An electric dipole rotates at constant angular velocity ωin thexy plane. (The charges,±q , are at r±=±R(cosωtx^+sinωty^); the magnitude of the dipole moment is p=2qR.)

(a) Find the interaction term in the self-torque (analogous to Eq. 11.99). Assume the motion is nonrelativistic ( ωR<<c).

(b) Use the method of Prob. 11.20(a) to obtain the total radiation reaction torque on this system. [answer: -μ0p2ω36πcz^]

(c) Check that this result is consistent with the power radiated (Eq. 11.60).

Short Answer

Expert verified

(a) The interaction term in the self-torque is Fradint=μ0q212πca·.

(b) The total radiation reaction torque on this systemμ0p02ω36πc

(c) The power radiated by the electrical dipole is consistent with power radiated by the accelerated charge.

Step by step solution

01

Write the given data from the question.

The angular velocity isω .

The magnitude of the dipole is p=2πR.

The charges are+q and -q.

The position of the charges±q=±R(cosωtx^+sinωty^) .

02

Determine the formulas to calculate the interaction term in the self-torque and total radiation reaction torque.

The expression for the potential due to osculation dipole along z-axis is given as follows.

role="math" localid="1658821706455" V=-p0ω4πε0crcosθr2sin[ω(t-rc)] …… (1)

The expression for the power radiated is given as follows.

P=Sda …… (2)

03

Calculate the interaction term in the self-torque.

The dipole moment of an electric dipole is given by,

p=2qr±

The rotating electric dipole can be taken as super position of dipole moments of two oscillating.

The dipole moment can be expressed as,

p=2qR(cosωtx^+sinωty^)

The total charge is divided into two halves separated by the distance; therefore, the radiation reaction force is given by,

Fradend=μ0q226πca·Fradend=μ0q224πca·

The interaction force is given by,

localid="1658821862972" Fradint=μ0q212πca·

The total radiation force is the sum of the radiation force at both the end.

Frad=Fradend+Fradint

Substitute μ0q224πca· for localid="1658821934982" Fradend and μ0q212πca· for Fradintinto above equation.

localid="1658825657309" Frad=μ0q224πca·+μ0q212πca·Frad=μ0q212πca·×32Frad=μ0q26πca·…… (3)

If the total force is F(q)=Fint(q)+2Fq2. The forceFq2is independent of distance then the interaction forceFint(q)part.

From the equation 11.1, the interaction force is given by,

localid="1658822132351" Fint(q)=μ0q212πca· …… (4)

Now compare the equation (3), the interaction term in the self-torque isFradint=μ0q212πca·which is analogous to equation (4).

Hence the interaction term in the self-torque is Fradint=μ0q212πca·.

04

Calculate the total radiation reaction torque on this system.

The magnitude of the position vector is given by,

r=x2+y2+z2rcosθ=z

Calculate the expression for the potential,

Substitute x2+y2+z2for rand zfor rcosθinto equation (1).

V=p0ω4πε0cxx2+y2+z2sinωtrc

The potential due to rotating electrical dipole is given by,

V=p0ω4πε0cxx2+y2+z2sinωtrcp0ω4πε0cyx2+y2+z2cosωtrcV=p0ω4πε0csinθcosϕrsinωtrcsinθsinϕrcosωtrc

The vector potential due to osculation dipole is given by,

A(r,θ,t)=μ0p0ω4πrsinωtrcz^

The vector potential due to rotating dipole is given by,

A(r,θ,t)=μ0p0ω4πrsinωtrcx^+cosωtrcy^

The intensity is given by.

S=1μ0(E×B)

Substitute 1c(r^×E) for Binto above equation.

S=1μ0E×1c(r^×E)S=1μ0c(E2r^(Er^)E)S=1μ0c(E2r^(0)E)S=1μ0c(E2r^) ……. (5)

The electric strength is given by,

E=VAtE=μ0p0ω24πrsinθrcosωtrcθ^

The electric strength can be expressed as,

cosωtrcx^rcr^+sinωtrcy^yrr^

Take a square of both the sides of the above equation,

E2=μ0p0ω24πr2cosωtrcx^rcr^+sinωtrcy^yrr^2E2=μ0p0ω24πr2x^rcr^2cos2ωtrc+y^yrr^sin2ωtrc2x^rcr^y^yrr^sinωtrccosωtrc …… (6)

Calculate the value of x^rcr^2.

x^rcr^2=1+x2r22x2r2x^rcr^2=1x2r2

Similarly,

y^yrr^2=1y2r2

Calculate the value of x^rcr^y^yrr^.

x^rcr^y^yrr^=x^y^+xy2xrr^y^yrx^r^x^rcr^y^yrr^=0+xyr2xyr2xyr2x^rcr^y^yrr^=xyr2

Substitutexyr2 forx^rcr^y^yrr^, 1y2r2 fory^yrr^2and1x2r2forx^rcr^2into equation (6).

localid="1658824474855" E2=μ0p0ω24πr21x2r2cos2ωtrc+1y2r2sin2ωtrc2xyr2sinωtrccosωtrcE2=μ0p0ω24πr21x2r2cos2ωtrc+1y2r2sin2ωtrc+2xyr2sinωtrccosωtrcE2=μ0p0ω24πr211r2xcosωtrc+ysinωtrc2

Substitute rsinθcosϕfor x, and rsinθsinϕfor yinto above equation.

E2=μ0p0ω24πr211r2rsinθcosϕcosωtrc+rsinθsinϕsinωtrc2E2=μ0p0ω24πr21sin2θcosϕcosωtrc+sinϕsinωtrc2E2=μ0p0ω24πr21sin2θcosωtrcϕ2]r^

Substitute μ0p0ω24πr21sin2θcosωtrcϕ2r^ forE2into equation (5).

S=1μ0cμ0p0ω24πr21sin2θcosωtrcϕ)2r^S=μ0cp0ω24πr22112sin2θr^

Calculate the power radiated dipole,

Substitute localid="1658825122009" μ0cp0ω24πr22112sin2θr^for Sinto equation (3).

localid="1658825212175" P=μ0cp0ω24πr22112sin2θdaP=μ0cp0ω24πr222π112sin2θr2sinθdθdϕP=μ0cp0ω24πr220π02π112sin2θsinθdθdϕP=μ0cp0ω24πr222π0π112sin2θsinθdθdϕ

Solve further as,

P=μ0p02ω48πc0πsinθdθ120πsin3θdθP=μ0p02ω48πc21243P=μ0p02ω46πc

The relationship between the power, torque and velocity is given by,

τ=RvP

Substitute Rωfor vinto above equation.

τ=RRωPτ=1ωP

Substitute μ0p02ω46πcfor Pinto above equation.

τ=1ωμ0p02ω46πcτ=μ0p02ω36πc

Hence the total radiation reaction torque on this system μ0p02ω36πc

05

Calculate the total power radiated.

(c)

The total power radiated from the equation 11.60 is given by,

Prad(t0)μ06πcp··(t0)2 …… (7)

The calculated total power radiated is given by,

P=μ0p02ω46πc …… (8)

By comparing the equations (7) and (8), the power radiated by the electrical dipole is consistent with power radiated by the accelerated charge.

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Most popular questions from this chapter

(a) Does a particle in hyperbolic motion (Eq. 10.52) radiate? (Use the exact formula (Eq. 11.75) to calculate the power radiated.)

(b) Does a particle in hyperbolic motion experience a radiation reaction? (Use the exact formula (Prob. 11.33) to determine the reaction force.)

[Comment: These famous questions carry important implications for the principle of equivalence.]

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.

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.

8 Suppose the (electrically neutral) yz plane carries a time-dependent but uniform surface current K (t) Z.

(a) Find the electric and magnetic fields at a height x above the plane if

(i) a constant current is turned on at t = 0:

K(t)={0,     t0K0,   t>0}

(ii) a linearly increasing current is turned on at t = 0:

K(t)={0,     t0αt,   t>0}

(b) Show that the retarded vector potential can be written in the form, and from

A(x,t)=μ0c2z^0K(txcu)du

And from this determine E and B.

(c) Show that the total power radiated per unit area of surface is

μ0c2[K(t)]2

Explain what you mean by "radiation," in this case, given that the source is not localized.22

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.]

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