Relativistic Frames of Reference

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[math]\displaystyle{ \textbf{\underline{Navigation}} }[/math]

[math]\displaystyle{ \vartriangleleft }[/math] [math]\displaystyle{ \triangle }[/math] [math]\displaystyle{ \vartriangleright }[/math]

Relativistic Frames of Reference

From the Galilean description of motion for a frame of reference moving relative to another frame considered stationary we know that


Galilean Frames of Reference
Figure 2.1: Primed reference frame moving in the z direction with velocity v.


[math]\displaystyle{ t= t' }[/math]
[math]\displaystyle{ x=x' }[/math]
[math]\displaystyle{ y=y' }[/math]
[math]\displaystyle{ z=z'+vt }[/math]


Using Einstein's Theory of Relativity, we know that the speed of light is a constant, c, for all reference frames. In the unprimed frame, from the definition of speed:


[math]\displaystyle{ speed=\frac{\Delta Distance}{\Delta Time} }[/math]


[math]\displaystyle{ c=\frac{\Delta d}{\Delta t} }[/math]


where

[math]\displaystyle{ c=3E8\ m/s }[/math]

Using the distance equation in a Cartesian coordinate system, the change in distance becomes


[math]\displaystyle{ c=\frac{\sqrt{(\Delta x)^2+(\Delta y)^2+(\Delta z)^2}}{\Delta t} }[/math]




[math]\displaystyle{ \textbf{\underline{Navigation}} }[/math]

[math]\displaystyle{ \vartriangleleft }[/math] [math]\displaystyle{ \triangle }[/math] [math]\displaystyle{ \vartriangleright }[/math]