Relativistic Frames of Reference: Difference between revisions
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<center><math> | <center><math>\frac{(\Delta x')^2+(\Delta y')^2+(\Delta z')^2}{(\Delta t')^2}= c^2=\frac{(\Delta x)^2+(\Delta y)^2+(\Delta z)^2}{(\Delta t)^2}</math></center> | ||
This is possible since the ratios of distance to time are multiples of the same base, i.e. <math>\frac{3\times 10^8\ m}{s}</math> | |||
Revision as of 04:07, 3 June 2017
[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

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:
where
Using the distance equation in a Cartesian coordinate system, the equation for the speed of light becomes
Following the postulate of Special Relativity, this implies for the primed frame
We can rewrite this as
This is possible since the ratios of distance to time are multiples of the same base, i.e. [math]\displaystyle{ \frac{3\times 10^8\ m}{s} }[/math]
[math]\displaystyle{ \vartriangleleft }[/math] [math]\displaystyle{ \triangle }[/math] [math]\displaystyle{ \vartriangleright }[/math]