How to really kill a new physics model · production process gg → h is multiplied by a factor of...

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How to really kill a new physics model Alexander Lenz (CERN) Bern, May 16th, 2012

Transcript of How to really kill a new physics model · production process gg → h is multiplied by a factor of...

Page 1: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

How to really kill a new physics model

Alexander Lenz (CERN)

Bern, May 16th, 2012

Page 2: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Greek Mythology I

Hydra: υδρα

◮ Snakelike monster with nine heads◮ Sister of Cerberos, Chimaira and Sphinx◮ Bad for hunters: When you cut off one head, two new ones grow...

Common folklore: Hydra was killed by Herakles

The painting:Antonio Pollaiuolo (1431-1498)Florence; 17.5 cm x 12 cm

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Contents

Hydra = SM4

Herakles (Langacker,Erler; Peskin; ATLAS; CMS;...) claimed manytimes that he killed Hydra; e.g. 1110.3805First, the idea of a sequential fourth generation of quarks and leptons is in

serious trouble. If there exist new heavy quarks U and D that couple to the

Standard Model as a conventional quark doublet, the cross section for the

production process gg → h is multiplied by a factor of 9. Given the fact that

Higgs limits are now within a factor of a few of the Standard Model

expectation, this excludes fourth generation models over the entire range of

Higgs mass, excepting only high values above 550 GeV. It is important to

note that other types of exotic fermions are still in play and are even

interesting...

But another head grew and Hydra is still aliveStatements like: mH in the range of 120 to 550 GeV is excluded in

the case of the SM4 are not (yet) correct

Iolaos has to helpAlexander Lenz How to really kill a new physics model (16. 03. 2012) 3 / 44

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The SM4 - the simplest extension of the SM

Another sequential generation of fermions

Leptons:

(

νee

)

,

(

νµµ

)

,

(

νττ

)

,

(

ν4ℓ4

)

Quarks:

(

u

d

)

,

(

c

s

)

,

(

t

b

)

,

(

t ′

b′

)

New parameters

4 Fermion masses

5 CKM parameters

5 PMNS parameters (Dirac neutrinos)

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The deaths of Hydra

History of the investigation of the SM4

Classical Period: Soni, Hou, et al 1986...

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The deaths of Hydra

History of the investigation of the SM4

Classical Period: Soni, Hou, et al 1986...

Death #1: LEP: Nν = 3

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The deaths of Hydra

History of the investigation of the SM4

Classical Period: Soni, Hou, et al 1986...

Death #1: LEP: Nν = 3

Death #2: S ,T ,U Langacker und Erler

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The deaths of Hydra

History of the investigation of the SM4

Classical Period: Soni, Hou, et al 1986...

Death #1: LEP: Nν = 3

Death #2: S ,T ,U Langacker und Erler

Resurrection: Kribs et al 2007; Vysotsky, Okun, et al. 2000-...Electro-weak Observables do not exclude a fourth family!

mt′ −mb′ =

(

1−1

5ln

mH

115GeV

)

· 50GeV

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Page 9: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

The deaths of Hydra

History of the investigation of the SM4

Classical Period: Soni, Hou, et al 1986...

Death #1: LEP: Nν = 3

Death #2: S ,T ,U Langacker und Erler

Resurrection: Kribs et al 2007; Vysotsky, Okun, et al. 2000-...Electro-weak Observables do not exclude a fourth family!

mt′ −mb′ =

(

1−1

5ln

mH

115GeV

)

· 50GeV

Interesting features found in precision analyses:◮ Scans over the CKM4 parameter regions

Bobrowski, A.L., Riedl, Rohrwild; Chanowitz; Soni,...; Buras et al.;Eberhardt, A.L., Rohrwild;...

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The deaths of Hydra

History of the investigation of the SM4

Classical Period: Soni, Hou, et al 1986...

Death #1: LEP: Nν = 3

Death #2: S ,T ,U Langacker und Erler

Resurrection: Kribs et al 2007; Vysotsky, Okun, et al. 2000-...Electro-weak Observables do not exclude a fourth family!

mt′ −mb′ =

(

1−1

5ln

mH

115GeV

)

· 50GeV

Interesting features found in precision analyses:◮ Scans over the CKM4 parameter regions

Bobrowski, A.L., Riedl, Rohrwild; Chanowitz; Soni,...; Buras et al.;Eberhardt, A.L., Rohrwild;...

Death #3: Higgs non-production at LHC

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The deaths of Hydra

History of the investigation of the SM4

Classical Period: Soni, Hou, et al 1986...

Death #1: LEP: Nν = 3

Death #2: S ,T ,U Langacker und Erler

Resurrection: Kribs et al 2007; Vysotsky, Okun, et al. 2000-...Electro-weak Observables do not exclude a fourth family!

mt′ −mb′ =

(

1−1

5ln

mH

115GeV

)

· 50GeV

Interesting features found in precision analyses:◮ Scans over the CKM4 parameter regions

Bobrowski, A.L., Riedl, Rohrwild; Chanowitz; Soni,...; Buras et al.;Eberhardt, A.L., Rohrwild;...

Death #3: Higgs non-production at LHC

?Real Death or Resurrection?

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Main old arguments against the fourth family

History of the PDG reviews

1994: “one heavy generation of ordinary fermions is allowed at 95% CL”

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Main old arguments against the fourth family

History of the PDG reviews

1994: “one heavy generation of ordinary fermions is allowed at 95% CL”

1998: “an extra generation of ordinary fermions is now excluded at the99.2% CL”

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Main old arguments against the fourth family

History of the PDG reviews

1994: “one heavy generation of ordinary fermions is allowed at 95% CL”

1998: “an extra generation of ordinary fermions is now excluded at the99.2% CL”

2002: “an extra generation of ordinary fermions is excluded at the 99.8% CLon the basis of the S parameter alone. [. . . ] This result assumes [. . . ] thatany new families are degenerate. This restriction can be relaxed [. . . ] to95%.”

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Page 15: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Main old arguments against the fourth family

History of the PDG reviews

1994: “one heavy generation of ordinary fermions is allowed at 95% CL”

1998: “an extra generation of ordinary fermions is now excluded at the99.2% CL”

2002: “an extra generation of ordinary fermions is excluded at the 99.8% CLon the basis of the S parameter alone. [. . . ] This result assumes [. . . ] thatany new families are degenerate. This restriction can be relaxed [. . . ] to95%.”

2010: “an extra generation of ordinary fermions is excluded at the 6 σ levelon the S parameter alone. This result assumes [. . . ] that any new familiesare degenerate. [. . . ] a fourth family is disfavored but not excluded bycurrent data.”

Erler/Langacker

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Status of 2007

Kribs, Plehn, Tait, Spannowsky; PRD 2007

SM4 is not excluded - in particular: δS vs. δT

mt′ −mb′ =

(

1−1

5ln

mH

115GeV

)

· 50GeV

CKM-mixing was neglected in electro-weak sector to obtain thisresult

Triggered some activity: 305 citations ≈ 60 per year

Several things were published before by Vysotsky, Rozanov, et al.;He, Polonsky, Su but widely ignored

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Constraints on the SM4

Direct constraints

Mass constraints (quarks, leptons)

Direct measurements of CKM elements

Phase constraints on the CKM matrix

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Constraints on the SM4

Direct constraints

Mass constraints (quarks, leptons)

Direct measurements of CKM elements

Phase constraints on the CKM matrix

Indirect constraints

FCNC

Lepton observables

Electro-weak precision observables

Higgs-production

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Direct mass limits: be careful, always assumptions...

t ′

b′

ℓ4

ν4

t

b

τ

ντ

c

s

µ

νµ

u

d

e

νe

Up-typeQuarks

Down-typeQuarks

ChargedLeptons

Neutrinos

m1 eV 1 keV 1 MeV 1 GeV 1 TeV

mq′ > O(550 − 100GeV): ATLAS; CMS, D0, CDF:e.g. Flacco et al. 2010

mν4 > O(50GeV): LEP ml4 > O(100GeV): LEP(mH /∈ [120 GeV, 550GeV]:ATLAS, CMS, CDF, D0)

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Tree level constraints

ff ′

W

VCKM4 =

Vud Vus Vub Vub′

Vcd Vcs Vcb Vcb′

Vtd Vts Vtb Vtb′

Vt′d Vt′s Vt′b Vt′b′

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Tree level constraints

Vud Vus Vub Vub′

Vcd Vcs Vcb Vcb′

Vtd Vts Vtb Vtb′

Vt′d Vt′s Vt′b Vt′b′

β decays

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Tree level constraints

Vud Vus Vub Vub′

Vcd Vcs Vcb Vcb′

Vtd Vts Vtb Vtb′

Vt′d Vt′s Vt′b Vt′b′

β decays

semileptonic

meson decays

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Tree level constraints

Vud Vus Vub Vub′

Vcd Vcs Vcb Vcb′

Vtd Vts Vtb Vtb′

Vt′d Vt′s Vt′b Vt′b′

β decays

semileptonic

meson decays (single) top production

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Tree level constraints

Vud Vus Vub Vub′

Vcd Vcs Vcb Vcb′

Vtd Vts Vtb Vtb′

Vt′d Vt′s Vt′b Vt′b′

β decays

semileptonic

meson decays (single) top production

The latest PDG value for Vtb is 0.88 ± 0.07.

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Tree level constraints alone

0

0.5

1

0.7 0.8 0.9 1

1-CL

|Vtb|

0

0.5

1

0 0.2 0.4 0.6 0.8

1-CL

θ34

Still huge mixing with a fourth familiy possible!⇒ include also loop observables!

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Page 26: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Further constraints: FCNC

Flavour observables:

d u, c , t, t ′

b

W W

d

b

u, c , t, t ′

Bd Bd

b s

γqq

W

u, c , t, t ′

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Page 27: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

CKM Fits

CKM picture works very well ⇒ corrections should be small

γ

γ

αα

dm∆Kε

sm∆ & dm∆

ubV

βsin 2

(excl. at CL > 0.95) < 0βsol. w/ cos 2

excluded at CL > 0.95

α

βγ

ρ-1.0 -0.5 0.0 0.5 1.0 1.5 2.0

η

-1.5

-1.0

-0.5

0.0

0.5

1.0

1.5excluded area has CL > 0.95

Summer 11

CKMf i t t e r

Similar results from UTfit and Lunghi et al.

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Page 28: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

FCNC in the SM4

Analysis: still huge corrections possible!

There are two effects that change the value of M12 in the SM4

t ′ running in the loop

The t loop is also changed, because now the CKM elements from the3x3 fit can not be use anymore!This was overseen many times!

Huge cancellations between these two effects are possible0902.4883,1005.3505: Parameter sets with O(300%) effects foundSimilar results from Buras et al. ’10; Chanowitz ’09,’10; Soni et al.’09,’10,’11; Hou et al...

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Bounds from FCNC

Observables used as bounds

∆Ms , ∆Md , ∆MD

ǫK : CP violation in K decays

b → sγ, Bs → µµ

Semileptonic asymmetries, Dimuonasymmetry

sin2β from Bd → ψKs

sin2βs from Bs → ψφ

Observables not yet used

B → K (∗)ll

Rare K decays

∆ACP

...

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Bounds on the CKM element Vtd

Im Vtd vs. Re Vtd

Eberhardt, A.L., Rohrwild: 1005.3505

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Bounds on the CKM element Vts

Im Vts vs. Re Vts

Eberhardt, A.L., Rohrwild: 1005.3505

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Bounds on the CKM element Vtb

Im Vtb vs. Re Vtb

Eberhardt, A.L., Rohrwild: 1005.3505

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Page 33: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

— Lesson #1 —

Even if CKM looks perfect - huge effects possible

Cancellations

If VCKM3 is not unitary, Vtx can differ sizeably from their SM3 values.

Effects of a new particle (e.g. t ′) of up to several hundred per centcan be compensated by δVtx

Keep this in mind, when discussing e.g. MFV or other models withnon-unitary VCKM3

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What are S , T and U?

Self-energy contributions by the fourth family

Z , γ Z , γt ′

t ′

Z , γ Z , γb′

b′

W Wu

b′

W Wc

b′

W Wt

b′

W W

d

t ′

W W

s

t ′

W W

b

t ′

W Wt ′

b′

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Explicit expressions

The exact formulae for S and T

Sferm =Nc

(U,D)

[

1−2

3ln

(

mU

mD

)]

+1

(ν,l)

[

1 + 2 ln

(

ml

)]

Tferm =Nc

16πs2c2M2Z

i=U,D

m2i − 4

U,D

∣V(CKM)UD

2 m2Um

2D

m2U −m2

D

ln

(

mU

mD

)

+1

16πs2c2M2Z

i=ν,l

m2i − 4

ν,l

∣V(PMNS)νl

2 m2νm2

l

m2ν−m2

l

ln

(

ml

)

≥ 0

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The S-T ellipse: Experimental values

S ,T

+0.1

−0.2

−0.4

−0.6

time

[PDG ’94] [PDG ’02] [Gfitter ’09] [PDG ’10]

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The S-T ellipse: Experimental values

S ,T

+0.1

−0.2

−0.4

−0.6

time

[PDG ’94] [PDG ’02] [Gfitter ’09] [PDG ’10]

S

T

95% CLBest fit

SM

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Fermion mass difference

Neglecting the leptons

0

0.5

1

-50 0 50

1-CL

mt’-mb’

(V CKM = 1)

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Fermion mass difference

Neglecting the leptons

0

0.5

1

-50 0 50

1-CL

mt’-mb’

Excludedat 6σ

(V CKM = 1)

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Fermion mass difference

Neglecting the leptons

0

0.5

1

-50 0 50

1-CL

mt’-mb’

Excludedat 6σ

0

0.5

1

-50 0 50

1-CL

mt’-mb’

(V CKM = 1) (V CKM 6= 1)

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Fermion mass difference

Taking also the leptons into account:

-100 -50 0 50 100mt’-mb’ [GeV]

-200

0

200

mν4-ml4

[GeV]

0

0.2

0.4

0.6

0.8

1

[GeV]4

d - m4um

-100 -50 0 50 100

[GeV

]4l

- m

4νm

-200

-150

-100

-50

0

50

100

150

2004th Generation

68%, 95%, 99% CL fit contours (allowed)

=120 GeVHMpreliminary

[GeV]4

d - m4um

-100 -50 0 50 100

[GeV

]4l

- m

4νm

-200

-150

-100

-50

0

50

100

150

200

G fitter SMB

Aug 10

(V CKM = 1)

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Fermion mass difference

Taking also the leptons into account:

-100 -50 0 50 100mt’-mb’ [GeV]

-200

0

200

mν4-ml4

[GeV]

0

0.2

0.4

0.6

0.8

1

-100 -50 0 50 100mt’-mb’ [GeV]

-200

0

200

mν4-ml4

[GeV]

0

0.2

0.4

0.6

0.8

1

(V CKM = 1) (V CKM 6= 1)

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The impact of S and T

Tree-level

0

0.5

1

0.7 0.8 0.9 1

1-CL

|Vtb|

0

0.5

1

0 0.2 0.4 0.6 0.8

1-CL

θ34

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The impact of S and T

Tree-level+ S and T

0

0.5

1

0.7 0.8 0.9 1

1-CL

|Vtb|

0

0.5

1

0 0.2 0.4 0.6 0.8

1-CL

θ34

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— Lesson #2 —

CKM4 dependence is essential for e-weak precision observables

For the first time fully included in 1005.3505

Eberhardt, A.L., Rohrwild

Qualitative changes

|mb′ −mt′ | < 80 GeV

|ml4 −mν4| < 140 GeV

Use full e-weak precision observables instead of S,T,UImplemenation of Zfitter in CKMfitter in progress

◮ 1105.3434 Gonzales, Rohrwild, Wiebusch◮ Eberhardt, Herbert, Lacker, A.L., Menzel, Nierste, Wiebusch =

CKM4Fitter 1204.3872

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 26 / 44

Page 46: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Higgs production and decay

Common folklore

σSM4(gg → h) ≈ 9σSM3(gg → h)

NLO e-weak corrections to production and decay are dominated bylight fermions, i.e. contribution of fourth family is negligible

A large range of higgs mass values in the SM4 is already excluded bythe non-observation of a higgs boson at LHC

Higgs limits assuming a 4th

generation heavy fermions

!"##$%$&'(('##$ )*$+,-./0$1,22-$-3.4563-$,7$)8!)9$ TU$

!"#!$%

863$5@F<,73C$=EE34$B,F,>$@7$>63$1,22-$<@-@7$E4@C=5/@7$54@--$-35/@7$,7$>63$?4.F3G@4i$@?$.$

9>.7C.4C$D@C3B$G,>6$>63$.CC,/@7$@?$.$63.Ya$?@=4>6$23734./@7$@?$?34F,@7-$C,Y,C3C$<a$,>-$

3ZE35>./@7$.-$.$?=75/@7$@?$GQ',-$,7C,5.>3C$<a$>63$-@B,C$B,73*$86,-$,-$.$V:c$I!$B,F,>$=-,72$>63$

I!-$F3>6@C*$$

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 27 / 44

Page 47: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Higgs production and decay

The facts

The possibility H → ν4ν4 was not considered - Why?

NLO e-weak corr. were reinvestigated and turned out to be hugeg

g

H

(a)

g

g

H

(b)

Figure 1: Examples of two-loop diagrams contributing to gg → H.

G. Passarino, C. Sturm, S. Uccirati 1108.2025;

A. Denner, S. Dittmaier, A. Muck, G. Passarino, M. Spira, C. Sturm, S. Uccirati, M.M. Weber 1111.6395

Leading behaviour known since a long time - why negelcted?Djouadi, Gambino 1994; Djouadi, Gambino, Kniehl 1997

This is currently implemented in the experimental search:LHC Higgs Cross Section Working Group

Conclusions will change dramatically!

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 28 / 44

Page 48: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

H → ν4ν4

PDG bounds mν4 > 90 GeV holds only for a unstable neutrino

pure mass term mixed mass term

unstable 80...90 62.1

stable (θi4 < 3 · 10−6) 45 33.5

Bulanov et al. 0301268; Carpenter, Rajamaran 1005.0628; Carpenter 1010.5502

H → ν4ν4 will be one of the dominant channels!

Khoze 0105069;

Arik et al. 0203257;

Belotsky et al. 0210153;

...

Higgs boson mass [GeV]110 120 130 140 150 160 170 180 190 200

SM3

BR)

×σ /

SM4

BR)

×σ(

-110

1

10Fourth family neutrino with mass 60 GeV

(Dirac) , ZZ, ff-W+ W→ H →(Majorana) gg(Dirac) γγ→ H →(Majorana) gg

Figure 4: Same as Fig. 1 but for mν4= 60 GeV.

Higgs boson mass [GeV]110 120 130 140 150 160 170 180 190 200

SM3

BR)

/ SM

4BR

)(

-110

1

10Fourth family neutrino with mass 70 GeV

(Dirac) , ZZ, ff-W+ W H (Majorana) gg(Dirac) H (Majorana) gg

Higgs boson mass [GeV]110 120 130 140 150 160 170 180 190 200

SM3

BR)

/ SM

4BR

)(

-110

1

10Fourth family neutrino with mass 80 GeV

(Dirac) , ZZ, ff-W+ W H (Majorana) gg(Dirac) H (Majorana) gg

Higgs boson mass [GeV]110 120 130 140 150 160 170 180 190 200

SM3

BR)

/ SM

4BR

)(

-110

1

10Fourth family neutrino with mass 90 GeV

(Dirac) , ZZ, ff-W+ W H (Majorana) gg(Dirac) H (Majorana) gg

Cetin et al. 1108.4071; also Carpenter 1110.4895; Rozanov, Vysotsky 1012.1483

Might be tested via heavy lepton searches and electro-weak precision observables

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 29 / 44

Page 49: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

NLO e-weak corrections I

Were not included in the LP2011 analyses

Turned out to be huge: up to −60%!

Are currently implemented in experimental analyses

[GeV]H

M100 200 300 400 500 600 700 800 900 1000

[%]

EW

-70

-60

-50

-40

-30

-20

-10

0

10

20 WW ZZ tt

100 200 300 400

2

4

6

8

10

12

Figure 1: Relative corrections in SM4 (t′−b′ and l′−νl′ doublets) due to two-loop EW correctionsto gg→ H. The masses of the 4th-generation fermions are chosen according to Eq. (2.1). In theinset a blow-up of the small-MH region is shown.

Table 7: Higgs branching fractions for the γγ decay channel without and with NLO EW correc-tions.

MH [GeV] w/o NLO EW w/ NLO EW

100 1.31 · 10−4 4.65 · 10−5

110 1.72 · 10−4 4.40 · 10−5

120 2.26 · 10−4 3.77 · 10−5

130 2.95 · 10−4 2.71 · 10−5

140 3.81 · 10−4 1.30 · 10−5

150 4.74 · 10−4 1.42 · 10−6

Denner et al. 1111.6395

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 30 / 44

Page 50: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

NLO e-weak corrections II

But!: Currently NLO e-weak corrections are only available for

ml4 = mν4 = mb′ = 600 GeV

mt′ = mb′ + 50 GeV (1− 0.2lnMH/115 GeV )

Vx4 = 0

PROBLEMS:

Cover the whole SM4 parameter space◮ also MH > 2mν4

◮ numerical integrations may take some time◮ Include CKM mixing in the corrections? This was crucial for S,T,U

Corrections are huge → convergence is questionable

1111.6395v2 by A.Denner et al.

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 31 / 44

Page 51: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

What does the Higgs search of LHC tell at LP2011?

Higgs limits assuming a 4th

generation heavy fermions

!"##$%$&'(('##$ )*$+,-./0$1,22-$-3.4563-$,7$)8!)9$ TU$

!"#!$%

863$5@F<,73C$=EE34$B,F,>$@7$>63$1,22-$<@-@7$E4@C=5/@7$54@--$-35/@7$,7$>63$?4.F3G@4i$@?$.$

9>.7C.4C$D@C3B$G,>6$>63$.CC,/@7$@?$.$63.Ya$?@=4>6$23734./@7$@?$?34F,@7-$C,Y,C3C$<a$,>-$

3ZE35>./@7$.-$.$?=75/@7$@?$GQ',-$,7C,5.>3C$<a$>63$-@B,C$B,73*$86,-$,-$.$V:c$I!$B,F,>$=-,72$>63$

I!-$F3>6@C*$$

ml4 = mν4 = mb′ = 600 GeV

mt′ = mb′ + 50 GeV (1− 0.2lnMH/115 GeV )

Vx4 = 0NLO-eweak is negligible

with the followingspecial properties:

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 32 / 44

Page 52: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Status: May 2012

Theory status:

HDECAY includes now NLO-eweak corrections for general SM4parameters - still no CKM4 mixing

H → ν4ν4 taken into account

S, T, U replaced by the explicit observables (Zfitter)

Michael Spira; A.L., Djouadi 1204.1252; Eberhardt et al. 1204.3872

Experimental News:

TeVatron sees hints for Higgs in associated Vector boson productionand subsequent Higgs decay in bb

Moriond 2012

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 33 / 44

Page 53: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Status: May 2012

Higgs Branching Ratios before full NLO-eweak for H → γγ

gg

γγ

VV

bb

MH=125 GeV

BR(H→XX)|SM4/SM

mν′ [GeV]45 62.5 100 200 300 400 500 600

10

1

0.1

0.01

A.L., Djouadi 1204.1252SM4 might be consistent with SM3, if

Gluon fusion enhanced by a factor of 9

Associated vector boson production not affected BUT 1 & 2

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 34 / 44

Page 54: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Status: May 2012

BUT 1: Full NLO-eweak for H → γγ ⇒ SM4 is dead, if signal stays

mb′ =mt′+50 GeV=600 GeV

“approx” NLO

MH=125 GeV

“exact” NLO

σ(gg→H→γγ)|SM4/SM

mν′ = mℓ′ [GeV]100 200 300 400 500 600

1

0.1

SM4 is in H → γγ a factor of 10 below the SM3Anti-BUT 1: HUGE NLO-eweak corrections!!

maybe not relieable and perturbativity is violated ???

A.L., Djouadi 1204.1252

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 35 / 44

Page 55: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Status: May 2012

BUT 2: The final Killer: The Tevatron signal, if it stays

mb′ =mt′+50 GeV=600 GeV

g2

HVV|SM4/SM

MH=125 GeV

σ(Vbb)|SM4/SM

VH→Vbb at Tevatron

mν′ = mℓ′ [GeV]100 200 300 400 500 600

1

0.1

Associated vector boson production is also reducedp + p → Hbb is in the SM4 only about 20% − 35% of the SM3

thus invisible at Tevatron!

A.L., Djouadi 1204.1252

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 36 / 44

Page 56: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Status: May 2012

What did we learn so far?

In ancient times it was believed that the SM4 leads to a significantenhancement of all Higgs decays, this could only be compensated by theinvisible decay H → ν4ν4, which was neglected in many analyses.

News since about March 2012: Under-production might kill the SM4

The numbers of γγ from a Higgs (for mH = 125 GeV) is in the SM4about a factor of 10 below the SM3This channel should be currently not detectable(Is perturbativity still valid?)

The number of bb from associated Higgs-vector boson production (formH = 125 GeV) is in the SM4 only about 20% − 35% of the SM3This channel should be currently not detectable

Higgs should actually be called AEBHGHK

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 37 / 44

Page 57: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Status: May 2012

Take the currently low significance of the Higgs signals into account

gg → H → γγ

V V → H → γγ

pp→ H →WW

pp→ H → ZZ

pp→ H → bb

−3σ −2σ −1σ +1σ +2σ +3σ

Pulls of the Higgs signal strengths

SM3

SM4

SM4+EWPO

SM4 is disfavoured (SM3 also) but not yet ruled outEberhardt et al. 1204.3872

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 38 / 44

Page 58: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Status: May 2012

Take the currently low significance of the Higgs signals into account

0

20

40

60

80

100

120

50 60 70 80 90 100

c2

mn4 [GeV]

SM4 with EWPO and H->ttSM4 w/o EWPO with H->ttSM4 with EWPOSM3 with EWPOSM4 w/o EWPOSM3 w/o EWPO

SM4 is disfavoured (SM3 also) but not yet ruled out Eberhardt et al.1204.3872

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 39 / 44

Page 59: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Conclusions

Interestings results from investigations of SM4

Huge invisible effects in the flavor sector not excluded!Compare this with MFV-paradigm

Totgesagte leben langer — It is difficult to rule out a model◮ CKM4 dependence turned out to be crucial◮ Higgs killing arguments turned around completely

Over-production ⇒ Under-production

Current status of SM4:◮ MH 6= 125 GeV

⇒ SM4 viable◮ MH = 125 GeV

⇒ SM4 is disfavoured (SM3 also) for light ν4, else stronger disfavoured◮ MH = 125 GeV and central values of Higgs signal will stay in 2012

⇒ ruled out

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 40 / 44

Page 60: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Conclusions

Next Steps

Include flavor observables - in progress CKM4fitter,...

There are some problem, which might be cured by the SM4

LHC will tell this year, if MH = 125 GeV is real

If LHC will not clearly rule out the SM4:

Include flavor observables - in progress CKM4fitter,...

Include lepton sector and CKM4 dependence of direct mass limitsCKM4fitter,...

all e-weak corrections at 2-loop order + full CKM4 dependence?

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 41 / 44

Page 61: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Greek Mythology II

Herakles did not manage to kill Hydra, because whenever he cut offone head, two new ones grow...

Iolaos the nephew of Herakles also joined this adventureWhenever Herakles cut off one head and the new ones started togrow, Iolaos burned them

Hydra was killed - Herakles became famous for it - but he would nothave managed without Iolaos help

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 42 / 44

Page 62: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

Perturbative SM4 is not yet excluded by experimental data

How the story really will be :-)

ATLAS;CMS Erler,LangackerPeskin,...

Cetin et al.; CKM4fitter,

Beham, (Hans) Sebald (1500-1550)

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 43 / 44

Page 63: How to really kill a new physics model · production process gg → h is multiplied by a factor of 9. Given the fact that Higgs limits are now within a factor of a few of the Standard

One head will always survive:

A non-perturbative fourth family

Work by

K. Jansen et al. - Lattice

P.Q. Hung et al.

G. Hou et al.

Alexander Lenz How to really kill a new physics model (16. 03. 2012) 44 / 44