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Use Stokes' Theorem to derive the integral form of Faraday's law, $$ \int_{C} \mathbf{E} \cdot d \mathbf{s}=-\frac{\partial}{\partial t} \iint_{D} \mathbf{B} \cdot d \mathbf{S} $$ from the differential form of Maxwell's equations.

Short Answer

Expert verified
By applying Stokes' theorem to the differential form of Faraday's law drawn from Maxwell's equations, we can successfully transform it and arrive at its integral form which is \( \int_{C} \mathbf{E} \cdot d \mathbf{s}=-\frac{\partial}{\partial t} \iint_{D} \mathbf{B} \cdot d \mathbf{S} \)

Step by step solution

01

Recall Maxwell's equations and the differential form of Faraday's law

Applying the differential form of Faraday's law from Maxwell's equation we derive that, \( \nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t} \)
02

Recognizing Stokes' Theorem and its application

The Stokes' theorem states that for any vector field, its curl integrated over some surface is equal to the line integral of the vector field around the boundary of the surface. That is if \( \mathbf{F} \) is a vector field, then \( \int_{C} \mathbf{F} \cdot d \mathbf{s} = \iint_{D} \nabla \times \mathbf{F} \cdot d \mathbf{S} \), where \( D \) is a surface bounded by the closed contour \( C \).
03

Apply Stokes' Theorem

Stokes' theorem allows us to transform the right hand side of the equation. From \( \nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t} \), we substitute this into Stokes’s theorem, obtaining \( \iint_{D} (\nabla \times \mathbf{E}) \cdot d \mathbf{S} = -\frac{\partial}{\partial t} \iint_{D} \mathbf{B} \cdot d \mathbf{S} \)
04

Derive the integral form of Faraday's law

On the left side of the equation, by definition of the surface integral of a curl of a vector field over a surface, we can rewrite this as a line integral along the boundary of that surface. Therefore, we obtain the final form of the Faraday's law in integral form: \( \int_{C} \mathbf{E} \cdot d \mathbf{s}=-\frac{\partial}{\partial t} \iint_{D} \mathbf{B} \cdot d \mathbf{S} \)

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Faraday's Law
Faraday's Law is a fundamental principle in electromagnetism that explains how a magnetic field can produce an electric field, a phenomenon known as electromagnetic induction. At its core, Faraday's Law links the change in magnetic field over time to the electric field generated by that change. This concept is pivotal in understanding how electric generators and transformers work. In its integral form, Faraday's Law states:
  • \( \int_{C} \mathbf{E} \cdot d \mathbf{s} = -\frac{\partial}{\partial t} \iint_{D} \mathbf{B} \cdot d \mathbf{S} \)
This equation tells us that the electric field \( \mathbf{E} \) around a closed loop \( C \) is equal to the negative rate of change of the magnetic flux \( \mathbf{B} \) through the surface \( D \).
This integral form of Faraday's Law is especially useful when analyzing systems with changing magnetic fields, such as inductors and transformers.
In practical applications, Faraday's Law is used to devise electric circuits that can harness energy from varying magnetic fields, enabling technologies like wireless charging and electric generators.
Maxwell's Equations
Maxwell's Equations are the set of four equations that form the foundation of classical electromagnetism, classical optics, and electric circuits. They beautifully unify all previous electric and magnetic theories into a single, consistent framework. Maxwell's Equations consist of:
  • Gauss's law for electricity
  • Gauss's law for magnetism
  • Faraday's law of induction
  • Ampère's law with Maxwell's addition
These equations describe how electric charges produce electric fields (Gauss's law for electricity), how magnetic poles (if they existed) do not exist (Gauss’s law for magnetism), how time-varying magnetic fields induce electric fields (Faraday's law, which we derived the integral form of using Stokes' theorem), and how currents and changing electric fields produce magnetic fields (Ampère's law with Maxwell's addition).
In the context of the exercise, we specifically used the differential form of Faraday's Law:
  • \( abla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t} \)
This equation expresses the relationship between time-varying magnetic fields and the curls (or loops) in the electric field.
Vector Calculus
Vector calculus is an essential mathematical tool used in the study of fields like physics and engineering. It involves vector fields and operations on these fields, such as divergence, gradient, and curl. In understanding electromagnetism, vector calculus is crucial for describing how fields vary in space and time.
One key concept used in the original exercise is the curl of a vector field, denoted as \( abla \times \mathbf{E} \). The curl measures the rotation at a point in the field, which in this case, translates to how a changing magnetic field creates an electric field.
  • Divergence measures how much a point acts as a source or sink of the field.
  • Gradient provides the direction and rate of fastest increase of a scalar field.
  • Curl indicates how much a field tends to swirl around a point.
For the problem at hand, Stokes' Theorem plays a pivotal role in transitioning from differential to integral forms of equations. Stokes' Theorem relates a surface integral of a curl over a surface to a line integral around the boundary of that surface. This interpretation allows us to translate the local properties described by differential equations into global properties described by integrals.
By applying Stokes' Theorem, we moved from the differential expression \( abla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t} \) to the integral result \( \int_{C} \mathbf{E} \cdot d \mathbf{s} = -\frac{\partial}{\partial t} \iint_{D} \mathbf{B} \cdot d \mathbf{S} \), bridging the gap between local and global understanding.

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Most popular questions from this chapter

Zaphod Beeblebrox was in trouble after the infinite improbability drive caused the Heart of Gold, the spaceship Zaphod had stolen when he was President of the Galaxy, to appear between a small insignificant planet and its hot sun. The temperature of the ship's hull is given by \(T(x, y, z)=\) \(e^{-k\left(x^{2}+y^{2}+z^{2}\right)}\) Nivleks. He is currently at \((1,1,1)\), in units of globs, and \(k=2\) globs \(^{-2}\). (Check the Hitchhikers Guide for the current conversion of globs to kilometers and Nivleks to Kelvin.) a. In what direction should he proceed so as to decrease the temperature the quickest? b. If the Heart of Gold travels at \(e^{6}\) globs per second, then how fast will the temperature decrease in the direction of fastest decline?

Let \(T^{\alpha}\) be a contravariant vector and \(S_{\alpha}\) be a covariant vector. a. Show that \(R_{\beta}=g_{\alpha \beta} T^{\alpha}\) is a covariant vector. b. Show that \(R^{\beta}=g^{\alpha \beta} S_{\alpha}\) is a contravariant vector.

For cylindrical coordinates, $$ \begin{aligned} x &=r \cos \theta \\ y &=r \sin \theta \\ z &=z \end{aligned} $$ find the scale factors and derive the following expressions: $$ \begin{gathered} \nabla f=\frac{\partial f}{\partial r} \hat{\mathbf{e}}_{r}+\frac{1}{r} \frac{\partial f}{\partial \theta} \hat{\mathbf{e}}_{\theta}+\frac{\partial f}{\partial z} \hat{\mathbf{e}}_{z} \\ \nabla \cdot \mathbf{F}=\frac{1}{r} \frac{\partial\left(r F_{r}\right)}{\partial r}+\frac{1}{r} \frac{\partial F_{\theta}}{\partial \theta}+\frac{\partial F_{z}}{\partial z} \\ \nabla \times \mathbf{F}=\left(\frac{1}{r} \frac{\partial F_{z}}{\partial \theta}-\frac{\partial F_{\theta}}{\partial z}\right) \hat{\mathbf{e}}_{r}+\left(\frac{\partial F_{r}}{\partial z}-\frac{\partial F_{z}}{\partial r}\right) \hat{\mathbf{e}}_{\theta}+\frac{1}{r}\left(\frac{\partial\left(r F_{\theta}\right)}{\partial r}-\frac{\partial F_{r}}{\partial \theta}\right) \\\ \nabla^{2} f=\frac{1}{r} \frac{\partial}{\partial r}\left(r \frac{\partial f}{\partial r}\right)+\frac{1}{r^{2}} \frac{\partial^{2} f}{\partial \theta^{2}}+\frac{\partial^{2} f}{\partial z^{2}}. \end{gathered} $$

Newton's Law of Gravitation gives the gravitational force between two masses as $$ \mathbf{F}=-\frac{G m M}{r^{3}} \mathbf{r} $$ a. Prove that \(\mathbf{F}\) is irrotational. b. Find a scalar potential for \(\mathbf{F}\).

A particle moves on a straight line, \(\mathbf{r}=t \mathbf{u}\), from the center of a disk. If the disk is rotating with angular velocity \(\omega\), then \(\mathbf{u}\) rotates. Let \(\mathbf{u}=\) \((\cos \omega t) \mathbf{i}+(\sin \omega t) \mathbf{j}\) a. Determine the velocity, \(\mathbf{v}\). b. Determine the acceleration, a. c. Describe the resulting acceleration terms identifying the centripetal acceleration and Coriolis acceleration.

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