Check that the retarded potentials of an oscillating dipole (Eqs. 11.12 and 11.17) satisfy the Lorenz gauge condition. Do not use approximation 3.

Short Answer

Expert verified

The retarded potentials of an oscillating dipole satisfy the Lorenz gauge condition.

Step by step solution

01

Expression for the Lorenz gauge condition:

Write the expression for the Lorenz gauge condition.

·A=-μ0ε0(Vt) …… (1)

Here,μ0 is the magnetic permeabilityε0 is the magnetic permittivity, A is the vector potential, and V is the scalar potential.

02

Determine the value of ∇·A :

Write the expression for the vector potential (using equation 11.17 ).

A=-μ0p0ω4π1rsinωt-rcz^A=-μ0p0ω4π1rsinωt-rccosθr^-sinθθ^

Calculate the value of ·A.

·A=1r2rr2Ar+1rsinθθsinθAθ+1rsinθϕϕ·A=1r2rr2-μ0p0ω4π1rsinωt-rccosθ1rsinθθ-μ0p0ω4π1rsinωt-rc-sin2θ+·A=-μ0p0ω4π1r2r1rr2sinωt-rccosθ-ωrccosωt-ωrccosθ-2sinθcosθr3sinθsinωt-ωrc·A=-μ0p0ω4π1r2sinωt-ωrcωrccosωt-ωrc-2r2sinωt-ωrccosθ

On further solving, the above equation becomes,

localid="1653907297258" ·A=-μ0p0ω4π2-1r2sinωt-ωrc+ωrccosωt-ωrccosθ·A=-μ0ωp0ω4πε01r2sinωt-rc+ωrccosωω-rccosθ....(1)

03

Determine the Lorenz gauge condition:

Write the expression for the scalar potential for an oscillating dipole potential (using equation 11.12 ).

V=p0cosθ4πε0r-ωcsinωt-rc+1rcosωt-rc

Calculate the value of Vt.

Vt=p0cosθ4πε0r-ω2ccosωt-rc-ωrsinωt-rcVt=p0ω4πε01r2sinωt-rc+ωrccosωt-rccosθ.......(2)

From equations (1) and (2),

·A=-μ0ωVt

Therefore, the retarded potentials of an oscillating dipole satisfy the Lorenz gauge condition.

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Most popular questions from this chapter

Use the “duality” transformation of Prob. 7.64, together with the fields of an oscillating electric dipole (Eqs. 11.18 and 11.19), to determine the fields that would be produced by an oscillating “Gilbert” magnetic dipole (composed of equal and opposite magnetic charges, instead of an electric current loop). Compare Eqs. 11.36 and 11.37, and comment on the result.

As you know, the magnetic north pole of the earth does not coincide with the geographic north pole—in fact, it’s off by about 11°. Relative to the fixed axis of rotation, therefore, the magnetic dipole moment of the earth is changing with time, and the earth must be giving off magnetic dipole radiation.

(a) Find the formula for the total power radiated, in terms of the following parameters:ψ (the angle between the geographic and magnetic north poles), M (the magnitude of the earth’s magnetic dipole moment), andω (the angular velocity of rotation of the earth). [Hint: refer to Prob. 11.4 or Prob. 11.11.]

(b) Using the fact that the earth’s magnetic field is about half a gauss at the equator, estimate the magnetic dipole moment Mof the earth.

(c) Find the power radiated. [Answer: 4×10-5W]

(d) Pulsars are thought to be rotating neutron stars, with a typical radius of 10 km, a rotational period of 10-3s, and a surface magnetic field of 108T. What sort of radiated power would you expect from such a star? [Answer: 2×1036W].

A parallel-plate capacitor C, with plate separation d, is given an initial charge (±)Q0. It is the0n connected to a resistor R, and discharges, Q(t)=Q0e-t/RC.

(a) What fraction of its initial energy(Q02/2C) does it radiate away?

(b) If C=1pF,R=1000Ω,and role="math" localid="1653972749344" d=0.1mm, what is the actual number? In electronics we don’t ordinarily worry about radiative losses; does that seem reasonable, in this case?

Use the duality transformation (Prob. 7.64) to construct the electric and magnetic fields of a magnetic monopole qmin arbitrary motion, and find the “Larmor formula” for the power radiated.

RepeatProb. 11.19, but this time let the external force be a Dirac delta function:F(t)=k(t)(for some constant k)[Note that the acceleration is now discontinuous att=0(though the velocity must still be continuous); use the method ofProb. 11.19(a) to show thatΔa=k/. In this problem there are only two intervals to consider: (i)t<0and (ii)t>0.]

(b) As inProb. 11.30, check that energy is conserved in this process.

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