00:02
Okay, so i like this problem.
00:05
Basically, here you have, again, the same players in the story, a shell, a charge in the middle.
00:15
However, the shell has a nice property that its density changes as you go outward.
00:22
So it gets smaller and smaller.
00:25
So row equals a over r.
00:31
And you're given that this charge in the middle is 45 femtoculomes and you're given a so plot spoiler alert i think that's the only one that you actually need just two centimeters and never too early to convert a number to si so 0 .02 meters and the goal is to get figure out what a is such that this um the field is spatially uniform even though the charge density isn't.
01:18
So basically first we need to solve for the field within here.
01:22
So we're going to use galses law to do that.
01:25
I'm going to do that on the next page.
01:29
Oh, why are there three? okay, well now i'm on two.
01:33
Okay, so gouse's law, i'll redraw the sphere.
01:41
You want to put your gaussian surface within here.
01:47
And so this is, now we're going to be able to see.
01:50
Evaluating the electric field at some radius are.
01:55
So start with our usual gauces law.
01:59
So e times the integral of e .da equals q and closed over epsilon not.
02:10
And a is, we chose our galsian surface nicely such that it was, excuse me, such that the integral is a constant.
02:26
So it doesn't change river space.
02:31
And the integral of da is just 4 pi r squared.
02:35
The dot product of e and da are the same everywhere along our surface.
02:41
And so, yeah, we get this left side, which you've probably seen before.
02:46
But q enclosed is a little more complicated because q is changing in space.
02:51
So we do need to integrate to figure out that.
02:53
So i'm going to kind of do this side integral over here.
02:56
I'll do it in blue because i kind of anticipate a lot of stuff on this page.
03:03
So q and closed, it's just in general, it's the integral of the density times a dv -d -volume element.
03:12
And our density is a over our, oh, look at that integral sign.
03:17
And the element of, like the differential element for spherical coordinates, especially, especially one that's symmetric, asymmutally, and with respect to all angles, basically, that's going to be r -squared 4 -pi dr.
03:41
So hopefully you've seen that in some kind of calculus class.
03:46
So that cancels that, and then we can pull our 4 -pi out.
03:51
And the bounds of our integral are from r to a, because that's where the charge is.
03:57
So it's just an integral of r...