/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q11.5P Calculate the electric and magne... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

Calculate the electric and magnetic fields of an oscillating magnetic dipole without using approximation . [Do they look familiar? Compare Prob. 9.35.] Find the Poynting vector, and show that the intensity of the radiation is exactly the same as we got using approximation .

Short Answer

Expert verified

The electric fields of an oscillating magnetic dipole is E=μ0m0Ӭ4πsinθr1rsinӬt−rc+ӬccosӬt−rcϕ.

The magnetic fields of an oscillating magnetic dipole is

B=μ0m04π2cosθr21rcosӬ1−rc−ӬcsinӬt−rcr^−sinθr−1r2cosӬt−rc+ӬrcsinӬt−rc+Ӭc2cosӬt−rc.

The average value of Poynting vector intensity is ⟨S⟩=μ0m02Ӭ432π2c3sin2θr2r^ .

Step by step solution

01

Write the given data from the question.

Consider that the intensity of the radiation is exactly the same as we got using approximation 3.

02

Determine the formula of electric and magnetic fields of an oscillating magnetic dipole and average value of Poynting vector intensity.

Write the formula ofelectric fields of an oscillating magnetic dipole.

E=∂A∂t …… (1)

Here,A is vector potential of an Oscillating magnetic dipole.

Write the formula ofmagnetic fields of an oscillating magnetic dipole.

B=∇×A …… (2)

Here, A is vector potential of an Oscillating magnetic dipole.

Write the formula ofaverage value of Poynting vector intensity.

. S=1C(E×B) …… (3)

Here, E is electric field of an oscillating magnetic dipole, C is speed of sound and B is magnetic field of an oscillating magnetic dipole.

03

Determine the electric and magnetic fields of an oscillating magnetic dipole and average value of Poynting vector intensity.

The vector potential of an Oscillating magnetic dipole is:

A(r,θ,t)=μ0m04πsinθr1rcosӬt−rc−ӬcsinӬt−rcφ^

Here, μ0is permeability of free space, m0is the mass, K is the wave number, Cis the speed of sound, Ӭis the angular frequency, and t is the time.

Determine theelectric fields of an oscillating magnetic dipole.

Substitute μ0m04πsinθr1rcosӬt−rc−ӬcsinӬt−rcφ^ for Ainto equation (1).

E=μ0m04πsinθr1rcosӬt−rc−ӬcsinӬt−rcφ^=−μ0m04πsinθr1rӬsinӬt−rc−Ӭ2ccosӬt−rcϕ^=μ0m0Ӭ4πsinθr1rsinӬt−rc+ӬccosӬt−rcϕ^

Therefore, the electric fields of an oscillating magnetic dipole is

role="math" localid="1658930668909" E=μ0m0Ӭ4πsinθr1rsinӬt−rc+ӬccosӬt−rcϕ.

Determine the magnetic fields of an oscillating magnetic dipole.

Substitute μ0m0Ӭ4πsinθr1rsinӬt−rc+ӬccosӬt−rcϕ for Ainto equation (2).

∇×A=1rsinθ∂∂θ(sinθAϕ)−∂Aθrθr^+1sinθ∂Ar∂ϕ−∂∂r(rAϕ)ϕ^+1r∂∂rrAθ1−dAr∂θϕ^

Here, Arand A0are not taken then:

role="math" localid="1658931445531" ∇×A=1rsinθ∂∂θ(sinθAϕ)r^1r∂∂r(rAϕ)θ^∇×A=μ0m04π1rsinθ∂∂θsinθsinθr1rcosӬt−rc−ӬcsinӬt−rcr^−1r∂∂rr⋅sinθr1rcos[Ӭt−rc−ӬcsinӬt−rc]θ^B=μ0m04π2cosθr21rcosӬt−rc−ӬcsinӬt−rcr^−sinθr−1r2cosӬt−rc+ӬrcsinӬt−rc+Ӭc2cosӬt−rcθ^

In problem 9.33 the result is A=μ0m0Ӭ24πc

Determine the average value of Poynting vector intensity.

Substitute μ0m0Ӭ4πsinθr1rsinӬt−rc+ӬccosӬt−rc]ϕ^ for Eand

B=μ0m04π2cosθr21rcosӬt−rc−ӬcsinӬt−rcr^−sinθr−1r2cosӬt−rc+ӬrcsinӬt−rc+Ӭc2cosӬt−rc for Binto equation (3).

S=1c(E×B)S=μ0m02Ӭ316π2c2sinθr22cosθr1−c2Ӭ2r2sinucosu+cӬr(cos2u−sin2u)θ^+sinθ−2r+c2Ӭ2r3sinucosu+Ӭccos2u+cӬr2(sin2u−cos2u)r^

Here, u=−Ӭt−rc

Then average value of Poynting vector is intensity

⟨S⟩=μ0m02Ӭ432π2c3sin2θr2r^

This is the same radiation intensity that we estimated using approximations.

Therefore, the average value of Poynting vector intensity is <S>=μ0m02Ӭ432π2c3sin2θr2r^ .

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 91Ó°ÊÓ!

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

Find the radiation resistance of the wire joining the two ends of the dipole. (This is the resistance that would give the same average power loss—to heat—as the oscillating dipole in fact puts out in the form of radiation.) Show thatR=790(dλ)2Ω , whereλ is the wavelength of the radiation. For the wires in an ordinary radio (say, d = 5 cm ), should you worry about the radiative contribution to the total resistance?

A positive charge q is fired head-on at a distant positive charge Q (which is held stationary), with an initial velocityv0 . It comes in, decelerates to v=0, and returns out to infinity. What fraction of its initial energy(12mv02) is radiated away? Assume v0≪c, and that you can safely ignore the effect of radiative losses on the motion of the particle. [ Answer (1645)(qQ)(v0c)3. ]

As a model for electric quadrupole radiation, consider two oppositely oriented oscillating electric dipoles, separated by a distance d, as shown in figure in Fig. 11.19. Use the results of Sect. 11.1.2 for the potentials of each dipole, but note that they are not located at the origin. Keeping only the terms of first order in d:

(a) Find the scalars and vector potentials

(b) Find the electric and magnetic fields.

(c) Find the pointing vector and the power radiated

A charged particle, traveling in from −∞ along the x axis, encounters a rectangular potential energy barrier

U(x)={U0, if 0<x<L,0, otherwise}

Show that, because of the radiation reaction, it is possible for the particle to tunnel through the barrier-that is, even if the incident kinetic energy is less thanU0, the particle can pass through 26.[Hint: Your task is to solve the equation

a=τa˙+Fm

Subject to the force

F(x)=U0[−δ(x)+δ(x−L)]

Refer to Probs. 11.19 and 11.31, but notice that this time the force is a specified function ofx, nott. There are three regions to consider: (i)x<0, (ii) 0<x<L, (iii)x>L. Find the general solution fora(t), Ï…(t), andx(t)in each region, exclude the runaway in region (iii), and impose the appropriate boundary conditions at x=0andx=L. Show that the final velocity (Ï…f)is related to the time spent traversing the barrier by the equation

,L=υfT−U0mυf(τe−T/τ+T−τ)

and the initial velocity (atx=−∞) is

υi=υf−U0mυf[1−11+υ0mvf2(e−T/τ−1)]

To simplify these results (since all we're looking for is a specific example), suppose the final kinetic energy is half the barrier height. Show that in this case

υi=υf1−(L/υfτ)

In particular, if you choose L=υfτ/4 , then υi=(4/3)υf, the initial kinetic energy is (8/9)U0, and the particle makes it through, even though it didn't have sufficient energy to get over the barrier!]

A current I(t)flows around the circular ring in Fig. 11.8. Derive the general formula for the power radiated (analogous to Eq. 11.60), expressing your answer in terms of the magnetic dipole moment, m(t) , of the loop.

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.