The particle has E=0.

(a) Show that the potential energy for x>0is given by

U(x)=-2am1x+2a22m

(b) What is the potential energy for x<0?

Short Answer

Expert verified

(a) The potential energy for x>0 isU(x)=-2amx+2a22m .

(b) The potential energy is zero for x<0.

Step by step solution

01

Step 1:Understandingthe time independent Schrodinger equation.

The time independent Schrodinger equation relates the energy of the particle, Eto the potential energy, U, the mass of the particle, m, the position of the particle, X, and the wave function, ψ

-2mddxψ(x)+U(x)=(x)

If the energy of the particles is 0 , then the potential energy can be is isolated by adding the first term to the other side and divided by the wave function.

02

Part (a)Step 2: Applying Schrodinger equation.

The wave function of the particle isψx .

ψ(x)={2a3xe-axx>00x<0

The time-independent Schrodinger equation relates the energy of the particle, E to the potential energy, U, the mass of the particle, m, the position of the particle, X, and the wave function,ψ

-2mddxψ(x)+U(x)=(x)

If the energy of the particles is 0 , then the potential energy can be isolated by adding the first term to the other side and divided by the wave function.

U(x)=1ψ(x)22md2dx2ψ(x)=eax2a3x22md2dx2(2a3xe-ax)=2eax4mxa32a3[-2ae-ax+xa2e-ax]=-2amx+2a22m

Therefore, the potential energy for X > 0 is U(x)=-2amx+2a22m.

03

Part (b)Step 3: Applying Schrodinger equation.

The wave function of the particle is ψ(x).

ψ(x)={2a3xe-axx>00x<0

Calculation:

The time-independent Schrodinger equation relates the energy of the particle, E to the potential energy, U, the mass of the particle, m, the position of the particle, X, and the wave function, ψ

-2mddxψ(x)+U(x)=(x)

If the energy of the particles is 0 , then the potential energy can be is isolated by adding the first term to the other side and divided by the wave function.

U(x)=1ψ(x)22md2dx2ψ(x)

For

x<0,ψ(x)=0U(x)=0

Thus, the potential energy is zero for X<0.

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Most popular questions from this chapter

An electron in the n=4 state of a 5 nm wide infinite well makes a transition to the ground state, giving off energy in the form of photon. What is the photon’s wavelength?

Consider a particle bound in a infinite well, where the potential inside is not constant but a linearly varying function. Suppose the particle is in a fairly high energy state, so that its wave function stretches across the entire well; that is isn’t caught in the “low spot”. Decide how ,if at all, its wavelength should vary. Then sketch a plausible wave function.

Consider the wave function that is a combination of two different infinite well stationary states the nth and the mth

ψx,t=12ψnxe-iEn/t+12ψme-iEm/t

  1. Show that the ψx,tis properly normalized.
  2. Show that the expectation value of the energy is the average of the two energies:E¯=12En+Em
  3. Show that the expectation value of the square of the energy is given by .
  4. Determine the uncertainty in the energy.

It is possible to take the finite well wave functions further than (21) without approximation, eliminating all but one normalization constant C . First, use the continuity/smoothness conditions to eliminate A, B , andG in favor of Cin (21). Then make the change of variables z=x-L/2 and use the trigonometric relations

sin(a+b)=sinacosb+cosasinband

cos(a+b)=cosacosb-sinasinbon the

functions in region I, -L/2<z<L/2. The change of variables shifts the problem so that it is symmetric about z=0, which requires that the probability density be symmetric and thus that ψ(z)be either an odd or even function of z. By comparing the region II and region III functions, argue that this in turn demands that (α/k)sinkL+coskL must be either +1 (even) or -1 (odd). Next, show that these conditions can be expressed, respectively, as αk=tankL2 and αk=-cotkL2. Finally, plug these separately back into the region I solutions and show that

ψ(z)=C×{eα(z+L/2)          z<L/2coskzcoskL2          -L/2<z<L/2e-α(z-L/2)          z>L/2


or

ψ(z)=C×{eα(z+L/2)          z<L/2-sinkzsinkL2          -L/2<z<L/2e-α(z-L/2)          z>L/2

Note that Cis now a standard multiplicative normalization constant. Setting the integral of |ψ(z)|2 over all space to 1 would give it in terms of kand α , but because we can’t solve (22) exactly for k(or E), neither can we obtain an exact value for C.

For the harmonic oscillator potential energy, U=12kx2, the ground-state wave function is ψ(x)=Ae-(mk/2)x2, and its energy is 12k/m.

(a) Find the classical turning points for a particle with this energy.

(b) The Schrödinger equation says that ψ(x) and its second derivative should be of the opposite sign when E > Uand of the same sign when E < U . These two regions are divided by the classical turning points. Verify the relationship between ψ(x)and its second derivative for the ground-state oscillator wave function.

(Hint:Look for the inflection points.)

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