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.

Short Answer

Expert verified

1. R=19

2. The potential energy drops discontinuously from to at , but comparing this to a car that drops off a cliff, its potential energy drops continuously from to linearly. i.e. , where x is the vertical

height.

3.T=89

Step by step solution

01

Forming ordinary differential equation as the time-independent Schrödinger equation

Schrodinger equation is given by,

hψt=-ih2m2ψx2+V(x,t)ψ(x,t)-<x<,t>0

Where, the drop in potential energy is,

V(x,t)=V(x)=0,x0-V0,x>0

Assuming,

ψ(x,t)=ψ(x)ϕ(t)

We get two separate equations as:

hϕ'(t)ϕ(t)=E-h22mψ''(x)ψ(x)+v(x)=E

Therefore the Schrodinger equation will be :

d2ψdx2=2mh2V(x)-Eψ

02

Splitting up the time-independent Schrodinger equation for the intervals of V(x)

d2ψdx2=2mh2(-E)ψ,forx0d2ψdx2=2mh2(-V0-E)ψ,forx>0For,E=V03d2ψdx2=2mV03h2(-E)ψ,forx0d2ψdx2=8mV03h2ψ,forx>0

Hence, the general solution would be:

ψ(x)=Aexpi2mV03h3x+Bexp-i2mV03h3x,x0Cexpi8mV03h3x+Dexp-i8mV03h3x,x>0

Solving the ordinary differential equation in t, we get ϕ(t)=e-iEt/h, Hence ψ(x,t)=ψ(x)ϕ(t)is a linear combination of waves traveling to the left and right.

Here, we assume the wave to only be incident from the left, which yields D = 0.

Hence,

ψ(x)=Aeikx+Be-ikxx0Ce2ikxx>0

Where,k=2mV03h2

03

Defining the reflection coefficient a)

The reflection coefficient is defined as the magnitude of the ratio of the reflected probability current to the incident probability current.

Where the probability current is,

J(x,t)=ih2mψψ*x-ψ*ψxJ(x,t)=ih2m[ψ(x)e-Et/h]x[ψ*(x)eiEt/h]-[ψ*(x)eiEt/h]x[ψ(x)e-iEt/h]J(x,t)=ih2m[ψ(x)e-Et/h]dψ*xeiEt/h-[ψ*(x)eiEt/h]dψdxe-iEt/hJ(x,t)=ih2mψdψ*dx-ψ*dψdx

Hence, the reflection coefficient,

localid="1658228499814" R=i2m(Be-ikx)ddx(B*eikx)-(B*eikx)ddx(Be-ikx)i2m(Aeikx)ddx(A*e-ikx)-(A*e-ikx)ddx(Aeikx)R=(Be-ikx)(B*eikx)-(B*eikx)(Be-ikx)(Aeikx)(A*e-ikx)-(A*e-ikx)(Aeikx)R=2ikBB*-2ikAA*R=B2A2

04

Calculating the reflection coefficient

To determine one of the constants, the wave function needs to x = 0 be continuous at

i.e.

limx0-ψ(x)=limx0+ψ(x)

A + B = C

Let μbe a very small number, and integrate the time-independent Schrodinger equation with respect to x from-μtoμ

-μμd2ψdx2dx=-μμ2mh2V(x)-Eψ(x)dxdψdx-μμ=-μ02mh2(-E)ψ(x)dx+0μ2mh2(-V0-E)ψ(x)dxdψdx-μμ=2mh2(-E)ψ(0)-μ0dx+2mh2(-V0-E)ψ(0)0μdxdψdx-μμ=2mh2(-E)ψ(0)μ+2mh2(-V0-E)ψ(0)μ

Taking the limit asμ0

dψdx0-0+=0

Hence, ψxis continuous at x = 0

So,

limx0-dψdx=limx0+dψdxik(A-B)=2ikCik(A-B)=2ik(A+B)B=-13A

Therefore, the reflection coefficient, and hence, the probability that the mass will turn back at x = 0 is,

R=BABA*R=-13-13*R=-13-13R=19

Thus, 1/9 is the probability that it will “reflect” back.

05

Explanation of part (b)

Here, the potential energy (V(x)) drops discontinuously from 0 to -V0at x = 0, but comparing this to a car that drops off a cliff, its potential energy drops continuously from 0 to -V0linearly.

i.e. Vcar(x)=-mgx, where x is the vertical height.

06

Defining the transmission coefficient c)

Since a neutron has energy E=4MeV, which is equal to a third of V0=12MeV, so, the previous analysis holds true.

The transmission coefficient is defined by the magnitude of the ratio of the transmitted probability current to the incident probability current.

j(x,t)=ih2mψdψdx*-ψ*dψdx

For,

ψ(x)=Aeikx+Be-ikx,x0Ce2ikx,x>0

Hence, the transmission coefficient,

T=ih2m(Ce-ikx)ddx(C*e-2ikx)-(C*e-2ikx)ddx(Ce2ikx)ih2m(Aeikx)ddx(A*e-ikx)-(A*e-ikx)ddx(Aeikx)T=(Ce2ikx)(-2ikC*e-2ikx)-(C*e-2ikx)(2ikCe2ikx)(Aeikx)(-ikA*e-ikx)-(A*e-ikx)(ikAeikx)T=-4ikCC*-2ikAA*T=2C2A2

At : x = 0

role="math" localid="1658229056899" limx0-ψ(x)=limx0+ψ(x)A+B=C

And

limx0-dψdx=limx0+dψdxik(A-B)=2ikC

Adding both the equations,

2A=3CC=23A

Therefore, the transmission coefficient, i.e., the probability that the neutron will enter the nucleus is,

T=2CACA*T=22323T=89

Thus, the transmission coefficient, i.e., the probability that the neutron will enter the nucleus is 8/9. Hence, R + T = 1

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