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(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:Ӭ.Ӭ(t)=Acos(Ӭt)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.

Short Answer

Expert verified

(a) The power delivered by the extra force is Pe=μ0q26πcӬ2v2. The power delivered is equal to power radiated.

(a) The power when motion is simple harmonic is μ0q26πcӬ4A2sin2(Ӭt). The energy which is been radiating is the same as that of the energy input.

(b)The radiation reaction force isFe=0. The power radiated is Prad=μ0q26πcg2.

Step by step solution

01

Understand the motion of the charged particle

When a charged particle or any matter rotates in a circular path, that matter experiences two forces.

One force of the forces out of them is directed towards the rotation axis called centripetal force. Another force acts outside the charged particle called centrifugal force.

02

Step 2: Identifythe given data

The given data can be listed as:

  • The charged particle isq
  • The radius of the circle is R.
  • The constant velocity is v.
  • The force exerted over the particle is Fe.
  • Thepower is Pe.
03

(a) Determinethepower when the particle is in a circular motion

We know that to counteract the radiation reaction we must have to exert a force of

Fe=−μ0q26πca˙ … (i)

Here, Feis the force of radiation,μ0is the permeability of free space,cis the velocity of light in a vacuum, qis the charged particle,a˙=dadtis the rate of change ofacceleration.

For circular motion

r(t)=R[cos(Ӭt)x^+sin(Ӭt)y^] … (ii)

We can write from equation (ii) that

v(t)=r˙=drdt=ddt(R[cos(Ӭt)x^+sin(Ӭt)y^])=RӬ[−sin(Ӭt)x^+cos(Ӭt)y^]

Here,Ris the radius of the circular path,Ó¬is the angular frequency, x^andy^are the unit vectors in the direction of the horizontal and vertical axis respectively,vis the velocity.

Now, from equation (ii) we can write

a(t)=v˙=ddtv=ddt(RӬ[−sin(Ӭt)x^+cos(Ӭt)y^])=−RӬ2[cos(Ӭt)x^+sin(Ӭt)y^]

It is further solved as

a(t)=−Ӭ2ra=v˙

Here,a is the acceleration of the body.

Now,the rate of change of acceleration

a˙=dadt=ddt(−Ӭ2r)=−Ӭ2drdt=−Ӭ2r˙

It is further solved as

a˙=−Ӭ2v … (iii)

Therefore, putting equation (iii) in equation (i), we get:

Fe=−μ0q26πc(−Ӭ2v)=μ0q26πcӬ2v

Hence, the force of radiation is μ0q26πcӬ2v.

Now, as we know that

Power=Force×velocity

Therefore

Pe=Fe×v=μ0q26πcӬ2v×v=μ0q26πcӬ2v2

… (iv)

Here,Peis the power which extra force delivers.

Thus, the power delivered is μ0q26πcӬ2v2.

Meanwhile, we know that

Prad=μ0q26πca2

Here, Pradis the power radiated.

We know that

a=−Ӭ2r

Therefore

a2=-Ó¬2r2=Ó¬4r2=Ó¬4r2=Ó¬2v2

Hence, we can write putting the value in equation (iv) as

Pe=μ0q26πca2=Prad

Thus, the power delivered is equal to power radiated.

04

(b) Determination of power when the particle is in a simple harmonic motion (SHM)

For simple harmonic motion, it isgiven that

r=Acos(Ӭt)z^ … (v)

Here,z^ is the unit vector along thez-direction

Now, to calculate velocity, we have

role="math" localid="1658752719009" v(t)=Ӭ˙=drdt=ddt(Acos(Ӭt))z^=−AӬsin(Ӭt)z^ … (vi)

Now, to calculate acceleration

a(t)=v˙=dvdt=ddt(−AӬsin(Ӭt))z^=−AӬ2cos(Ӭt)z^ … (vii)

Now, from the equation (vii) and (v), we can write

a=−Ӭ2r

Now, the rate of change of acceleration

a˙=dadt=ddt(−Ӭ2r)=−Ӭ2r˙=−Ӭ2v

Therefore, from equation(i) we can write

Fe=−μ0q26πca˙=−μ0q26πc(−Ӭ2v)=μ0q26πcӬ2v

Thus, the radiation reaction force isμ0q26πcӬ2v.

Hence, power can be calculated as

Pe=μ0q26πcӬ2v×v=μ0q26πcӬ2v2

Thus, the power is μ0q26πcӬ2v2.

Now, as we know from part (a) that

a2=Ó¬4r2

Substitute equation (v) in the above expression.

Therefore

a2=Ó¬4r2=Ó¬4Acos(Ó¬t)2=Ó¬4A2cos2(Ó¬t)

Ó¬2v2=Ó¬4A2sin2(Ó¬t)

Hence, the radiated power is

Prad=μ0q26πca2=μ0q26πcA2Ӭ4cos2(Ӭt) … (viii)

Pe=μ0q26πcӬ2v2=μ0q26πcӬ4A2sin2(Ӭt)

Therefore,Prad is not equal to Pewhen the body moves in SHM.This occurs because we know that over a full cycle the time average ofsin2(Ó¬t) andcos2(Ó¬t)are equal.Hence, the energy which is radiating is the same as that of the energy input.

05

(c)Determination of power when the particle is in a free falling state

We know that for a free-falling body with constant acceleration g, the displacement of that particle will be

s=12gt2y^

Here,y^is the unit vector along the vertical direction.

Therefore, velocity is given as

v(t)=s˙v=dsdt=ddt(12gt2)=gty^

Here,y^is the unit vector along the vertical direction. is the acceleration due to gravity, and tis the time.

Therefore, the acceleration is

a(t)=vË™=dvdt=ddt(gt)y^=gy^

Hence, the change in acceleration is

aË™=dadt=ddtg=0

Here, a is equal to g.

Substitute the value in equation (1).

Fe=−μ0q26πca˙Fe=0

Therefore,the radiation reaction force is equal to zero.

Substitute the value in the equationPe=Fe×v from equation (i).

Pe=Fe×vPe=0

Hence, thereaction power is zero.

Now, puta=g in the expression of radiated power from equation (viii).

Prad=μ0q26πcg2

Hence, due to this reason, energy will be taken from the nearby fields.So, in this exact solution the paradox stays.

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Most popular questions from this chapter

Calculate the electric and magnetic fields of an oscillating magnetic dipole without using approximation . [Do they look familiar? Compare Prob. 9.35.] Find the Poynting vector, and show that the intensity of the radiation is exactly the same as we got using approximation .

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 thatΔ²¹=−k/³¾Ï„. 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.

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]

A positive charge q is fired head-on at a distant positive charge Q (which is held stationary), with an initial velocityv0 . It comes in, decelerates to v=0, and returns out to infinity. What fraction of its initial energy(12mv02) is radiated away? Assume v0≪c, and that you can safely ignore the effect of radiative losses on the motion of the particle. [ Answer (1645)(qQ)(v0c)3. ]

A charged particle, traveling in from −∞ along the x axis, encounters a rectangular potential energy barrier

U(x)={U0, if 0<x<L,0, otherwise}

Show that, because of the radiation reaction, it is possible for the particle to tunnel through the barrier-that is, even if the incident kinetic energy is less thanU0, the particle can pass through 26.[Hint: Your task is to solve the equation

a=τa˙+Fm

Subject to the force

F(x)=U0[−δ(x)+δ(x−L)]

Refer to Probs. 11.19 and 11.31, but notice that this time the force is a specified function ofx, nott. There are three regions to consider: (i)x<0, (ii) 0<x<L, (iii)x>L. Find the general solution fora(t), Ï…(t), andx(t)in each region, exclude the runaway in region (iii), and impose the appropriate boundary conditions at x=0andx=L. Show that the final velocity (Ï…f)is related to the time spent traversing the barrier by the equation

,L=υfT−U0mυf(τe−T/τ+T−τ)

and the initial velocity (atx=−∞) is

υi=υf−U0mυf[1−11+υ0mvf2(e−T/τ−1)]

To simplify these results (since all we're looking for is a specific example), suppose the final kinetic energy is half the barrier height. Show that in this case

υi=υf1−(L/υfτ)

In particular, if you choose L=υfτ/4 , then υi=(4/3)υf, the initial kinetic energy is (8/9)U0, and the particle makes it through, even though it didn't have sufficient energy to get over the barrier!]

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