Let a black-hole moves linearly at a constant speed, $v$. We set $x$-axis parallel to $v$.
I suppose $v$ is fast enough to cannot ignore the Relativistic effects.
My question.
How is the mathematical formula Schwarzschild radius of the black-hole when it moves linearly at a constant speed such that the Relativistic effects cannot be ignored.
Note: My question is focused on the mathematical expression how the Schwarzkopf radius changes by constant-velocity linear motion using mathematical expressions.
In the 3436, there are some discussion about "Can an object near the speed of light become a black hole (due to an increase in mass)"? However, in this question, it does not matter whether or not a black hole is formed.
Furthermore, no one has answered how the Schwartz-Schuld radius specifically changes- This is the core of my question-.
To make the question simpler, I restricted the question if the star was originally a black hole.
【Comments】 I tried to calculate using a formula that could be used. The results are as follows:
Let ${M}_{0}$ be a Rest mass of the star, $G$ be a constant of gravitation, and $c$ be the speed of light.
According to the Wikipedia. the Relativistic mass, $M$ is represented by the following formula:
$$M=\frac{M_0}{\sqrt{1-\dfrac{v^2}{c^2}}}$$
The Schwarzschild radius is represented by the following formula:
$$r_s=\frac{2GM}{c^2}$$
On the other hand, an object of length ${L}_{0}$ shrinks to length $L$ by the Lorentz contraction as follows. $$L={L_0}\sqrt{1-\frac{v^2}{c^2}}$$
Therefore, it might be $$r_s=\frac{2GM}{c^2}\sqrt{1-\frac{v^2}{c^2}}\ =\frac{2G{M_0}}{c^2}.$$