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