Assume and put
The nonzero four-velocity equations are
with and . Hence
Integrating from the origin gives the uniformly accelerated trajectory
The light ray has . At interception, , so
A finite solution exists exactly when
Then
and, writing ,
At interception is approached only as , and for it never occurs. The limiting backward light ray is the Rindler horizon of the accelerated particle.
Again let . For , the Lorentz-force equations are
The sum is constant and initially equals . Therefore
A further integration gives
Eliminating between and yields
a semicubical parabola, with the physical branch selected by for the signs shown.

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