Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal...

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Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of Mass

Transcript of Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal...

Page 1: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Francesco Sannino

Zakopane 2009

Conformal Dynamics from LHC to Cosmology III

C P 3 - O r i g i n s

Particle Physics & Origins of Mass

Page 2: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Technicolor

Page 3: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

SM is Unnatural

DEWSB

Need for Conformal Dynamics

Lecture 1

Page 4: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Atoms4%

Dark Matter22%

Dark Energy74%

Page 5: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Dark Matter

!DM

!B! 5

Page 6: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

U(1) baryon number approx. conserved.

We observe a B - Anti B asymmetry.

EW unbroken B - L allows B to survive the EW transition.

B - L need not to be conserved at GUT scales

!B

Page 7: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

A particle similar to the nucleon

But electrically neutral

At most EW-type cross sections

Great if connected to the ESWB

What if DM is due to an asymmetry?

Page 8: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Technibarion is similar to the nucleon

TB number like the B number

At most EW-type cross sections

EW scale and interactions built in

Technicolor is a natural example(TIMP)

Nussinov, 86Barr - Chivukula - Farhi 90Sarkar 96Gudnason - Kouvaris - F.S. 06

Ultra Minimal Technicolor is the first physical realization Ryttov - F.S. 08

PAMELA/ATIC Decaying Dark Matter + Unification, Nardi, F.S., Strumia, 08.

Page 9: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

TIMP can be a Boson or a Fermion

Can be (or not) neutral w.r.t. Weak Interactions

Within Technicolor

TIMP is a pseudo Goldstone-boson

Ultra Minimal Technicolor

Ryttov - F.S. 08

Composite Unparticle + TC F.S. - Zwicky 08

Unbaryon (To investigate)

Page 10: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Plus sign minus signCDMS II Ge CombinedXENON10 2007 Projected superCDMS

Foadi, Frandsen, F.S. 08

(GeV)

10 50 100 500 1000 5000 1! 10410"45

10"44

10"43

10"42

10"41M#

$nucleon!cm"

2 "

!nucleon =µ2

4"

!Z

A

8" # dB

!2+

dM fmN

M2HM!

"2

µ = M!mN/(M! + mN )

MH = 300 GeV

dB = ±1! =3 TeV

dM = 1

Earth Based Constraints

Page 11: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Asymmetric DM Relic Density

mTB

mp! 1 TeV

1 GeV= 103

TB

B! exp

!"mTB(T !)

T !

"# 10"3 T ! ! 200 GeV

!TB

!B=

TB

B

mTB

mp! O(1)

Page 12: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

ConditionsUniverse Electric Neutrality

Chemical Equilibrium

EW Sphaleron Processes, Kuzmin-Rubakov-Shaposhnikov

TB - B violated at High Energies & approx. conserved at EW

(Extra) EW Phase Transitions

Cline, Jarvinen, F.S. 08Jarvinen, Ryttov, F.S. 09

Baryogenesis

Page 13: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Lecture 2

Phases of Gauge Theories

Gauge Theories Knobs:

Nf, Nc, Representations, Temperature, ...

Discoveries:

IR CD for low number of flavors!

Universal Structure

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Fund

2A

2S Adj

Ladder

Catterall, SanninoDel Debbio, Patella,PicaCatterall, Giedt, Sannino, SchneibleHietanen, Rummukainen, Tuominen

Iwasaki et al.

Appelquist, Fleming, NeilDeuzeman, Lombardo, Pallante

×

×

! = 1 ! = 2

Shamir, Svetitsky, DeGrand

Non-SUSY Phase Diagram Bound

Ryttov and F.S. 07

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5 6 7 8 9 100

5

10

15

20

N

Nf

A.F.B.F. & γ= 2 SD

SO(N)

SO(N) Phase Diagram

F.S. 09

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Sp(2N) Phase Diagram

F.S. 092 3 4 5 60

5

10

15

20

25

30

35

N

N Wf

A.F. B.F. & γ= 2 SD

SP(2N)

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Conformal House

Ryttov and F.S. 09

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2 Rep. ExampleSU(N) Adjoint & Fundamental Dirac Matter

010

20

Nf !F"

0.00.5

1.01.5

Nf !Adj"2

4

6

8

10

N

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Lecture 3

Minimal Walking Models

Predictions for LHC

Unification

Page 20: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Minimal Walking Technicolor

F.S. and Tuominen 04

Dietrich, F.S. Tuominen 06

Foadi, Frandsen, Ryttov, F.S. 07Cline, Jarvinen, F.S. 08

Belyaev, Foadi, Frandsen, Jarvinen, Pukhov, F.S. 08

Gudnason, Kouvaris, F.S. 06Gudnason, Ryttov, F.S. 06

Page 21: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

SU(3)

SU(2)

U(1)

U

D

Gt-up

t-down

t-glue SU(2)

NExtraNeutrino

EExtra Electron

U and D: Adj of SU(2)

Page 22: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

MWT versus EWPD

Y=-3/2 for Leptons

S

T

1 TeV

117 GeV

LEP EWG Summer 2006

100 Gev < M1 < 800 Gev

100 Gev < M2 < 1000 Gev

Page 23: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

SLeptons =16!

!1! 2Y ln

"M1

M2

#2

+1 + 8Y

20

"mZ

M1

#2

+1! 8Y

20

"mZ

M2

#2

+ O

"m4

Z

M4i

#$

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The most economical WT theory

Compatible with precision measurements

Possible DM candidates and Unification investigated

Can support 1st order Electroweak Phase Transition

Can support exotic electric charges

Lattice studies have begun

MWT Features

Page 25: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Ultra Minimal Walking TechnicolorRyttov and F.S. 08

Eichten and Lane

Page 26: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

SU(3)

SU(2)

U(1)

U

D

Gt-up

t-down

t-glue SU(2)

!2!1

t-lambda

U and D: Fund of SU(2)

t-lambdas: Adj of SU(2) Singlet of SM

Weyl Fermions

Page 27: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

The most economical “2 rep” WT theory

Smallest naive S-parameter & # of fermions

Natural DM candidate visible at LHC

Order of the Electroweak PT under investigation

Rich unexplored Collider Phenomenology

UMT Features

Page 28: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Minimal Walking Technicolor

Back to

Page 29: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

The Minimal Walking Theory

2 Adj. Dirac Flavors of SU(2)

Page 30: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

The MWT Lagrangian

What you see is “not” what LHC will see

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Heavy V/V coupling

Bare mass of the Axial

MWT effective lagrangian

L(Composites) + L(Mixing with SM) + L(New Leptons) + L(SM!Higgs)

Initial investigation we include:

Composite Higgs H

Composite Axial - Vector States R1,2

MA

Page 32: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

LHC Phenomenology

A. Belyaev R. Foadi M. T. FrandsenM. O. JarvinenA. Pukhov

In collaboration with

CalcHepBFFJPS arXiv:0809.0793

Page 33: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

An!ls and Demons of LHC

Page 34: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Comprehensive Effective Technicolor Lagrangian

Vector Mesons

Yukawas

** Link to MWT via Modified Weinberg Sum Rules **

Written in a renormalizable form

With imposed constraints from Precision Data

Foadi, Frandsen, Ryttov & F.S. 07

A working technicolor benchmark

Page 35: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Composite Higgs Signals

Associate Higgs Production BFFJPS 08, Zerwekh 05

Higgs To be done! ! !!

Page 36: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

pp! HV

Page 37: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Walking/Higher dim. rep. can allow for:

Light Composite Higgs F.S. 08 Hong, Hsu, F.S. 04 Dietrich, F.S., Tuominen 05 Doff, Natale, Rodrigues da Silva 08 Doff, Natale, 09.

Light Composite Axial Foadi, Frandsen, Ryttov F.S., 07 Eichten, Lane 07

pp! HV

Page 38: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

|!J | < 4.5, pjT > 30 GeV, |!l| < 2.5, pl

T > 15 GeV, !R(jj/jl) > .5

65 GeV < Mjj < 95 GeV

The way this event plot is done in a simple way.

1]Cross section is computed only for pp -> HW

2] Then CalcHEP adds decays of H to ZZ and on top of that it adds decay of W and ZZ to 4l and 2j.

A better way (we have not done)

pp -> WZZ. This means CalcHEP will need to compute many more diagrams. However, if we had done this fully. Once we added the cuts the results should be the same.

Why is the purple event distribution so sharp to the right.

pp! HW± !W±ZZ ! 4l + 2j

10-2

10-1

1

10

10 2

400 600 800 1000 1200

S=0.3g̃=5MH=400!s=14 TeV

M4ljj (GeV)Num

ber o

f eve

nts/

20 G

eV @

100

fb-1

10-2

10-1

1

10

10 2

400 600 800 1000 1200

S=0.3g̃=5MH=200!s=14 TeV

M4ljj (GeV)Num

ber o

f eve

nts/

20 G

eV @

100

fb-1

Page 39: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

|!J | < 4.5, pjT > 30 GeV, |!l| < 2.5, pl

T > 15 GeV, !R(jj/jl) > .5

65 GeV < Mjj < 95 GeV

10-2

10-1

1

10

10 2

400 600 800 1000 1200

S=0.3g̃=5MH=200!s=10 TeV

M4ljj (GeV)Num

ber o

f eve

nts/

20 G

eV @

10

fb-1

10-2

10-1

1

10

10 2

400 600 800 1000 1200

S=0.3g̃=5MH=400!s=10 TeV

M4ljj (GeV)Num

ber o

f eve

nts/

20 G

eV @

10

fb-1

pp! HW± !W±ZZ ! 4l + 2j

Page 40: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Further Signatures

New SM Fermions

DM candidates

Dietrich, F.S., Tuominen 05Gudnason, Ryttov & F.S. 08

Foadi, Frandsen, FS. 08Ryttov & F.S. 08Gudnason, Kouvaris & F.S. 05Kainulainen, Tuominen, Virkajarvi 06Kouvaris 07; Kouvaris, Khlopov 08

Page 41: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Unification

Farhi-Susskind, 79 Gudnason-Ryttov-F.S. 06

Page 42: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

!!1n (µ) = !!1

n (MZ)! bn

2"ln

MZ

"

BTh !b3 " b2

b2 " b1=

!!13 " !!1 sin2 "w

(1 + c2)!!1 sin2 "w " c2!!1# BExp

MGUT = MZ exp!2!

"!12 (MZ)! "!1

1 (MZ)b2 ! b1

"

Degree of SU(3)xSU(2)xU(1) Unification

1 - loop running for SU(n)

Unification Scale

Page 43: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

b3 =43Ng ! 11

b2 =43Ng !

223

+16!"#$

Higgs

b1 =35

%209

Ng +16

&=

43Ng +

110!"#$

Higgs

BTh ! 0.53 BExp ! 0.72

BTh ! 0.68 BExp ! 0.72

b3 =43Ng ! 11

b2 =43Ng !

223

+23

12

!2(2 + 1)

2+ 1

"=

43

(Ng + 1)! 223

b1 =35

!209

Ng +209

"=

43

(Ng + 1)

Standard Model

Minimal Walking Technicolor

Page 44: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of
Page 45: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Adding Adjoint SM Matter

Page 46: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Minimal Walking Technicolor + SM Adjoint Matter

Colored Octet of Majorana Particles

Weak Triplet of Majorana Fermions

Extra SM Weyl Singlet

b3 =43Ng ! 11 + 2

b2 =43!Ng + 1

"! 22

3+

43

b1 =43!Ng + 1

"

BTh = 13/18 = 0.72(2) versus BExp ! 0.72

Gudnason-Ryttov-F.S. ph/0612230

Bajc-Senjanovic ph/0612029

Page 47: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

MSSM

MWT + SM Adjoint Fermions

Zoom in MWT + SM Adjoint Fermions

Page 48: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

• Composite States: Technirho, composite (light) Higgs

• Detect Light Higgs: “Elementary or Composite ?”

• Study:

• 4th Family of Leptons no Quarks

What LHC can see and how may it deceive you

pp! HV

Page 49: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

• wino/bino/gluino-like produced. Have you seen SUSY, WTC or ... ?

• Study their couplings to SM fermions

What LHC can see and how may it deceive you

Unpleasant scenario:

• WW scatttering is unitarized at the tree level up to 4 TeV with new vectors states of about 1.5 TeV. LHC and ILC will not discover! (Foadi and FS 08)

Page 50: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

• Introduced different types of viable technicolor theories

• Phase Diagram for Gauge Theories

• Presented Minimal Walking Technicolor

• Dark Matter as a technibaryon

• Unification

Summary

Page 51: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Unifying also TC Cartoon!

Page 52: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

• (Ultra) Minimal Walking Technicolor

• Associate Production of the Composite Higgs

• Heavy Vectors are best produced and detected via Drell-Yan

Summary

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Beyond S-T-U

Burgess et al.Barbieri et al.

Page 54: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Beyond S-T-U

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Recovering S and T

Page 56: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Computing the Parameters for (Minimal) Walking Technicolor

Foadi, Frandsen, Ryttov, F.S.Foadi, Frandsen, F.S.

Page 57: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

95% confidence level error ellipsesSolid line , dashed-line , dotted one

Closest point M_A=600 GeV, Further away M_A=150 GeV. Foadi, Frandsen, F.S.

Page 58: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Custodial Technicolor

S=0

Novel Symmetry

S=0S=0

Appelquist, F.S.

Page 59: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Still Constrained

Page 60: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Low Energy Scalar Sector

Page 61: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Low Energy Vector Sector

Page 62: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of
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Higgsless versus Higgsful

Page 67: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Higgsless:

Higgsful:

Page 68: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Spectrum of Hadronic/Technihadronic States

Using ‘t Hooft Large N and Unitarity in Pion-Pion Scattering in QCD

Vector Meson is a quark-antiquark state:

Broad Sigma of multiquark nature

F.S. & Schechter, 95Harada, F.S. and Schechter, 03Caprini, Colangelo,Leutwyler 05Maiani,Piccinini, Polosa, Riquer 04F.S. and Schechter, 07

QCD is NOT higgsless!

Page 69: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Higgsless: ‘t Hooft Limit

MT! =!

2v0

F"

!3!

ND NTCm!

MTf0 =!

2v0

F"!

ND

!NTC!

3

" p!12

mf0

v0 ! 250GeV

MT!(TeV)

MTf0(TeV)

ND = 2NTC

ND =NTF

2

F.S. 07

p ! 1

3 4 5 6 7 8 90.7

0.8

0.9

1.0

1.1

1.2

1.3

1.4

Page 70: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

M_H/M_V < 1 in 2-index theories (Corrigan - Ramond Limit)

Page 71: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Signals Independent

of the

Composite Higgs

Page 72: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Drell-Yan production of heavy vectors

Vector Boson Fusion production of heavy vectors

Heavy Vectors Signals

R1,2

Page 73: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Drell Yan Production

q

q̄!

R1,2

Page 74: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Drell-Yan

1

10

10 2

10 3

10 4

500 1000 1500 2000

S=0.3g̃=2

Mll (GeV)Num

ber o

f eve

nts/

20 G

eV @

100

fb-1

1

10

10 2

10 3

10 4

500 1000 1500 2000

S=0.3g̃=5

Mll (GeV)Num

ber o

f eve

nts/

20 G

eV @

100

fb-1

√s = 14 TeV √s = 14 TeV

Page 75: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Drell-Yan

Undetectable

g̃ = 5

1

10

10 2

10 3

10 4

500 1000 1500 2000

S=0.3g̃=2!s=10 TeV

Mll (GeV)Num

ber o

f eve

nts/

20 G

eV @

10

fb-1

Page 76: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

DY visible at small due to large mixing with W/Z

At small we observe near Vector-Axial degeneracy

Stronger coupling of the technirho to fermions.

Page 77: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Drell-Yan

10-1

1

10

10 2

500 1000 1500 2000

S=0.3g̃=2

MT3l (GeV)Nu

mbe

r of e

vent

s/20

GeV

@ 1

00 fb

-1

10-1

1

10

10 2

500 1000 1500 2000

S=0.3g̃=5

MT3l (GeV)Nu

mbe

r of e

vent

s/20

GeV

@ 1

00 fb

-1

√s = 14 TeV √s = 14 TeV

Page 78: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Peaks merge at large Mass because of the inversion point.

We still see a signal at large since now R decays via WZ which grows with

Page 79: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Vector-Axial Spectrum

MA (TeV)

Mas

s Sp

ectru

m (T

eV)

R±2,0

R±1,0 S=0.3

g̃=50.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2

2.2

0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 2.2

Page 80: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Vector Resonances Branching Ratios

Mass (TeV)

BR(R

± 1)

tb

ffnl

W±Z

W±H

S=0.3g̃=5

10-6

10-5

10-4

10-3

10-2

10-1

1

0.6 0.8 1 1.2 1.4 1.6 1.8 2 2.2

Mass (TeV)

BR(R

0 1)

ff

ll

W+W-

ZH

S=0.3g̃=5

10-6

10-5

10-4

10-3

10-2

10-1

1

0.6 0.8 1 1.2 1.4 1.6 1.8 2 2.2

For light masses (Below vector/axial inversion) and large : R1 -> HV is dominant. M_H = 200 GeV.

Page 81: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

Vector Resonances Decays

M_H = 200 GeV.

Mass (TeV)

! (G

eV)

R±2

R±1

S=0.3g̃=5

10-1

1

10

10 2

10 3

0.6 0.8 1 1.2 1.4 1.6 1.8 2 2.2

Mass (TeV)

! (G

eV)

R02

R01

S=0.3g̃=5

10-1

1

10

10 2

10 3

0.6 0.8 1 1.2 1.4 1.6 1.8 2 2.2

Page 82: Conformal Dynamics from LHC to Cosmology IIIth- · Francesco Sannino Zakopane 2009 Conformal Dynamics from LHC to Cosmology III C P 3 - O r i g i n s Particle Physics & Origins of

pp! HV

MA

!(p

p "

H W

+ ) (pb

)

MH=200 GeV, S=0.3, g̃=5#s=14 TeV#s=10 TeV

10-3

10-2

10-1

1

600 800 1000 1200 1400

MA

!(p

p "

H W

+ ) (pb

)

MH=400 GeV, S=0.3, g̃=5#s=14 TeV#s=10 TeV

10-3

10-2

10-1

1

600 800 1000 1200 1400