Minkowski Spacetime


This section requires some knowledge of calculus, and possibly vectors as well. If you do not understand integration, try our page on Bondi k-calculus


Minkowski spacetime was developed shortly after Einstein published his paper on the theory of special relativity. It extends the 'standard' equations of relativity to arbitrary paths through space, and is best suited to regions of space devoid of large amounts of matter and energy.
 

In space, Pythagoras' theorem states that if a line has components along the x,y, and z axis of dx,dy, and dz respectively, then the total length of the line, ds, is given by

ds2 = dx2 + dy2 + dz2


In Minkowski spacetime, this equation is changed slightly to

ds2 = c2 dt2 - ( dx2 + dy2 + dz2 )

where dt is the component of the line along the time axis.

Now suppose A is a nonaccelerating observer travelling along the time axis. (So their position is constant for all time) Suppose that B travels at a constant velocity, v , along the x-axis with respect to A.

The velocity, as every novice physics student knows, is v = dx/dt where dx and dt are changes in position and time. Thus, using the distance defined above,

ds2 = c2 dt - dx2= c2dt2(1 - v2/c2)

So the length of B's path is a constant multiple of A's length as assumed in Bondi's k-calculus! The key to using Minkowski spacetime is knowing (without proving here) that the time experienced by an observer is related to the length of its path in spacetime. Actually,

dT2 = ds2 / c2

which gives the standard equation of relativity:

dt = dT / (1-v2/c2)1/2




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