When we defined the velocity above, we took dX/dt where dt refers to our "stationary frame" clock. Perhaps we should refer to the moving clock, dt'=dt/γ (moving clocks run slow) then
Think about it... now every frame should get the same result because all use the same clock ... the clock attached to the object. The time atached to the object is called the proper time and is usually denoted τ instead of t'. This is why you get the same value for the norm².
Now evaluate V² in the rest frame where v=vi=0 and γ=1 and we get ... c² again! But now if we apply a Lorentz X-boost of B you should get ß'=(ß+B)/(1+ßB) where ß=speed in S and B is speed of S w.r.t. S'....See what you get if you give a particle two boosts.
The spacelike part mγv reduces to the "usual" definition of momentum
Next, define the timelike part mγc=E/c that is, define the relativistic energy E=mγc².
Recall γ=(1-β²)½~1+½β²+... for small β²=v²/c².
Then the relativistic energy becomes E=mc²+½mv²+...
The ½mv² you recognise as the kinetic energy K in nonrelativistic mechanics. We should really define K=E-mc².
The mc² you recognise as Einstein's E=mc², and it is! mc² is the rest mass energy.
We have E=mγc² and p=mγv (p and v are magnitudes)
the ratio p/E=v/c² or p=Ev/c². For photons v=c and p=E/c.
Also, E2-p2c2 = m2γ2c4-m2γ2v2c2 = m2c4γ2(1-v2/c2) = m2c4.
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