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So now that has come to an exercise for you, we want to calculate the electric field and the electrostatic

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potential for a charged sphere so the tasks that you have to solve are calculate the electric field

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of a homogeneously charged sphere.

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And as a hint, you have to distinguish the inside region of the sphere and the outside region of the

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sphere.

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And you should use the rotational symmetry of the problem to make it a lot simpler for you to solve

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the integral.

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And you have to consider that homogeneously charged means that this row here it is charged density is

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constant.

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So it means you can pull it out of the integral.

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And then the second task is quite easy when you have determined the electric field from the electric

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field to calculate the electrostatic potential.

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So if you want to have another Hynde's, please keep on watching the video, otherwise you can now stop

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the video and go ahead and solve the problem yourself.

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So the bigger hint is that, of course, we have already solved this problem for the region outside

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of the sphere.

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So this was as a solution to Coulomb stop where we have integrated here over the charged density and

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got to that charge.

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Q And on the left hand side, we could pull out to the electric field because we have this dependence

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artist, a cemetery where the electric field is always pointing along the radio direction.

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So this vector here is parallel to the vector from the integral.

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And so this term here would just be the surface of the sphere that we are considering for our integration.

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And so this gave us the electric field, which is proportional to you, divide divided by our square.

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So the first part we have actually already solved, but still it's a nice exercise to do it yourself

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once again.

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And now what is about the region inside of the sphere?

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So this you really have to do yourself.

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So please post a video and just continue when you have tried for a few minutes.

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So since this is the first time you are doing this, please don't expect to be able to solve it just

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right away, because even though it may be easy, once you have seen the solution, sometimes it can

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be quite difficult to get the right idea and to come up with a solution.

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So please don't give up.

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Just really spend some minutes trying to solve this.

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And when you've done it or when you need more hints, please continue the video.

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And now I will present you the solution.

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So everything that we need is the Maxwell equation and its integral formulation.

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So this one here, then we need the symmetry of the problem, which allows us to write down the electric

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field as a scalar function multiplied by this vector are.

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So it means the electric field is always pointing along the radio direction.

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And so this means that this is always parallel to this D.R.C. here.

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Now, in previous light, I have already shown you what the solution looks like outside of the sphere,

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so this means this small R is larger than this capital R, which is the radius of the sphere.

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And so our right hand side of this solution is always the volume of this sphere.

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So it is four divided by three times PI times capital R to the power of three.

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And in this charge density and of course this one, we could also write down as the inclosed charge,

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but it's not really necessary.

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Now, the left hand side you can see here, I've already pulled out this E of our so we are just left

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with the surface integral of the way of the sphere that we are considering here.

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So this would be this black Dasht sphere with the radius small R and not capital R, so the surface

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of a sphere is four pi times the radius square.

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So this is what we have here.

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So as you have seen on the previous slides, this is already a solution.

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We just have to divide by Epsilon zero by four pi r square.

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And so this is the solution that we come up with so we can express it like this or we can reintroduce

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the inclose charge and then we get the result that we had previously.

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Now, if you have the solution, it is not so difficult to find a solution for the inside region.

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The main difference here is that the right hand side of this equation looks different because here the

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right hand side of this equation was always the volume of our charge, so of our charged sphere.

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So this is because this road density is only finite for this sphere.

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And in this wide region here, it would be zero.

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So it would not contribute here to this integral.

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However, now if we look on the inside, this black Dasht sphere here would be inside of this blue sphere.

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So this means now the radius of the black sphere really plays a role.

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So this means here for this integral, we do not have to consider the radius of the black out of the

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blue sphere capital R, but we have to consider the radius of the black sphere smaller.

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So this means here the left hand side is exactly the same, but the right hand side is now four pi four

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divided by three times pi times smaller to the power of three times real.

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And this means that this is now our solution, so why we had to hear a one of our square dependent's

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we have now here and our dependence, and this is, of course, because here instead of this capital,

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are we have now a small R and so these power of three and this power of two, they council and we are

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left with power of one.

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Now we can look at this electric field and you can see that on the inside we get our dependence.

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So it's a linear function.

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It increases, which is, of course, because when we go far away from the center of this sphere, we

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have more a charge generating these electric fields.

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So this means here we have this linear increase in the electric field.

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And when we are outside of the sphere, the electric field decreases with the power of one over R to

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the power of two.

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And at the position are we can also calculate the value.

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This would be divided by three epsilon zero times capital R.

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And as you can see, this is this value we get from both solutions, of course, because the electric

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field has to be steady.

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So here we would get capital R straightforwardly and here we would get R to the power of three divided

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by R to the power of two, which gives us the same value.

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Now, the second task was calculate the electrostatic potential, and so here we just have to take our

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solutions from inside and outside of the sphere for the electric field.

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And now we have to calculate the electrostatic potential by this equation here.

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So basically, we just have to integrate over the electric field.

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So here we get as a solution that we get here an exponential of this hour that is increased by one.

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So instead of R to the power of minus two, we get R to the power of minus one or we can write it down

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as one of R and then we would also get a minus sign.

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But he is also a minus sign.

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So these cancel out.

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So this is what we get for the electrostatic potential.

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And of course, you can remember that we could add here any constant to this electrostatic potential

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because we can shift our zero position of the electromagnetic potential as we wish.

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But here I have chosen it such that it is zero when we take the position vector to infinity.

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So if you go with R to infinity, this whole thing here would go to zero, which is something that,

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yeah, looks good or makes sense physically, but it's actually not that important.

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It's important that you have this term and then you would have here another constant possibly.

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Now for the inside region, we also have to integrate here.

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So what we get is we have to increase this exponent here so we get all square and then we have to divide

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by two.

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And then also we get you just minus sign from this minus sign.

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So this is what we get for the electrostatic potential.

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But also we get here another constant.

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And now this time the constant is really important because at the position are is equal to capital.

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Are these two electrostatic potentials need to match each other.

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So it must be a continuous function.

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So if we have assumed here that our constant is zero, we can now determine the constant here so that

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these to match at the position are equal capital R so you can see that this solution and we can also

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write it like this.

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And if you now put in here to Capital R, you will see that you will get here two times Capital R Square.

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So you get real divided by three Epsilon, zero Times Capital R Square and you, you get the same thing

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because you used to cancel out and we are only left with a capital R Square.

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And so this is what the electrostatic potential looks like.

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So it keeps on decreasing yappers basically because of the shape of our electric field on the previous

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slide.

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And then we have here a continuous function and to position R, which is really important.

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So I'm just saying this one more time.

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You could add here a different constant and then you would have to add here the same constant additional

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to this constant.

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So when you plot your electrostatic potential, it should look exactly like this, but this whole function

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could be shifted by any value.
