GeV

p = MH(⇤) = 250GeV

MH⇠= 2

sNCm4

t + dTCM4U

NCm2t + dTCM2

U

�tt!tt0+ (p) = m

2t

m

2tNC(p2 � 4m2

t )

8⇡2

Z 1

0dx ln

✓⇤2

m

2t � p

2x(1 � x)

+m

2UNTC(p2 � 4m2

U)

8⇡2

Z 1

0dx ln

✓⇤2

m

2U � p

2x(1 � x)

◆��1

This has a pole at

##2mU2mt

mt(⇤) = 118GeV,mU(⇤) = 126GeVat ⇤ = 500TeVNC = 3, NTC = 15) MH = 250GeV

p = MH(⇤) = 250GeV

MH⇠= 2

sNCm4

t + dTCM4U

NCm2t + dTCM2

U

�tt!tt0+ (p) = m

2t

m

2tNC(p2 � 4m2

t )

8⇡2

Z 1

0dx ln

✓⇤2

m

2t � p

2x(1 � x)

+m

2UNTC(p2 � 4m2

U)

8⇡2

Z 1

0dx ln

✓⇤2

m

2U � p

2x(1 � x)

◆��1

N.B.: These are masses at !scale — to be renormalized to

⇤⇤EW

⇢H and aHThe Higgs’ heavy vector partners —

• ⇢H and aH are the most accessible technihadron partners of H(125)

Describe them via Hidden Local Symmetry as the gauge bosons of an flavor symmetry.SU(2)L ⌦ SU(2)R

KL & Luke Pritchett, PLB 753, 211-214; 1507.07102

⇢H and aH

! gL = gR ⌘ g⇢H = 3 � 5

! ⇢0H ! W+

L W�L , ⇢±

H ! W±L ZL

! a0H ! ZLH, a±

H ! W±L H

TC interactions are vectorial, isospin and parity-invariant: ⇢H and aH(minimizes S from too!)

The Higgs’ heavy vector partners —

• ⇢H and aH are the most accessible technihadron partners of H(125)

• Describe them via Hidden Local Symmetry as the gauge bosons of an flavor symmetry.SU(2)L ⌦ SU(2)R

KL & Luke Pritchett, PLB 753, 211-214; 1507.07102

(the Goldstone bosons of EWSB)

) M⇢H⇠= MaH

Decay rates and Cross sections

�(⇢0H ! W+W�) ⇠= �(⇢±H ! W±Z) ⇠=g2⇢H

M⇢H

48⇡

�(a0 ! ZH) ⇠= �(a± ! W±H) ⇠=g2⇢H

MaH

48⇡

�(a0H ! W+W�) ⇠= �(a±H ! W±Z) ⇠=g2⇢H

M2WM3

aH

24⇡M4⇢H

H,W±L , ZL

⇢H and aH are parity-doubled isotriplets

Near the EW phase transition are a degenerate (2,2) quartet => equal decay rates!

M⇢H(MaH

= 1.05M⇢H) �(⇢H ! V V ) (GeV) �(aH ! V H) (GeV) �(aH ! V V ) (GeV)

1800 178 184 0.82

1900 188 196 0.78

2000 198 208 0.74

for g⇢H= 3.86

M⇢H(MaH

= 1.05M⇢H) �(⇢H ! V V ) (GeV) �(aH ! V H) (GeV) �(aH ! V V ) (GeV)

1800 178 184 0.82

1900 188 196 0.78

2000 198 208 0.74

N.B.: These widths may be significantly depleted (⇠ 1/4?)

by the content of tt, tb H,WL, ZL

⇢H , aH ! V V, V H cross sections

⇢H , aH are mainly produced at LHC via Drell-Yan.

⇢HLarge VV coupling of

aH

=> appreciable VBF too.

=> NO appreciable VBF. Small VV coupling of

ps (TeV) M⇢H (GeV) �(⇢±

H) (fb)(DY + V BF )

�(⇢0H) (fb)

(DY + V BF ) �(a±H) (fb) �(a0

H) (fb)

8 1800 1.53+0.36 0.74+0.18 0.71 0.37

8 1900 1.05+0.24 0.50+0.12 0.51 0.27

8 2000 0.73+0.15 0.36+0.08 0.36 0.17

13 1800 7.61+3.67 3.74+1.93 4.65 2.23

13 1900 5.74+2.62 2.81+1.37 3.16 1.69

13 2000 4.37+1.90 2.16+0.99 2.39 1.27

for g⇢H= 3.86, MaH

= 1.05M⇢H, YTL

= 0, YUR= �YDR

=

12

⇢H , aH ! V V, V H cross sections

⇢H , aH are mainly produced at LHC via Drell-Yan.

⇢HLarge VV coupling of

aH

=> appreciable VBF too.

=> NO appreciable VBF.

�DY (aH) ' 0.5�DY (⇢H)

�DY (13TeV) = 5� 7 �DY (8TeV)

�V BF (aH) < 0.01 �V BF (⇢H)

rising to about

12�DY (⇢H) at 13TeV

�V BF (⇢H) ' 14�DY (⇢H) at

ps = 8TeV,

proton pdf’s

Small VV coupling of

) �(⇢±H) ' �(⇢+H) ' 2�(⇢0H) uniformly

ditto for aH) W+Z � W�Z, W+H � W�H

!!

• VV production from W±Z,W+W�⇢H only: but NO ZZ !

=> Distinguish W from Z — using leptonic decays.

Predictions & recommendations for Run 2-300 fb�1!

W±Z,W+W�⇢H only: but NO ZZ !•

=> Distinguish W from Z — using leptonic decays. VV production from

aH ⇢H . How to distinguish if degenerate?VH due to not

Predictions & recommendations for Run 2-300 fb�1!

W±Z,W+W�⇢H only: but NO ZZ !•

=> Distinguish W from Z — using leptonic decays. VV production from

aH ⇢H . How to distinguish if degenerate?VH due to not 1/3 of VV, not VH, production is VBF, with forward jets!

Predictions & recommendations for Run 2-300 fb�1!

W±Z,W+W�⇢H only: but NO ZZ !

=> Distinguish W from Z — using leptonic decays. VV production from

aH ⇢H . How to distinguish if degenerate?VH due to not 1/3 of VV, not VH, production is VBF, with forward jets!

Predictions & recommendations for Run 2-300 fb�1!

Difficult to explain DY+VBF > few fb at 8 TeV. Therefore, Run 1 was an up-fluctuation — like H(125)! This was confirmed (!!) last December.

W±Z,W+W�⇢H only: but NO ZZ !

=> Distinguish W from Z — using leptonic decays. VV production from

aH ⇢H . How to distinguish if degenerate?VH due to not 1/3 of VV, not VH, production is VFB, with forward jets!

Predictions & recommendations for Run 2-300 fb�1!

Difficult to explain DY+VBF > few fb at 8 TeV. Therefore, Run 1 was an up-fluctuation — like H(125)! This was confirmed (!!) last December.

• There will be NO top & W partners. Our model doesn’t need them!

That’s all, Folks!