← Quantum Mechanics

Applications of the Schrödinger Equation

Sunday, February 27, 2022

Constant Potential Energy

If the potential energy is constant, the Schrödinger equation becomes:

22md2ψdx2+U0ψ(x)=Eψ(x)-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2}+U_0\psi\left(x\right)=E\psi\left(x\right)

Assuming E>U0E\gt U_0

Then using the fact that

d2ψdx2=k2ψ(x)\frac{d^2\psi}{dx^2}=-k^2\psi\left(x\right)

from the equation for the wave function, ψ\psi, the wave number, kk, can be represented as

k=2m(EU0)2k=\sqrt{\frac{2m\left(E-U_0\right)}{\hbar^2}}

The solution to this equation gives a form where the second derivative is equal to itself multiplied by a negative constant, meaning it can be represented in the form

ψ(x)=Asinkx+Bcoskx\psi\left(x\right)=A\sin{kx}+B\cos{kx}

If E<U0E\lt U_0 (forbidden region)

Rewriting the solution for the case where E<U0E\lt U_0, we get

d2ψdx2=k2ψ(x)\frac{d^2\psi}{dx^2}=k'^2\psi\left(x\right)

where

k=2m(U0E)2k'=\sqrt{\frac{2m\left(U_0-E\right)}{\hbar^2}}

In this case, the solution can generally be written as

ψ(x)=Aekx+Bekx\psi\left(x\right)=Ae^{k'x}+Be^{-k'x}

The Free Particle

For any free particle, the force it experiences is 0. This means the potential energy is constant (we say U0=0U_0=0), so the energy of the particle is

E=2k22mE=\frac{\hbar^2k^2}{2m}

using the form ψ(x)=Asinkx+Bcoskx\psi\left(x\right)=A\sin{kx}+B\cos{kx}. Notice how kk can have any value, meaning the energy is not quantized.

Normalization integral

Since this cannot be integrated from -\infty to ++\infty, we cannot normalize the wave function in this form. Instead, we use the complex exponentials:

ψ(x)=A(eikxeikx2i)+B(eikx+eikx2)=Aeikx+Beikx\psi\left(x\right)=A\left(\frac{e^{ikx}-e^{-ikx}}{2i}\right)+B\left(\frac{e^{ikx}+e^{-ikx}}{2}\right)=A'e^{ikx}+B'e^{-ikx}

where

A=A/2i+B/2B=A/2i+B/2A'=A/2i+B/2\newline B'=-A/2i+B/2

The interpretation of this solution relies on the time-dependent version of the Schrödinger equation:

Ψ(x,t)=(Aeikx+Beikx)eiωt=Aei(kxωt)+Bei(kx+ωt)\Psi\left(x,t\right)=\left(A'e^{ikx}+B'e^{-ikx}\right)e^{-i\omega t}=A'e^{i\left(kx-\omega t\right)}+B'e^{-i\left(kx+\omega t\right)}

The first term represents a wave moving to the right with amplitude AA', whereas the second term represents a wave moving to the left with amplitude BB'.

Beam of particles

To represent a beam of particles moving in the +x+x direction, set B=0B'=0. Then, the probability density function becomes

P(x)=ψ(x)2=A2eikxeikx=A2P\left(x\right)=\left|\psi\left(x\right)\right|^2=\left|A'\right|^2e^{ikx}e^{-ikx}=\left|A'\right|^2

which makes sense because the particles are equally likely to be found anywhere along the xx axis, giving a completely unlocalized wave.

Infinite Potential Energy Well

Setup

The particle is trapped in a region of width LL between two infinitely high walls of infinite potential energy. It makes perfectly elastic collisions with either side, so its energy is completely confined to the region. It is said that

U(x)={00xLx<0,x>LU\left(x\right)=\begin{cases} 0 && 0\leq x\leq L \newline \infty && x\lt 0,x\gt L \end{cases}

Outside the region

To find the solution outside the region, it is quite clear that ψ\psi must be 0 so that UψU\psi is not infinite (since U=U=\infty). Additionally, if the particle is always contained in the region, the probability of finding it outside the region must be 00.

ψ(x)=0        x<0,x>L\psi\left(x\right)=0~~~~~~~~x\lt 0, x\gt L

Inside the region

Knowing U(x)=0U\left(x\right)=0 inside the region, the solution becomes

ψ(x)=Asinkx+Bcoskx        0xL\psi\left(x\right)=A\sin{kx}+B\cos{kx}~~~~~~~~0\leq x\leq L

where

k=2mE2k=\sqrt{\frac{2mE}{\hbar^2}}

To ensure the equation for the wave is continuous at the boundaries where x=0x=0 and x=Lx=L, we set the following restrictions:

ψ(0)=Asin0+Bcos0=0ψ(L)=AsinkL+BcoskL=0\psi\left(0\right)=A\sin{0}+B\cos{0}=0\newline \psi\left(L\right)=A\sin{kL}+B\cos{kL}=0

The first of these equations gives B=0B=0, leaving AsinkL=0A\sin{kL}=0. Either A=0A=0 (which would mean the wave is 0 everywhere) or sinkL=0\sin{kL}=0, which is only true when

kL=nπ        n=1,2,3,...kL=n\pi~~~~~~~~n=1,2,3,...

Solving for the wavelength, we find that λ=2L/n\lambda=2L/n.

The solution to the Schrödinger equation for a particle trapped in a linear region is a series of standing de Broglie waves

And since only certain wavelengths are permitted, we also can see that

En=2k22m=2π2n22mL2=h2n28mL2        n=1,2,3,...E_n=\frac{\hbar^2k^2}{2m}=\frac{\hbar^2\pi^2n^2}{2mL^2}=\frac{h^2n^2}{8mL^2}~~~~~~~~n=1,2,3,...

The energy is quantized as well

Allowed energies

Setting E0=h2/8mL2E_0=h^2/8mL^2, we find that En=n2E0E_n=n^2E_0. Therefore, only square integer multiples of E0E_0 are allowed. E0E_0, when n=1n=1, is called the ground state, and all other values of nn are called the excited states.

By absorbing or releasing energy equal to the difference in energy states, the particle can transition between one excited state and another.

Normalization

The final step in the solution for ψ(x)\psi\left(x\right) is to determine the value of AA that normalizes the function:

0LA2sin2nπxL dx=1\int_0^LA^2\sin^2{\frac{n\pi x}{L}}~dx=1

Solving this makes A=2/LA=\sqrt{2/L}, so

ψn(x)=2LsinnπxL        n=1,2,3,...\psi_n\left(x\right)=\sqrt{\frac{2}{L}}\sin{\frac{n\pi x}{L}}~~~~~~~~n=1,2,3,...

Between two points, the wave function and probability distributions look something like this for the first few values of nn:

Probabilities of finding a particle in an infinite energy potential well

This is very strange behavior since it means a particle can go between two locations in space without going in the spaces in between them.

Motion of the particle

For this trapped particle, the uncertainty in position would be Δx=L1/121/2π2n2\Delta x=L\sqrt{1/12-1/2\pi^2 n^2} and the uncertainty in momentum would be Δp=hn/2L\Delta p=hn/2L. Therefore, the product of these two uncertainties is

ΔxΔp=hn211212π2n2=h2n21212π2\Delta x\Delta p=\frac{hn}{2}\sqrt{\frac{1}{12}-\frac{1}{2\pi^2 n^2}}=\frac{h}{2}\sqrt{\frac{n^2}{12}-\frac{1}{2\pi^2}}

This means the product of the uncertainties grows as nn increases. The minimum value occurs when n=1n=1:

ΔxΔp=0.090h=0.57\Delta x\Delta p=0.090h=0.57\hbar

Finite Potential Energy Well

A finite potential energy well can be defined as such:

U(x)={00xLU0x<0,x>LU\left(x\right)=\begin{cases} 0 && 0\leq x\leq L \newline U_0 && x\lt 0,x\gt L \end{cases}

Inside the region

Inside the region is the same as it was for an infinite energy potential well:

ψ(x)=Asinkx+Bcoskx\psi\left(x\right)=A\sin{kx}+B\cos{kx}

although the values for AA and BB are not valid in this calculation.

For the region x<0x \lt 0

In this case, the energy of the particle is less than its potential energy, so we must use the form ψ(x)=Cekx+Dekx\psi\left(x\right)=Ce^{k'x}+De^{-k'x}. However, since the region includes x=x=-\infty, the second term would become infinite. Therefore, D=0D=0 and the equation becomes

ψ(x)=Cekx\psi\left(x\right)=Ce^{k'x}

For the region x>Lx \gt L

In this region, we must again use the form ψ(x)=Fekx+Gekx\psi\left(x\right)=Fe^{k'x}+Ge^{-k'x}. However, since this region includes x=+x=+\infty, F=0F=0. Therefore,

ψ(x)=Gekx\psi\left(x\right)=Ge^{-k'x}

Solving

We now have five unknowns: coefficients AA, BB, CC, GG, and the energy, EE. Additionally, we have four equations from the boundary conditions (continuity for ψ\psi and now dψ/dxd\psi/dx at both x=0x=0 and x=Lx=L) and one equation from the normalization condition.

The energy values must be determined numerically given the situation since the resulting equation results in a transcendental equation that cannot be solved algebraically.

These equations can be solved with specific numbers, given a problem. The key quality of any solution however is that at the boundary conditions, the wave function satisfies both the continuity of the function itself and the continuity of the first derivative of the function, such as the examples shown below:

Finite potential energy well probabilities

In these graphs, the penetration property is also clearly seen, as the sinusoidal functions transition into exponential ones at the boundaries. Note that for higher energy levels, the wave penetrates further into the forbidden region.

Two-Dimensional Infinite Potential Energy Well

Extending the Schrödinger equation to two dimensions, we get:

22m(2ψ(x,y)x2+2ψ(x,y)y2)+U(x,y)ψ(x,y)=Eψ(x,y)-\frac{\hbar^2}{2m}\left(\frac{\partial^2\psi\left(x,y\right)}{\partial x^2}+\frac{\partial^2\psi\left(x,y\right)}{\partial y^2}\right)+U\left(x,y\right)\psi\left(x,y\right)=E\psi\left(x,y\right)

And the two-dimensional version of the infinite potential energy well is defined as follows:

U(x,y)={00xL;0yLotherwiseU\left(x,y\right)=\begin{cases} 0 && 0\leq x\leq L;0\leq y\leq L \newline \infty && \text{otherwise}\end{cases}

This represents a particle confined in an L×LL \times L square, where the corners are (0,0)\left(0,0\right), (0,L)\left(0,L\right), (L,0)\left(L,0\right), and (L,L)\left(L,L\right). Collisions with the lines x=0x=0, x=Lx=L, y=0y=0, and y=Ly=L are perfectly elastic.

Just like the previous one-dimensional wells, we assume the function is 0 in the forbidden regions. But now, we also assume the wave function is separable in the well. That is,

ψ(x,y)=f(x)g(y)\psi\left(x,y\right)=f\left(x\right)g\left(y\right)

where

f(x)=Asinkxx+Bcoskxxg(y)=Csinkyy+Dcoskyyf\left(x\right)=A\sin{k_xx}+B\cos{k_xx}\newline g\left(y\right)=C\sin{k_yy}+D\cos{k_yy}

Applying the boundary conditions, we see that

ψ(0,y)=0    and    ψ(L,y)=0    for all yψ(x,0)=0    and    ψ(x,L)=0    for all x\psi\left(0,y\right)=0~~~~\text{and}~~~~\psi\left(L,y\right)=0~~~~\text{for all}~y\newline \psi\left(x,0\right)=0~~~~\text{and}~~~~\psi\left(x,L\right)=0~~~~\text{for all}~x

Using these conditions, we see that B=D=0B=D=0, just like the one-dimensional case. We also see that since sinkxL=0\sin{k_xL}=0 and sinkyL=0\sin{k_yL}=0, kxLk_xL and kyLk_yL must be integer multiples of π\pi (but not necessarily the same multiple).

Putting it all together, we see that

ψ(x,y)=AsinnxπxLsinnyπyL\psi\left(x,y\right)=A'\sin{\frac{n_x\pi x}{L}}\sin{\frac{n_y\pi y}{L}}

We can find coefficient AA' using the normalization of the function:

ψ2 dx dy=1\int\int\psi^2~dx~dy=1

Or for this situation,

0Ldy0LA2sin2nxπxLsin2nyπyLdx=1\int_0^Ldy\int_0^LA'^2\sin^2{\frac{n_x\pi x}{L}}\sin^2{\frac{n_y\pi y}{L}}dx=1

Solving this equation gives us that

A=2LA'=\frac{2}{L}

Energy

Plugging this solution into the energy equation, we find that the allowed energies for values of nxn_x and nyn_y are

E=2π22mL2(nx2+ny2)=h28mL2(nx2+ny2)E=\frac{\hbar^2\pi^2}{2mL^2}\left(n_x^2+n_y^2\right)=\frac{h^2}{8mL^2}\left(n_x^2+n_y^2\right)

The ground state for this situation occurs when nx=ny=1n_x=n_y=1:

E0=2π22mL2=h28mL2E_0=\frac{\hbar^2\pi^2}{2mL^2}=\frac{h^2}{8mL^2}

Therefore,

E=E0(nx2+ny2)E=E_0\left(n_x^2+n_y^2\right)

nxn_x and nyn_y are called quantum numbers, and different combinations of each of them produce different probability density distributions. Just like the one dimensional case, where the value of ψ2\psi^2 is highest, we expect to find the particle and where it is 0, we do not expect to find the particle. See the examples below:

2-dimensional infinite potential energy well probabilities

Experimental accuracy

This exact probability distribution can be observed using an electron microscope. Below is a picture of a ring of iron atoms, whose probabilities are shown as peaks:

A ring of iron atoms

Degeneracy

It is possible for multiple pairs of quantum numbers to result in the same energy level. This situation is known as degeneracy and the energy levels are called degenerate.

For example, the energy state E=13E0E=13E_0 can be obtained with nx=3n_x=3 and ny=2n_y=2 or nx=2n_x=2 and ny=3n_y=3. This is not as dramatic as, say, E=50E0E=50E_0 being obtained by nx=1n_x=1 and ny=7n_y=7 versus nx=5n_x=5 and ny=5n_y=5. 13E013E_0 is said to have two-fold degeneracy, whereas 50E050E_0 has three-fold degeneracy (it can also be represented by nx=7n_x=7 and ny=1n_y=1).