JDude13
- 95
- 0
So I was bored and decided to find some simple equations to deal with relativistic geometric edges and angles at an angle to the direction of movement.
L=L_0\sqrt{(\frac{\cos(\Delta\theta_0)}{\gamma})^2+(1-\cos(\Delta\theta_0)^2)^2}
\Delta\theta=\tan^{-1}(\gamma\frac{\sqrt{1-\cos(\Delta\theta_0)^2}}{\cos(\Delta\theta_0)}
Where
L is the relativistic length of the edge
L_0 is the rest length of the edge
\Delta\theta is the “relativistic angle” between the edge and the direction of motion.
\Delta\theta_0 is the “rest angle” between the edge and the direction of motion.
\gamma is the Lorentz factor of the object, \frac{1}{\sqrt{1-\beta^2}}
Tell me what you think.
L=L_0\sqrt{(\frac{\cos(\Delta\theta_0)}{\gamma})^2+(1-\cos(\Delta\theta_0)^2)^2}
\Delta\theta=\tan^{-1}(\gamma\frac{\sqrt{1-\cos(\Delta\theta_0)^2}}{\cos(\Delta\theta_0)}
Where
L is the relativistic length of the edge
L_0 is the rest length of the edge
\Delta\theta is the “relativistic angle” between the edge and the direction of motion.
\Delta\theta_0 is the “rest angle” between the edge and the direction of motion.
\gamma is the Lorentz factor of the object, \frac{1}{\sqrt{1-\beta^2}}
Tell me what you think.
Last edited: