I am searching for formulae to convert Euclidean distance into hyperbolic distance.
The problem that I am confronting is that I want to calculate if a bug travels $x$ units in Euclidean space, how much distance would that be in hyperbolic space. I am aware of the following formula
$$d_h\ =\frac{\sinh ^{-1}\left(\frac{\sqrt{\left| k\right| } d_e}{2}\right)}{\sqrt{\left| k\right| }}$$ where $k$: Gaussian Curvature, $d_e$ : Euclidean distance and $d_h$: hyperbolic distance.
[there is a formula from Poincaré disk
$$d_h\ =2 \tanh ^{-1}(r)$$ where $r$ is distance from the center of the disk.
But it is not very helpful since Euclidean distance inside the disk is limited by the size of the disk]
Are there other formulae, which can convert any Euclidean distance into hyperbolic distance?
Thank you!
Thanks Andrey. I have a thought about comparing Euclidean world with hyperbolic world at least from the point of view of distance covered by the bug. See if this makes sense. Please tell me if I am completely off the mark.
In any unit disk model of hyperbolic world (Poincaré, Klein etc.) we have no comparison of Euclidean world since it is constrained by the size of the disk. How about if we create a unit disk model of Euclidean world [like A Euclidean Model for Euclidean Geometry by Mader ].
In this Euclidean model if we assume the distance from the origin of this disk along the diameter to be $r$ where $r<1$ and Euclidean distance in Euclidean space to be $d_e$. Now $d_e$ and $r$ are related by $d_e=\frac{r}{\sqrt{1-r^2}}$which is $r=\frac{d_e}{\sqrt{1+d_e^2}}$
If we now superimpose this disk on Poincaré disk and again assume $r$ to be the distance from the origin along the diameter in Poincaré disk. We know $d_h=2 \tanh ^{-1}(r)$. If we substitute $r$ with $r=\frac{d_e}{\sqrt{1+d_e^2}}$ we get $$d_h=2 \tanh ^{-1}\left(\frac{d_e}{\sqrt{d_e^2+1}}\right)$$.
Will this be a reasonable way to compare Euclidean distance covered by the bug with hyperbolic distance?