In Prob. 2.25, you found the potential on the axis of a uniformly charged disk:

V(r,0)=σ2ε0(r2+R2r)

(a) Use this, together with the fact that Pi(1)=1to evaluate the first three terms

in the expansion (Eq. 3.72) for the potential of the disk at points off the axis, assuming r>R.

(b) Find the potential for r<Rby the same method, using Eq. 3.66. [Note: You

must break the interior region up into two hemispheres, above and below the

disk. Do not assume the coefficients A1are the same in both hemispheres.]

Short Answer

Expert verified

(a) The first three terms in the expansion for the potential r>Ris σR24ε0r1R28r23cos2θ1+.

(b) The first three terms in the expansion for the potential r<Risσ2ε0R+rcosθ+r28R3cos2θ1+

Step by step solution

01

Define functions

Write the expression for the potential outside the disk in spherical polar co-ordinates.

V(r,θ)=l=0Birt1Pi(cosθ){for r<R] …… (1)

Given that, the potential on the axis is,

V(r,0)=σ2ε0(r2+R2r) …… (2)

02

Determine part (a)

a)

From the equation (1)

V(r,θ)=i=0n=Birl=1P1(cosθ)

=i=0Birl=1Pi(1)

V(r,θ)=i=0Biri=1

Then,j=0irBjrj1=σ2ε0r7+Rr

As, r>Rfor this region

r2+R2=r1+R2r22

=r1+12R2r218R4r4+

This is done by (x+1)12.

r2+R2=1+12x123x2+

l=0Bjrl1=σ2ε01+12R2r218R4r4+1

=σ2ε0R22r18R4r3+……. (3)

Substitute I=0in equation (3), then

B0=σR24ε0

B1=0

B2=σR416s0

Now,

V(r,0)=σR24ε0rσR416ε0r3P2(cos0)+

=σR24ε0r1rR24r3P2(cosθ)+

=σR24ε0r1R28r23cos2θ1+

Hence, the first three terms in the expansion for the potentialr>R is σR24ε0r1R28r23cos2θ1+

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

Show that the electric field of a (perfect) dipole (Eq. 3.103) can be written in the coordinate-free form

Edip(r)=14πε014πε01r3[3p·^rr-p]

A long cylindrical shell of radius Rcarries a uniform surface charge σ0on the upper half and an opposite charge -σ0on the lower half (Fig. 3.40). Find the electric potential inside and outside the cylinder.

(a) Show that the quadrupole term in the multipole expansion can be written as

V"quad"(r)=14πε01r3(i,j=13r^ir^jQij.....(1)

(in the notation of Eq. 1.31) where

localid="1658485520347" Qij=12[3ri'rj'-(r')2δij]ρ(r')dτ'.....(2)

Here

δ_ij={1ifi=j0ifij.....(3)

is the Kronecker Deltalocalid="1658485013827" (Qij)and is the quadrupole moment of the charge distribution. Notice the hierarchy

localid="1658485969560" Vmon=14πε0Qr;Vdip=14πε0r^ipjr2;Vquad(r)=14πε01r3i,j=13r^ir^jQIJ;...

The monopole moment localid="1658485018381" (Q) is a scalar, the dipole moment localid="1658485022577" (p) is a vector, the quadrupole moment localid="1658485026647" (Qij)is a second rank tensor, and so on.

(b) Find all nine components of localid="1658485030553" (Qij)for the configuration given in Fig. 3.30 (assume the square has side and lies in the localid="1658485034755" x-y plane, centered at the origin).

(c) Show that the quadrupole moment is independent of origin if the monopole and

dipole moments both vanish. (This works all the way up the hierarchy-the

lowest nonzero multipole moment is always independent of origin.)

(d) How would you define the octopole moment? Express the octopole term in the multipole expansion in terms of the octopole moment.

Show that the average field inside a sphere of radius R, due to all the charge within the sphere, is

Eave=-14πε0ρR3

Where ρis the total dipole moment. There are several ways to prove this delightfully simple result. Here's one method:

(a) Show that the average field due to a single chargeqat point r inside thesphere is the same as the field at r due to a uniformly charged sphere with

ρ=q/(43πR3), namely

14πε0(43πR3)qr2rdζ'

Where r is the vector from r to dζ

(b) The latter can be found from Gauss's law (see Prob. 2.12). Express the answerin terms of the dipole moment of q.

(c) Use the superposition principle to generalize to an arbitrary charge distribution.

(d) While you're at it, show that the average field over the volume of a sphere, dueto all the charges outside, is the same as the field they produce at the center.

In Ex. 3.8 we determined the electric field outside a spherical conductor

(radiusR)placed in a uniform external field E0. Solve the problem now using

the method of images, and check that your answer agrees with Eq. 3.76. [Hint:Use

Ex. 3.2, but put another charge, -q,diametrically opposite q.Leta, with14πε02qa2=-E0held constant.]

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