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2D Infinite Well Quantum Wave Function Plotter

Last Updated on September 16, 2024 by Max

To derive the wave function for a particle in a 2D infinite potential well, we start by considering a quantum mechanical particle confined within a rectangular region of space with infinite potential walls.

This means that the particle is trapped in a box where it cannot escape, and its wave function must satisfy certain boundary conditions imposed by the walls of the well.

Dimensions of the Infinite Well

  • The potential well has a length L_x in the x -direction and a length L_y in the y -direction.
  • Inside the well (for 0 \leq x \leq L_x and 0 \leq y \leq L_y ), the potential V(x, y) = 0 .
  • Outside the well, the potential V(x, y) = \infty .

Schrödinger Equation:

The time-independent Schrödinger equation for a particle of mass m confined in a 2D infinite potential well is given by:

-\frac{\hbar^2}{2m} \left( \frac{\partial^2 \psi(x, y)}{\partial x^2} + \frac{\partial^2 \psi(x, y)}{\partial y^2} \right) = E \psi(x, y),

where \hbar is the reduced Planck’s constant, \psi(x, y) is the wave function of the particle, and E is the energy of the particle.

To solve the Schrödinger equation, we use the method of separation of variables. We assume the solution can be written as a product of two functions, one depending only on x and the other only on y :

\psi(x, y) = X(x) Y(y).

Substituting this into the Schrödinger equation gives:

-\frac{\hbar^2}{2m} \left( \frac{d^2 X(x)}{dx^2} Y(y) + X(x) \frac{d^2 Y(y)}{dy^2} \right) = E X(x) Y(y).

Dividing both sides by X(x) Y(y) , we obtain:

-\frac{\hbar^2}{2m} \left( \frac{1}{X(x)} \frac{d^2 X(x)}{dx^2} + \frac{1}{Y(y)} \frac{d^2 Y(y)}{dy^2} \right) = E.

Since the left side is a sum of two terms, one depending only on x and the other only on y , each term must be equal to a constant. Let’s denote these separation constants by E_x and E_y such that:

\frac{1}{X(x)} \frac{d^2 X(x)}{dx^2} = -\frac{2mE_x}{\hbar^2}, \quad \frac{1}{Y(y)} \frac{d^2 Y(y)}{dy^2} = -\frac{2mE_y}{\hbar^2}.

Thus, the total energy E of the system is:

E = E_x + E_y.

The differential equation for X(x) is:

\frac{d^2 X(x)}{dx^2} + \frac{2mE_x}{\hbar^2} X(x) = 0.

This is a standard form of the second-order differential equation whose solutions are sinusoidal functions:

X(x) = A \sin\left(k_x x\right) + B \cos\left(k_x x\right),

where k_x = \sqrt{\frac{2mE_x}{\hbar^2}} .

To satisfy the boundary conditions:

\psi(x, y) = 0 at x = 0 and x = L_x ,

We find:

  1. At x = 0 : X(0) = A \sin(0) + B \cos(0) = B = 0 \Rightarrow B = 0 .
  2. At x = L_x : X(L_x) = A \sin(k_x L_x) = 0 .

For a non-trivial solution, A \neq 0 , so:

k_x L_x = n_x \pi, \quad \text{where } n_x = 1, 2, 3, \ldots

Thus, k_x = \frac{n_x \pi}{L_x} , and the solution for X(x) becomes:

X(x) = A \sin\left( \frac{n_x \pi x}{L_x} \right).

Similarly, for the y -direction, the differential equation for Y(y) is:

\frac{d^2 Y(y)}{dy^2} + \frac{2mE_y}{\hbar^2} Y(y) = 0,

with solutions:

Y(y) = C \sin\left(k_y y\right) + D \cos\left(k_y y\right),

where k_y = \sqrt{\frac{2mE_y}{\hbar^2}} .

Applying the boundary conditions:

\psi(x, y) = 0 at y = 0 and y = L_y ,

We find:

  1. At y = 0 : Y(0) = C \sin(0) + D \cos(0) = D = 0 \Rightarrow D = 0 .
  2. At y = L_y : Y(L_y) = C \sin(k_y L_y) = 0 .

For a non-trivial solution, C \neq 0 , so:

k_y L_y = n_y \pi, \quad \text{where } n_y = 1, 2, 3, \ldots

Thus, k_y = \frac{n_y \pi}{L_y} , and the solution for Y(y) becomes:

Y(y) = C \sin\left( \frac{n_y \pi y}{L_y} \right).

The general solution for the wave function \psi(x, y) is the product of the solutions in the x - and y -directions:

\psi(x, y) = X(x) Y(y) = A C \sin\left( \frac{n_x \pi x}{L_x} \right) \sin\left( \frac{n_y \pi y}{L_y} \right).

The normalization condition requires that the total probability of finding the particle in the well is 1:

\int_0^{L_x} \int_0^{L_y} |\psi(x, y)|^2 \, dx \, dy = 1.

Substitute the wave function:

\int_0^{L_x} \int_0^{L_y} A^2 C^2 \sin^2\left( \frac{n_x \pi x}{L_x} \right) \sin^2\left( \frac{n_y \pi y}{L_y} \right) \, dx \, dy = 1.

Separate the integrals:

A^2 C^2 \left( \int_0^{L_x} \sin^2\left( \frac{n_x \pi x}{L_x} \right) \, dx \right) \left( \int_0^{L_y} \sin^2\left( \frac{n_y \pi y}{L_y} \right) \, dy \right) = 1.

Each integral evaluates to \frac{L_x}{2} and \frac{L_y}{2} respectively, so:

A^2 C^2 \left( \frac{L_x}{2} \right) \left( \frac{L_y}{2} \right) = 1.

Solving for A C :

A C = \frac{2}{\sqrt{L_x L_y}}.

Thus, the normalized wave function is:

\psi(x, y) = \frac{2}{\sqrt{L_x L_y}} \sin\left( \frac{n_x \pi x}{L_x} \right) \sin\left( \frac{n_y \pi y}{L_y} \right).

The energy levels of the particle in the 2D infinite well are given by:

E_{n_x, n_y} = \frac{\hbar^2 \pi^2}{2m} \left( \frac{n_x^2}{L_x^2} + \frac{n_y^2}{L_y^2} \right), \quad \text{where } n_x, n_y = 1, 2, 3, \ldots

The wave function \psi(x, y) describes the quantum state of a particle confined in a 2D infinite potential well, and the energy levels are quantized based on the quantum numbers n_x and n_y . The derived wave function shows the sinusoidal nature of the probability amplitude, with nodes determined by the quantum numbers, reflecting the particle’s confinement within the well.

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