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So let us now come to our exercises, and if you had problems calculating these examples, please don't

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feel discouraged, because the truth is in theoretical physics, the exercises are most often quite

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difficult and you have to spend a lot of time solving them, and especially you have to spend the time

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to get the right idea.

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So now I will present the solutions for the three examples.

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So the first task was about the electric field and point charges, and we had three different tasks.

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First of all, we had to write down the electric field of the positive charge and we had to draw the

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electric field lines that after we had to do the same thing with a negative charge, and then we had

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to consider a combination of two charge that half a distance of the length A.

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So first of all, let us write down the electric field for A and B, and in both cases, the result

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is directly given by the Cullum's law.

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So we have a one over R-squared dependence and here we have a positive charge plus.

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Q And here we get the same results but with a negative charge minus Q.

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And in both cases, we also want to know about the orientation, so here the orientation is always along

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the radial direction.

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So from the center where our charge is located, the orientation E.R. goes along the radial direction

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and it also determines the direction of the electric field.

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Now, for see, the result is actually quite simple to write down, because we want to consider our

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first charge plus queue at the position of zero.

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So it is just the field of eight and then the other charge is negative.

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So it's similar results to be, but it's displaced by a.

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So we have to account for this by shifting our vector here so we get our minus a square.

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And also we need to be very careful because the orientation is now different.

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It is still a radial orientation, but not with respect to zero, but with respect to the position of

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the second charge, which is displaced by a.

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So while this is written down, quite simply, it's actually very hard to really write down the exact

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form because of this R minus a vector here, which is different from E r, so we have to be really careful.

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And you will see later in this course we will determine the electric field of such a dipole.

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This is what it is called.

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But we can already draw the field lines, which is quite easy because we know that for a the field lines

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look like this.

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So it's along the radial direction.

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So they pointier away from the center of this CU charge.

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And for B it's the same thing.

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But just with it, with the different sine.

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OK, so now let's really consider these two charges as pears.

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So this is the solution for see where these are displaced by a distance of a.

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So what we have to do is we have to add up all of these vectors here.

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So, of course, they will also be vectors in this wide space here.

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So if we do this, we get something like this, which is the electric field of the dipole.

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Now, the second task was about the induction law, so we had to consider a current loop with an area

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of a square and it is dragged from outside of the magnetic field to the inside of a magnetic field,

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which is constant and is pointing along the perpendicular direction compared to just plain here.

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So we could say it's pointing along the Z direction.

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And what we want to do is we want to bring this current look inside of the field.

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So as you have just seen, we've brought it inside and then out again.

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But here in this example, we just want to bring it inside and we want to calculate the voltage that

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emerges.

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And as we have learned, the induction voltage is given by the temporal change, this derivative of

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the magnetic flux.

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So basically, all we have to figure out is the magnetic flux of this example.

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So the magnetic flux is given by this integral here where we have to integrate the magnetic fields in

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the area of this current loop in this area.

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And this this here is a vector that points along the Z direction.

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So it's parallel to be.

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So this means we can just calculate B times day.

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And since our yeah, our area does not change, we can also write it down as B zero times the area of

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aid that is inside of the field region.

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So now we just have to think about how does the field rate region change over time when we move this

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this loop here with the velocity of V?

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So of course the area that is included is given by the length A, which was this one here.

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And then we have another length which I called A in, which is the length of this side here that is

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inside of the field.

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So right now it is zero.

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But if you bring this loop completely into the field, then it is a and this of course, given by the

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velocity times the time because we considered a motion with a constant velocity.

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V So we have our flux which is given by that one, and we can easily calculate the partial derivative

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versus back to T.

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So it's just minus B zero times.

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Eight times V.

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Now, of course, you also have to consider that once this whole loop is inside of the field and you

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keep on moving it inside of the field, then the voltage will drop to zero.

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This is because then the flux will be constant.

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It will just be be zero times a day and then the time derivative will be zero.

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Now, the third task is a bit more difficult.

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So here we have to consider a straight wire that goes along the direction and we have the magnetic field

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that has a profile that is given by this by this polar direction.

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There's a certain cylindrical coordinates.

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So these we have discussed in the mathematical tutorial section.

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But even if you're not familiar with the with cylindrical coordinates, you can still solve this example

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if you just use this representation of this vector here in Cartesian coordinates.

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So it's it's helpful to know about cylindrical coordinates in this example, but it is not necessary.

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So what we have to do here is we have to take amperes law.

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And I just want you to check that it is correct so that this can be a correct solution.

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So we have to verify that the Kerl or the rotation of B is given by zero times to the current density.

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And here I have already given you a hint.

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It's very important to realize that our current density is zero everywhere, except for the position

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of the wire, which is for real equal to zero.

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So this means we have to verify that this one here is zero for every point except for row zero.

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So let's do it.

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And here you can see the whole solution.

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I mean, I already show you that result.

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But let me briefly go through this calculation.

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So what I have done here is just I have just written down the Knobler vector and then here we have the

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magnetic fields.

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And here I have used this F.I. vector, which is this one here, and I have used that row is given by

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the square root of X squared plus Y square.

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So this is sincere.

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We have row and here we have one overall, we get one overall square, which is why we have here X squared

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plus Y square.

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Now the next step I have calculated this vector product here and if you look at it carefully, you will

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see that this expression here only has a Z component.

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This is where you calculate the X derivative of the Y component of this one here, minus the Y derivative

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of the X component, which is this one here.

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So we get these two terms and in both cases we have to use the product rule because we have a product

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of X times one over X squared plus Y square.

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And both of these functions are X dependent here and here.

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So this means for both of these terms we get two additional terms.

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So, of course, the first one is very easy.

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We just have to differentiate X, which gives us one times the other function, which is one of X squared

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plus Y square.

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And then for the other derivative, we have to take X times the derivative of one over X squared plus

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Y square and one of X equals Y square is the same as saying in brackets X squared plus Y square to depart

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from minus one.

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So we have to multiply by minus one, increase the Powerball, but I just say decrease the power, which

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gives us power of minus two, which is this one here.

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And then we have to account for the inner derivative, which is 2x X, which is this one.

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And then we do the same thing for the other component.

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We have to I have to apologize.

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Here's a mistake.

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This is not X, this is, of course, Y and this is X.

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There's a I've made a typo when I wrote down the equation.

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So this one must be y times to Y divided by X squared plus Y square squared.

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OK, so if we have done this, we have this term here twice, so we have to over X squared plus Y square

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and then we have here two Times Square over X squared plus by square.

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And then the other term where we have this typo here we have two Times Square over X squared plus Y

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square squared.

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And then you can see that you can here get rid of this power too and get rid of this one.

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So we have to over X squared plus Y square, minus two of X squared plus Y square, which is zero.

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So this means we have verified that this is indeed zero.

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But please be careful.

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We have divided here by row, which means our whole calculation is only true for row different from

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zero, which in this case is all we wanted to know.

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We will learn later, underscores how we can really determine this relation here.

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So we will really derive it.

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We will go the other way around.

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We will start from the umpire's law and then we will derive that the field looks like this.

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And at the moment we cannot really do this because this calculation here is not valid for the position

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are equal to zero.

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So please stay tuned and continue watching the course and then you will see that we can also solve the

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whole problem later on.
