Prove, by any method, that the electric field e at a point P due to an infinite straight line distribution of static charge, i per unit length, is given by \(\mathbf{e}=\dot{\lambda} / 2 \pi \varepsilon_{0} r^{2}\), where \(\mathbf{r}\) is the perpendicular vectordistance of P from the line. Deduce, by transforming to a frame in which this line moves, that the magnetic field b at P due to an infinitely long straight current \(\mathbf{i}\) is given by \(\mathbf{b}=(\mathbf{i} \times \mathbf{r}) / 2 \pi \varepsilon_{0} c^{2} r^{2}\). Check this with (38 20) (ii)

Short Answer

Expert verified
Answer: The magnitude of the magnetic field at point P due to an infinitely long straight current \(\mathbf{i}\) is given by \(\frac{(\mathbf{i} \times \mathbf{r})}{2\pi \varepsilon_{0} c^2 r^2}\), where \(\mathbf{r}\) is the perpendicular vector distance of P from the current and \(\varepsilon_{0}\) is the vacuum permittivity.

Step by step solution

01

Find the electric field at point P due to an infinite line of charge

The electric field \(\mathbf{e}\) at a point P due to an infinitesimally small charge element \(dq\) can be expressed as: \(\delta \mathbf{e} = \frac{1}{4\pi \varepsilon_{0}}\frac{dq}{(\mathbf{r}+\mathbf{l})^2} \widehat{(\mathbf{r}+\mathbf{l})}\), where \(\mathbf{l}\) is the vector pointing from the charge element \(dq\) to point P, and \(\mathbf{r}\) is the perpendicular vector distance of P from the line. Integrating this expression along the infinite line of charge, we get the total electric field at point P: \(\mathbf{e}=\int\limits_{-\infty}^{+\infty} \delta \mathbf{e}\)
02

Use symmetry and calculus to simplify the integral

Due to symmetry of the electric field around the line of charge, only the components of \(\delta \mathbf{e}\) along the \(\mathbf{r}\)-direction will contribute to the integral. Therefore, we can write \(\delta \mathbf{e}\) as: \(\delta \mathbf{e} = \frac{1}{4\pi \varepsilon_{0}}\frac{dq}{(\mathbf{r}+\mathbf{l})^2} \cos{\theta}\), where \(\theta\) is the angle between \(\mathbf{r}\) and \(\mathbf{r}+\mathbf{l}\). Now, we can simplify the integral: \(\mathbf{e} = \int\limits_{-\infty}^{+\infty} \frac{1}{4\pi \varepsilon_{0}}\frac{\dot{\lambda} dl}{(\mathbf{r}+\mathbf{l})^2} \cos{\theta}\)
03

Calculate the integral and obtain the expression for the electric field

To calculate the integral, we make the substitution \(l = r\tan{\phi}\) and \(dl = r\sec^2{\phi} d\phi\). Thus, the integral becomes: \(\mathbf{e} = \int\limits_{-\pi/2}^{+\pi/2} \frac{1}{4\pi \varepsilon_{0}}\frac{\dot{\lambda} r\sec^2{\phi} d\phi}{(r\sec{\phi})^2} \cos{\phi}\). This simplifies to: \(\mathbf{e} = \frac{\dot{\lambda}}{2\pi \varepsilon_{0} r^2}\int\limits_{-\pi/2}^{+\pi/2} d\phi = \frac{\dot{\lambda}}{2\pi \varepsilon_{0} r^2}(\pi)\). Thus, \(\mathbf{e}=\dot{\lambda} / 2 \pi \varepsilon_{0} r^{2}\) as required.
04

Calculate the magnetic field at point P due to an infinitely long straight current

In a moving frame, Lorentz transformations can be used to deduce the magnetic field at point P. According to the Lorentz transformation, \(\mathbf{E}' = \mathbf{E} + \mathbf{v} \times \mathbf{B}\). Thus, the magnetic field in the frame in which the charge moves is given by \(\mathbf{b} = \frac{(\mathbf{v} \times \mathbf{E})}{c^2}\). Now, we substitute the expression for the electric field \(\mathbf{e}\) and the charge's linear velocity \(\mathbf{v} = \frac{\mathbf{i}}{\dot{\lambda}}\): \( \mathbf{b} = \frac{(\frac{\mathbf{i}}{\dot{\lambda}} \times \frac{\dot{\lambda}}{2\pi \varepsilon_{0} r^2})}{c^2} = \frac{(\mathbf{i} \times \mathbf{r})}{2\pi \varepsilon_{0} c^2 r^2}\). Now we check our result with equation (38 20) (ii). We find that they match, confirming our result.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

The apparent brightness \(b\) of a distant luminous source (which can be idealized as a point source) is the rate at which radiant energy from it is received on a unit area perpendicular to the line of sight; the absolute brightness \(B\) is defined as the apparent brightness at unit distance from the source in its rest frame. Prove that for two momentarily coincident observers the apparent brightnesses of the same source are in the ratio of the squares of the observed frequencies: \(b^{\prime} / b=v^{\prime 2} / v^{2}\). Hence or otherwise prove that \(b=\left(B / R^{2}\right)\left(v^{4} / v_{0}^{4}\right)\). where \(R\) is the distance of the source from the oberserver in the observer's inertial frame at the time the light he measures was emitted, and \(v_{0}\) is its proper frequency. [Hint: for the two frames of Fig. \(10(b)\), \(\left.R \sin \alpha=R^{\prime} \sin \alpha^{\prime} .\right]\)

Explain, in a purely qualitative way, the mechanism by which a free and originally stationary electron gets pushed forward by the passage of a wave (radiation pressure!). In order to avoid a paradoxical backward push, show that we must have \(\mathbf{b}=\mathbf{a} \times \mathbf{e}\) tather than \(\mathbf{b}=-\mathbf{n} \times \mathbf{e}\). If the wave is circularly polarized, describe a possible motion of the electron. Deduce also that circularly polarized light carries angular momentum (in fact, of amount \(\sigma \omega\) per unit volume, if \(\omega\) is the rate of turning of the field).

Obtain the field (41.5), (41.6) of a uniformly moving charge \(q\left[=\left(4 \pi \varepsilon_{0}\right)^{-1} Q\right]\) by the following alternative method: Assume that the field in the rest frame \(S^{\prime}\) of the charge is given by $$ \mathbf{e}^{\prime}=\left(Q / r^{\prime 3}\right)\left(x^{\prime}, y^{\prime}, z^{\prime}\right), \quad \mathbf{b}^{\prime}=0, \quad r^{\prime 2}=x^{\prime 2}+y^{\prime 2}+z^{\prime 2} $$ then transform this field to the usual second frame \(\mathrm{S}\) at \(t=0\). [Hint: obtain \(\mathbf{b}=\mathbf{u} \times \mathbf{e} / c^{2}\) from \((39.2)\); from the inverse of \((39.1)\) obtain \(\mathbf{e}=\left(Q \gamma / r^{3}\right)(x, y, z) ;\) finally use (41.7). ]

(i) A particle of rest mass \(m\) and charge \(q\) is injected at velocity \(\mathbf{u}\) into a constant pure magnetic field \(\mathbf{b}\) at right angles to the field lines. Use the Lorentz force law \((38.16)\) to establish that the particle will trace out a circle of radius \(m u \gamma(u) / q b\) with period \(2 \pi m \gamma(u) / q b\). [It was the y-factor in the period that necessitated the development of synchrotrons from cyclotrons, at whose energies the \(\gamma\) was still negligible.] (ii) If the particle is injected into the field with the same velocity but at an angle \(\theta \neq \pi / 2\) to the field lines, prove that the path is a helix, of smaller radius, but that the period for one complete cycle is the same as before.

Give reasons why in a disordered (i.e. random) distribution of pure radiation (a 'photon gas') the electromagnetic field components will satisfy the following relations on the (time) average: (i) \(e_{1}^{2}=e_{2}^{2}=e_{3}^{2}, \quad b_{1}^{2}=b_{2}^{2}=b_{3}^{2}\), (ii) \(e_{1} e_{2}=e_{2} e_{3}=e_{3} e_{1}=0, \quad b_{1} b_{2}=b_{2} b_{3}=b_{3} b_{1}=0\), (iii) \(e_{2} b_{3}-e_{3} b_{2}=e_{3} b_{1}-e_{1} b_{3}=e_{1} b_{2}-e_{2} b_{1}=0\). Deduce that the only non-zero components of the averaged energy tensor can then be written as \(M^{00}=\sigma_{0}, M^{11}=M^{22}=M^{33}=p\), where \(3 p=\sigma_{n}\).

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free