Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics...

68
Francesco Sannino Composite Conformal Dynamics Nagoya March 2012

Transcript of Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics...

Page 1: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

September 2011

Francesco Sannino

Composite Conformal Dynamics

CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Page 2: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Atoms4%

Dark Matter22%

Dark Energy74%

??

Riddles

Page 3: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Beyond?

Theoretical blah blah blah...Carlo Rubbia

Planck Scale

Page 4: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

© Francesco Sannino

Page 5: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

๏ Gauge bosons

Spin 1

Thinking Slow

๏ FermionsSpin 1/2

๏ Graviton Spin 2

๏ Dark matter sector ๏ Inflationary sector? ?

Page 6: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Lorentz Group basics

๏ Lorentz group is SL(2, C)

๏ Spin 1/2 is the fund. representation

๏ All other spins are derived

๏ No need for fund. scalars

Supersymmetry is an emergent theory

What about Supersymmetry?

See for example Antipin, Mojaza, Pica and Sannino arXiv:1105.1510

Page 7: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

SM - GeometrySU(3)

SU(2)L

U(1)⊂SU(2)R

U (1)Q

SU(3)

<H>

Higgs

L-Leptons

R-Quarks

Weak GBGluons

R-Leptons

L-Quarks

Hyper - GB

Branish

Higgs Sector

Page 8: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

M2H = 2� v2

Fermi Scale

Page 9: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Natural SM mass spectrum

MH = �p2 v ⇡ � 345 GeV

mf = �fvp2⇡ �f 174 GeV

MW = gv

2⇡ g 123 GeV

Top has the right energy scale!

Light quarks and leptons are odd!

Page 10: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

O’ Higgs, where art thou!

Page 11: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Light Higgs Anatomy

pp ! WW ⇤ ! `+⌫`0�⌫0 4.7fb�1no excess R = 0.16+0.6

�0.6@126GeV

pp ! �� 4.9fb�1 mH = 126.5 ± 0.7 GeV R = 2+0.9�0.7

pp ! ZZ⇤ ! `+`�`0�`0+ 4.8fb�1 mH = 126± 2 GeV R = 1.2+1.2�0.8

Page 12: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Light Higgs Anatomy cont.pp ! �� 4.8fb�1 mH = 125 GeV R = 1.65+0.67

�0.6

pp ! WW ⇤ ! `+⌫`0�⌫0 4.6fb�1no excess R = 0.4+0.6

�0.55@126GeV

pp ! ZZ⇤ ! `+`�`0�`0+ 4.7fb�1 mH = 125± 2 GeV R = 0.58+1.0�0.58

H ! bb 10/9.7 fb�1 mH = 115� 135 GeV R = 1.6+0.6�0.6@120 GeV

Page 13: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

What if Higgs-like state is there?

“Higgs” @ 125 GeV vs unitarity scale:

MH

1.2 TeV' 0.1

MH

4⇡v' 0.04

๏ Mass of the “Higgs” versus EW ChPT convergence radius scale:

๏ Compare with mass of the pion versus ChPT convergence radius:

M⇡

4⇡F⇡' 0.1 Goldstone

Conformal Goldstone

Page 14: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Conformal Goldstone

๏ Spontaneous breaking of scale (conformal) symmetry

@µDµ = ⇥µ

µ =X

i

�(gi)@L@gi

๏ Dilaton mass and decay constant

hD|@µDµ|0i = �fDm2D

๏ In near-conformal technicolor like models

fD = v mD = MH

Page 15: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

LHC Higgs “potential” discovery

๏ Would imply

mD ⌧ 4⇡fD , mD < fD

๏ For comparison in QCD

M⇡ ⌧ 4⇡F⇡ , M⇡ ' F⇡

๏ What kind of models can do this?

fD = v mD = MH

Page 16: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Near Conformal Models

critical exponent⌫

N cf critical number of techniflavors for conformality

๏ Other examples?Calculable perturbative examples

Antipin, Mojaza, Sannino 1107.2932

๏ Conformal technicolor models (Light Composite Higgs)

MH

v' (N c

f �Nf )⌫ Dietrich, Sannino, Tuominen hep-ph/0510217

Dietrich, Sannino hep-ph/0611341

Grinstein, Uttayarat 1105.2370

Page 17: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Technicolor - Geometry

U (1)Q

SU(3)SU(3)

SU(2)L

U(1)⊂SU(2)R

TC

< Q Q>_

R-TQuarks

L-TQuarks

Technicolor

Page 18: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Dots are partially fixed by Anomalies as well as other principles

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q�µDµQ + · · ·

· · · ⇥ L(New SM Fermions)

Dynamical EW Breaking

Page 19: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Wanted!

๏ Minimal Technicolor passing precision tests

๏ ETC for Fermion masses generation

๏ Non QCD dynamics/Walking

๏ Large mass anomalous dimensions ?

๏ Dark matter candidates

Page 20: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

iWalk

© Francesco Sannino

Page 21: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

No seriously, Walking?

How can one tune an integer number?

Anomalous dimensions may be small

© Francesco Sannino

Dietrich Sannino 06Fukano & Sannino 10

Page 22: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

ideal Walking = iWalkFukano & Sannino 10

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q�µDµQ + · · ·

© Francesco Sannino

Appelquist, Soldate, Takeuchi and Wijewardhana, 88Miranky and Yamawaki 88Kondo, Mino, Yamawaki 89Takeuchi 96Yamawaki, Kurachi and Shrock 08

Page 23: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Gauged Nambu Jona-Lasinio

As if the number of flavors is continuous

Anomalous dimensions increase

2 3 4 5 6 7 8 9 100

5

10

15

20

N

Nf

Fukano & Sannino 10� ' 1.73

Phenomenologically viable

Being tested!

Fukano & Sannino 10

© Francesco Sannino

Page 24: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Discovering Working Technicolor

Page 25: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Tevatron

Consistency of the theory

YW

CMS Data �1⇥5 fb�1, 3 ⇥5 fb�1, 5 ⇥13 TeV, 100 fb�1, 3 ⇥13 TeV, 100 fb�1, 5 ⇥

0.5 1.0 1.5 2.0 2.5

2

4

6

8

10

12

MA ⇤TeV⌅

g⇤Walking

Running

Andersen, Hapola, Sannino 11Belyaev, Foad, Frandsen, Jarvinen, Pukhov, Sannino 08

Much unexplored !

Page 26: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Need to go beyond QCD

Page 27: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Gauge Group, i.e. SU, SO, SP

Matter Representation

# of Flavors per Representation

Knobs

NfQCD IR Conformal Infrared free

?

Page 28: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

α

Energy

Interesting structure at large Nf

A novel phase @ large Nf

NfQCD IR Conformal Asymp. Safe

First coefficients at large Nf are knownPica & Sannino 10

�UV =3⇥

TFNf

Ciuchini, Derkachov, Gracey, Manashov ‘99

Page 29: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

1 2 3 4 x

-14

-12

-10

-8

-6HHxL

Ciuchini, Derkachov, Gracey, Manashov ‘99

A novel phase @ large Nf

Pica & Sannino 10

�UV =3⇥

TFNf

B. Holdom, 2010

Page 30: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Perturbation theory

Page 31: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Nf

N

ElectricPerturbative region

Page 32: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

da

d lnµ2= �(a) = ��0a

2 � �1a3 � �2a

4 � �3a5 +O(a6) ,

� d lnm

d lnµ2=

�(a)

2= �0a+ �1a

2 + �2a3 + �3a

4 +O(a5) ,

Low Energy Effective TheoryFour loops

Van Ritbergen, Vermaseren, Larin 97Vermaseren, Larin, Van Ritbergen, 97

a =↵

4⇡=

g2

16⇡2

Mojaza, Pica, Sannino 10

Generalized 4th order Casimirs for SU(N), SO(N) and SP(N)

Page 33: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Low Energy Effective TheoryZero’s - Dynamics

Page 34: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

4 - loop Zerology

a⇤ =2

⇡arctan (5a) Pica, Sannino 10

Page 35: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

4 - Zerology

SU(2), SU(3) SU(4) - SU(11)

SU(>11)

FUNDAMENTAL

SU(>1)

ADJOINT

Page 36: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

�(↵) =@↵

@↵�(↵) ,

�(↵) = �(↵)� �(↵)@ln zm@↵

�0 , �0 and �1 are universal

↵ =1X

n=1

hn↵n , with h1 = 1 ,

m = mzm (↵) = m1X

n=0

`n↵n , with `0 = 1

FP Ɣ is physical

Page 37: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

0.4 0.5 0.6 0.7 0.8 0.9 1.0

-0.5

0.0

0.5

1.0

1.5

nfn f

gƔ - Fundamental

3-loops

4-loops

All ordersPica - Sannino 10Ryttov - Sannino 07

2-loops

Ryttov, Shrock 10

Pica, Sannino 10

Page 38: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

0.4 0.5 0.6 0.7 0.8 0.9 1.0

0.5

1.0

1.5

nfn f

g

Ɣ - Minimal Walking

2-loops

3-loops

4-loops

All ordersPica - Sannino 10Ryttov - Sannino 07

Pica, Sannino 10Ryttov, Shrock 10

Page 39: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Universal Picture

Page 40: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

SU(N)

2 3 4 5 6 7 8

2

4

6

8

10

12

14

16

18

N

n f

Fund

A-Sym

Sym

Adj

Ryttov & Sannino 07Dietrich & Sannino 07Sannino & Tuominen 04

Ryttov & Shrock 10

Very interesitng

Poppitz & Unsal 9, 10

Pica & Sannino 10

SU(N) Phase Diagram

Page 41: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

A Perturbative Dilaton ModelO. Antipin, M. Mojaza, F. Sannino - hep-ph/1107.2932

L = �1

2TrF 2 +

NfX

j

i j /D j

+yH iHij j + h.c.+Tr |@µH|2 � u1

�TrH†H

�2 � u2Tr�H†H

�2

+i�a�µDabµ �

b

QCD-like Adjoint fermion

Higgs-sector ~ Mesons

Gauge-gauge (EM) duality & the Standard Model Mojaza et al. (hep-th/1101.1522) and Sannino (hep-th/1102.5100)

H ⇠

Spectrum extremely close to the wanted one!

Page 42: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Infrared physics

Perturbative IR stable fixed point (a la Banks-Zaks)

{g⇤2, y⇤H2, u⇤

1, u⇤2} ⇠ ✏

Nf/Nc ⌘ x = xAF(1� ✏) < xAF

-0.4 -0.2 0.0 0.2

0.00

0.05

0.10

0.15

0.20

0.25

0.30

z1

z 2

g ⇡ g⇤ , yH ⇡ y⇤Hu1

u2

IR conformal or?

L = LK(Fµ⌫ ,�, , H; g) + yH H � u1

�TrH†H

�2 � u2Tr�H†H

�2

Page 43: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Spontaneous symmetry breaking

H. Yamagishi, 1980Coleman-Weinberg mechanism

Hcij = �c�ij

dV RGe↵

dµ=

µ

@

@µ+X

i

�(gi)@

@gi+ ���c

@

@�c

!V RGe↵ = 0

L = LK(Fµ⌫ ,�, , H; g) +r

aHNf

H � z1N2

f

�TrH†H

�2 � z2Nf

Tr�H†H

�2

Page 44: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

The Light Dilaton

-0.4 -0.2 0.0 0.20.00

0.05

0.10

0.15

0.20

0.25

0.30

z1

z 2

g ⇡ g⇤ , yH ⇡ y⇤H

separatrixV RGe↵

0(�c) = 0

V

RGe↵

00(�c) = 0 )

m

(1)

2 / 4z22 � xaH = 0IR Conformal

�SB

V RGe↵ (�c) = 0

� 4z22 � xaH = � smallarbitrarily light by tuning:

Page 45: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Is it the Dilaton?

@µDµ = ⇥µ

µ =X

i

�(gi)@L@gi

hD|@µDµ|0i = �fDm2D

⇥µµ / (�1 + �2)�+ · · · since �(g),�(yH) ⇡ 0 at µ0

�(µ0) . ✏

Page 46: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

g

g*

The Complete Picture

µ

g*

IR Conformal

Walking �(g)

µ

g

m ⇤SYM

h��i = � 9

32⇡2⇤3SYM ⇤

2SYM = v2

✓3

11✏

◆2/3

exp

✓� 6

22✏

◆.

�(µ0) < 0

�(µ0) > 0

�SB - , H decoupling

Super-Yang Mills

Walking Dynamics

Page 47: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Full Spectrum of Broken Phase

µ

Mass eigenstates of quarks and mesons

Hij ⇡ (�c + �+ i⇡0)�ij + haT aij + i⇡aT a

ij , a = 1, . . . N2f � 1

µm2 ⇠ m2

h ⇠ ✏m2d ⇠ �✏m2

SYM ⇠ e�1/✏m2NGB = 0

1N2f 4NfNc + (N2

f � 1)4(N2c � 1)

EWHiggsDM

Page 48: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Minimal Working TC

UD

Minimal WT

Next to MWT

Orthogonal

SU(2)TC

SU(3)TC

SO(4)TC

Ultra MTSU(2)TC

NE

Frandsen, Sannino 09

Ryttov & Sannino 08

Sannino & Tuominen 04Dietrich, Sannino, Tuominen 05

Dietrich, Sannino, Tuominen 05

Sannino, Tuominen 04UD

UD

UD

Frandsen, Masina, Sannino 09

Vanilla TC

Page 49: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Minimal Walking Technicolor

Page 50: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Extra Electron SU(3)

SU(2)

U(1)

U

D

Gt-up

t-down

t-glue SU(2)

NExtraNeutrino

U and D: Adj of SU(2)

F.S. + Tuominen 04Dietrich, F.S., Tuominen 05

Page 51: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

S = S(W )TC + SNS

Offset the first term

S beyond TC...

Page 52: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

New Leptons & Precision Data

1 TeV

117 GeV

300 GeV

Exotic Leptonic hypercharge Y=-3/2 Standard Model Leptonic hypercharge

Page 53: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Conclusions

๏ DEWSB can naturally occur at the LHC

๏ Phase Diagram of strongly interacting theories

๏ Minimal models of technicolor

๏ Composite Dark Matter and Inflation (... another time)

Page 54: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

MWT Features

๏ The most economical WT theory

๏ Compatible with precision measurements

๏ Possible DM candidates

๏ Light Composite Higgs

๏ Under investigation on the Lattice

Page 55: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Composite Higgs H

Composite Axial - Vector States

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

R1,2

MWT Effective Lagrangian

Heavy Electron

2 Heavy Majoranas N1 N2

Frandsen, Masina, Sannino 09

Hapola, Masina, Sannino 11 Foadi, Frandsen, Ryttov & F.S. 07

Page 56: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Tevatron

Consistency of the theory

YW

CMS Data �1⇥5 fb�1, 3 ⇥5 fb�1, 5 ⇥13 TeV, 100 fb�1, 3 ⇥13 TeV, 100 fb�1, 5 ⇥

0.5 1.0 1.5 2.0 2.5

2

4

6

8

10

12

MA ⇤TeV⌅

g⇤

Walking

Running

Constraining MWT

Andersen, Hapola, Sannino 11Belyaev, Foad, Frandsen, Jarvinen, Pukhov, Sannino 08

Page 57: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Conclusions

๏ DEWSB can naturally occur at the LHC

๏ Phase Diagram of strongly interacting theories

๏ Minimal models of technicolor

๏ Composite Dark Matter

๏ Composite inflation.

Page 58: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Back - up

© Francesco Sannino

Page 59: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Atoms4%

Dark Matter22%

Dark Energy74%

Dark Matter

�DM

�B� 5

Francesco Sannino

Page 60: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

�B DM asymmetry

A particle similar to the nucleon

Electrically neutral

At most EW-type cross sections

Great if connected to EW (Observable at LHC)

Page 61: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Puzzle

7.5 8.0 8.5 9.010-42

10-41

10-40

10-39

Mf in GeV

spincm

2 CoGeNT

DAMA

Xenon 100Xenon 10

CDMS

Page 62: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Higgs

Del Nobile, Kouvaris, Sannino 11

DarkMatter

DarkMatter

+ �

Quantum Mechanics

Page 63: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Interfering Composite ADM

CoGeNT and DAMA Del Nobile, Kouvaris, Sannino 11

7.5 8.0 8.5 9.0

10-38

10-37

Mf in GeV

spincm

2 CoGeNT

DAMA

Xenon 100Xenon 10CDMS

Chang et al. 2010, Feng et al, 2011, Frandsen et al. 2011

Page 64: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

What makes DM?

Atoms4%

Dark Matter22%

?Francesco Sannino

Composite

???

DM Particle

Elementary

Oversimplification

Page 65: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Composite Dark Matter

TIMPs Masses Annih. Asymm Symm Models

TC-Baryon (1 - 3) TeV - X -Complex-RepTraditional TC

TC-PGB 5 GeV - .5 TeV X X X(Pseudo)-Real

(UMT, MWT, OT)

Unbaryon (1 - 10) GeV X X X Techni-unparticle

(Un)TC Interact. Massive Particle (u)TIMP

TC-PGB Ryttov - Sannino 08Frandsen & Sannino. 09

Gudnason - Kouvaris - Sannino. 06

TC-Baryon

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

Nardi, Sannino., Strumia, 08.Foadi, Frandsen, Sannino 09

Sannino, 10Related Kouvaris 06,07,10Kainulainen, Virkajarvi, Tuominen 06,09,10

Belyaev, Frandsen, Sannino, Sarkar 10

Mixed TIMP DM

Unbaryon Sannino, Zwicky 09Frandsen, Sarkar, 10

D.B. Kaplan 92

Page 66: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

�TB

�B=

TB

B

mTB

mp� O(1)

DM and GUTs

� ⇠ M4GUT

m5TB

⇠ 1026sec

GUTs

� ⇠ M4GUT

m5TB

⇠ 3⇥ 1037sec

Nardi, FS, Strumia, 08.

Gudnason, Ryttov, FS 06

TB

B� O(1)

Light

mTB ⇠ 5 GeV

TB

B⇡ exp

h�mTB

T ⇤

i

Heavy

mTB ⇡ (1� 3) TeV

Francesco Sannino

Page 67: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

Not the Coldplay album

New life in Technicolor

Page 68: Francesco Sannino€¦ · September 2011 Francesco Sannino Composite Conformal Dynamics CP3-DESY-Goettingen School 11-14 October 2011Nagoya March 2012

�B The model

L = �1

2TrF 2

+

NfX

j

i j /D j

+yH iHij j + h.c.