dynamical electroweak breaking @ lhcconsistency of the theory yw cms data 1 5 fb1, 3 5 fb1, 5 13...

September 2011

Francesco Sannino

Composite Dynamics

CP3-DESY-Goettingen School 11-14 October 2011Vienna - November 25 - 2011

Francesco Sannino

Riddles

Atoms4%

Dark Matter22%

Dark Energy74%

Francesco Sannino

Riddles

Atoms4%

Dark Matter22%

Dark Energy74%

Francesco Sannino

Riddles

Atoms4%

Dark Matter22%

Dark Energy74%

Francesco Sannino

Riddles

Atoms4%

Dark Matter22%

Dark Energy74%

?Francesco Sannino

Riddles

Atoms4%

Dark Matter22%

Dark Energy74%

??Francesco Sannino

Riddles

Francesco Sannino

Standard Model

SM

Francesco Sannino

Standard Model

SM - GeometrySU(3)

SU(2)L

U(1)⊂SU(2)R

L-Leptons

R-Quarks

Weak GBGluons

R-Leptons

L-Quarks

Hyper - GBFrancesco Sannino

SM - GeometrySU(3)

SU(2)L

U(1)⊂SU(2)R

Higgs

L-Leptons

R-Quarks

Weak GBGluons

R-Leptons

L-Quarks

Hyper - GB

Higgs Sector

Francesco Sannino

SM - GeometrySU(3)

SU(2)L

U(1)⊂SU(2)R

<H>

Higgs

L-Leptons

R-Quarks

Weak GBGluons

R-Leptons

L-Quarks

Hyper - GB

Higgs Sector

Francesco Sannino

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

Higgs Sector

Francesco Sannino

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

Francesco Sannino

O’ Higgs, where art thou!

© Francesco Sannino

© Francesco Sannino

MSSM Status

© Francesco Sannino

© Francesco Sannino

MSUGRA/CMSSM = five parameters: the universal scalar mass m0, gaugino mass m1/2, the trilinear scalar coupling A0, tan β: the ratio of the VEV of the two Higgses the sign of the higgsino mass parameter μ.

ATLAS Experiment © 2011 CERN

ATLAS Experiment © 2011 CERN

What else has LHC not seen ?

© Francesco Sannino

ATLAS Experiment © 2011 CERN

What about Technicolor ?

© Francesco Sannino

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

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 !

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 !

Technicolor - Geometry

SU(3)

SU(2)L

U(1)⊂SU(2)R

Francesco Sannino

Technicolor - Geometry

SU(3)

SU(2)L

U(1)⊂SU(2)R

TC

R-TQuarks

L-TQuarks

Technicolor

Francesco Sannino

Technicolor - Geometry

SU(3)

SU(2)L

U(1)⊂SU(2)R

TC

< Q Q>_

R-TQuarks

L-TQuarks

Technicolor

Francesco Sannino

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

Francesco Sannino

Dynamical EW Breaking

Francesco Sannino

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q̄�µDµQ + · · ·

Dynamical EW Breaking

Francesco Sannino

Dots are partially fixed by Anomalies as well as other principles

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q̄�µDµQ + · · ·

Dynamical EW Breaking

Francesco Sannino

Dots are partially fixed by Anomalies as well as other principles

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q̄�µDµQ + · · ·

· · · ⇥ L(New SM Fermions)

Dynamical EW Breaking

Francesco Sannino

-0.2 0.0 0.2 0.4-0.1

0.0

0.1

0.2

0.3

0.4

0.5

S

T

SU(3) + 1 Fund. Doublet Weinberg, Susskind1 TeV

Large & Positive S from QCD-like Technicolor

Need novel dynamics

SM Fermion Masses

Francesco Sannino

L̄ · HeR ⇥ L̄Q̄Q

�2ETC

eR

Extending Technicolor

Francesco Sannino

Different Approaches

Francesco Sannino

Scalar-less New Gauge Interactions (Extended TC)

Different Approaches

Francesco Sannino

Scalar-less New Gauge Interactions (Extended TC)

Marry SUSY and Technicolor

Different Approaches

Francesco Sannino

Scalar-less New Gauge Interactions (Extended TC)

Marry SUSY and Technicolor

Add New Scalars in the Flavor Sector

Different Approaches

Francesco Sannino

Scalar-less New Gauge Interactions (Extended TC)

Marry SUSY and Technicolor

Add New Scalars in the Flavor Sector

.....

Different Approaches

Francesco Sannino

Naive Extended Technicolor

Eichten & Lane 80

Francesco Sannino

Naive Extended Technicolor

Eichten & Lane 80

Recent investigationsRyttov & Shrock 10

Francesco Sannino

Naive Extended Technicolor

Eichten & Lane 80

Recent investigationsRyttov & Shrock 10

Francesco Sannino

PNGMasses

Naive Extended Technicolor

Eichten & Lane 80

Recent investigationsRyttov & Shrock 10

Francesco Sannino

PNGMasses

SM-FermionMasses

Naive Extended Technicolor

Eichten & Lane 80

Recent investigationsRyttov & Shrock 10

Francesco Sannino

PNGMasses

SM-FermionMasses

FCNCOperators

Naive Extended Technicolor

Eichten & Lane 80

Recent investigationsRyttov & Shrock 10

Francesco Sannino

PNGMasses

SM-FermionMasses

FCNCOperators

Naive Extended Technicolor

Modifies TC dynamics

Eichten & Lane 80

Recent investigationsRyttov & Shrock 10

Francesco Sannino

PNGMasses

SM-FermionMasses

FCNCOperators

Naive Extended Technicolor

Modifies TC dynamics

Eichten & Lane 80

Recent investigationsRyttov & Shrock 10

Francesco Sannino

Antola, Di Chira, Sannino, Tuominen 10,11

Francesco Sannino

mf �g2

ETC

�2ETC

< Q̄Q >ETC⇤ETC

Francesco Sannino

mf �g2

ETC

�2ETC

< Q̄Q >ETC⇤ETC

⇤TC Electroweak breaks

Francesco Sannino

mf �g2

ETC

�2ETC

< Q̄Q >ETC⇤ETC

⇤TC Electroweak breaks

< Q̄Q >ETC ⇥< Q̄Q >TC � �3TC

Francesco Sannino

mf �g2

ETC

�2ETC

< Q̄Q >ETC⇤ETC

⇤TC

mf �g2

ETC

�2ETC

< Q̄Q >ETC ⇥ mTop

Electroweak breaks

< Q̄Q >ETC ⇥< Q̄Q >TC � �3TC

Francesco Sannino

Need to go beyond QCD

Francesco Sannino

Near Conformal

Francesco Sannino

Near Conformal

UVIR

Francesco Sannino

Near Conformal

UVIR

IR Conformal behavior

Francesco Sannino

Near Conformal

UVIR

IR Conformal behavior

Francesco Sannino

Why walking helps?

Francesco Sannino

QCD-Like

~

Why walking helps?

Francesco Sannino

QCD-Like

Near the conformal window

~

~

Why walking helps?

Francesco Sannino

QCD-Like

Near the conformal window

~

~

Why walking helps?

Francesco Sannino

mf �g2

ETC

�2ETC

< Q̄Q >ETC=g2

ETC

�2ETC

��ETC

�TC

⇥⇥m(��)

< Q̄Q >TC

If large anomalous dimension, around ⇥m(�⇤) ⇠ 1.7

Francesco Sannino

mf �g2

ETC

�2ETC

< Q̄Q >ETC=g2

ETC

�2ETC

��ETC

�TC

⇥⇥m(��)

< Q̄Q >TC

If large anomalous dimension, around ⇥m(�⇤) ⇠ 1.7

Francesco Sannino

mf �g2

ETC

�2ETC

< Q̄Q >ETC=g2

ETC

�2ETC

��ETC

�TC

⇥⇥m(��)

< Q̄Q >TC

If large anomalous dimension, around ⇥m(�⇤) ⇠ 1.7

Fermion Mass Enhancement & FCNC decoupling

Francesco Sannino

Ingredients

Francesco Sannino

๏ Understand Phase Diagram of gauge theories

๏ Understand Phase Diagram of gauge theories

๏ Walking: Is it really phenomenologically viable?

๏ Understand Phase Diagram of gauge theories

๏ Walking: Is it really phenomenologically viable?

๏ Need a working example of ETC

Phase diagram

Francesco Sannino

Knobs

Francesco Sannino

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

Knobs

Francesco Sannino

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

Matter Representation

Knobs

Francesco Sannino

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

Matter Representation

# of Flavors per Representation

Knobs

Francesco Sannino

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

Matter Representation

# of Flavors per Representation

Knobs

Nf

Francesco Sannino

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

Matter Representation

# of Flavors per Representation

Knobs

NfQCD

Francesco Sannino

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

Matter Representation

# of Flavors per Representation

Knobs

NfQCD IR Conformal

Francesco Sannino

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

Matter Representation

# of Flavors per Representation

Knobs

NfQCD IR Conformal Infrared free

Francesco Sannino

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

Matter Representation

# of Flavors per Representation

Knobs

NfQCD IR Conformal Infrared free

Francesco Sannino

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

Matter Representation

# of Flavors per Representation

Knobs

NfQCD IR Conformal Infrared free

Francesco Sannino

?

A novel phase @ large Nf

NfQCD IR Conformal

Francesco Sannino

Pica & Sannino 10

Interesting structure at large Nf

A novel phase @ large Nf

NfQCD IR Conformal

Francesco Sannino

Pica & Sannino 10

Interesting structure at large Nf

A novel phase @ large Nf

NfQCD IR Conformal

Francesco Sannino

Entire series at large Nf is known

Pica & Sannino 10

α

Energy

Interesting structure at large Nf

A novel phase @ large Nf

NfQCD IR Conformal Asymp. Safe

Francesco Sannino

Entire series at large Nf is known

Pica & Sannino 10

α

Energy

Interesting structure at large Nf

A novel phase @ large Nf

NfQCD IR Conformal Asymp. Safe

Francesco Sannino

Entire series at large Nf is known

Pica & Sannino 10

�UV =3⇥

TFNf

Universal Picture

Francesco Sannino

Fund

2A

2S

Adj

Ladder

Ryttov & Sannino 07

SU(N) Phase Diagram

Dietrich & Sannino 07

Sannino & Tuominen 04

Pica & Sannino 10

Francesco Sannino

Fund

2A

2S

Adj

Ladder

Ryttov & Sannino 07

SU(N) Phase Diagram

Dietrich & Sannino 07

Sannino & Tuominen 04

Pica & Sannino 10

Francesco Sannino

Fund

2A

2S

Adj

Ladder

Ryttov & Sannino 07

SU(N) Phase Diagram

Dietrich & Sannino 07

Sannino & Tuominen 04

Pica & Sannino 10

Francesco Sannino

Fund

2A

2S

Adj

Ladder

Ryttov & Sannino 07

SU(N) Phase Diagram

Dietrich & Sannino 07

Sannino & Tuominen 04

Pica & Sannino 10

Francesco Sannino

Very interesitng

Lattice SU(N) Phase Diagram

Fund

2A

2SAdj

�SD ' 1�PS = 1

�PS = 0.5

iWalk

© Francesco Sannino

iWalk = ideal Walking

© Francesco Sannino

Dietrich Sannino 06Fukano & Sannino 10

iWalk = ideal Walking

Walking is fine tuned

© Francesco Sannino

Dietrich Sannino 06Fukano & Sannino 10

iWalk = ideal Walking

Walking is fine tuned

Anomalous dimensions may be small

© Francesco Sannino

Dietrich Sannino 06Fukano & Sannino 10

iWalkFukano & Sannino 10

© Francesco Sannino

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

iWalkFukano & Sannino 10

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q̄�µDµQ + · · ·

© Francesco Sannino

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

iWalkFukano & Sannino 10

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q̄�µDµQ + · · ·

© Francesco Sannino

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

iWalkFukano & Sannino 10

L(H)⇤ �14F aµ⇥F a

µ⇥ + i Q̄�µDµQ + · · ·

© Francesco Sannino

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

Gauged Nambu Jona-Lasinio

2 3 4 5 6 7 8 9 100

5

10

15

20

N

Nf

Fukano & Sannino 10� ' 1.73

Fukano & Sannino 10

© Francesco Sannino

Gauged Nambu Jona-Lasinio

As if the number of flavors is continuous

2 3 4 5 6 7 8 9 100

5

10

15

20

N

Nf

Fukano & Sannino 10� ' 1.73

Fukano & Sannino 10

© Francesco Sannino

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

Fukano & Sannino 10

© Francesco Sannino

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

Fukano & Sannino 10

© Francesco Sannino

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

Minimal Working TC

UD

Francesco Sannino

Minimal Working TC

UD

Minimal WT

SU(2)TCNE

Sannino & Tuominen 04

Dietrich, Sannino, Tuominen 05

Frandsen, Masina, Sannino 09

Francesco Sannino

Minimal Working TC

UD

Minimal WT

Next to MWT

SU(2)TC

SU(3)TC

NE

Sannino & Tuominen 04

Dietrich, Sannino, Tuominen 05

Dietrich, Sannino, Tuominen 05

Sannino, Tuominen 04UD

Frandsen, Masina, Sannino 09

Francesco Sannino

Minimal Working TC

UD

Minimal WT

Next to MWT

Orthogonal

SU(2)TC

SU(3)TC

SO(4)TC

NE

Frandsen, Sannino 09

Sannino & Tuominen 04

Dietrich, Sannino, Tuominen 05

Dietrich, Sannino, Tuominen 05

Sannino, Tuominen 04UD

UD

Frandsen, Masina, Sannino 09

Francesco Sannino

Minimal Working TC

UD

Minimal WT

Next to MWT

Orthogonal

SU(2)TC

SU(3)TC

SO(4)TC

Ultra MT

SU(2)TC

NE

Frandsen, Sannino 09

Ryttov & Sannino 08

Sannino & Tuominen 04

Dietrich, Sannino, Tuominen 05

Dietrich, Sannino, Tuominen 05

Sannino, Tuominen 04UD

UD

UD

Frandsen, Masina, Sannino 09

Francesco Sannino

Vanilla TC

Minimal Walking Technicolor

SU(3)

SU(2)

U(1)

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

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

⇣

S beyond TC...

S = S(W )TC + SNS

S beyond TC...

S = S(W )TC + SNS

S beyond TC...

S = S(W )TC + SNS

Offset the first term

S beyond TC...

New Leptons & Precision Data

1 TeV

117 GeV

300 GeV

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

MWT Features

MWT Features

๏ The most economical WT theory

MWT Features

๏ The most economical WT theory

๏ Compatible with precision measurements

MWT Features

๏ The most economical WT theory

๏ Compatible with precision measurements

๏ Possible DM candidates

MWT Features

๏ The most economical WT theory

๏ Compatible with precision measurements

๏ Possible DM candidates

๏ Under investigation on the Lattice

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

MWT Effective Lagrangian

Foadi, Frandsen, Ryttov & F.S. 07

Composite Higgs H

Composite Axial - Vector States

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

R1,2

MWT Effective Lagrangian

Foadi, Frandsen, Ryttov & F.S. 07

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

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

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

Dark Matter

Francesco Sannino

Atoms4%

Dark Matter22%Dark Energy

74%

Dark Matter

Francesco Sannino

Atoms4%

Dark Matter22%Dark Energy

74%

Dark Matter

�DM

�B� 5

Francesco Sannino

What makes DM?

Atoms4%

Dark Matter22%

Francesco Sannino

What makes DM?

Atoms4%

Dark Matter22%

?Francesco Sannino

What makes DM?

Atoms4%

Dark Matter22%

?Francesco Sannino

???

DM Particle

What makes DM?

Atoms4%

Dark Matter22%

?Francesco Sannino

???

DM Particle

Elementary

What makes DM?

Atoms4%

Dark Matter22%

?Francesco Sannino

Composite

???

DM Particle

Elementary

What makes DM?

Atoms4%

Dark Matter22%

?Francesco Sannino

Composite

???

DM Particle

Elementary

Oversimplification

�B DM asymmetry

�B DM asymmetry

A particle similar to the nucleon

�B DM asymmetry

A particle similar to the nucleon

Electrically neutral

�B DM asymmetry

A particle similar to the nucleon

Electrically neutral

At most EW-type cross sections

�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)

Composite Dark Matter (Un)TC Interact. Massive Particle (u)TIMP

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

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

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

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

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

DM and GUTs

Francesco Sannino

�TB

�B=

TB

B

mTB

mp� O(1)

DM and GUTs

Francesco Sannino

�TB

�B=

TB

B

mTB

mp� O(1)

DM and GUTs

TB

B� O(1)

Light

mTB ⇠ 5 GeV

Francesco Sannino

�TB

�B=

TB

B

mTB

mp� O(1)

DM and GUTs

TB

B� O(1)

Light

mTB ⇠ 5 GeV

TB

B⇡ exp

h�mTB

T ⇤

i

Heavy

mTB ⇡ (1� 3) TeV

Francesco Sannino

�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

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

Higgs

Del Nobile, Kouvaris, Sannino 11

DarkMatter

DarkMatter

+ �

Quantum Mechanics

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

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

Conclusions

๏ DEWSB can naturally occur at the LHC

Conclusions

๏ DEWSB can naturally occur at the LHC

๏ Phase Diagram of strongly interacting theories

Conclusions

๏ DEWSB can naturally occur at the LHC

๏ Phase Diagram of strongly interacting theories

๏ Minimal models of technicolor

Conclusions

๏ DEWSB can naturally occur at the LHC

๏ Phase Diagram of strongly interacting theories

๏ Minimal models of technicolor

๏ Composite Dark Matter

Conclusions

๏ DEWSB can naturally occur at the LHC

๏ Phase Diagram of strongly interacting theories

๏ Minimal models of technicolor

๏ Composite Dark Matter

๏ Composite inflation... another time

Conclusions