-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.

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Most popular questions from this chapter

A particle of mass m and kinetic energy E > 0 approaches an abrupt potential drop V0 (Figure 2.19).

(a)What is the probability that it will “reflect” back, if E = V0/3? Hint: This is just like problem 2.34, except that the step now goes down, instead of up.

(b) I drew the figure so as to make you think of a car approaching a cliff, but obviously the probability of “bouncing back” from the edge of a cliff is far smaller than what you got in (a)—unless you’re Bugs Bunny. Explain why this potential does not correctly represent a cliff. Hint: In Figure 2.20 the potential energy of the car drops discontinuously to −V0, as it passes x = 0; would this be true for a falling car?

(c) When a free neutron enters a nucleus, it experiences a sudden drop in potential energy, from V = 0 outside to around −12 MeV (million electron volts) inside. Suppose a neutron, emitted with kinetic energy 4 MeV by a fission event, strikes such a nucleus. What is the probability it will be absorbed, thereby initiating another fission? Hint: You calculated the probability of reflection in part (a); use T = 1 − R to get the probability of transmission through the surface.

The scattering matrix. The theory of scattering generalizes in a pretty obvious way to arbitrary localized potentials to the left (Region I),V(x)=0soψ(x)=Aeikx+Be-ikx,wherek2mE

To the right (Region III),V(x)is again zero, soψ(x)=Feikx+Ge-ikxIn between (Region II), of course, I can't tell you what is until you specify the potential, but because the Schrödinger equation is a linear, second-order differential equation, the general solution has got to be of the form

ψwhere f(x)and g(x)are two linearly independent particular solutions. 48 There will be four boundary conditions (two joining Regions I and II, and two joining Regions II and III). Two of these can be used to eliminate C and D, and the other two can be "solved" for B and F in terms of \(A\) and G

B=S11A+S12G.F=S21A+S22G

The four coefficientsSijwhich depend on k (and hence on E), constitute a2×2matrix s called the scattering matrix (or S-matrix, for short). The S-matrix tells you the outgoing amplitudes (B and F) in terms of the incoming amplitudes (A and G):

(BF)=(S11S21S21S22)(AG)

In the typical case of scattering from the left, G=0so the reflection and transmission coefficients are

Rl=|B|2|A|2|G=0=|S11|2.TI=|F|2|A|2|G=0=|S2|2.

For scattering from the right, and

Rr=|F|2|G|2A=0=|S22|2.Tr=|B|2|G|2A=0=|S12|2.

(a) Construct the S-matrix for scattering from a delta-function well (Equation 2.114). (b) Construct the S-matrix for the finite square well (Equation 2.145). Hint: This requires no new work, if you carefully exploit the symmetry of the problem.

Analyze the odd bound state wave functions for the finite square well. Derive the transcendental equation for the allowed energies and solve it graphically. Examine the two limiting cases. Is there always an odd bound state?

If two (or more) distinct44solutions to the (time-independent) Schrödinger equation have the same energy E . These states are said to be degenerate. For example, the free particle states are doubly degenerate-one solution representing motion to the right. And the other motion to the left. But we have never encountered normalizable degenerate solutions, and this is no accident. Prove the following theorem: In one dimension45 there are no degenerate bound states. Hint: Suppose there are two solutions, ψ1and ψ2with the same energy E. Multiply the Schrödinger equation for ψ1by ψ2and the Schrödinger equation for ψ2by ψ1and subtract, to show that ψ2dψ1/dx-ψ2dψ1/dxis a constant. Use the fact that for normalizable solutions ψ0at±to demonstrate that this constant is in fact zero.Conclude that ψ2s a multiple of ψ1and hence that the two solutions are not distinct.

Show that E must be exceed the minimum value of V(x) ,for every normalizable solution to the time independent Schrodinger equation what is classical analog to this statement?

d2Ψdx2=2mh2[V(x)E]Ψ;

IfE<Vmin thenΨ and its second derivative always have the same sign. Is it normalized?

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