00:01
All right, so let's say we have a formula for the relativistic doppler effect.
00:06
And so this is our source frequency times the square of 1 minus v squared over c squared, divided by 1 minus v over c times the cosine of theta.
00:18
So if you have a ray of light moving with respect to, or a source emitting light, excuse me, if that's a, you know, traveling to the speed v, then in the case where they are parallel or anti -parallel, theta, or let's take the case where they're parallel, theta is going to be zero in that case.
00:40
And so the coasts or anti -paralleled, actually kind of like, the only difference would be a negative sign.
00:46
The cosine of zero is one.
00:50
And so in this case, this frequency, we would just plug in as a one for the cosine.
00:54
So what we'll get is the square root of 1 minus v squared over c squared over 1 minus v over c.
01:02
And the numerator we can write as the square root of 1 minus v square, or sorry, square root of 1 minus v over c times 1 plus v over c...