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

U(x)={U0,if0<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(xL)]

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), υ(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 (υf)is related to the time spent traversing the barrier by the equation

,L=υfTU0mυf(τeT/τ+Tτ)

and the initial velocity (atx=) is

υi=υfU0mυf[111+υ0mvf2(eT/τ1)]

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!]

Short Answer

Expert verified

(a) The value of radiation reaction subject to the force is Δa=±U0mtν.

(b) Region (i): The value of 3th region the general solution isa(t)=0 , υ(t)=B3and.x(t)=B3t+C3

(c) Region (ii): The value of 2nd region the general solution isa(t)=U0mtνfe(tT)t, and x(t)=L+νf(tT)+U0mvf[te(tT)tt+Tt]

(d) Region (iii): The value of 1st region the general solution isa(t)=A1el/t , and x(t)=A1t2el/t+B1t+C1.

Step by step solution

01

Write the given data from the question

Consider acharged particle, traveling in from along the x axis, encounters a rectangular potential energy barrier.

Consider the initial velocity (atx=).

Consider the following boundary conditions:

(1) x Continuous atx=0 and.x=L

(2) νContinuous at x=0and.x=L

(3) Δa=±U0mtν (Plus at x=0, minus at x=L.

02

Determine the formula of radiation reaction subject to the force,3rd  ,  2nd and 1stregion of the general solution a(t) ,  υ(t) and x(t) .

Write the formula ofradiation reaction subject to the force.

a=τa˙+Fm …… (1)

Here, a˙is radiation of reaction, Fis force and mis mass of the particle.

Write the formula ofregion of the general solution of.

a(t)=Aet/τ…… (2)

Here, A is runway we pick.

Write the formula ofregion of the general solution of ν(t).

. ν(t)=Atet/τ …… (3)

Here, A is runway we pick, t is time.

Write the formula ofregion of the general solution of x(t).

x(t)=At2et/τ …… (4)

Here, A is runway we pick, t is time.

03

Step 3:(a) Determine the radiation reaction subject to the force.

The third of these follows from integrating the equation of motion:

Determine theradiation reaction subject to the force.

Substitute U0[δ(x)+δ(xL)] for F into equation (1).

dvdtdt=tdadtdt+U0m[δ(x)+δ(xL)dt]Δν=tΔa+U0m[δ(x)+δ(xL)]dtdxdx=0Δa=U0m1ν[δ(x)+δ(xL)]dxΔa=±U0mtν

Therefore, the value of radiation reaction subject to the force is Δa=±U0mtν.

04

(b) Determine the value of  3th region of the general solution.

In each of the three regions the force is zero (it acts only at x=0andx=l).

For.(x>L)

Determine the3thregion the general solution is.a(t)

Substitute 0 for A3into equation (2).

a(t)=0

Determine the3thregion the general solution is .

Substitute 0for A3 into equation (3).

ν(t)=B3

Determine the3thregion the general solution is .

Substitute 0 forA3 into equation (4).

x(t)=B3t+C3

Let the final velocity beνf(=B3), set the clock so that t=0 when the particle is at x=0, and let T be the time it takes to transverse the barrier.

So, x(T)=L=νfT+C3 and hence C3=LνfT

Thena(t)=0 ; ν(t)=νf,

x(t)=L+νf(tT)

Therefore, the value of 3th region the general solution isa(t)=0 , υ(t)=B3 and .x(t)=B3t+C3

05

(c) Determine the value of  2nd region of the general solution.

For (0<x<L)

Determine the 2ndregion the general solution is a(t).

Substitute U0mtνfeT/t for A2into equation (2).

a(t)=U0mtνfeT/τet/τ=U0mtνfe(tT)τ

Determine the2nd region the general solution isν(t).

Substitute U0mtνfeT/t for A2and νfU0mνf for B2 into equation (3).

ν(t)=νfU0mνf+U0mtνfeT/τ=νf+U0mνf[e(tT)τ1]

Determine the 2ndregion the general solution isx(t).

Substitute U0mtνfeT/t for A2 and LνfT+U0mνf(Tt)for C2into equation (4).

x(t)=L+νf(tT)+U0mνf[te(tT)τt+Tt]

Therefore, thevalue of 2nd region the general solution isa(t)=U0mtνfe(tT)t, ν(t)=νf+U0mνf[etTt1]and x(t)=L+νf(tT)+U0mvf[te(tT)tt+Tt]

Note:[The particle may reverse course before reaching L if the barrier is sufficiently wide (or high), but we're interested in the case when it actually tunnels through.]

In particular for t=0 (Whenx=0)

0=LνfT+U0mνf[teTτ+Tt]

Thus L=νfTU0mνf[teT/τ+Tt]

06

(d) Determine the value of  1st region of the general solution.

For (x<0)

Determine the1st region the general solution is a(t).

a(t)=A1et/τ

Determine the1st region the general solution is .ν(t)

ν(t)=A1tet/τ+B1

Determine the1st region the general solution is x(t).

x(t)A1t2et/τ+B1t+C1

Therefore, the

Let νi be the incident velocity (at t); then B1=νicondition (3) says

U0mtνfeT/tA=U0mtν0

Where, ν0is the speed of the particle as it passes x=0. From the solution in region (ii) it follows the ν0=νf+U0mνf(eT/t1). But we can also express it in terms of the solution in region (i).

ν0=A1t+νi

Therefore, the value of 1st region the general solution is a(t)=A1el/t, ν(t)=A1tel/t+B1and .x(t)=A1t2el/t+B1t+C1


νi=νf+U0mνf(eTt1)A1t=νf+U0mνf(eTt11)+U0mν0U0mνfeTt=νfU0mνf+U0mν0=νfU0mνf(1νfν0)=νfU0mνf{1νfνf+U0mνf[eT/t1]}

If 12mνf2=12U0, then

Determine the inductance.

L=νfTνf[teT/t+Tt]=νf[TteT/tT+t]=tνf(1eT/t)

Now incident voltage will be:

νi=νfνf[111+eTt1]=νf(11+eTt)=νfeTt

Putting these together since, Ltνf=1eTtthen eTt=1Ltνf

Since,eT/t=11(Ltνf)

Thus νi=νf1(Lνft)

In particular, for ,L=νft4solve as:

νi=νf114=43νf

So incident kinetic energy will be:

KEiKEf=12mvi212mvi2KEiKEf=(vivf)2KEiKEf=169KEi=169KEf

Solve further as

KEi=16912U0=89U0

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Assuming you exclude the runaway solution in Prob. 11.19, calculate

(a) The work done by the external force,

(b) The final kinetic energy (assume the initial kinetic energy was zero),

(c) The total energy radiated.

Check that energy is conserved in this process.

A radio tower rises to height h above flat horizontal ground. At the top is a magnetic dipole antenna, of radius b, with its axis vertical. FM station KRUD broadcasts from this antenna at (angular) frequency ω, with a total radiated power P (that’s averaged, of course, over a full cycle). Neighbors have complained about problems they attribute to excessive radiation from the tower—interference with their stereo systems, mechanical garage doors opening and closing mysteriously, and a variety of suspicious medical problems. But the city engineer who measured the radiation level at the base of the tower found it to be well below the accepted standard. You have been hired by the Neighborhood Association to assess the engineer’s report.

(a) In terms of the variables given (not all of which may be relevant), find the formula for the intensity of the radiation at ground level, a distance R from the base of the tower. You may assume that bc/ωh. [Note: We are interested only in the magnitude of the radiation, not in its direction—when measurements are taken, the detector will be aimed directly at the antenna.]

(b) How far from the base of the tower should the engineer have made the measurement? What is the formula for the intensity at this location?

(c) KRUD’s actual power output is 35 kilowatts, its frequency is 90 MHz, the antenna’s radius is 6 cm, and the height of the tower is 200 m. The city’s radio-emission limit is 200 microwatts/cm2. Is KRUD in compliance?

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.]

As you know, the magnetic north pole of the earth does not coincide with the geographic north pole—in fact, it’s off by about 11°. Relative to the fixed axis of rotation, therefore, the magnetic dipole moment of the earth is changing with time, and the earth must be giving off magnetic dipole radiation.

(a) Find the formula for the total power radiated, in terms of the following parameters:ψ (the angle between the geographic and magnetic north poles), M (the magnitude of the earth’s magnetic dipole moment), andω (the angular velocity of rotation of the earth). [Hint: refer to Prob. 11.4 or Prob. 11.11.]

(b) Using the fact that the earth’s magnetic field is about half a gauss at the equator, estimate the magnetic dipole moment Mof the earth.

(c) Find the power radiated. [Answer: 4×10-5W]

(d) Pulsars are thought to be rotating neutron stars, with a typical radius of 10 km, a rotational period of 10-3s, and a surface magnetic field of 108T. What sort of radiated power would you expect from such a star? [Answer: 2×1036W].

a)Find the radiation reaction force on a particle moving with arbitrary velocity in a straight line, by reconstructing the argument in Sect. 11.2.3 without assuming υ(tr)=0. [Answer: (μ0q2γ4/6πc)(a˙+3γ2a2υ/c2)]

(b) Show that this result is consistent (in the sense of Eq. 11.78) with the power radiated by such a particle (Eq. 11.75).

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free