The trajectory of an observer with a uniform proper acceleration $a$ (Rindler) in an inertial frame $(t,z)$ can be described by the hyperbola \begin{equation} \left(z+\frac{\gamma_{0}}{a}\right)^{2} - \left(t+\frac{\gamma_{0}\beta_{0}}{a}\right)^{2} = \frac{1}{a^2}\,, \end{equation} where $\beta_{0}$ is the initial velocity and $\gamma_{0} = 1/\sqrt{1-\beta_{0}^{2}}$ the initial Lorentz factor. Plotting this gives the following figure.
There is, of course, another hyperbola when you rotate this hyperbola by $90$ degrees and I'm interested in studying this situation. Purely mathematically, this hyperbola gets described by \begin{equation} \left(z+\frac{\gamma_{0}}{a}\right)^{2} - \left(t+\frac{\gamma_{0}\beta_{0}}{a}\right)^{2} = -\frac{1}{a^2}\,, \end{equation} where there is now a minus sign in the right hand side and is plotted below.
However, this makes not much sense since in this (superluminal) regime, the initial velocity $\beta_{0}$ is larger than one such that the initial Lorentz factor $\gamma_{0}$ becomes imaginary.
My question is if there is a way to work around this. How can we describe this regime such that it physically also makes sense?