New physics, Observables, and Quantum Field Theory

New physics, Observables, and Quantum Field Theory Axel Maas 13th of March 2015 Institute of High Energy Physics Vienna Austria Overview ● ● Setti...
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New physics, Observables, and Quantum Field Theory Axel Maas 13th of March 2015 Institute of High Energy Physics Vienna Austria

Overview ●



Setting the scene Why to wonder about seeing the W/Z and the Higgs



Resolving the paradox



Confirming the resolution



Implications for new Physics



Summary

Short version: 1502.02421

Main messages

Main messages ●

For theory ●





That perturbation theory works in the standard model is not trivial That it works can be explained using field theory It does not need to work beyond-thestandard model

Main messages ●

For theory ●







That perturbation theory works in the standard model is not trivial That it works can be explained using field theory It does not need to work beyond-thestandard model

For experiment ●



Predictions for new physics signatures may be too optimistic Theories can be better constrained/falsified

What is non-perturbative? ●

Standard statement: When couplings are small/weak enough everything is perturbative

What is non-perturbative? ●



Standard statement: When couplings are small/weak enough everything is perturbative Strong interactions are non-perturbative ●

Like QCD

What is non-perturbative? ●



Standard statement: When couplings are small/weak enough everything is perturbative Strong interactions are non-perturbative ●



Like QCD

But not entirely true: Weak interactions can be non-perturbative ●



QED is weakly interacting, but has nonperturbative features like atoms, molecules, matter with phase structure,... Bound states, phase transitions,...

What is non-perturbative? ●



Standard statement: When couplings are small/weak enough everything is perturbative Strong interactions are non-perturbative ●



But not entirely true: Weak interactions can be non-perturbative ●





Like QCD

QED is weakly interacting, but has nonperturbative features like atoms, molecules, matter with phase structure,... Bound states, phase transitions,...

Are there (relevant) non-perturbative effects at the electroweak scale?

Setting the scene

Standard model



Particles can be grouped according to the forces

Standard model



Electromagnetic sector u

c

t

d

s

b

e







Particles can be grouped according to the forces ●

Electromagnetic sector (QED)

Standard model



Strong sector

Electromagnetic sector g

u

c

t

d

s

b

e







Particles can be grouped according to the forces ●

Electromagnetic sector (QED)



Strong sector (QCD)

Standard model



Strong sector

Electromagnetic sector g

u

c

t

d

s

b

e







W

e

Z

 

Weak sector

Particles can be grouped according to the forces ●

Electromagnetic sector (QED)



Strong sector (QCD)



Weak sector

Standard model



Strong sector

Electromagnetic sector g

u

c

t

d

s

b

W

Z

Higgs sector h

e

 



e

 

Weak sector

Particles can be grouped according to the forces ●

Electromagnetic sector (QED)



Strong sector (QCD)



Weak sector



Higgs sector

Standard model



Strong sector

Electromagnetic sector g

u

c

t

d

s

b

W

Z

Higgs sector h

e

 



e

 

Weak sector

Particles can be grouped according to the forces ●

Electromagnetic sector (QED)



Strong sector (QCD)



Weak sector



Higgs sector – actually 13 different interactions

The Brout-Englert-Higgs effect



The Higgs is assumed to create much of the mass

The Brout-Englert-Higgs effect 100% 80% 60%

Strong Higgs

40% 20% 0%



u

d

s

c

b

t

W

Z Leptons

The Higgs is assumed to create much of the mass

The Brout-Englert-Higgs effect 100%

h h

80%

h h h

60%

Strong Higgs

40% 20% 0%

u

d

s

c

b

t

W

Z Leptons



The Higgs is assumed to create much of the mass



Mechanism: “Higgs condenses”

The Brout-Englert-Higgs effect 100%

h h

80%

h t h

h

60% 40% 20% 0%





Strong Higgs

u

d

s

c

b

t

W

Z Leptons

The Higgs is assumed to create much of the mass Mechanism: “Higgs condenses and the particles are slowed (gain mass)”

The Brout-Englert-Higgs effect 100%

h h

80%

h t h

h

60% 40% 20% 0%







Strong Higgs

u

d

s

c

b

t

W

Z Leptons

The Higgs is assumed to create much of the mass Mechanism: “Higgs condenses and the particles are slowed (gain mass)” Higgs only particle which has a static mass

The elusiveness of the Higgs

The elusiveness of the Higgs



Higgs couples to a particle proportional to its mass

The elusiveness of the Higgs



[ATLAS & CMS, '11+'12 data]

Higgs couples to a particle proportional to its mass

The elusiveness of the Higgs

[ATLAS & CMS, '11+'12 data]

h h



Higgs couples to a particle proportional to its mass



Required almost 2 years of data taking ●

But twice as many data by the end of this year



10 times more until 2020 (perhaps 100 times by 2025...)

Questions to the standard model ●

Why does the Higgs has the mass it has? ●

Could have any mass

Questions to the standard model ●

Why does the Higgs has the mass it has? ●



Could have any mass

Why does it interact the way it does? ●

Why are the masses of the matter particles so different?

Questions to the standard model ●

Why does the Higgs has the mass it has? ●



Why does it interact the way it does? ●



Could have any mass Why are the masses of the matter particles so different?

Why is there the Brout-Englert-Higgs effect? ●

No intrinsic reason

Questions to the standard model ●

Why does the Higgs has the mass it has? ●



Why does it interact the way it does? ●



No intrinsic reason

Why have electrons the same charge as protons? ●



Why are the masses of the matter particles so different?

Why is there the Brout-Englert-Higgs effect? ●



Could have any mass

...

Could have any rational ratio

The Higgs – a touchstone ●

Why do we observe the Higgs at all? ●

From a theoretical point of view, this is not obvious

Why to wonder

Coordinates



Space-time

Coordinates



Space-time is a set of points

Coordinates



Space-time is a set of points ●

Coordinate systems are used to describe them

Coordinates



Space-time is a set of points ●



Coordinate systems are used to describe them

Coordinates must not be the usual cartesian ones ●

E.g. spherical coordinates

Coordinate transformations



Coordinates systems are made by humans ●

Points do not care about them

Coordinate transformations

= ●

Coordinates systems are made by humans ●

Points do not care about them



Physics must be independent of coordinates



Or: Physics is the same in any coordinate system

Coordinate transformations

= ●

Coordinates systems are made by humans ●

Points do not care about them



Physics must be independent of coordinates



Or: Physics is the same in any coordinate system



There is a transformation between them ●

Coordinate transformation

Redundant coordinates



Coordinates are not always independent ●



Some coordinates may be redundant

Something moving in the plane, but described also by height

Redundant coordinates



Coordinates are not always independent ●



Some coordinates may be redundant

Something moving in the plane, but described also by height

Redundant coordinates



Coordinates are not always independent ●





Some coordinates may be redundant

Something moving in the plane, but described also by height One can eliminate the additional coordinates ●

Can be technically helpful

Redundant coordinates



Coordinates are not always independent ●





Something moving in the plane, but described also by height One can eliminate the additional coordinates ●



Some coordinates may be redundant

Can be technically helpful

But this is not necessary

External space-time

Space ●

Particle physics takes place in space-time

Time

External space-time

Time

Space ●



Particle physics takes place in space-time Space-time is then just the arena where particle physics happens

External space-time

Time

Space ●



Particle physics takes place in space-time Space-time is then just the arena where particle physics happens

External space-time

Time

Space ●



Particle physics takes place in space-time Space-time is then just the arena where particle physics happens

External space-time

Time

Space ●





Particle physics takes place in space-time Space-time is then just the arena where particle physics happens Space-time is therefore called the external space

Internal space



Space-time

Particles have more properties than just position and speed

Internal space

Space-time e Spin





Particles have more properties than just position and speed Example: Spin (internal angular momentum) ●

Electrons have spin ½



This spin has a direction



That is an additional information



This requires one more coordinate

Internal space

Space-time e Spin







Particles have more properties than just position and speed Example: Spin (internal angular momentum) ●

Electrons have spin ½



This spin has a direction



That is an additional information



This requires one more coordinate

It is thus internal: It belongs to the electron, not to space-time

Internal space



There are much more possibilities

Internal space p ●

There are much more possibilities ●

E.g.: Proton and neutron

n

Internal space p ●

N

n

There are much more possibilities ●

E.g.: Proton and neutron



The Strong nuclear force cannot distinguish them



Behaves like a single particle: Nucleon

Internal space

-

+

p ●

N

Isospin

n

There are much more possibilities ●

E.g.: Proton and neutron



The Strong nuclear force cannot distinguish them



Behaves like a single particle: Nucleon



Can be described by an internal space: Isospin



Isospin + is a proton, Isospin – is a neutron

Internal space

-

+

p ●

N

Isospin

n

There are much more possibilities ●

E.g.: Proton and neutron



The Strong nuclear force cannot distinguish them



Behaves like a single particle: Nucleon



Can be described by an internal space: Isospin



Isospin + is a proton, Isospin – is a neutron



Other forces can distinguish

Internal space

-

+

p ●



N

Isospin

n

There are much more possibilities ●

E.g.: Proton and neutron



The Strong nuclear force cannot distinguish them



Behaves like a single particle: Nucleon



Can be described by an internal space: Isospin



Isospin + is a proton, Isospin – is a neutron



Other forces can distinguish

To be proton or neutron is an internal (discrete) coordinate

Internal space

-

+

p



N

Isospin

n

Where is then the difference, if one neglects everything but the strong nuclear force?

Internal space

-

+

p





N

Isospin

n

Where is then the difference, if one neglects everything but the strong nuclear force? None

Internal space

-

+

p







N

Isospin

n

Where is then the difference, if one neglects everything but the strong nuclear force? None The system does not care whether the thing is a proton or neutron

Internal space

-

+

p







N

Isospin

n

Where is then the difference, if one neglects everything but the strong nuclear force? None The system does not care whether the thing is a proton or neutron



Can be changed, and the physics remains unchanged



What is called proton or neutron does not matter



Just a coordinate system

Internal space

-

+

p







N

Isospin

n

Where is then the difference, if one neglects everything but the strong nuclear force? None The system does not care whether the thing is a proton or neutron



Can be changed, and the physics remains unchanged



What is called proton or neutron does not matter



Just a coordinate system



Physics must be independent of this

Classical electrodynamics ●

Triumph of classical physics in the 19th century

Classical electrodynamics ●

Triumph of classical physics in the 19th century



Formulated as the Maxwell equations ●

Vacuum:

∇ E=0 ∇×B=∂t E

∇ B=0 ∇×E=−∂t B

Classical electrodynamics ●

Triumph of classical physics in the 19th century



Formulated as the Maxwell equations ●



Vacuum:

∇ E=0 ∇×B=∂t E

∇ B=0 ∇×E=−∂t B

Rewriting with the vector potential (ϕ , A)

B=∇ × A

E=−∇ ϕ−∂ t A

Classical electrodynamics ●

Triumph of classical physics in the 19th century



Formulated as the Maxwell equations ●



Vacuum:

∇ E=0 ∇×B=∂t E

Rewriting with the vector potential (ϕ , A)

B=∇ × A ●

∇ B=0 ∇×E=−∂t B

E=−∇ ϕ−∂ t A

Invariant under so-called gauge transformations

A→ A+∇ Λ

ϕ→ϕ−∂t Λ

Λ arbitrary

Classical electrodynamics ●

Triumph of classical physics in the 19th century



Formulated as the Maxwell equations ●



Vacuum:

∇ E=0 ∇×B=∂t E

Rewriting with the vector potential (ϕ , A)

B=∇ × A ●

E=−∇ ϕ−∂ t A

Invariant under so-called gauge transformations

A→ A+∇ Λ ●

∇ B=0 ∇×E=−∂t B

ϕ→ϕ−∂t Λ

Λ arbitrary

Extreme case of coordinate transformations ●

Some part of the vector potential is redundant

The Higgs sector as a gauge theory ●

The Higgs sector is a gauge theory

1 a μν L=− W μ ν W a 4 a a a W μ ν=∂μ W ν−∂ ν W μ



Ws

W

a μ

W

The Higgs sector as a gauge theory ●

The Higgs sector is a gauge theory

1 a μν L=− W μ ν W a 4 a a a a b c W μ ν=∂μ W ν−∂ ν W μ + gf bc W μ W ν



Ws



Coupling g and some numbers f abc

W

a μ

W

W

W

The Higgs sector as a gauge theory ●

The Higgs sector is a gauge theory

1 a μν L=− W μ ν W a 4 a a a a b c W μ ν=∂μ W ν−∂ ν W μ + gf bc W μ W ν



Ws

W

W

a μ



No QED: Ws and Zs are degenerate



Coupling g and some numbers f abc

h h

W

W

The Higgs sector as a gauge theory ●

The Higgs sector is a gauge theory

1 a μν ij j + μ L=− W μ ν W a + ( Dμ h ) D ik h k 4 a a a a b c W μ ν =∂μ W ν−∂ ν W μ + gf bc W μ W ν D ijμ =δij ∂μ





Ws

W Higgs hi

a μ



No QED: Ws and Zs are degenerate



Coupling g and some numbers f abc

W h

W

W

The Higgs sector as a gauge theory ●

The Higgs sector is a gauge theory

1 a μν ij j + μ L=− W μ ν W a + ( Dμ h ) D ik h k 4 a a a a b c W μ ν =∂μ W ν−∂ ν W μ + gf bc W μ W ν Dμij =δij ∂μ −igW μa t ija





Ws

W Higgs hi

a μ



No QED: Ws and Zs are degenerate



Coupling g and some numbers f abc and taij

W h

W

W

h W

The Higgs sector as a gauge theory ●

The Higgs sector is a gauge theory

1 a μν ij j + μ a + 2 2 L=− W μ ν W a +( Dμ h ) D ik hk +λ (h ha −v ) 4 a a a a b c W μ ν =∂μ W ν −∂ ν W μ + gf bc W μ W ν W W W ij ij a ij D μ =δ ∂μ −igW μ t a





Ws

W Higgs hi

a μ

h

h W h h



No QED: Ws and Zs are degenerate



Couplings g, v, λ and some numbers f abc and taij

The Higgs sector as a gauge theory ●

The Higgs sector is a gauge theory

1 a  ij j   a  2 2 L=− W   W a  D  h  D ik h k  h h a −v  4 a a a a b c W   =∂  W  −∂  W   gf bc W  W  W W W ij ij a ij D  = ∂ −igW  t a





Ws

W Higgs hi

a μ

h

h W h h



No QED: Ws and Zs are degenerate



Couplings g, v, λ and some numbers f abc and taij



If not stated differently: Tree-level masses as in SM

Symmetries 1 a μν ij j + μ a + 2 2 L=− W μ ν W a + ( Dμ h ) D ik h k + λ(h ha −v ) 4 a a a a b c W μ ν =∂μ W ν −∂ ν W μ + gf bc W μ W ν Dμij =δij ∂μ −igW μa t ija

Symmetries 1 a μν ij j + μ a + 2 2 L=− W μ ν W a + ( Dμ h ) D ik h k + λ(h ha −v ) 4 a a a a b c W μ ν =∂μ W ν −∂ ν W μ + gf bc W μ W ν Dμij =δij ∂μ −igW μa t ija ●

Local SU(2) gauge symmetry ●

a

Invariant under arbitrary gauge transformations   x  a 

a 

a b

a bc

c 

W W  ∂ −g f W 

b

ij a

a

hi  hi g t  h j

Symmetries 1 a μν ij j + μ a + 2 2 L=− W μ ν W a + ( Dμ h ) D ik h k + λ(h ha −v ) 4 a a a a b c W μ ν =∂μ W ν −∂ ν W μ + gf bc W μ W ν Dμij =δij ∂μ −igW μa t ija ●

Local SU(2) gauge symmetry ●

a

Invariant under arbitrary gauge transformations   x  a 

a 

a b

a bc

c 

W W  ∂ −g f W  ●

b

ij a

a

hi  hi g t  h j

Global SU(2) Higgs custodial (flavor) symmetry ●

Acts as right-transformation on the Higgs field only a μ

W →W

a μ

ij

ij



hi → hi + a h j + b h j

The trouble with the Higgs ●

Weak interactions are an extreme case of redundancy ●

Strong interactions also; same story, different details

The trouble with the Higgs ●

Weak interactions are an extreme case of redundancy ●



Strong interactions also; same story, different details

Elementary particles are auxiliary objects ● ●

Depend on a coordinate system in internal space Properties can change under coordinate transformation

The trouble with the Higgs ●

Weak interactions are an extreme case of redundancy ●



Elementary particles are auxiliary objects ● ●



Strong interactions also; same story, different details Depend on a coordinate system in internal space Properties can change under coordinate transformation

Getting a coordinate-independent object requires at least a combination (bound-state) of two h

h

Resolving the paradox

The trouble with the Higgs ●

But what is then this?

The trouble with the Higgs ●

But what is then this?



Field theory

The trouble with the Higgs ●

But what is then this?



Field theory: h

h

The trouble with the Higgs ●

But what is then this?



Field theory: h

h

[Fröhlich et al. PLB 80]

⟨(h

+

h)( x)(h

+

h)( y)⟩

The trouble with the Higgs ●

But what is then this?



Field theory: h h

h



h

+

h h

h

h

+ something small

h

[Fröhlich et al. PLB 80]

⟨(h

+

h)( x)(h

+

h=v+η + 3 h)( y)⟩ ≈ const .+⟨η (x) η( y)⟩+O (η )

The trouble with the Higgs ●

But what is then this?



Field theory: h h



h



h

+

h h

h

h

+ something small

h

Touchstone ●

Compare theory and experiment



Will require much more data

⟨(h

+

h)( x)(h

+

[Fröhlich et al. PLB 80]

h=v+η + 3 h)( y)⟩ ≈ const .+⟨η (x) η( y)⟩+O (η )

Confirming the resolution

Confirming the resolution Requires a (non-perturbative) suitable method

Confirming the resolution Requires a (non-perturbative) suitable method: Lattice gauge theory

Lattice calculations ●

Take a finite volume – usually a hypercube

L

Lattice calculations ●



Take a finite volume – usually a hypercube Discretize it, and get a finite, hypercubic lattice

a L

Lattice calculations ●





Take a finite volume – usually a hypercube Discretize it, and get a finite, hypercubic lattice Calculate observables using path integral ●

Can be done numerically



Uses Monte-Carlo methods

a L

Lattice calculations ●







Take a finite volume – usually a hypercube Discretize it, and get a finite, hypercubic lattice Calculate observables using path integral ●

Can be done numerically



Uses Monte-Carlo methods

Artifacts ●

Finite volume/discretization a L

Lattice calculations ●







Take a finite volume – usually a hypercube Discretize it, and get a finite, hypercubic lattice Calculate observables using path integral ●

Can be done numerically



Uses Monte-Carlo methods

Artifacts ●

Finite volume/discretization



Masses vs. wave-lengths

a L

Lattice calculations ●







Take a finite volume – usually a hypercube Discretize it, and get a finite, hypercubic lattice Calculate observables using path integral ●

Can be done numerically



Uses Monte-Carlo methods

Artifacts ●

Finite volume/discretization



Masses vs. wave-lengths

a L

Lattice calculations ●







Take a finite volume – usually a hypercube Discretize it, and get a finite, hypercubic lattice Calculate observables using path integral ●

Can be done numerically



Uses Monte-Carlo methods

Artifacts ●

Finite volume/discretization



Masses vs. wave-lengths



Euclidean formulation

a L

Masses from Euclidean propagators

Masses from Euclidean propagators

D( p)=〈O



+

( p)O(− p)〉

Masses can be inferred from propagators

Masses from Euclidean propagators

D( p)=〈O



+

1 ( p)O(− p)〉∼ 2 2 p +m

Masses can be inferred from propagators

Masses from Euclidean propagators

1 D( p)=〈O ( p)O(−p)〉∼ 2 2 p +m + C (t )=〈O ( x)O( y )〉∼exp(−m Δ t ) +



Masses can be inferred from propagators

Masses from Euclidean propagators

D( p)=〈O

+

( p)O(− p)〉∼∑

ai 2

2 i

p +m + C (t )=〈O (x)O( y )〉∼∑ ai exp(−mi Δ t) ∑ ai=1∧m0< m1< ... ●

Masses can be inferred from propagators



Long-time behavior relevant ●

No exact results on time-like momenta

Masses from Euclidean propagators



Masses can be inferred from propagators



Long-time behavior relevant ●

No exact results on time-like momenta

Masses from Euclidean propagators



Masses can be inferred from propagators



Long-time behavior relevant ●

No exact results on time-like momenta

Masses from Euclidean propagators



Masses can be inferred from propagators



Long-time behavior relevant ●

No exact results on time-like momenta

Higgsonium

h



+

h

Simpelst 0 bound state h + ( x)h( x)

Higgsonium

h



h

+

Simpelst 0 bound state h + ( x)h( x) ●

Same quantum numbers as the Higgs ●

No weak or flavor charge

Higgsonium

[Maas et al. '13]

h



h

+

Simpelst 0 bound state h + ( x)h( x) ●

Same quantum numbers as the Higgs ●

No weak or flavor charge

Higgsonium

[Maas et al. '13]

Influence of heavier states

h

h

Finite-volume effects



Finite-volume effects

+

Simpelst 0 bound state h + ( x)h( x) ●

Same quantum numbers as the Higgs ●

No weak or flavor charge

Higgsonium

[Maas et al. '13]

h

h

Finite-volume effects



+

Simpelst 0 bound state h + ( x)h( x) ●

Same quantum numbers as the Higgs ●



No weak or flavor charge

Mass is about 120 GeV

Higgsonium

[Maas et al. '13]

h

h

Finite-volume effects



Finite-volume effects

+

Simpelst 0 bound state h + ( x)h( x) ●

Same quantum numbers as the Higgs ●



No weak or flavor charge

Mass is about 120 GeV

Higgsonium

[Maas et al. '13]

Influence of heavier states

h

h

Finite-volume effects



Finite-volume effects

+

Simpelst 0 bound state h + ( x)h( x) ●

Same quantum numbers as the Higgs ●



No weak or flavor charge

Mass is about 120 GeV

Mass relation - Higgs ●

[Fröhlich et al. PLB 80 Maas'12, Maas & Mufti'13]

Higgsonium: 120 GeV, Higgs at tree-level: 120 GeV ●

Scheme exists to shift Higgs mass always to 120 GeV

Mass relation - Higgs ●

Higgsonium: 120 GeV, Higgs at tree-level: 120 GeV ●



[Fröhlich et al. PLB 80 Maas'12, Maas & Mufti'13]

Scheme exists to shift Higgs mass always to 120 GeV

Demonstrates the relation ●

Duality between elementary states and bound states [Fröhlich et al. PLB 80]

⟨(h

+

h)( x)(h

+

h=v+η + 3 h)( y)⟩ ≈ const .+⟨η (x) η( y)⟩+O (η )



Same poles to leading order



Fröhlich-Morchio-Strocchi (FMS) mechanism

Mass relation - Higgs ●

Higgsonium: 120 GeV, Higgs at tree-level: 120 GeV ●



Scheme exists to shift Higgs mass always to 120 GeV

Demonstrates the relation ●

Duality between elementary states and bound states [Fröhlich et al. PLB 80]

⟨(h



[Fröhlich et al. PLB 80 Maas'12, Maas & Mufti'13]

+

h)( x)(h

+

h=v+η + 3 h)( y)⟩ ≈ const .+⟨η (x) η( y)⟩+O (η )



Same poles to leading order



Fröhlich-Morchio-Strocchi (FMS) mechanism

Deeply-bound relativistic state ●

Mass defect~constituent mass



Cannot describe with quantum mechanics



Very different from QCD bound states

Isovector-vector state

W



h h

Vector state 1- with operator

+

h a h tr t Dμ + √h h √h + h



Only in a Higgs phase close to a simple particle



Higgs-flavor triplet, instead of gauge triplet

Isovector-vector state

W



[Maas et al. '13]

h h

Vector state 1- with operator

+

h a h tr t Dμ + √h h √h + h



Only in a Higgs phase close to a simple particle



Higgs-flavor triplet, instead of gauge triplet

Isovector-vector state

W



[Maas et al. '13]

h h

Vector state 1- with operator

+

h a h tr t Dμ + √h h √h + h



Only in a Higgs phase close to a simple particle



Higgs-flavor triplet, instead of gauge triplet



Mass about 80 GeV

Mass relation - W ●

Vector state: 80 GeV



W at tree-level: 80 GeV ●

W not scale or scheme dependent

[Fröhlich et al. PLB 80 Maas'12]

Mass relation - W ●

Vector state: 80 GeV



W at tree-level: 80 GeV ●



W not scale or scheme dependent

Same mechanism 〈(h

+

Dμ h)( x)(h

+

Dμ h)( y)〉

[Fröhlich et al. PLB 80 Maas'12]

Mass relation - W

[Fröhlich et al. PLB 80 Maas'12]



Vector state: 80 GeV



W at tree-level: 80 GeV ●



W not scale or scheme dependent

Same mechanism +

+

〈(h D μ h)( x)(h Dμ h)( y)〉 h=v+ η 3 ≈ const.+ 〈W μ ( x)W μ ( y)〉+ O (η ) ∂ v=0

Mass relation - W

[Fröhlich et al. PLB 80 Maas'12]



Vector state: 80 GeV



W at tree-level: 80 GeV ●



W not scale or scheme dependent

Same mechanism +



+

〈(h D μ h)( x)(h Dμ h)( y)〉 h=v+ η 3 ≈ const.+ 〈W μ ( x)W μ ( y)〉+ O (η ) ∂ v=0 Same poles at leading order ●

At least for a light Higgs

Mass relation - W

[Fröhlich et al. PLB 80 Maas'12]



Vector state: 80 GeV



W at tree-level: 80 GeV ●



W not scale or scheme dependent

Same mechanism +



+

⟨(h Dμ h)( x)(h Dμ h)( y)⟩ h=v + η 3 ≈ const .+⟨W μ ( x)W μ ( y)⟩+O (η ) ∂ v=0 Same poles at leading order ●

At least for a light Higgs



Remains true beyond leading order

What about the rest?

What about the rest? ●

Quarks and gluons ●

Anyhow bound by confinement in bound states ●

Top subtle, but same principle

What about the rest? ●

Quarks and gluons ●

Anyhow bound by confinement in bound states ●



Top subtle, but same principle

Leptons ●

Actually Higgs-lepton bound-states ●

Enormous mass defects



Requires confirmation



Except for right-handed (Dirac) neutrino

What about the rest? ●

Quarks and gluons ●

Anyhow bound by confinement in bound states ●



Leptons ●

Actually Higgs-lepton bound-states ●



Top subtle, but same principle

Enormous mass defects



Requires confirmation



Except for right-handed (Dirac) neutrino

Photons ●

QED similar but simpler

How events looks like (LEP/ILC) e--H bound state

μ --H bound state

Z-H-H bound state e+-H bound state ●

Collision of bound states

μ+-H bound state

How events looks like (LEP/ILC) e--H bound state

μ --H bound state

Z-H-H bound state e+-H bound state ●

Collision of bound states



'Constituent' particles

μ+-H bound state

How events looks like (LEP/ILC) e--H bound state

μ --H bound state

Z-H-H bound state e+-H bound state ●

Collision of bound states



'Constituent' particles



Higgs partners just spectators ●

Similar to pp collisions

μ+-H bound state

How events looks like (LEP/ILC) e--H bound state

μ --H bound state

Z-H-H bound state e+-H bound state ●

Collision of bound states



'Constituent' particles



Higgs partners just spectators ●



Similar to pp collisions

Sub-leading contributions

μ+-H bound state

How events looks like (LEP/ILC) e--H bound state

μ --H bound state

Z-H-H bound state e+-H bound state ●

Collision of bound states



'Constituent' particles



Higgs partners just spectators ●



Similar to pp collisions

Sub-leading contributions ●

Ordinary ones: Large and detected

μ+-H bound state

How events looks like (LEP/ILC) e--H bound state

μ --H bound state

Z-H-H bound state

μ+-H bound state

e+-H bound state ●

Collision of bound states



'Constituent' particles



Higgs partners just spectators ●



Similar to pp collisions

Sub-leading contributions ●

Ordinary ones: Large and detected



New ones: Small, require more sensitivity

Implications

Ground states ●

For W and Higgs exist gauge-invariant composite/bound states of the same mass ●

Play the role of the experimental signatures



“True” physical states



Reason for the applicability of perturbation theory for electroweak physics

Ground states ●

For W and Higgs exist gauge-invariant composite/bound states of the same mass ●

Play the role of the experimental signatures



“True” physical states





Reason for the applicability of perturbation theory for electroweak physics

Is this always true? ●

Full standard model: Probably



Other parameters?

Phase diagram (Lattice-regularized) phase diagram

f(Classical Higgs mass)



[Fradkin & Shenker PRD'79 Caudy & Greensite PRD'07]

 g(Classical gauge coupling)

Phase diagram (Lattice-regularized) phase diagram

f(Classical Higgs mass)



[Fradkin & Shenker PRD'79 Caudy & Greensite PRD'07]

Higgs “phase”

 g(Classical gauge coupling)

Phase diagram (Lattice-regularized) phase diagram

f(Classical Higgs mass)



[Fradkin & Shenker PRD'79 Caudy & Greensite PRD'07]

Higgs “phase”

Confinement “phase”  g(Classical gauge coupling)

Phase diagram (Lattice-regularized) phase diagram

f(Classical Higgs mass)



[Fradkin & Shenker PRD'79 Caudy & Greensite PRD'07]

Higgs “phase”

Confinement “phase”  g(Classical gauge coupling)

Phase diagram (Lattice-regularized) phase diagram continuous

f(Classical Higgs mass)



[Fradkin & Shenker PRD'79 Caudy & Greensite PRD'07]

Crossover

Higgs “phase”

1st order

Confinement “phase”  g(Classical gauge coupling)

Phase diagram (Lattice-regularized) phase diagram continuous ●

Separation only in fixed gauges

f(Classical Higgs mass)



[Fradkin & Shenker PRD'79 Caudy & Greensite PRD'07]

Crossover

Higgs “phase” Coulomb gauge

Landau gauge

1st order

Confinement “phase”  g(Classical gauge coupling)

Phase diagram (Lattice-regularized) phase diagram continuous ●





Separation only in fixed gauges

f(Classical Higgs mass)



[Fradkin & Shenker PRD'79 Caudy & Greensite PRD'07]

Crossover

Same asymptotic states in confinement and Higgs pseudo-phases

Higgs “phase”

1st order

Confinement “phase”  g(Classical gauge coupling)

Same asymptotic states irrespective of coupling strengths

Typical spectra



[Maas, Mufti '13,'14, Evertz et al.'86, Langguth et al.'85,'86]

Generically different low-lying spectra

Typical spectra



[Maas, Mufti '13,'14, Evertz et al.'86, Langguth et al.'85,'86]

Generically different low-lying spectra ●

0+ lighter in QCD-like region



1- lighter in Higgs-like region

Typical spectra

[Maas, Mufti '13,'14, Evertz et al.'86, Langguth et al.'85,'86]

“Higgs”





Generically different low-lying spectra ●

0+ lighter in QCD-like region



1- lighter in Higgs-like region

Use as operational definition of phase

“QCD”

Phase diagram

“QCD”

[Maas, Mufti,'14]

“Higgs”



Complicated phase diagram



QCD-like behavior even for negative bare mass



Similar bare couplings for both physics types

Development in the Higgs channel [Maas, Mufti'14]

Unstable Physical



QCD-like

Three distinct regions

Development in the Higgs channel [Maas, Mufti'14]

● ●

Base-line Lowest state as expected above threshold: 2 almost non-interacting ”Ws”

Development in the Higgs channel [Maas, Mufti'14]





Next state within errors essentially trivial throughout No discernible resonances

Development in the Higgs channel [Maas, Mufti'14]



Next state within errors essentially trivial throughout



No discernible resonances



Also true for the next level



Different from perturbation theory

Implications for Higgsed theories [Maas,'15]



Higgsed theories appear a lot in BSM ●

GUTs, 2HDM, (some) SUSY models,...

Implications for Higgsed theories [Maas,'15]



Higgsed theories appear a lot in BSM ●



GUTs, 2HDM, (some) SUSY models,...

Structure observed here is not generic ●



Mass relation of elementary states and observable states only possible for light but not too light Higgs Global symmetries determines observable state spectrum ●

SM Higgs sector is special because custodial and gauge group are the same

Implications for Higgsed theories [Maas,'15]



Higgsed theories appear a lot in BSM ●



GUTs, 2HDM, (some) SUSY models,...

Structure observed here is not generic ●



Mass relation of elementary states and observable states only possible for light but not too light Higgs Global symmetries determines observable state spectrum ●



SM Higgs sector is special because custodial and gauge group are the same

Each case may be different

Implications for 2HDM [Maas,'15]



Simple example: Additional Higgs doublet a

Implications for 2HDM [Maas,'15]





Simple example: Additional Higgs doublet a Standard scenario: Both Higgs condense ● ●

SM condensate is a mixture All additional Higgs particles are states, but heavier than the SM Higgs

Implications for 2HDM [Maas,'15]





Simple example: Additional Higgs doublet a Standard scenario: Both Higgs condense ● ●



SM condensate is a mixture All additional Higgs particles are states, but heavier than the SM Higgs

Perturbatively, the state space has just four more (heavier) Higgs

Implications for 2HDM [Maas,'15]





Simple example: Additional Higgs doublet a Standard scenario: Both Higgs condense ● ●





SM condensate is a mixture All additional Higgs particles are states, but heavier than the SM Higgs

Perturbatively, the state space has just four more (heavier) Higgs Non-perturbative?

Implications for 2HDM [Maas,'15]



FMS states

Implications for 2HDM [Maas,'15]



FMS states: ●

Higgs 1:

⟨(h

+

h)(x)(h

+

+ h

3 h

h)( y )⟩ ≈ const .+⟨ η (x )ηh ( y )⟩+O(η )

Implications for 2HDM [Maas,'15]



FMS states: ●

Higgs 1:

⟨(h ●

+

h)(x)(h

+ h

3 h

+

3

+

h)( y )⟩ ≈ const .+⟨ η (x )ηh ( y )⟩+O(η )

+

a)( y )⟩ ≈ const .+⟨ ηa (x)ηa ( y)⟩+O(ηa )

Higgs 2:

⟨(a

+

a)(x)(a

Implications for 2HDM [Maas,'15]



FMS states: ●

Higgs 1:

⟨(h ●

h)(x)(h

+ h

3 h

+

3

+

h)( y )⟩ ≈ const .+⟨ η (x )ηh ( y )⟩+O(η )

+

a)( y )⟩ ≈ const .+⟨ ηa (x)ηa ( y)⟩+O(ηa )

Higgs 2:

⟨(a ●

+

+

a)(x)(a

W 1: ⟨(h + Dμ h)(x )(h + D μ h)( y)⟩ ≈ const .+⟨W μ ( x)W μ ( y)⟩+O(η3h )

Implications for 2HDM [Maas,'15]



FMS states: ●

Higgs 1:

⟨(h ●

h)(x)(h

+ h

3 h

+

3

+

h)( y )⟩ ≈ const .+⟨ η (x )ηh ( y )⟩+O(η )

+

a)( y )⟩ ≈ const .+⟨ ηa (x)ηa ( y)⟩+O(ηa )

Higgs 2:

⟨(a ●

+

+

a)(x)(a

W 1: ⟨(h + Dμ h)(x )(h + D μ h)( y)⟩ ≈ const .+⟨W μ ( x)W μ ( y)⟩+O(η3h )



W 2:

⟨(a + Dμ a)(x)(a + D μ a)( y )⟩ ≈ const .+⟨W μ ( x)W μ ( y )⟩+O(η3a )

Implications for 2HDM [Maas,'15]



FMS states: ●

Higgs 1:

⟨(h ●

h)(x)(h

+ h

3 h

+

3

+

h)( y )⟩ ≈ const .+⟨ η (x )ηh ( y )⟩+O(η )

+

a)( y )⟩ ≈ const .+⟨ ηa (x)ηa ( y)⟩+O(ηa )

Higgs 2:

⟨(a ●

+

+

a)(x)(a

W 1: ⟨(h + Dμ h)(x )(h + D μ h)( y)⟩ ≈ const .+⟨W μ ( x)W μ ( y)⟩+O(η3h )



W 2:

⟨(a + Dμ a)(x)(a + D μ a)( y )⟩ ≈ const .+⟨W μ ( x)W μ ( y )⟩+O(η3a ) ●

Twice as many W ●

Beyond expansion: Lattice is running

Implications for other BSM scenarios [Maas,'15]



Grand-unified theories ●

All gauge interactions from a single one at a high scale (>1015 GeV)



Broken by a second BEH effect



Explains relations of electric charges



Explains gauge coupling unification



Explains intrafamily relations ●



Anomaly-freeness of the standard model

Most prominent signature: Proton decay

Implications for other BSM scenarios [Maas,'15]



Grand-unified theories ●

All gauge interactions from a single one at a high scale (>1015 GeV)



Broken by a second BEH effect



Explains relations of electric charges



Explains gauge coupling unification



Explains intrafamily relations ●

Anomaly-freeness of the standard model



Most prominent signature: Proton decay



Impact: Structure restricted

Implications for other BSM scenarios [Maas,'15]



Technicolor ●

Higgs replaced by new fermions (techniquarks) and new gauge interaction (technicolor)

Implications for other BSM scenarios [Maas,'15]



Technicolor ●



Higgs replaced by new fermions (techniquarks) and new gauge interaction (technicolor) FMS mechanism cannot work

Implications for other BSM scenarios [Maas,'15]



Technicolor ●

● ●

Higgs replaced by new fermions (techniquarks) and new gauge interaction (technicolor) FMS mechanism cannot work Observable states must still be gaugeinvariant

Implications for other BSM scenarios [Maas,'15]



Technicolor ●

● ●



Higgs replaced by new fermions (techniquarks) and new gauge interaction (technicolor) FMS mechanism cannot work Observable states must still be gaugeinvariant Needs to create signals by bound states: W/Z and Higgs Has not been adressed so far ● Only effective theories ●

Summary ●



Higgs sector with light Higgs successfully described by perturbation theory around classical physics Bound-state/elementary state duality ●

Highly relativistic bound states

Summary ●



Higgs sector with light Higgs successfully described by perturbation theory around classical physics Bound-state/elementary state duality ●





Highly relativistic bound states

Permits physical interpretation of resonances in cross sections Generalizations to other BSM theories with Higgs effect possible ●

Required to understand observable spectrum



Differences to perturbative one possible

Summary ●



Higgs sector with light Higgs successfully described by perturbation theory around classical physics Bound-state/elementary state duality ●





Highly relativistic bound states

Permits physical interpretation of resonances in cross sections Generalizations to other BSM theories with Higgs effect possible ●

Required to understand observable spectrum



Differences to perturbative one possible



New restrictions and opportunities for falsification



Could qualitatively alter experimental signatures