For , choose and parametrize one clockwise orbit by and . Over , the relativistic charged-particle action is
The same formula with applies for either orbit orientation.
Lorentz-force equation from the worldline action Created 2026-09-24 Updated 2026-09-24
Varying the relativistic charged-particle action with fixed endpoints gives
or the equivalent raised-index equation.
Use Minkowski spacetime signature and write . The reparametrization-invariant relativistic charged-particle action is
The first term is because
An electromagnetic gauge transformation is
It leaves the electromagnetic field tensor unchanged because antisymmetrized second derivatives commute. The action changes only by
This endpoint term has zero variation for fixed endpoints, which is the gauge invariance of the charged-particle worldline action.
Because is constant, . The coordinate speed along the circle is consequently
so
For the convention in the question, take , so and .
On the circular solution, the free part of the relativistic charged-particle action is
In the gauge , the interaction is the closed line integral
The orbit is clockwise for , so . Thus
Combining the two terms and using gives the charged-particle action over one relativistic cyclotron orbit
Although the intermediate magnetic line integral depends on the chosen magnetic vector potential, the closed-orbit result is gauge invariant.
For a timelike worldline, . Its square root is a Lorentz scalar, and
Thus the first term is the Lorentz-invariant free-particle action . Written as a line element, it is also invariant under a change of the worldline parameter .
The interaction is the scalar line integral
Under an electromagnetic gauge transformation
it changes only by
This endpoint term does not affect a fixed-endpoint variational problem. Hence both Lorentz invariance and gauge invariance select the displayed relativistic charged-particle action, with the expected free-particle and minimal-coupling terms.