Mutual Inductance (1-12-2021)

There are two circular loops of wire

Loop 1 (parallel to the y z yz plane):

x 1 = 1 y 1 = cos θ 1 z 1 = 2 + sin θ 1 0 θ 1 2 π x_1 = 1 \\ y_1 = \cos \theta_1 \\ z_1 = 2 + \sin \theta_1 \\ 0 \leq \theta_1 \leq 2 \pi

Loop 2 (in the x y xy plane):

x 2 = cos θ 2 y 2 = sin θ 2 z 2 = 0 0 θ 2 2 π x_2 = \cos \theta_2 \\ y_2 = \sin \theta_2 \\ z_2 = 0 \\ 0 \leq \theta_2 \leq 2 \pi

What is the mutual inductance between the two loops?

Details and Assumptions:
1) Magnetic permeability μ 0 = 1 \mu_0 = 1
2) All quantities are in standard S I SI units


The answer is 0.0738.

This section requires Javascript.
You are seeing this because something didn't load right. We suggest you, (a) try refreshing the page, (b) enabling javascript if it is disabled on your browser and, finally, (c) loading the non-javascript version of this page . We're sorry about the hassle.

2 solutions

Steven Chase
Jan 13, 2021

Essentially, the idea here is to pass one unit of current through one of the coils, and measure the resulting flux in the other coil. There are two ways to solve this, as indicated below:

ϕ = S B d S = S ( × A ) d S = C A d \phi = \iint_S \vec{B} \cdot \vec{dS} = \iint_S (\nabla \times \vec{A}) \cdot \vec{dS} = \oint_C \vec{A} \cdot \vec{d \ell}

An integral is required to determine the field B \vec{B} or A \vec{A} from the source. And then integrating over a surface requires two additional integrals, whereas integrating over a boundary curve requires one additional integral. So the left side ultimately requires a triple integral, and the right side requires a double integral. The surfaces and boundary curves are all very well defined in this problem, so that isn't much of a concern. When integrating numerically, for a given amount of computation, you get a better result using the magnetic vector potential method. @Karan Chatrath has shown the triple integral method, and has remarked on the numerical difficulties. For reference, to get an answer close to that of the vector potential method, I divided each spatial parameter into 1000 1000 pieces, resulting in a billion loop iterations. Of course, it took forever to run. By contrast, with the vector potential method, I got good results with "just" 25 25 million loop iterations. By "good results", I mean that the answers were all roughly equal with 25 25 million, 100 100 million, and 400 400 million loop iterations.

@Steven Chase Nice solution upvoted.

Talulah Riley - 5 months ago
Karan Chatrath
Jan 13, 2021

I got lucky while solving this one, on the last try. This is because of my choice of numerical resolution and problem approach. My first approach is as follows:

r 1 = ( 1 , r cos t 1 , 2 + r sin t 1 ) \vec{r}_1 = (1,r\cos{t_1},2+r\sin{t_1}) r 2 = ( cos t 2 , sin t 2 , 0 ) \vec{r}_2 = (\cos{t_2},\sin{t_2},0) d r 2 = ( sin t 2 , cos t 2 , 0 ) d t 2 d\vec{r}_2 = (-\sin{t_2},\cos{t_2},0) \ dt_2

Magnetic field due to an elementary arc of loop 2 at a point in the plane of loop 1:

d B = 1 4 π d r 2 × ( r 1 r 2 ) r 1 r 2 3 d\vec{B} = \frac{1}{4\pi} \frac{d\vec{r}_2 \times (\vec{r}_1-\vec{r}_2)}{\lvert \vec{r}_1-\vec{r}_2\rvert^3}

The elementary flux through loop 1:

d Φ = d B ( r d r d t 1 i ^ ) = f ( r , t 1 , t 2 ) d t 1 d t 2 d r d\Phi = d\vec{B} \cdot \left (r \ dr \ dt_1 \ \hat{i}\right) = f(r,t_1,t_2) dt_1 \ dt_2 \ dr

Φ = 0 1 0 2 π 0 2 π f ( r , t 1 , t 2 ) d t 1 d t 2 d r 0.0763 \Phi = \int_{0}^{1} \int_{0}^{2\pi} \int_{0}^{2\pi} f(r,t_1,t_2) dt_1 \ dt_2 \ dr \approx 0.0763

Simplifications left out. Numerical resolution: d r = 0.001 ; d t 1 = d t 2 = π / 100 dr = 0.001 \ ; \ dt_1 = dt_2 = \pi/100 .


The approach that actually worked was:

r 1 = ( 1 , cos t 1 , 2 + sin t 1 ) \vec{r}_1 = (1,\cos{t_1},2+\sin{t_1}) r 2 = ( r cos t 2 , r sin t 2 , 0 ) \vec{r}_2 = (r\cos{t_2},r\sin{t_2},0) d r 1 = ( 0 , sin t 1 , cos t 1 ) d t 1 d\vec{r}_1 = (0,-\sin{t_1},\cos{t_1}) \ dt_1

Magnetic field due to an elementary arc of loop 1 at a point in the plane of loop 2:

d B = 1 4 π d r 1 × ( r 2 r 1 ) r 2 r 1 3 d\vec{B} = \frac{1}{4\pi} \frac{d\vec{r}_1 \times (\vec{r}_2-\vec{r}_1)}{\lvert \vec{r}_2-\vec{r}_1\rvert^3}

The elementary flux through loop 2:

d Φ = d B ( r d r d t 2 i ^ ) = f ( r , t 1 , t 2 ) d t 1 d t 2 d r d\Phi = d\vec{B} \cdot \left (r \ dr \ dt_2 \ \hat{i}\right) = f(r,t_1,t_2) dt_1 \ dt_2 \ dr

Φ = 0 1 0 2 π 0 2 π f ( r , t 1 , t 2 ) d t 1 d t 2 d r 0.0741 \Phi = \int_{0}^{1} \int_{0}^{2\pi} \int_{0}^{2\pi} f(r,t_1,t_2) dt_1 \ dt_2 \ dr \approx 0.0741

Simplifications left out. Numerical resolution: d r = 0.001 ; d t 1 = d t 2 = π / 100 dr = 0.001 \ ; \ dt_1 = dt_2 = \pi/100 .

@Karan Chatrath Nice solution. Upvoted

Talulah Riley - 5 months ago

0 pending reports

×

Problem Loading...

Note Loading...

Set Loading...