00:01
Here we're looking at the relativistic definition of momentum, that it is gamma times the classical expression, mv, where gamma, the lorentz factor, is a nonlinear function of the velocity.
00:18
It's one over the square root of one minus v.
00:23
C squared.
00:24
So we're going to start off and let our momentum work with v.
00:29
Over sea is 40 % the speed of light.
00:33
So in order to calculate the momentum, we need the gamma factor.
00:39
The lorentz factor is simply putting in 4 .4 o .c and dividing out the c.
00:50
We wind up getting something a little bit over one.
00:54
Classically, gamma is always identical to 1, and we get roughly 1 .091.
01:12
So almost 10 % away from exactly 1.
01:17
So we can now calculate our momentum is 1 .091 times 0 .4 aught aught times c times the mass of the particle.
01:46
Okay, now let's see what happens if we double the velocity...