-consider the “step” potential:

v(x)={0,ifx0,V0,ifx>0,

a.Calculate the reflection coefficient, for the case E < V0, and comment on the answer.

b. Calculate the reflection coefficient, for the case E >V0.

c. For potential such as this, which does not go back to zero to the right of the barrier, the transmission coefficient is not simply F2A2(with A the incident amplitude and F the transmitted amplitude), because the transmitted wave travels at a different speed . Show thatT=E-V0V0F2A2,for E >V0. What is T for E < V0?

d. For E > V0, calculate the transmission coefficient for the step potential, and check that T + R = 1.


Short Answer

Expert verified

a) The reflection coefficient is 1 when E < V0.

b) The reflection coefficient is R=(E-E-V0)4V02when E > V0.

c) The transmission coefficient is T=F2-V0+EA2Ewhen E > V0and zero when E< V0.

d) Th transmission coefficient calculated as T=4E-V0+E+E-(-V0+E)2V02and R + T = 1.

Step by step solution

01

Define the Schrödinger equation

A differential equation describes matter in quantum mechanics in terms of the wave-like properties of particles in a field. Its answer relates to a particle's probability density in space and time.

02

a) Reflection coefficient when E < V0

Step potential is given as:

V(x)=0ifx0V(x)=V0ifx>0

The Schrodinger equation can be calculated as:

-h22md2Ψdx2+V(x)Ψ=EΨ

For x0

role="math" localid="1658127639629" -h22md2Ψ2dx2=EΨ1

For

-h22md2Ψ2dx2+V0Ψ2=EΨ2

Let,

k=2mEh2andα=2m(V0-E)h2

For x0

role="math" localid="1658127959257" d2Ψdx2+k2Ψ1=0

For x>0

d2Ψ2dx2-α2Ψ2=0

For x0

Ψ1(x)=Aeikx+Be-ikx

For x>0

Ψ2(x)=Feax+Ge-ax

In the above equations, F will be zero for E < V0 ( x+) the wave function will not be,then only wave function will be continuous across the boundry. Thus, the solution will be:

role="math" localid="1658128607114" Ψ1(x)=Aeikx+Be-ikx(1)Ψ2(x)=Ge-αx(2)

Apply boundary conditions as:

Wave function and the derivative will be continous at x = 0, then:

Ψ1(0)=Ψ2(0) (3)

dΨ1dxx=0=dΨ2dxx=0 (4)

Using the equations above, we get,

A+B=Gik(A-B)=-αG

Solving the above equations and we get,

B=k-iαk+iαAG=2kk+iαA

Substituting the values in equations 1 and 2, we get,

Ψ1(x)=Aeikx+Ak-iαk+iαe-ikxΨ2(x)=A2kk+iαe-ikx

The reflection coefficient can be calculated as:

R=BA2

Substituting the values, and we get,

R=k-iαk-iα2=k2+α2k2+α22=1

Thus, the reflection coefficient is 1 when E< V0.

03

b) Reflection coefficient when E > V0

The Schrodinger equation can be calculated as:

-h22md2Ψdx2+V(x)Ψ=EΨ

For x0

-h22md2Ψ1dx2=EΨ1

For x>0

h22md2Ψ1dx2+V0Ψ2=EΨ2-

We know:

k=2mEh2,andβ=2m(-V0+E)h2

For x0

d2Ψ1dx2+k2Ψ1=0

For x>0

d2Ψ2dx2+β2Ψ2=0

For x0

localid="1658132108137" Ψ1(x)=Aeikx+Be-ikx

For x>0

localid="1658132126293" Ψ2(x)=Feiβx+Ge-iβx

In the above equations, G will be zero for E > V0 ( x),then only wave function will be continuous across the boundry. Thus, the solution will be:

localid="1658132145945" Ψ1(x)=Aeikx+Be-ikxΨ2(x)=Feiβx

Apply boundary conditions as:

Wave function and the derivative will be continous at x = 0, then:

Ψ10=Ψ20(7)dΨ1dxx=0=dΨ2dxx=0(8)

Ψ1(0)=Ψ2(0)dΨ

Using the equations above, we get,

A+B=Fik(A-B)=iβF(13)

Solving the above equations and we get,

-B1+kβ=A1-kβ(14)

The reflection coefficient can be calculated as:

R=BA2

Substituting the values, and we get,

R=1-(k/β)1+(k/β)2=β-kβ+k2β-kβ-k2=(β-k)4(β2+k2)(9)

We know:

k=2mEh2,andβ=2m(-V0+E)h2

k2=2mEh2β2=2m(-V+E)h2β2-k2=2m(-V+E)h2-2mEh2(β2-k2)2=2m(-V0)h22

And

β-k=2m(-V0+E)h2-2mEh2β-k=2mEh2(-V0+E-E)β-k4=2mh2(-V0+E-E)4

Substituting the values in equation 9, we get,

R=(E-E-V0)4V02

Thus, the reflection coefficient is R=(E-E-V0)4V02when E > V0.

04

c) Transmission coefficient  For E > V0

From the definition of the transmission coefficient:

T=probabilityoftransmittedparticletotherightofthebarriesprobabilityoffindingincidentparticleinthebox

Let's take the time interval dt here. The probability of finding the transmitted particle to the right of the barrier is Pt, and the probability of finding the incident particle in the box to the left of the barrier is Pi.

The above expression for transmission coefficient can be written as:

T=PtPi

From the definition of probabilities:

PtPi=F2vtA2vi (11)

Here viand vt are the speed of the incident particle and transmitted particle, respectively.

From the definition of velocity:

v=hk2m

Thus the velocities can be calculated as:

vt=hβ2mvi=hk2m

Substitute the values in equation 11, and we get,

role="math" localid="1658204796438" PtPi=F2hβ2mA2hk2m (12)

Substitute values, and we get,

PtPi=F22m(-V0+E)hh2mA22mEh2h2mPtPi=F2(-V0+E)A2E

Thus, the transmission coefficient will be:

role="math" localid="1658205459586" T=F2(-V0+E)A2E

For E < V0

F = 0 thus,

T = 0

Thus, the transmission coefficient is T=F2(-V0+E)A2Ewhen E > V0and zero when

E < V0.

05

d) Transmission coefficient for step potential E > V0

From equation 12, the transmission coefficient can be calculated as:

T=PtPi=F2hβ2mA2hk2m

Solving the equation further:

T=PtPi=F2βA2k

From equations 13 and 14:

-B1+kβ=A1-kβA+B=F

Substituting the value of B in the above expression, we get,

A-A1-kβ1+kβ=FF=A1-1-kβ1+kβFA=1+kβ-1+kβ1+kβFA=2kββ+kβFA=2kβ+k

The transmission coefficient can be written as:

T=PtPi=2kβ+k2βkT=4kβ(β+k)2

The transmission coefficient can be written as:

T=PtPi=2kβ+k2βkT=4kββ+k2

Substituting values in the above expression, we get,

role="math" localid="1658209317653" T=2mEh242m(-V0+E)h22m(-V0+E)h2+2mEh22T=4E-V0+EE+(-V0+E)2×E(-V0+E)2E(-V0+E)2=4E-V0+E×E(-V0+E)2E+(-V0+E)2T=4E-V0+E×E--V0+E(V0)2

From subpart b, the reflection coefficient is:

R=β-k4β2-k22R+T=β-k4β2-k22+4kββ+k2=(β4+k4-4β3k+6β2k2-4βk3)(β2+k2+2kβ)+4kββ4+k4-2β2k2(β2+k2+2kβ)β4+k4-2β2k2=β2β4+k2β4+2kββ4+k4β2+k4k2+k42kβ-4β3kk2-4β3k2kβ+6β2k2β2+6β2k2k2+6β2k22kβ-4βk3k2-4βk3k2-4βk32kβ+4kββ4+4kβk4-4kβ2β2k2β2β4+β2k4-β22β2k2+k2k4-k22β2k2+2kββ2+2kβk4-2kβ2β2k2

Solving further as:

β6+k2β4+2kβ5+k4β2+k6+k52β-4β5k-4β3k3-8β4k2+6k2β4+6β2k4+12β3k3-4k3β3-4βk5-8β2k4+4kβ5R+T=+4βk5-8β3k3β6+β2k4-2β4k2+k2β4+k6-2β2k4+2kβ5+2βk54β3k3=β6+β2k4-2β4k2+k2β4+k6-2β2k4+2kβ5+2βk54β3k3β6+β2k4-2β4k2+k2β4+k6-2β2k4+2kβ5+2βk54β3k3R+T=1

Thus, the transmission coefficient is calculated as

T=4E-V0+E×4E(-V0+E)2(V0)2andR+T=1.

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

In this problem we explore some of the more useful theorems (stated without proof) involving Hermite polynomials.

a. The Rodrigues formula says thatHn(ξ)=(1)neξ2(d)neξ2

Use it to derive H3 and H4 .

b. The following recursion relation gives you Hn+1 in terms of the two preceding Hermite polynomials: Hn+1(ξ)=2ξHn(ξ)2nHn1(ξ)

Use it, together with your answer in (a), to obtain H5 and H6 .

(c) If you differentiate an nth-order polynomial, you get a polynomial of

Order (n-1). For the Hermite polynomials, in fact,

dHn=2nHn1(ξ)

Check this, by differentiatingH5and H6.

d. Hn(ξ)is the nth z-derivative, at z = 0, of the generating function exp(z2+2ξz)or, to put it another way, it is the coefficient ofznn! in the Taylor series expansion for this function: ez2+2ξz=n=0znn!Hn(ξ)

Use this to obtain H0,H1and H2.

Show that

Ψ(x,t)=(mωπh)1/4exp[-mω2hx2+a221+e-2iωt+ihtm-2axe-iωt]

satisfies the time-dependent Schrödinger equation for the harmonic oscillator potential (Equation 2.43). Here a is any real constant with the dimensions of length. 46

(b) Find|Ψ(x,t)|2 and describe the motion of the wave packet.

(c) Compute <x> and <p> and check that Ehrenfest's theorem (Equation 1.38) is satisfied.

Evaluate the following integrals:

(a)-3+1(x3-3x2+2x-1)δ(x+2)dx.

(b).0[cos(3x)+2]δ(x-π)dx

(c)_1+1exp(lxl+3)δ(x-2)dx

A particle in the infinite square well has as its initial wave function an even mixture of the first two stationary states:

Ψ(x,0)=A[ψ1(x)+ψ2(x)]

You can look up the series

116+136+156+=π6960

and

114+134+154+=π496

in math tables. under "Sums of Reciprocal Powers" or "Riemann Zeta Function."

(a) Normalize Ψ(x,0) . (That is, find A. This is very easy, if you exploit the orthonormality of ψ1and ψ2 Recall that, having ψnormalized at , t=0 , you can rest assured that is stays normalized—if you doubt this, check it explicitly after doing part(b).

(b) Find Ψ(x,t)and |Ψ(x,t)|2Express the latter as a sinusoidal function of time. To simplify the result, let ωπ22ma2

c)Compute x . Notice that it oscillates in time. What is the angular frequency of the oscillation? What is the amplitude of the oscillation?(If your amplitude is greater than a2 , go directly to jail.

(d) Compute p

(e) If you measured the energy of this particle, what values might you get, and what is the probability of getting each of them? Find the expectation value ofH.How does it compare with E1 and E2

Solve the time-independent Schrodinger equation with appropriate boundary conditions for the “centered” infinite square well: V(x)=0(for-a<x<+a), V(x)=α(otherwise). Check that your allowed energies are consistent with mine (Equation 2.30), and confirm that your ψ'scan be obtained from mine (Equation 2.31) by the substitution x → (x + a)/2 (and appropriate renormalization). Sketch your first three solutions, and compare Figure 2.2. Note that the width of the well is now 2a.

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