olgerm said:
These are quantities that describe location in SR-spacetime.
No, they aren't. We are not dealing with spacetime position vectors here--if we were, everything that has been written in this thread would be nonsense.
olgerm said:
I am not sure what kind of answer you espect.
In other words, you don't know.
The standard math of SR describes the worldline of a particle with a 4-
velocity vector, usually denoted ##u##, which is a unit vector tangent to the worldline at a particular event. If we have two particles in relative motion, we can choose the event to be the point in spacetime where they pass each other, and then we have two 4-velocity vectors ##u_1## and ##u_2##. Their dot product is ##u_1 \cdot u_2 = \gamma##, where ##\gamma## is the relativistic gamma factor corresponding to the ordinary "relative velocity" between the particles, i.e., ##\gamma = 1 / \sqrt{1 - v^2}##.
In terms of rapidity, we have ##\gamma = \cosh \alpha##, and also ##v = \tanh \alpha##. From this it is easy to calculate that ##\gamma v = \sinh \alpha##. So we have ##u_1 \cdot u_2 = \cosh \alpha##. Note that, since ##u_1## and ##u_2## are both unit vectors, we could indeed write the dot product as ##u_1 \cdot u_2 = |u_1| |u_2| \cosh \alpha##, since both magnitudes are ##1##. But ##\alpha## here, as has been said, is the rapidity; it is not an "angle in spacetime between the worldlines" in any useful sense, since it is not limited to the range ##0## to ##2 \pi##.