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Deduce Eq. 11.100 from Eq. 11.99. Here are three methods:

(a) Use the Abraham-Lorentz formula to determine the radiation reaction on each end of the dumbbell; add this to the interaction term (Eq. 11.99).

(b) Method (a) has the defect that it uses the Abraham-Lorentz formula—the very thing that we were trying to derive. To avoid this,F(q) let be the total d-independent part of the self-force on a charge q. Then

F(q)=Fint(q)+2F(q2)

WhereFint is the interaction part (Eq. 11.99), andF(q2) is the self-force on each end. Now,F(q) must be proportional to q2, since the field is proportional to q and the force is qE. SoF(q2)=(14)F(q) Take it from there.

(c) Smear out the charge along a strip of length L oriented perpendicular to the motion (the charge density, then, is λ=qL); find the cumulative interaction force for all pairs of segments, using Eq. 11.99 (with the correspondence q2→λdy, at one end and at the other). Make sure you don’t count the same pair twice.

Short Answer

Expert verified

(a) Equation 11.100 using Abraham-Lorentz formula is Frad=μ0q26πca˙.

(b) Equation 11.100 usingFq=Fintq+2Fq2 is Frad=μ0q26πca˙.

(c) Equation 11.100 using cumulative interaction force is Frad=μ0q26πca˙.

Step by step solution

01

Expression for the Abraham-Lorentz formula:

Write the expression for the Abraham-Lorentz formula.

Frad=μ0q26Πca˙

Here, q is the point charge, c is the speed of light, andaË™ is the time rate of the acceleration.

02

Deduce equation 11.100 using Abraham-Lorentz formula:

(a)

Write the expression for the radiation reaction force at the end of the dumbbell.

Fradend=μ0q226πca˙Fradend=μ0q224πca˙

Write the expression for the interaction force (using equation 11.99).

Fradint=μ0q212πca˙

Hence, the total radiation force in dumbbell will be,

Frad=2Fradend+FradintFrad=2μ0q224πca˙+μ0q212πca˙Frad=μ0q212πca˙1+1Frad=μ0q26πca˙˙

Therefore, the equation 11.100 is deduced.

03

Deduce equation 11.100 using F(q)=Fint(q)+2F(q2) :

(b)

Consider is the totalFqd-independent part of the self-force that acts on the charge q, then,

Fq=Fintq+2Fq2 …… (2)

Here,Fq2 is the self-force on each end of the dumbbell andFintq is the interaction force part.

Write the relation betweenFq and Fq2.

Fq2=14Fq

SubstituteFrad=μ0q26πca˙ andFq2=14Fq in equation (2).

Fq=μ0q212πca˙+214FqFintq=FradintFq-12Fq=μ0q212πca˙Fq=μ0q26πca˙

Therefore, equation 11.100 is deduced.

04

Deduce equation 11.100 using cumulative interaction force:

(c)

Write the cumulative interaction force expression on all the pairs of segments.

F=μ012πca˙∫0y12λdy22dy1

Integrate from 0 to L and divide the result with L.

role="math" localid="1653989418237" F=μ012πca˙4λ2∫0Ly1dy1F=μ012πca˙4λ2L22F=μ06πca˙λ2L2

Here, λ=qL.

Hence, the above equation becomes,

F=μ06πca˙qL2L2F=μ06πca˙q2

Therefore, equation 11.100 is deduced.

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Most popular questions from this chapter

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 ε→0.

(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^ â¶Ä‰â¶Ä‰â¶Ä‰(−∞<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 particle of mass m and charge q is attached to a spring with force constant k, hanging from the ceiling (Fig. 11.18). Its equilibrium position is a distance h above the floor. It is pulled down a distance d below equilibrium and released, at timet=0.

(a) Under the usual assumptions (d≪λ≪h), calculate the intensity of the radiation hitting the floor, as a function of the distance R from the point directly below q. [Note: The intensity here is the average power per unit area of floor.]

FIGURE 11.18

At whatR is the radiation most intense? Neglect the radiative damping of the oscillator.

(b) As a check on your formula, assume the floor is of infinite extent, and calculate the average energy per unit time striking the entire floor. Is it what you’d expect?

(c) Because it is losing energy in the form of radiation, the amplitude of the oscillation will gradually decrease. After what timebhas the amplitude been reduced to d/e? (Assume the fraction of the total energy lost in one cycle is very small.)

An electron is released from rest and falls under the influence of gravity. In the first centimeter, what fraction of the potential energy lost is radiated away?

Use the result of Prob. 10.34 to determine the power radiated by an ideal electric dipole, , at the origin. Check that your answer is consistent with Eq. 11.22, in the case of sinusoidal time dependence, and with Prob. 11.26, in the case of quadratic time dependence.

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