Energy stored in a magnetic field!

An infinite straight solid cylindrical wire contains a uniform current density of magnitude J J (the direction of the current is along the axis of the cylinder). Find the energy stored in the magnetic field (in S.I. units) within a cylindrical volume of radius R R and length L L whose axis is parallel to that of the wire and at a distance of d d from it.

Details and Assumptions: \text{Details and Assumptions:}

\bullet Assume that the radius of the wire is sufficiently large so that the cylinder is entirely contained within it.

\bullet The magnetic energy density is given by B B 2 μ 0 \dfrac{\mathbf{B}\cdot\mathbf{B}}{2\mu_{0}} where B \mathbf{B} is the magnetic field.

\bullet J = 1 0 3 π A/m 2 J=\dfrac{10^{3}}{\pi}\text{A/m}^{2}

\bullet R = 2 m R=2 \text{m}

\bullet L = 2 m L=2 \text{m}

\bullet d = 2 2 m d=2\sqrt{2} \text{m}


The answer is 4.

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2 solutions

Karthik Kannan
Oct 24, 2014

The magnetic energy stored in the cylinder is given by:

E = cylinder B B 2 μ 0 d V E=\displaystyle\iiint_{\text{cylinder}}\frac{\mathbf{B}\cdot\mathbf{B}}{2\mu_{0}}\text{d}V

Now the trick here to avoid difficult calculations is to split the field at any point inside the cylinder into two components:

The first of these components arises only due to the current flowing in the cylindrical region. Let us call it B cylinder \mathbf{B}_{\text{cylinder}} .

The second component is the field due to the remaining part of the wire assuming the cylinder is removed. Let us call it B remaining \mathbf{B}_{\text{remaining}} .

Thus B = B cylinder + B remaining \mathbf{B}=\mathbf{B}_{\text{cylinder}}+\mathbf{B}_{\text{remaining}}

Therefore E = cylinder B cylinder B cylinder 2 μ 0 d V + cylinder B remaining B remaining 2 μ 0 d V + cylinder 2 B cylinder B remaining 2 μ 0 d V E=\displaystyle\iiint_{\text{cylinder}}\frac{\mathbf{B}_{\text{cylinder}}\cdot\mathbf{B}_{\text{cylinder}}}{2\mu_{0}}\text{d}V+\displaystyle\iiint_{\text{cylinder}}\frac{\mathbf{B}_{\text{remaining}}\cdot\mathbf{B}_{\text{remaining}}}{2\mu_{0}}\text{d}V+\displaystyle\iiint_{\text{cylinder}}\frac{2\mathbf{B}_{\text{cylinder}}\cdot\mathbf{B}_{\text{remaining}}}{2\mu_{0}}\text{d}V

= E 1 + E 2 + E 3 =E_{1}+E_{2}+E_{3}

Computing E 1 : \text{Computing }E_{1}\text{:}

It can be easily shown that B cylinder = μ 0 J x 2 \mathbf{B}_{\text{cylinder}}=\dfrac{\mu_{0}Jx}{2} where x x is the distance from the axis of the cylinder.

Consider a small cylindrical shell of thickness d x \text{d}x at a radial distance of x x :

d E 1 = 1 2 μ 0 μ 0 2 J 2 x 2 4 ( 2 π x l d x ) \text{d}E_{1}=\dfrac{1}{2\mu_{0}}\dfrac{\mu_{0}^{2}J^{2}x^{2}}{4}(2\pi xl\text{d}x)

E 1 = μ 0 J 2 π l 4 0 R x 3 d x = μ 0 J 2 π l R 4 16 \therefore E_{1}=\dfrac{\mu_{0}J^{2}\pi l}{4}\displaystyle\int_{0}^{R} x^{3}\text{d}x=\dfrac{\mu_{0}J^{2}\pi lR^{4}}{16}

Computing E 2 : \text{Computing }E_{2}\text{:}

First we shall find B remaining \mathbf{B}_{\text{remaining}} .

Refer the diagram above. We want to find the field at a point whose position vector w.r.t. the center of the one of the cross sections of the cylinder is b \mathbf{b} . The position vector of the center of this cross section is a \mathbf{a} . Assume that the plane of the cylinder is the x y xy plane.

Thus B remaining = B B cylinder \mathbf{B}_{\text{remaining}}=\mathbf{B}-\mathbf{B}_{\text{cylinder}}

= μ 0 J 2 ( k ^ × ( a + b ) ) μ 0 J 2 ( k ^ × b ) =\dfrac{\mu_{0}J}{2}(\hat{k}\times(\mathbf{a}+\mathbf{b}))-\dfrac{\mu_{0}J}{2}(\hat{k}\times\mathbf{b})

= μ 0 J 2 ( k ^ × a ) =\dfrac{\mu_{0}J}{2}(\hat{k}\times\mathbf{a})

Thus B remaining = μ 0 J 2 ( k ^ × a ) \mathbf{B}_{\text{remaining}}=\dfrac{\mu_{0}J}{2}(\hat{k}\times\mathbf{a}) which is a constant!

Therefore E 2 = cylinder B remaining B remaining 2 μ 0 d V E_{2}=\displaystyle\iiint_{\text{cylinder}}\frac{\mathbf{B}_{\text{remaining}}\cdot\mathbf{B}_{\text{remaining}}}{2\mu_{0}}\text{d}V

= 1 2 μ 0 μ 0 2 J 2 d 2 4 × Volume of cylinder =\dfrac{1}{2\mu_{0}}\dfrac{\mu_{0}^{2}J^{2}d^{2}}{4}\times\text{Volume of cylinder}

E 2 = μ 0 J 2 π l R 2 d 2 8 \therefore E_{2}=\dfrac{\mu_{0}J^{2}\pi lR^{2}d^{2}}{8}

Computing E 3 : \text{Computing }E_{3}\text{:}

Refer the diagram above. Say we want to compute B cylinder B rremaining \mathbf{B}_{\text{cylinder}}\cdot\mathbf{B}_{\text{rremaining}} at a point A A . Now consider the diametrically opposite point B B in the diagram. If the angle between B cylinder \mathbf{B}_{\text{cylinder}} and B remaining \mathbf{B}_{\text{remaining}} at A A is θ \theta then the angle between them at point B B is 180 θ 180-\theta . Thus all the contributions due to B cylinder B rremaining \mathbf{B}_{\text{cylinder}}\cdot\mathbf{B}_{\text{rremaining}} cancel out.

So E 3 = cylinder 2 B cylinder B remaining 2 μ 0 d V = 0 E_{3}=\displaystyle\iiint_{\text{cylinder}}\frac{2\mathbf{B}_{\text{cylinder}}\cdot\mathbf{B}_{\text{remaining}}}{2\mu_{0}}\text{d}V=0

Thus E = E 1 + E 2 = μ 0 J 2 π R 2 l 8 ( R 2 2 + d 2 ) E=E_{1}+E_{2}=\boxed{\dfrac{\mu_{0}J^{2}\pi R^{2}l} {8}\left( \dfrac{R^{2}}{2}+d^{2}\right)}

Nice Solution!

jatin yadav - 6 years, 7 months ago

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Thanks Jatin! Your solution is nice too! Actually I first used the method that you used but I could not compute the resulting integral so I thought of this method. ¨ \ddot\smile

Karthik Kannan - 6 years, 7 months ago
Jatin Yadav
Oct 27, 2014

Using Ampere's Law, we get :

B ( r ) = μ 0 J r 2 B(r) = \dfrac{\mu_{0} J r}{2}

Consider a cross-section. On that , consider a circle of radius r r centered at axis of infinite cylinder. Consider the region where it intersects the given cylinder, as shown:

Clearly, using cosine rule,

cos ϕ = r 2 + d 2 R 2 2 d r \cos \phi = \dfrac{ r^2+d^2-R^2}{2dr}

Hence, d V = 2 r ϕ d r × L dV = 2r \phi dr \times L

Hence,

d E B = B 2 2 μ 0 d V = 1 2 μ 0 ( μ 0 J r 2 ) 2 2 L r arccos ( r 2 + d 2 R 2 2 d r ) d r dE_{B} = \dfrac{B^2}{2 \mu_{0}} dV = \dfrac{1}{2 \mu_{0}}\bigg(\dfrac{\mu_{0}J r}{2}\bigg)^2 2Lr \arccos\bigg(\dfrac{r^2+d^2-R^2}{2dr}\bigg) dr

= μ 0 J 2 4 r 3 arccos ( r 2 + d 2 R 2 2 d r ) d r \dfrac{\mu_{0} J^2}{4} r^3 \text{ } \arccos\bigg(\dfrac{r^2+d^2-R^2}{2dr}\bigg) dr

Hence, E = μ 0 J 2 L 4 d R d + R r 3 arccos ( r 2 + d 2 R 2 2 d r ) d r E = \dfrac{\mu_{0}J^2L}{4} \displaystyle \int_{d-R}^{d+R} r^3 \text{ } \arccos \bigg(\dfrac{r^2+d^2-R^2}{2dr}\bigg) {\mathrm dr}

= 1 5 π 2 2 2 2 2 + 2 r 3 arccos ( r 2 + 4 4 2 r ) d r \dfrac{1}{5 \pi} \displaystyle \int_{2\sqrt{2}-2}^{2\sqrt{2}+2} r^3 \text{ } \arccos \bigg(\dfrac{r^2+4}{4 \sqrt{2} r} \bigg) {\mathrm dr}

Use the substitution r = 2 x r = 2x , and then x + 1 / x = 2 2 cos θ x+1/x = 2 \sqrt{2} \cos \theta to get the answer as 4

I did the same way.

Ronak Agarwal - 6 years, 6 months ago

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