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This seems unnecessarily complicated. The quick way is to note that the world-line of an observer with constant proper acceleration is necessarily a hyperbola because anything else would not have constant curvature (just as a curve of constant curvature in Euclidean space is a circle). We therefore have (up to spacetime translations)Yuras said:I was totally sure I'll find it on wikipedia, but it's not there... Had to come up with something on the fly, so don't expect too much.
Basically you calculate hyperbolic angle (aka rapidity) between the initial 4-velocity ##u_0## and the current one ##u##. Start with their inner product ##cosh(w)=u_0\cdot u## and differentiate it by the proper time:
$$sinh(w)\dot w=u_0 \cdot \dot u = |\dot u| sinh(w)$$
The last step is analogous to ##cos(\frac{\pi}{2}+w)=-sin(w)## (note that ##u## and ##\dot u## are orthogonal). I don't know hyperbolic trigonometry enough to justify it right now, so I'm hand waving here, but in practice you of course just calculate ##u_0\cdot\dot u## in the reference frame of ##u##:
$$u_0\cdot\dot u=
\begin{pmatrix}
cosh(w) &
sinh(w) &
0 &
0
\end{pmatrix}
\cdot
\begin{pmatrix}
0 \\
|\dot u| \\
0 \\
0
\end{pmatrix}
$$
It's a bit of a cheating, but the statement itself is coordinate independent anyway.
One way or another, after cancelling ##sinh## we get the following:
$$\dot w = |\dot u|$$
If the (magnitude of the) 4-acceleration is constant, then we just have uniform hyperbolic rotation, i.e. a hyperbola.
Note that this method handles variable acceleration as long as it stays in the same plane as ##u_0## and ##u##. For more general case you have to stop before the last step:
$$sinh(w)\dot w=u_0 \cdot \dot u$$
(I really hope I didn't make any silly mistake, and all the above actually makes sense :) )
$$
t^2 - x^2 = - 1/a^2
$$
(the RHS must be negative for the hyperbola to be time-like)
It is simple to verify that ##a## is the proper acceleration:
Parametrize the hyperbola using the hyperbolic one*
$$
t = \sinh(as)/a, \quad x = \cosh(as)/a
$$
This gives ##dX/ds = (\cosh(as),\sinh(as))## which has norm 1 and is therefore the 4-velocity ##V## with ##s## being the proper time. It follows that
$$
A = \frac{dV}{ds} = a (\sinh(as), \cosh(as))
$$
which squares to ##\alpha^2 = -A^2 = a^2##.
* Here I obviously chose ##as## as the argument of the hyperbolic functions because I know that makes ##s## the proper time. However, it is also easy to make this a reasonable guess or just use a rapidity ##\theta## as the argument. In the latter case it immediately follows that rapidity is ##as## by rescaling to normalize 4-velocity (##\theta = as## this is the relativistic generalization of ##v = at## for constant proper acceleration).
The bottom line is you don’t have to delve deep into differentiating gamma factors and solving an ODE in ##t## to solve the case of constant proper acceleration.
Edit: ##\LaTeX## versions of the hyperbolic functions exist: \sinh -> ##\sinh## and \cosh -> ##\cosh## etc.