UNIFYING CHART 3: QED/FIELD THEORY OVERVIEW

Part 1.  From Field Equations to Propagators and Observables

Heisenberg Picture

 

 

Spin 0

Spin  

Spin 1

Free field equations

 

 

 

Lagrangian density, free

 

 

Minimal substitution

Not treated here  

 In free Lagrangian (density):   

Lagrangian, free plus interactions

Not treated here

      

Interacting fields equations

Not treated here

 

 

Conjugate momentum

 

 

 

Hamiltonian density

 

 

Free field solutions

 

 

 

Discrete eigenstates

(Plane waves, finite volume or periodic B.C.’s)

 

 

 

Continuous eigenstates

(Plane waves, infinite volume, no B.C.’s)

 

 spinor indices on ur, vr, and ψ  suppressed.  r = 1,2.

 

Second quantization

                  Ψr = any quantized field

All other commutators = 0.    Anti-commutator for spin  fields (use plus sign.)

 

  FREE FIELDS ONLY   

 

Using conjugate momenta expressions in the second quantization relation above yields

Equal time commutators

 

 

outer product, spinor indices α, β shown with α,β = 1,2,3,4.

 

 

Using free field solutions in the above and the 3D Dirac delta function (e.g., for discrete solutions,  ) yields the coefficient commutators (below).

Coefficient commutators

 

 

 

discrete

 

 

 

continuous

 

 

 

 

Using the free field solutions in the LHS below (covariant field commutators) and the relations above yields RHS of below.  (Note that different authors define the terms below slightly differently.)

Covariant commutators, continuous only

 

 

 

3-momentum space form

 

 

 

contour integral form

 

 

 

 

The coefficient commutation relations used with the Hamiltonian acting on states lead to creation and destruction operator interpretation of the coefficients and to the number operators below.

Operators:

 

 

 

creation

 

 

 

destruction

 

 

 

number

 

 

 

tot partic num

 

 

 

particle num:

lowering

 

 

 

raising

 

 

 

Normaliz factors

lowering

 

 

as with scalars

raising

 

 

as with scalars

 

Operations on states with creation, destruction, and number operators above yield the properties below.

Properties of states:

 

state symmetric under particle exchange, Bose-Einstein stats

 

state changes sign under particle exchange, Fermi-Dirac statistics

 

state symmetric under particle exchange, Bose-Einstein stats

Four currents (operators)

 

 

 

      = 0 for photons  

 

Emphasis in field theory is usually on the number of particles (N(k) operator), and particle probability densities are rarely used.  For completeness, however, and to make the connection with quantum mechanics, they are included below.  (Antiparticles would have negative values of those below!)

Single particle probability density (not operator)

 Note integration over , not x

For plane wave,  

As at left, but with Dirac j0 above.

= 0 for chargeless particles.  Led to conclusion that j0 is really proportional to charge probability density.

 

Creation and destruction of free particles (& antiparticles) and their propagation visualized below.

Feynman diagrams

 




Time ordered operator T

If ty < tx , , i.e., the  operates first, and should be placed on the right.

If tx < ty , , i.e, the  (x) operates first, and should be placed on the right.

Note that  (x) commutes with .   [Fermions would anti-commute.]

 

The operator fields in the T operator below will create and destroy kets on RHS.  In the wave mechanics formulation, bracket integration is over the dummy  variable in the bra and ket, not x,y of T operator. 

Transition amplitude density

 

 

 

The above represent both

1)      creation of a particle at y, destruction at x, and

2)      creation of an antiparticle at x, destruction at y

 

Fields such as  represent integration over all momenta.  The transition amplitude (density) above for fixed x and y equals the Feynman propagator  between x and y.  Note this is a number, not an operator.  Only the continuous field solutions are relevant as no boundary conditions exist in this case.

 

 

 

 

Feynman propagators

 

 

 

 

Evaluating the above in complex space and taking certain limits with contour integrals yields a form for Feynman propagators which works for any time ordering and will prove more convenient.

in physical space