Summary Notes of Free Particle and Momentum Operator
Free Particle
Function of a standing wave is:
\[\Psi(x) = A * e^{i k x} + B * e^{-i k x}\]Solve for the energy of the wave by applying the hamiltonian to Ψ
Apply the operator on the wavefunction
\[H\Psi = -\frac{\hbar^2}{2m} \nabla^2(A e^{i k x} + B e^{-i k x})\] \[= -\frac{\hbar^2}{2m}(A(i k)^2 e^{i k x} + B(-i k)^2 e^{-i k x})\] \[= -\frac{\hbar^2}{2m}(-A k^2 e^{i k x} - B k^2 e^{-i k x})\] \[E\Psi = -\frac{\hbar^2}{2m}(-k^2)(A e^{i k x} + B e^{-i k x})\]where \(E\) is the Energy (eigenvalue) and the wavefunction is returned (eigenfunction)
\[E = \frac{\hbar^2 k^2}{2m}(A e^{i k x} + B e^{-i k x})\]The free particle has no boundaries and is not confined in space, the spatial frequency, \(k\), and \(E\) values are not restricted and can be any number. Therefore, since they are not restricted, the system is not quantized.
Momentum Operator
Define momentum (\(\rho\)) via the de Broglie relation where \(\lambda = \frac{2\pi}{k}\) relating the wavelength (\(\lambda\)) to the spatial frequency (\(k\)).
\[\rho = \frac{h}{\lambda}\] \[\rho = \frac{h}{\lambda} = h*k\] \[\frac{2\pi}{\lambda} = \hbar * k\] \[\rho = \hbar * k\]Momentum operator (\(\rho\)):
The momentum operator makes changes to the wavefunction. Ask for momentum and get back the eigenfunction (\(\Psi\)) and eigenvalue (\(\rho\)) from operation.
Confirm this with an example where \(\rho = \frac{\hbar}{i} \frac{d}{dx}\).
\(\hat{\rho} \Psi =\)\rho(A e^{i k x}) = \frac{\hbar}{i} \frac{d}{dx}(A e^{i k x}) = \frac{\hbar}{i}A(i k)e^{i k x} = \hbar k A e^{i k x} = \rho A e^{i k x}$$
This returns the scalar momentum (\(\rho\)) times the eigenfunction (\(A e^{i k x}\)).
Now confirm for \(\rho^2\) where the Energy for classical physics is
\[E = \frac{1}{2}mv^2 = \frac{\rho^2}{2m}\] \[\hat{\rho^2} = \left(\frac{\hbar}{i}\frac{d}{dx}\right)^2 = \frac{\hbar^2}{i^2}\frac{d^2}{dx^2} = -\hbar^2 \frac{d^2}{dx^2}\] \[\frac{d^2}{dx^2} = \nabla^2\]confirms that this is a reasonable match to classical physics
\[\frac{\hat{\rho^2}}{2m} = H = -\frac{\hbar^2}{2m} \nabla^2\]