Lecture #1: Quantum electrodynamics

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Lecture #1: Quantum electrodynamics QED Lagrangian and Hamiltonian, equation of motion, scattering matrix, perturbation theory, Feynman rules, probability and effective cross section. Let us recall certain facts. Free electron, Dirac equation: 0 ) ( = x m x i ψ γ μ μ , or ( ) 0 ) ( = / x m p ψ , where μ μ μ μ γ x i p p p = = / , Solution for a free electron - flat wave*spin factor, corresponding to different helicity states (λ/2): ipx e p u x = ) ( ) ( λ ψ , where + + = λ λ λ χ ε λ χ ε m p m p u | | ) ( , = = + 1 0 , 0 1 χ χ More importantly (and very usefully!) = ± / = ± ± 2 , 1 ) ( ) ( λ λ λ m p p u p u Dirac equation for interacting electron: A e p p / + / / , ) ( μ μ μ μ μ μ μ γ γ γ eA x i A e x i + = + = 0 ) ( ) ( = + x m x eA x i ψ γ μ μ μ Photon- quantum of EM field: νμ μν F F = , l ikl ik H F ε = , i i iE F = 4 Or ν μ μ ν μν x A x A F = In vacuum: 0 ) ( = x F x μν ν Solution for free photon – flat wave*spin factor (s=1): ikx e k e A = ) ( μ μ , where μν ν μ μ δ = = e e k e * , 0 Interacting photons == Maxwell’s equations: (HW: show that this indeed is the case): ) ( ) ( x j x F x μ μν ν = ) ( ) ( ) ( x x e x j ψ γ ψ μ μ =

Transcript of Lecture #1: Quantum electrodynamics

Page 1: Lecture #1: Quantum electrodynamics

Lecture #1: Quantum electrodynamics QED Lagrangian and Hamiltonian, equation of motion, scattering matrix, perturbation theory, Feynman rules, probability and effective cross section. Let us recall certain facts. Free electron, Dirac equation:

0)( =⎟⎟⎠

⎞⎜⎜⎝

⎛−

∂∂ xmx

i ψγµ

µ , or ( ) 0)( =−/ xmp ψ , where µ

µµµγ xippp∂∂

==/ ,

Solution for a free electron - flat wave*spin factor, corresponding to different helicity states (λ/2):

ipxepux −= )()( λψ , where ⎟⎟⎟

⎜⎜⎜

+

+=λ

λ

λ χελ

χε

mpmpu ||)( , ⎟⎟

⎞⎜⎜⎝

⎛=⎟⎟

⎞⎜⎜⎝

⎛= −+ 1

0,

01

χχ

More importantly (and very usefully!) ∑=

±/=±±2,1

)()(λ

λλ mppupu

Dirac equation for interacting electron:

Aepp /+/→/ , )( µµ

µµµµ

µ γγγ eAx

iAex

i +∂∂

=+∂∂

=

0)()( =⎪⎭

⎪⎬⎫

⎪⎩

⎪⎨⎧

−⎟⎟⎠

⎞⎜⎜⎝

⎛+

∂∂ xmxeAx

i ψγ µµ

µ

Photon- quantum of EM field: νµµν FF −= , liklik HF ε= , ii iEF −=4

Or ν

µ

µ

νµν x

AxAF

∂−

∂∂

=

In vacuum:

0)( =∂∂ xFx µνν

Solution for free photon – flat wave*spin factor (s=1): ikxekeA −= )(µµ , where µννµµ δ== eeke *,0

Interacting photons == Maxwell’s equations: (HW: show that this indeed is the case):

)()( xjxFx µµνν

=∂∂

)()()( xxexj ψγψ µµ −=

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Lagrange equation for field φ :

,0,

=∂∂

−∂∂

∂∂

φφ µµ

LLx

where µµ

φφ ,=

∂∂x

We need a Lagrangian that will give us both Dirac and Maxwell equations (HW1):

ψγψ µµ

µµυ

µυ⎪⎭

⎪⎬⎫

⎪⎩

⎪⎨⎧

−+∂∂

+−= meAx

iFFL )(41

To decouple free particle pieces and interaction pieces let us rewrite it as

ψγψψγψ µµµ

µµυ

µυ eAmx

iFFL +⎪⎭

⎪⎬⎫

⎪⎩

⎪⎨⎧

−∂∂

+−=41

Interaction Lagrangian: µµµµ ψγψ AjeALI −==

Interaction Hamiltonian:

∫−= xdLH II3

Scattering matrix )(),()( −∞Φ−∞∞=∞Φ S

Perturbation theory tells us:

),()(),( 00 ttStHttSt

i I=∂∂

The solution in its exact form:

∫∫ =⎟⎟⎠

⎞⎜⎜⎝

⎛−=

+∞

∞−

))(exp()(exp 4xdxLiTdttHiTS II

Please note that in its exact form the S-matrix is always unitary: ),exp(iR where R is real. If the interaction is weak we can use the perturbative expansion of the exponent:

))()...()((...! 21

42

41

4)(nIIIn

nn xLxLxLTxdxdxd

niS ∫∫∫=

Thus, knowing (effective) Lagrangian one is able to write the scattering matrix. Or, closer to home

∫ /××/×/−

= nnnn

nn xdxdxdxxAxxxAxxxAx

nieS 4

24

14

222111)( ...)()()(...)()()()()()(

!)(

ψψψψψψ

Matrix element for process iàf can be written as fSiM n

if || )(= Each fermion’s wave function can be written as a sum of creation of fermions with certain quantum numbers ( sa )and destruction of antifermions ( sb+ ). Similarly, each antifermion’s wave function can be written as a sum of creation of antifermions with certain quantum numbers ( sb ) and destruction of fermions ( sa+ ):

Page 3: Lecture #1: Quantum electrodynamics

)(0|)(|1),(1|)(|0

),(0|)(|1),(1|)(|0

)()()(

;)()()(

)()(

)()(

)()(

)()(

xxxx

xxxx

xbxax

xbxax

rrrrrr

ssssss

rrr

sss

rrr

sss

−−−−−−

++++++

−++

−++

==

==

+=

+=

∑∑

∑∑

ψψψψ

ψψψψ

ψψψ

ψψψ

Now, in the expression for S we need to move all creation operators to the right and destruction operators to the left. Mind that bosons (photons) commute, while fermions (electrons) anticommute, thus you get a negative sign every time two fermions change place. Normally it does not matter, because we are interested in the square of the matrix element. It does matter when we’ll need to consider interference between two or more diagrams. Need to be careful with the relative sign of permutations. Field operators in momentum representation:

Inner photon line (Fourier transformation of the Green’s function))0(

)( 2 ikig

kD+

−= µν

µν

Massive boson )0()/(

)( 22

2

iMpMppgi

pD+−

−−= νµµν

µν

Inner electron line 0)(

0)( 22 imp

mpiimp

ipS+−

+/=+−/

=αβ

Photon operators )(1|)(|0 λµλµλ exA =

*)(0|)(|1 λµλµλ exA =

Electron operators )(1|)(|0 )()( pux µµµ ψ =++

)(0|)(|1 )()( pux µµµ ψ =++

)(1|)(|0 )()( pvx −=+− µµµ ψ

)(0|)(|1 )()( pvx −=−− µµµ ψ

Photon-fermion vertex µγie - energy momentum conservation at each vertex. But… Internal lines do not have to be “on mass shell”. 22 mp ≠ !!! Useful gamma-matrix trivia:

)(4)( ,0)#(4)( ,41

,

)( ,

0000

0

000

νσµδνδµσσδµνδσνµ

µννµ

µµµµ

γγγγγ

γγ

γγγγγγγγ

γψψ

γγγ

ggggggTroddTrgTrTr

I

+−==

==

==

=

==

++

+

+