Undergrad Affine parameter and non-geodesic null curves

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The discussion centers on the characteristics of a specific non-geodesic null curve in flat spacetime, defined by a parametric equation involving a positive constant R. It is established that this curve remains null, satisfying the conditions for both the first and second derivatives with respect to any monotonic reparametrization. The conversation explores whether an affine parameter can be defined for non-geodesic null curves, noting that existing criteria for affine parameters in timelike, spacelike, and null geodesic cases may not apply. A proposed solution suggests that the time coordinate in the reference frame can serve as an affine parameter due to the symmetry in the Euclidean length over uniform intervals. The discussion concludes with the acknowledgment of the unique challenges presented by non-geodesic null curves.
JimWhoKnew
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Is there a sensible way to define an affine parameter for non-geodesic null curves?
Consider the curve (thanks to SE) in flat spacetime, given in Cartesian coordinates by$$x^μ(λ)=\left(λ , R\cos\frac{\lambda⁡}{R} , R\sin\frac{\lambda}{⁡R} ,0\right)$$where ##~R~## is a positive constant. At each point$$\dot x^\mu \dot x_\mu=0$$so it is a null curve but not a geodesic (not a straight line). It also satisfies$$\ddot x^\mu \dot x_\mu=0 \quad .$$If I got the calculation right, it turns out that for any reparametrization ##~\lambda'~## , where ##~\lambda'(\lambda)~## is an arbitrary monotonic function, ##~\dot x^\mu \dot x_\mu=\ddot x^\mu \dot x_\mu=0~## holds in this particular case (dots here w.r.t. ##~\lambda'~##).

Is there a sensible way in which we can define an affine parameter for non-geodesic null curves like this, such that certain parametrizations are affine while others are not?

Edit: (We have criteria for parameters to "be affine" in the cases of timelike/spacelike curves and null geodesics. Is the non-geodesic null curve an exception?)
 
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For the particular example in OP, I think that the time coordinate ##~t~## of the specific reference frame can be regarded as an affine parameter. Because of the symmetry (the Euclidean length traced in each uniform interval ##~\Delta t~## is the same).
 
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