Apply Eqs. 11.59 and 11.60 to the rotating dipole of Prob. 11.4. Explain any apparent discrepancies with your previous answer

Short Answer

Expert verified

The equation of the Poynting vectorS=μ0p02ω416π2csin2θr2r^ disagrees with the value of Poynting vector S in problem 11.4 because, in this problem, the polar axis is along the direction ofpt0¨ .

For the case of total radiated power, the value ofPradt0=μ0p02ω46πc agrees with the value of P in problem 11.4 because, in this problem, the integration of all angles is calculated, and the orientation of the polar axis is irrelevant.

Step by step solution

01

Expression for the dipole moment of rotating dipole:

Write the expression for the dipole moment of the rotating dipole.

p(t)=p0cos(ωt)x^+p0sin(ωt)y^ …… (1)

Write the expression for the Poynting vector (using equation 11.59 ).

S=μ0p¨t216π2csin2θr2r^ …… (2)

Write the expression for the total radiated power (using equation ).

Pradt0μ06πcp¨t02 …… (3)

02

Determine the apparent discrepancies:

Take the double differentiation of equation (1).

p˙t=-p0ωsinωtx^+p0ωcosωty^p¨t=-p0ω2cosωtx^-p0ω2sinωty^p¨t=-p0ω2cosωtx^+sinωty^

Substitutep¨t=-p0ω2cosωtx^+sinωty^ in the above value in equation (2).

S=μ0-p0ω2cosωtx^+sinωty^216π2csin2θr2r^S=μ0p02ω416π2ccos2ωt+sin2ωtsin2θr2r^S=μ0p02ω416π2csin2θr2r^

Hence, the above equation disagrees with the value of Poynting vector S in problem 11.4 because, in this problem, the polar axis is along the direction of p¨t0.

Substitutep¨t=-p0ω2cosωtx^+sinωty^ in equation (3).

Pradt0μ06πc-p0ω2cosωtx^+sinωty^2Pradt0=μ0p02ω46πc

For the case of total radiated power, the value ofPradt0=μ0p02ω46πc agrees with the value of P in problem 11.4 because, in this problem, the integration of all angles is calculated, and the orientation of the polar axis is irrelevant.

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Most popular questions from this chapter

Find the radiation resistance (Prob. 11.3) for the oscillating magnetic dipole in Fig. 11.8. Express your answer in terms ofλand b , and compare the radiation resistance of the electric dipole. [ Answer: 3×105(bλ)4Ω]

With the inclusion of the radiation reaction force (Eq. 11.80) Newton’s second law for a charged particle becomes

a=τa˙+Fm

Where Fis the external force acting on the particle.

(a) In contrast to the case of an unchanged particle (a=Fm), acceleration (like position and velocity) must now be a continuous function of time, even if the force changes abruptly. (Physically, the radiation reaction damps out any rapid change in a). Prove that ais continuous at any time t, by integrating the equation of motion above from (t-ε)to (t+ε)and taking the limit ε0.

(b) A particle is subjected to constant force F, beginning at timet=0and lasting until time T. Find the most general solution role="math" localid="1658753661705" a(t)to the equation of motion in each of the three periods: (i) t<0; (ii) 0<t<T ; (iii) t>T.

(c) Impose the continuity condition (a) at t=0and t=T. Sow that you can either eliminate the runaway in region (iii) or avoid pre-acceleration in region (i), but not both.

(d) If you choose to eliminate the runaway, what is the acceleration as a function of time, in each interval? How about the velocity? (The latter must, of course, be continuous at t=0andt=T ). Assume the particle was originally at rest; v(-)=0.

(e) Plot a(t)and v(t), both for an uncharged particle and for a (non-runaway) charged particle, subject to this force.

An ideal electric dipole is situated at the origin; its dipole moment points in the z direction and is quadratic in time:

p(t)=12p¨0t2z^    (<t<)

wherep¨0is a constant.

  1. Use the method of Section 11.1.2 to determine the (exact) electric and magnetic fields for all r > 0 (there's also a delta-function term at the origin, but we're not concerned with that).
  2. Calculate the power, P(r,t), passing through a sphere of radius r.
  3. Find the total power radiated (Eq. 11.2), and check that your answer is consistent with Eq. 11.60.21

(a) A particle of charge qmoves in a circle of radiusRat a constant speedv. To sustain the motion, you must, of course, provide a centripetal forcemv2Rwhat additional force (Fe) must you exert, in order to counteract the radiation reaction? [It's easiest to express the answer in terms of the instantaneous velocityv.] What power (Pe) does this extra force deliver? ComparePewith the power radiated (use the Larmor formula).

(b) Repeat part (a) for a particle in simple harmonic motion with amplitudeand angular frequency:ω.ω(t)=Acos(ωt)z Explain the discrepancy.

(c) Consider the case of a particle in free fall (constant accelerationg). What is the radiation reaction force? What is the power radiated? Comment on these results.

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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