00:01
So for this problem, we want to start out by finding the joint pdf of x1 plus x2.
00:06
So we're using parameters and we have a pdf of x1 and a pdf of x2.
00:22
And both of the pdfs are the same.
00:25
So i'm going to write it like this, but you could do two separate ones.
00:29
And so we have parameter x because we're denoted this from one and two so if this was for two we would just say parameter two so we have parameter x times e times negative parameter lambda lambda y x1 and this is greater than some aspect of x so if this was x1 or x2 and this and there it's greater than zero and when we say that we're saying that it had to exist or it's otherwise zero and when you're trying to find a new random variable you're doing because that's what we're going to be doing you do you equals x1 plus x2 and then for v you have x1 over x1 plus x2 so let's keep that and let's remember that so we want to find the transformation and we're going to use this right here and so first we're going to consider v and then you so or we can start with you you is equal to x1 plus x2 so x2 is you and we're solving for you right now i mean we're solving for x squared so x squared it's u minus uv and the reason why that is is because you're going to see why in a second of why x1 changes i just wanted to show you kind of what we're going to be doing how we're going to be solving and so when we get to v it's x1 plus and you can't know v without you but i just want to show you the pattern so it's x1 plus x2 so when we're solving for x1 we bring it to that side and we have x1 plus x2 because we brought this one down there so next we are just going to solve.
03:11
And so x1 plus x2 is what? boom.
03:21
So this is supposed to be times.
03:26
So we have x1 is equal to vu.
03:33
And that's uv.
03:35
And so that's how when we get x1, then that becomes that.
03:38
And so that's how we find those random variables.
03:42
And so when we have that, we have let's write our new little piece of information that we need x1 is equal to uv and x2 is equal to uv u minus uv so now we need to calculate the jocobian transition and it's really hard and complicated well it's not hard and complicated but pretty much we have v here.
04:24
We have u...