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(a) Check Eq. 5.76 for the configuration in Ex. 5.9.

(b) Check Eqs. 5.77 and 5.78 for the configuration in Ex. 5.11.

Short Answer

Expert verified

(a) The equation 5.76 satisfies.

(b) The equations 5.77 and 5.78 is satisfied.

Step by step solution

01

Significance of magnetostatics

Magnetostatics is mainly used for predicting fast switching magnetic events which occur in less than a nanosecond. Moreover, magnetostatics is also a good approximation when there is no static current.

02

(a) Checking the equation 5.76

The equation 5.76 can be expressed as:

Babove-Bbelow=μ0(K×n^) …(i)

Here, Baboveand Bbeloware the magnetic field at the top and the bottom,μ0 is the permeability, k is the constant and n^is the position vector.

At the solenoid’s surface, the magnetic field at the top is zero.

The equation of the magnetic field at the bottom at solenoid’s surface is expressed as:

Bbelow=μ0nIz^

Here, lis the current andz^ is the position vector along the z axis.

Substitute for in the above equation.

Bbelow=μ0Kz^

Substitute -Kz^for(K×n^) in the equation (i).

Babove-Bbelow=-μ0Kz^

Thus, the equation 5.76 satisfies.

03

(b) Checking the equation 5.77 and 5.78

The equation in the example 5.11 is expressed as:

Ar,θ,ϕ=μ0Rωδ3rsinθϕ^rR=μ0R4ωδ3sinθr2ϕ^rR …(ii)

The equation 5.77 is expressed as:

Aabove=Abelow

The equation 5.78 is expressed as:

Aaboven-Abelown=-μ0K

In the equation of the example 5.11, the both the equations have the same values at the surface. Hence, it satisfies the equation 5.77 asAabove=Abelow .

Differentiating the equation (ii) with respect to the coordinate r in order to find the left side of the equation 5.78 .

ArR+=μ0R4ωδ3-2sinθr3ϕ^R=2μ0Rωδ3sinθϕ^=μ0Rωδ3sinθϕ^

The equation of the constant K is expressed as:

K=δV=δω×r=δωrsinθϕ^

Hence, the right and the left side of the equation 5.78 is satisfied.

Thus, the equations 5.77 and 5.78 is satisfied.

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Most popular questions from this chapter

Show that the magnetic field of a dipole can be written in coordinate-free form:

Bdip(r)=μ04π1r3[3(mr^)r^-m]

Suppose you have two infinite straight line chargesλ, a distance d apart, moving along at a constant speed υ(Fig. 5.26). How great would have tobe in order for the magnetic attraction to balance the electrical repulsion? Work out the actual number. Is this a reasonable sort of speed?

Use the results of Ex. 5.11to find the magnetic field inside a solid sphere, of uniform charge density ρand radius R, that is rotating at a constant angular velocity \omega.

A thin uniform donut, carrying charge Qand mass M, rotates about its axis as shown in Fig. 5.64.

(a) Find the ratio of its magnetic dipole moment to its angular momentum. This is called the gyromagnetic ratio (or magnetomechanical ratio).

(b) What is the gyromagnetic ratio for a uniform spinning sphere? [This requires no new calculation; simply decompose the sphere into infinitesimal rings, and apply the result of part (a).]

(c) According to quantum mechanics, the angular momentum of a spinning electron is role="math" localid="1658120028604" 12, where is Planck's constant. What, then, is the electron's magnetic dipole moment, in role="math" localid="1658120037359" A×M2 ? [This semi classical value is actually off by a factor of almost exactly 2. Dirac's relativistic electron theory got the 2right, and Feynman, Schwinger, and Tomonaga later calculated tiny further corrections. The determination of the electron's magnetic dipole moment remains the finest achievement of quantum electrodynamics, and exhibits perhaps the most stunningly precise agreement between theory and experiment in all of physics. Incidentally, the quantity (e2m ), where e is the charge of the electron and m is its mass, is called the Bohr magneton.]

What current density would produce the vector potential, A=kϕ^(where kis a constant), in cylindrical coordinates?

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