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 q2λdy, 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, anda˙ 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˙4λ20Ly1dy1F=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 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.

Question: In Ex. 11.3 we assumed the velocity and acceleration were (instantaneously,

at least) collinear. Carry out the same analysis for the case where they are

perpendicular. Choose your axes so that v lies along the z axis and a along the x axis

(Fig. 11.14), so thatv=vz^,a=ax^,andr^=sinθcosϕx^+sinv=vz^,a=ax^,andr^=sinθcosϕx^+sinsinϕy^+cosθz^Check that P is consistent with the Lienard formula.

dP=μ0q2a216π2c1-βcosθ2-1-β2sin2θcos2ϕ1-βcosθ5,P=μ0q2a2γ46πc[Answer: .For relativistic velocities ( β1) the radiation is again sharply peaked in the forward

direction (Fig. 11.15). The most important application of these formulas is to circular motion-in this case the radiation is called synchrotron radiation. For a relativistic electron, the radiation sweeps around like a locomotive's headlight as the particle moves.]

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.

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.

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.

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