(a) Use Ampère's law (8.6.4) to prove that the current density \(J(z)\) in the conductor of Fig. \(8.6 .2\) is related to the net magnetic field just outside the conductor by $$ B_{\text {outeide }}=\mu_{0} \int_{0}^{\infty} J(z) d z=\mu_{0} K, $$ where the integral symbolized by \(K\) has the dimensions of a surface current density, namely, amperes per meter. \((b)\) Consider an artificial model whereby the surface current \(K\) is distributed uniformly in the skin layer \(0

Short Answer

Expert verified
#Answer#: a) The relationship between the current density in the conductor and the net magnetic field just outside the conductor is given by: $$ B_\text{outside} = \mu_{0} \int_{0}^{\infty} J(z) d z = \mu_{0} K $$ where \(K\) is the surface current density. b) In the simplified model with a uniform surface current in the skin layer, the time-average power per unit area is: $$ \frac{\overline{B_\text{outside}^2}}{\mu_0^2 g \delta} $$ The resistance ratio of a round wire for high-frequency currents to direct current is: $$ \frac{R_\text{ac}}{R_\text{dc}} = \frac{2 \delta}{a} $$ where \(a\) is the radius of the wire.

Step by step solution

01

Part (a): Using Ampère's law to find the relationship between current density and magnetic field

Ampère's law states that the circulation of the magnetic field around a closed loop is equal to the product of the permeability \(\mu_0\) and the total current passing through the surface enclosed by the loop. For this exercise, we need to relate the current density \(J(z)\) to the net magnetic field just outside the conductor, \(B_\text{outside}\). We can write Ampère's law as: $$ \oint \vec{B} \cdot d\vec{l} = \mu_0 \int \vec{J} \cdot d\vec{A} $$ Consider a rectangular loop just outside the conductor of width \(dA\). The magnetic field is tangential to the conductor and has constant magnitude over the surface. Thus, the circulation of the magnetic field around the loop is equal to \(B_\text{outside}\times dA\). On the other hand, the total current passing through the surface enclosed by the loop is \(\int_0^\infty J(z) dz\). Substituting these expressions into Ampère's law, we get: $$ B_\text{outside} \times dA = \mu_0 \int_{0}^{\infty} J(z) dz $$ Dividing by \(dA\), we have: $$ B_\text{outside} = \mu_{0} \int_{0}^{\infty} J(z) d z = \mu_{0} K $$ where \(K\) has the dimensions of surface current density.
02

Part (b): Time-average power per unit area and resistance ratio for the simplified model

Let's consider the simplified model with a uniform surface current \(K\) distributed in the skin layer \(0 < z < \delta\), such that the current density is \(J_\text{skin} = \frac{K}{\delta}\). To find the time-average power per unit area, we use the following expression: $$ \left(\frac{\overline{J_\text{skin}^2}}{g}\right) \delta $$ Substituting \(J_\text{skin} = \frac{K}{\delta}\), we get: $$ \frac{\overline{K^2}}{g \delta} = \frac{\overline{B_\text{outside}^2}}{\mu_0^2 g \delta} $$ This result matches with the time-average power per unit area found in Prob. \(8.6.6 b\). Now, the resistance ratio of a round wire for high-frequency currents to direct current can be found using the ratio of effective areas: $$ \frac{R_\text{ac}}{R_\text{dc}} = \frac{2 \delta}{a} $$ where \(a\) is the radius of the wire. This concludes the exercise.

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Most popular questions from this chapter

A waveguide becomes a resonant cavity upon placing conducting walls at the two ends. Show that a resonance occurs when the length \(L\) is an integral number \(n\) of guide halfwavelengths \(\lambda_{e} / 2 ;\) specifically, \(\left(\frac{\omega}{c}\right)^{2}=\left(\frac{l \pi}{a}\right)^{2}+\left(\frac{m \pi}{b}\right)^{2}+\left(\frac{n \pi}{L}\right)^{2} \quad\) rectangular parallelepiped \(\left(\frac{\omega}{c}\right)^{2}=\left(\frac{u_{l m}}{a}\right)^{2}+\left(\frac{n \pi}{L}\right)^{2} \quad\) right circular cylinder. Cavity modes, requiring three integral indices, are named \(\mathrm{TE}_{l m n}\) or \(\mathrm{TM}_{l m n} . \mathrm{Make}\) a mode chart for cylindrical cavities by plotting loci of resonances on a graph of \((d / L)^{2}\) against \((f d)^{2}\), where \(d \equiv 2 a, f \equiv \omega / 2 \pi . \dagger\)

(a) Evaluate the energy density \(W_{1}\) and the Poynting vector \(s\) for the simple plane wave of Sec. \(8.3\) to show that the electric and magnetic energy densities are equal and that $$ |\mathbf{s}|=c\left(\boldsymbol{W}_{1}\right)_{\text {field }} $$ (b) Show that the time-average Poynting vector is $$ \mathrm{s}=\frac{E_{0}{ }^{2}}{2 Z_{0}} \hat{\mathrm{k}}=\frac{1}{2} H_{0}{ }^{2} Z_{0} \hat{\mathrm{k}}, $$ where \(E_{0}\) and \(H_{0}=B_{0} / \mu_{0}\) are the (peak) field amplitudes, \(Z_{0}\) is the wave impedance given by \((8.3 .10)\), and \(\hat{k}\) is a unit vector in the direction of propagation \((c)\) Evaluate the field-dependent terms in (8.4.15) for a plane wave to show that the time-average force density is $$ \vec{F}_{1}=-\nabla\left(\bar{W}_{1}\right) \text { field } $$ which is a simple generalization of the result quoted in (8.4.20).

(a) From \((8.7 .10)\) and \((8.7 .13)\), show that the guided ave impedance \(\left(E_{x}{ }^{2}+E_{y}{ }^{2}\right)^{1 / 2} /\) \(\left(H_{x}{ }^{2}+H_{z}{ }^{2}\right)^{1 / 2}\) is \(Z_{\mathrm{TE}}=\frac{Z_{0}}{\left[1-\left(\lambda_{0} / \lambda_{e}\right)^{2}\right]^{1 / 2}} \quad\) TE modes \(Z_{\text {T? }}=Z_{0}\left[1-\left(\lambda_{0} / \lambda_{c}\right)^{2}\right]^{1 / 2} \quad\) TM modes, where \(Z_{0}\) is the unbounded wave impedance \((8.3 .10)\) or, more generally, \((8.3 .12) .(b)\) For the TE o dominant mode in rectangular waveguide, show that the peak potential difference between opposite points in the cross section is $$ V_{0}=\left[\int_{0}^{b} E_{y}\left(x=\frac{1}{2} a\right) d y\right]_{p e s k}=b E_{0} $$ and that the peak axial current flowing in the top wall is $$ I_{0} \equiv\left[\frac{1}{\mu_{0}} \int_{0}^{a} B_{x}(y=b) d x\right]_{\text {pak }}=\frac{2 a E_{0}}{\pi Z_{\mathrm{TE}}} $$ Since the result of Prob. 8.7.10b can be written $$ \bar{P}=\frac{a b}{4} \frac{E_{0}{ }^{2}}{Z_{\mathrm{TB}}} $$ we can define three other (mode-dependent) waveguide impedances as follows: $$ \begin{aligned} &Z_{V, I}=\frac{V_{0}}{I_{0}}=\frac{\pi}{2}\left(\frac{b}{a} Z_{\mathrm{TE}}\right) \\ &Z_{P, V}=\frac{V_{0}{ }^{2}}{2 P}=2\left(\frac{b}{a} Z_{\mathrm{TE}}\right) \\\ &Z_{P, I}=\frac{2 \bar{P}}{I_{0}{ }^{2}}=\frac{\pi^{2}}{8}\left(\frac{b}{a} Z_{\mathrm{TE}}\right) \end{aligned} $$ which differ by small numerical factors. Only systems supporting a TEM mode (e.g., Sec. 8.1), have a unique impedance.

Show that $$ \begin{aligned} &\mathbf{E}=(1+j j) E_{1} e^{j(\omega t-\alpha o)} \\ &\mathbf{B}=(-1 j+j) \frac{E_{1}}{c} e^{j(\omega t-\alpha t)} \end{aligned} $$ represent a circularly polarised plane wave. (Note that \(j=\sqrt{-1}\), while \(\mathbf{1}, \mathbf{j}\) are the cartesian unit vectors in the \(x\) and \(y\) directions!) If you watch the time variation of the electric field at a fixed position, will the direction of the field rotate in the right-or left-handed sense with respect to the direction of travel \((+z) ?\) If you could take a snapshot of the electric field over space, in which sense would the direction rotate? Repeat these questions for the magnetic field. How would you represent a circularly polarized wave of the opposite handedness? Answer: Left-handed; right-handed; magnetic same as electric; reverse sign of \(j\) in coefficients.

Use Gauss' and Stokes' theorems (Appendix A) to convert Maxwell's differential equations for vacuum, \((82.1)\) to \((8.2 .4)\), to their integral form $$ \begin{aligned} &\oint_{S} \mathbf{E} \cdot d \mathbf{S}=\frac{q}{\epsilon_{0}} \\ &\oint_{L} \mathbf{E} \cdot d \mathbf{l}=-\frac{d \Phi_{m}}{d t} \\ &\oint_{S} \mathbf{B} \cdot d \mathbf{S}=0 \\ &\oint_{L} \mathbf{B} \cdot d \mathbf{l}=\mu_{0} I+\mu_{0} \frac{d \Phi_{*}}{d t} \end{aligned} $$ † See Sec. \(5.4\) and Prob. 8.2.4. where the closed surface \(S\) contains the net charge \(q\) and the closed line (loop) \(L\) is linked by the net current \(I\), the magnetic flux \(\Phi_{m}=\int \mathbf{B} \cdot d \mathbf{S}\), and the electric flux \(\Phi_{e}=\epsilon_{0} \int \mathbf{E} \cdot d \mathbf{S}\). Note: The corresponding equations for a general electromagnetic medium are developed in Prob. \(8.6 .1 .\)

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