|Quantum Field Theory|
|... no spooky action at a distance (Einstein)|
|Relativistic Quantum Mechanics|| Klein-Gordon Equation|
|The Dawn of QFT|| Spinors|
Feynman Slash Notation
Conformal Field Theory
Countdown to the Standard Model
|From a framework to a model|| Yang-Mills Theory|
|Semi-Classical Gravity and the Dark Age|| Hawking Radiation|
Problems with the Standard Model
|Beyond the Standard Model|| Beyond the Standard Model|
Theory of Everything
|Related||De Donder-Weyl Theory|
Quantum Electrodynamics, or QED in short, is a Quantum Field Theory relating to Electromagnetism and Light. It is a weakly-coupled theory, with a Fine-Structure Constant of as it's Coupling Constant yet there is a need for Renormalisation. Quantum Electrodynamics has a gauge group of .
Lagrangian DensityEdit this section
Lagrangian Density of Quantum Electrodynamics
Field EquationEdit this section
To begin, substituting the definition of into the Lagrangian gives us
Next, we can substitute this Lagrangian into the Euler–Lagrange Equation of motion for a field:
to find the field equations for QED.
The two terms from this Lagrangian are then
Substituting these two back into the Euler–Lagrange equation (2) results in
with complex conjugate
Bringing the middle term to the right-hand side transforms this second equation into
The left-hand side is like the original Dirac Equation and the right-hand side is the interaction with the electromagnetic field.
One further important equation can be found by substituting the Lagrangian into another Euler–Lagrange equation, this time for the field, :
The two terms this time are
and these two terms, when substituted back into (3) give us
Now, if we impose the Lorenz Gauge Condition, that the divergence of the four potential vanishes
then we get
which is a Wave Equation for the four potential, the Quantum Electrodynamical version of the classical Maxwell equations in the Lorenz gauge.
RenormalisationEdit this section
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Interaction PictureEdit this section
This theory can be straightforwardly quantized by treating bosonic and fermionic sectors as free. This permits us to build a set of asymptotic states which can be used to start a computation of the probability amplitudes for different processes. In order to do so, we have to compute a time-evolution operator that, for a given initial state , will give a final state in such a way to have
This technique is also known as the S-Matrix. The evolution operator is obtained in the Interaction Picture where time evolution is given by the interaction Hamiltonian, which is the integral over space of the second term in the Lagrangian density given above:
and so, one has
where is the time ordering operator. This evolution operator only has meaning as a series, and what we get here is a Perturbation Series with the Fine-Structure Constant as the development parameter. This series is called the Dyson Series.