Stationary states of free particle

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SUMMARY

The discussion focuses on obtaining the stationary states of a free particle in three dimensions using the time-dependent Schrödinger equation. The wavefunction is expressed as a product of spatial and temporal components: \psi(\mathbf{r},t) = \psi_1(x) \psi_2(y) \psi_3(z) \phi(t). By substituting this into the Schrödinger equation and setting potential energy U to zero, the equation simplifies to \frac{-\hbar^2}{2m} \nabla^2 \psi(\mathbf{r},t) = i\hbar \frac{\partial \psi(\mathbf{r},t)}{\partial t}. The separation of variables leads to three individual one-dimensional Schrödinger equations, with the temporal component described by \phi(t) = A e^{-iE t / \hbar}, where E is the separation constant.

PREREQUISITES
  • Understanding of Schrödinger's equation
  • Familiarity with wavefunctions and their properties
  • Knowledge of separation of variables technique
  • Basic concepts of quantum mechanics, particularly free particle behavior
NEXT STEPS
  • Study the derivation of the time-independent Schrödinger equation
  • Learn about the implications of boundary conditions in quantum mechanics
  • Explore the concept of infinite square wells and their energy levels
  • Investigate the role of the separation constant E in quantum systems
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Students and professionals in quantum mechanics, physicists working on wave-particle duality, and anyone interested in the mathematical foundations of quantum theory.

Mindscrape
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The problem is to obtain the stationary states for a free particle in three dimensions by separating the variables in Schrödinger's equation.

So take

\psi(\mathbf{r},t) = \psi_1(x) \psi_2(y) \psi_3(z) \phi(t)

and substitute it into the time-dependent Schrödinger equation. For the stationary states set U=0 and obtain

\frac{-\hbar^2}{2m} \nabla^2 \psi(\mathbf{r},t) = i\hbar \frac{\partial \psi(\mathbf{r},t)}{\partial t}

Then divide by the wavefunction, and I get

i\hbar \frac{\partial \phi(t)}{\partial t} = \frac{-\hbar^2}{2m} \left( \frac{\partial^2 \psi_1}{\partial x^2} + \frac{\partial^2 \psi_2}{\partial y^2} + \frac{\partial^2 \psi_3}{\partial z^2} )\right

I know that each one of the unknown functions must make a separate equation, but I don't know what to solve for without energy. For the time-independent equation they will all essentially be infinite square wells, but I don't know what to do with the time dependency.
 
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Mindscrape said:
The problem is to obtain the stationary states for a free particle in three dimensions by separating the variables in Schrödinger's equation.

So take

\psi(\mathbf{r},t) = \psi_1(x) \psi_2(y) \psi_3(z) \phi(t)

and substitute it into the time-dependent Schrödinger equation. For the stationary states set U=0 and obtain

\frac{-\hbar^2}{2m} \nabla^2 \psi(\mathbf{r},t) = i\hbar \frac{\partial \psi(\mathbf{r},t)}{\partial t}

Then divide by the wavefunction, and I get

i\hbar \frac{\partial \phi(t)}{\partial t} = \frac{-\hbar^2}{2m} \left( \frac{\partial^2 \psi_1}{\partial x^2} + \frac{\partial^2 \psi_2}{\partial y^2} + \frac{\partial^2 \psi_3}{\partial z^2} )\right

I know that each one of the unknown functions must make a separate equation, but I don't know what to solve for without energy. For the time-independent equation they will all essentially be infinite square wells, but I don't know what to do with the time dependency.

Oops. A correction. I had no noticed that you had put in the wavefunction and then divided by it.

Ok, so at first you should get



i\hbar \psi_1 \psi_2 \psi_3 \frac{\partial \phi(t)}{\partial t} = \frac{-\hbar^2}{2m} \left( \phi \psi_1 \psi_3 \frac{\partial^2 \psi_1}{\partial x^2} +\phi \psi_1 \psi_3 \frac{\partial^2 \psi_2}{\partial y^2} + \phi \psi_1 \psi_2 \frac{\partial^2 \psi_3}{\partial z^2} )\right

Then the next step is to divide everything by \phi \psi_1 \psi_2 \psi_3 and then you should get (instead of what you wrote):

i\hbar {1 \over <br /> \phi} \frac{\partial \phi(t)}{\partial t} = \frac{-\hbar^2}{2m} \left( {1 \over \psi_1} \frac{\partial^2 \psi_1}{\partial x^2} +{ 1 \over \psi_2} \frac{\partial^2 \psi_2}{\partial y^2} + {1 \over \psi_3} \frac{\partial^2 \psi_3}{\partial z^2} )\right
and then to use the usual argument of separation of variables to show that \phi(t) obeys
i \hbar {\partial \phi(t) \over \partial t} = E \phi(t) [/itex] where E is the constant of separation. So \phi(t) = A e^{-iE t / \hbar}. <br /> <br /> Then you go on to separate the equations in x, y and z. You end up with three separate 1-dimensional Schrödinger equations ).<br /> <br /> Hope this helps.<br /> <br /> Patrick
 
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