Particle Physics: The Standard Model · Particle Physics: The Standard Model Dirk Zerwas LAL...

Particle Physics: The Standard Model

Dirk Zerwas

LALzerwas@lal.in2p3.fr

March 15, 2012

Dirk Zerwas Particle Physics: The Standard Model

The HistoryThe LagrangianThe Feynman RulesMoeller ScatteringBhabha

The History

Introduction of particles (ατoµoς)

Particle-Wave dualism (deBroglie wave length)

Particles are fields in a quantum field theory

1941: Stueckelberg proposes to interpret electron linesgoing back in time as positrons

end of 1940s: Feynman, Tomonaga, Schwinger et aldevelop renormalization theory

anomalous magnetic moment predicted (not today)

Quantum Field Theory in a nutshell

Leading Order (LO)diagram is the simplestdiagram

The electron is on-shell(p2 = m2

e), no interactions

NLO (next-to-leadingorder) diagram

Process not allowed inclassical mechanics

Heisenberg: ∆E∆t ≥ 1 →process allowed forreabsorption after∆t ∼ 1/∆E

Quantum mechanics: addall diagrams, but thatwould also include Nγ = ∞Each vertex is aninteraction and eachinteraction has a strength(|M|2 ∼ α = 1/137)

Perturbation theory withSommerfeld convergence

Construct the Lagrangian of Free Fields

Introduce interactions via the minimal substitution scheme

Derive Feynman rules (→ courses by Adel Bilal, PierreBinetruy, Pierre Fayet, Matteo Cacciari, Slava Ryshkov)

Construct (ALL) Feynman diagrams of the process

Apply Feynman rules

Some aspects are not part of these lectures, but will sketch theideas

Remember the particle zoo

treat only the carrier of theinteraction γ

as well as the e

uR cR tRdR sR bR

eR µR τR

Remember the particle zoo

treat only the carrier of theinteraction γ

as well as the e

uR cR tRdR sR bR

eR µR τR

The photon

MAXWELL equations:

∂µFµν(x) = jν(x)ǫµνρσ∂νFρσ(x) = 0

with the photon field tensor:

Fµν(x) = ∂µAν(x) − ∂νAµ(x)

Fermions

The DIRAC equation:

(iγµ∂µ − m)ψ(x) = 0

leading to:

ψ(x)(iγµ∂µ − m)ψ(x)

with ψ = ψ†γ0 = ψT⋆

The free Lagrangian (L0)

L0 = −14

Fµν(x)Fµν(x) + ψ(x)(iγµ∂µ − m)ψ(x)

The photon

MAXWELL equations:

Fermions

The DIRAC equation:

(iγµ∂µ − m)ψ(x) = 0

leading to:

L0 = −14

The photon

MAXWELL equations:

Fermions

The DIRAC equation:

(iγµ∂µ − m)ψ(x) = 0

leading to:

L0 = −14

Minimal Substitution

i∂µ → i∂µ + eAµ(x)

ψ(x)γµi∂µψ(x)

→ ψ(x)γµ(i∂µ + eAµ(x))ψ(x)= ψ(x)γµi∂µψ(x) + eψ(x)γµAµ(x)ψ(x)

leads to a coupling between photon and fermion fields:

Interaction Lagrangian L′

L′ = −jµAµ = eψ(x)γµAµ(x)ψ(x)

the negative sign for jµ = −eψ(x)γµψ(x)

Gauge Invariance

Principle

Invariance of the Lagrangian under local U(1) transformationsor: why should physics at the Elysee be different at the ENS?

Aµ → Aµ + ∂µΛ(x)ψ(x) → exp (ieΛ(x))ψ(x)

L0 + L′ = L → LLocal gauge invariance under a U(1) gauge symmetry (1929Weyl)if Λ 6= f (x) it is a global U(1) symmetry.

U(1) Gauge invariance Photon field:

Proof.

Fµν = ∂µAν − ∂νAµ

= ∂µ(Aν + ∂νΛ) − ∂ν(Aµ + ∂µΛ)

= ∂µAν − ∂νAµ + ∂µ∂νΛ − ∂ν∂µΛ ∂µ∂ν = ∂ν∂µ

= ∂µAν − ∂νAµ

= Fµν

Photon field okDirk Zerwas Particle Physics: The Standard Model

Proof.

= ∂µ(Aν + ∂νΛ) − ∂ν(Aµ + ∂µΛ)

= Fµν

Proof.

= ∂µ(Aν + ∂νΛ) − ∂ν(Aµ + ∂µΛ)

= Fµν

Proof.

= ∂µ(Aν + ∂νΛ) − ∂ν(Aµ + ∂µΛ)

= Fµν

Proof.

= ∂µ(Aν + ∂νΛ) − ∂ν(Aµ + ∂µΛ)

= Fµν

Proof.

= ∂µ(Aν + ∂νΛ) − ∂ν(Aµ + ∂µΛ)

= Fµν

Fermion field

Proof.

ψ(iγµ∂µ − m)ψ

→ ψ† exp (−ieΛ)γ0(iγµ∂µ − m)(ψ exp (ieΛ))

= exp (−ieΛ)ψ(iγµ∂µ − m)(ψ exp (ieΛ))

= exp (−ieΛ)ψiγµ(∂µψ) exp (ieΛ)

+ exp (−ieΛ)ψiγµψ∂µ exp (ieΛ))

+ exp (−ieΛ)ψ(−m)ψ exp (ieΛ)

= ψiγµ(∂µψ)

+ ψ(−m)ψ

= ψ(iγµ∂µ − m)ψ − eψγµ(∂µΛ)ψ

Fermion field

Proof.

= ψ†γ0(iγµ∂µ − m)ψ

= ψiγµ(∂µψ)

+ ψ(−m)ψ

= ψ(iγµ∂µ − m)ψ − eψγµ(∂µΛ)ψDirk Zerwas Particle Physics: The Standard Model

Fermion field

Proof.

= ψ†γ0(iγµ∂µ − m)ψ

= ψiγµ(∂µψ)

+ ψ(−m)ψ

= ψ(iγµ∂µ − m)ψ − eψγµ(∂µΛ)ψDirk Zerwas Particle Physics: The Standard Model

Fermion field

Proof.

= ψiγµ(∂µψ)

+ ψ(−m)ψ

Fermion field

Proof.

= ψiγµ(∂µψ)

+ ψ(−m)ψ

Fermion field

Proof.

= ψiγµ(∂µψ)

+ ψ(−m)ψ

Fermion field

Proof.

= ψiγµ(∂µψ) + exp (−ieΛ)ψiγµψie∂µΛ exp (ieΛ)

+ ψ(−m)ψ

Fermion field

Proof.

= ψiγµ(∂µψ) + exp (−ieΛ)ψiγµψie∂µΛ exp (ieΛ)

+ ψ(−m)ψ

Fermion field

Proof.

= ψiγµ(∂µψ) − eψγµ(∂µΛ)ψ

+ ψ(−m)ψ

Fermion field

Proof.

= ψiγµ(∂µψ) − eψγµ(∂µΛ)ψ

+ ψ(−m)ψ

Interaction

Proof.

eψγµAµψ(x)= e exp (−ieΛ)ψγµ(Aµ + ∂µΛ)ψ exp (ieΛ)= eψγµ(Aµ + ∂µΛ)ψ= eψγµAµψ + eψγµ(∂µΛ)ψ

Interaction term combined with fermion field (−ieψγµ∂µΛψ)ok

gauge invariance of the fermion field cries for theintroduction of a gauge boson!

Interaction

Proof.

Interaction

Proof.

Interaction

Proof.

Interaction

Proof.

Interaction

Proof.

Interaction

Proof.

External lines

initial state electron u(p)initial state positron v(p)initial state photon ǫµ

final state electron u(p)final state positron v(p)final state photon ǫµ⋆

Internal lines and vertex

virtual photon −igµν

k2+iǫvirtual electron i 6p+m

p2−m2+iǫinteraction(vertex) ieγµ

Matrix element

|M|2 =′

TfiT †fi

Sum over final state, average over initial state

Moeller Scattering e−e− → e−e−

Simplest diagram with initial and final state of two electrons

conserve electric charge and momentum at each vertex

t channel only: C(e− + e−) = −2e 6= C(γ) = 0

p conservation at each vertex → 2 diagramsqγ = p2 − p3 6= p2 − p4

te−(p1)e−(p2) → e−(p3)e−(p4)

te−(p1)e−(p2) → e−(p4)e−(p3)

te−(p1)e−(p2) → e−(p3)e−(p4)

te−(p1)e−(p2) → e−(p4)e−(p3)

te−(p1)e−(p2) → e−(p3)e−(p4)

te−(p1)e−(p2) → e−(p4)e−(p3)

te−(p1)e−(p2) → e−(p3)e−(p4)

te−(p1)e−(p2) → e−(p4)e−(p3)

Fermion arrow tip to end

Interaction

propagator (internal line)

second graph p3 ↔ p4

graphs fermionpermutation: −k = f (pi)

Tfi = [ u(p4)(−ieγµ)u(p1)(−igµν )u(p3)(−ieγν)u(p2)

− u(p3)(−ieγρ)u(p1)(−igρσ )u(p4)(−ieγσ)u(p2)]

Interaction

Tfi = [ u(p4)(−ieγµ)u(p1)(−igµν

k2 )u(p3)(−ieγν)u(p2)

Interaction

− u(p3)(−ieγρ)u(p1)(−igρσ

k2 )u(p4)(−ieγσ)u(p2)]

Interaction

(p4−p1)2 )u(p3)(−ieγν)u(p2)

(p3−p1)2 )u(p4)(−ieγσ)u(p2)]

1i Tfi = 1

i [ u(p4)(−ieγµ)u(p1)(−igµν

(p4−p1)2 )u(p3)(−ieγν)u(p2)

(p3−p1)2 )u(p4)(−ieγσ)u(p2)]

= e2[ u(p4)γµu(p1)(

(p4−p1)2 )u(p3)γνu(p2)

− u(p3)γρu(p1)(

(p3−p1)2 )u(p4)γσu(p2)]

|M|2 =∑′

fi TfiT †fi

Calculation to be continued in Problem Solving

|M|2 =64π2α2

t2u2 [(s − 2m2)2(t2 + u2) + ut(−4m2s + 12m4 + ut)]

1i Tfi = 1

(p4−p1)2 )u(p3)(−ieγν)u(p2)

(p3−p1)2 )u(p4)(−ieγσ)u(p2)]

= e2[ u(p4)γµu(p1)(

(p4−p1)2 )u(p3)γνu(p2)

− u(p3)γρu(p1)(

(p3−p1)2 )u(p4)γσu(p2)]

|M|2 =∑′

fi TfiT †fi

|M|2 =64π2α2

t2u2 [(s − 2m2)2(t2 + u2) + ut(−4m2s + 12m4 + ut)]

1i Tfi = 1

(p4−p1)2 )u(p3)(−ieγν)u(p2)

(p3−p1)2 )u(p4)(−ieγσ)u(p2)]

= e2[ u(p4)γµu(p1)(

(p4−p1)2 )u(p3)γνu(p2)

− u(p3)γρu(p1)(

(p3−p1)2 )u(p4)γσu(p2)]

|M|2 =∑′

fi TfiT †fi

|M|2 =64π2α2

t2u2 [(s − 2m2)2(t2 + u2) + ut(−4m2s + 12m4 + ut)]

1i Tfi = 1

(p4−p1)2 )u(p3)(−ieγν)u(p2)

(p3−p1)2 )u(p4)(−ieγσ)u(p2)]

= e2[ u(p4)γµu(p1)(

(p4−p1)2 )u(p3)γνu(p2)

− u(p3)γρu(p1)(

(p3−p1)2 )u(p4)γσu(p2)]

|M|2 =∑′

fi TfiT †fi

|M|2 =64π2α2

t2u2 [(s − 2m2)2(t2 + u2) + ut(−4m2s + 12m4 + ut)]

1i Tfi = 1

(p4−p1)2 )u(p3)(−ieγν)u(p2)

(p3−p1)2 )u(p4)(−ieγσ)u(p2)]

= e2[ u(p4)γµu(p1)(

(p4−p1)2 )u(p3)γνu(p2)

− u(p3)γρu(p1)(

(p3−p1)2 )u(p4)γσu(p2)]

|M|2 =∑′

fi TfiT †fi

|M|2 =64π2α2

t2u2 [(s − 2m2)2(t2 + u2) + ut(−4m2s + 12m4 + ut)]

dσdΩ

= |M|2 164π2s

0 ≤ θ ≤ π/2 (electrons) me ≈ 0

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

s dσdΩ is scale invariant: measure of the pointlikeness of a particle

dσdΩ

= |M|2 164π2s

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

dσdΩ

= |M|2 164π2s

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

dσdΩ

= |M|2 164π2s

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

dσdΩ

= |M|2 164π2s

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

dσdΩ

= |M|2 164π2s

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

dσdΩ

= |M|2 164π2s

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

dσdΩ

= |M|2 164π2s

t = −2p1p3 = −2(√

s/2√

s/2 − s/4 cos θ) = −s/2(1 − cos θ)

u = −2p1p4 = −2(s/4 − ~p1~p4) = −2(s/4 + ~p1~p3)

= −2(s/4 + s/4 cos θ) = −s/2(1 + cos θ)

dσdΩ = α2

st2u2 [s2(t2 + u2) + u2t2]

s [ s2

u2 + s2

t2 + 1]

s(3+cos2 θ)2

sin4 θ

Stanford-PrincetonStorage ring

2e− beams√

s = 556MeV

limited detectoracceptance

differential cross sectionmeasurement andprediction

Typical t channelθ = 0 → dσ/dΩ → ∞Extremely good agreementbetween the measurementand the theory prediction

e−e− colliders discontinued(1971)

The Bhabha Process Homi Bhabha studied in the 1930s inGreat Britain, worked in India afterwards

tdσdΩ

16s(3 + cos2 θ)2

sin4 θ2

0 ≤ θ ≤ π

t channel: ∼ sin−4(θ/2)

s channel: ∼ 1 + cos2 θ

PETRA e+e− collider√s ≤ 35GeV

JADE, TASSO,CELLO

total cross section

differential crosssection

JADE, TASSO,CELLO

total cross section

JADE, TASSO,CELLO

total cross section

Excellent agreement with QED

Errors reflect statistics

QED deviation : s/Λ2 < 5% withs = 352GeV2

→ (~c)/Λ = (0.197GeV · fm)/Λ ≈0.13 · 10−3fm

N =∫

Ldt · σToday Bhabha is a luminositymeasurement

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