PHOT 301: Quantum Photonics
LECTURE 05
Michaël Barbier, Fall semester (2024-2025)
So far we looked at bound states
Different well potentials lead to different allowed energy levels
Narrower wells \(\longrightarrow\) less energy levels (more spread)
\[ -\frac{\hbar^2}{2m} \frac{d^2 \psi(x)}{dx^2} = E \psi(x), \quad \textrm{ as } V(x) = 0 \]
\[ \Rightarrow \quad \frac{d^2 \psi(x)}{dx^2} = - k^2 \psi(x), \quad \textrm{ with } k = \frac{\sqrt{2 m E}}{\hbar} \]
\[ \psi(x) = A e^{ikx} + B e^{-ikx} \]
\[ \psi(x) = A e^{ikx} + B e^{-ikx} \]
\[ \psi(x) = A e^{ikx} + B e^{-ikx} \]
\[ \begin{aligned} |\psi(x)|^2 &= \psi(x)^* \, \psi(x)\\ &= (A^* e^{-ikx} + B^* e^{ikx}) (A e^{ikx} + B e^{-ikx})\\ &= |A|^2 + |B|^2 + (A B^* e^{i2kx} + A^* B e^{-i2kx})\\ &= |A|^2 + |B|^2 + \Re\left(A B^* e^{i2kx}\right)\\ \Rightarrow \int_{-\infty}^{+\infty} |\psi(x)|^2 dx &= (|A|^2 + |B|^2) \, \infty + \int_{-\infty}^{+\infty} \Re\left(A B^* e^{i2kx}\right) dx\\ \end{aligned} \]
The last integral is bounded (oscillating between finite values)
The total integral \(\int |\psi|^2 dx \longrightarrow +\infty\), and therefore doesn’t exist.
We can rewrite \(\Psi(x, t) = \psi(x) e^{-iEt/\hbar}\) with \(E = \frac{\hbar^2 k^2}{2m}\):
\[ \begin{aligned} \Psi(x, t) &= A e^{ikx - iEt/\hbar} + B e^{-ikx - iEt/\hbar}\\ &= A e^{ikx - iEt/\hbar} + B e^{-ikx - iEt/\hbar}\\ &= A e^{ik(x - \frac{\hbar k}{2m}t)} + B e^{-ik(x - \frac{\hbar k}{2m}t)}\\ \end{aligned} \]
\[ \psi(x) = \sum_{n=-N}^N e^{i (k_0 + n\delta k) x} \]
Phase velocity \(v\)
\[ v = \frac{\omega}{k} \]
Group velocity:
\[ v_g = \frac{d\omega}{dk} \]
\[ \Psi(x, t) = \sum_{n=-N}^N e^{i (k_0 + n\delta k) x} \]
\[ \begin{aligned} \Psi(x, t) &= \frac{1}{\sqrt{2\pi}}\int \phi(k) e^{i (k x - \omega t)}\\ \end{aligned} \]
Assume \(\phi(k)\) around \(k_0\)
\[ \begin{aligned} \Psi(x, t) &\approx \frac{1}{\sqrt{2\pi}}\int \phi(k_0 + s) e^{i ((k_0 +s) x - (\omega_0 + s\omega_0') t)}\\ &\approx \frac{1}{\sqrt{2\pi}} e^{i (k_0 x - \omega_0 t)} \int \phi(k_0 + s) e^{i s(x - \omega_0' t)}\\ \end{aligned} \]
Finite square potential well
Bound states \(0 < E < V_0\)
Scattering states \(E > V_0\)
Schrodinger equation:
\[ - \frac{\hbar^2}{2m} \frac{d^2 \psi(x)}{dx^2} = \left(E - V(x)\right) \, \psi(x) \]
For bound states \(0 < E < V_0\)
\[ \textrm{inside: }\quad \psi(-a < x < a) = C \sin(\lambda x) + D \cos(\lambda x) \qquad \lambda = \frac{\sqrt{2 m E}}{\hbar} \]
\[ \textrm{outside:} \quad \begin{aligned} \psi(x < -a) &= A e^{-\kappa x} + B e^{\kappa x} = B e^{\kappa x}\\ \psi(x > a) &= F e^{-\kappa x} + G e^{\kappa x} = F e^{-\kappa x} \end{aligned} \qquad \kappa = \frac{\sqrt{2 m (V_0 - E)}}{\hbar} \]
Since \(\psi(x)\) is continuous in \(x = -a\) and \(x = a\):
\[ \begin{aligned} B e^{-\kappa a} &= -C \sin(\lambda a) + D \cos(\lambda a)\\ F e^{-\kappa a} &= C \sin(\lambda a) + D \cos(\lambda a)\\ \end{aligned} \qquad \psi(x) \textrm{ continuous in } x = -a, a \]
\[ \begin{aligned} B \kappa e^{-\kappa a} &= \lambda C \cos(\lambda a) + D \sin(\lambda a)\\ -F \kappa e^{-\kappa a} &= \lambda C \cos(\lambda a) - \lambda D \sin(\lambda a)\\ \end{aligned} \qquad \frac{d\psi(x)}{dx} \textrm{ continuous in } x = -a, a \]
\[ \begin{aligned} B e^{-\kappa a} &= -C \sin(\lambda a) + D \cos(\lambda a)\\ F e^{-\kappa a} &= C \sin(\lambda a) + D \cos(\lambda a)\\ \end{aligned} \qquad \psi(x) \textrm{ continuous in } x = -a, a \]
\[ \begin{aligned} B \kappa e^{-\kappa a} &= \lambda C \cos(\lambda a) + \lambda D \sin(\lambda a)\\ -F \kappa e^{-\kappa a} &= \lambda C \cos(\lambda a) - \lambda D \sin(\lambda a)\\ \end{aligned} \qquad \frac{d\psi(x)}{dx} \textrm{ continuous in } x = -a, a \]
Add the first two equations and subtract the others:
\[ \begin{aligned} (B + F) e^{-\kappa a} &= 2 D \cos{\lambda a}\\ (B + F) \frac{\kappa}{\lambda} e^{-\kappa a} &= 2 D \sin{\lambda a}\\ \end{aligned} \]
And divide them \(\Leftrightarrow B \neq -F\)
\[ \begin{aligned} \frac{\kappa}{\lambda} &= \tan{\lambda a}\\ \end{aligned} \]
\[ \begin{aligned} B e^{-\kappa a} &= -C \sin(\lambda a) + D \cos(\lambda a)\\ F e^{-\kappa a} &= C \sin(\lambda a) + D \cos(\lambda a)\\ \end{aligned} \qquad \psi(x) \textrm{ continuous in } x = -a, a \]
\[ \begin{aligned} B \kappa e^{-\kappa a} &= \lambda C \cos(\lambda a) + \lambda D \sin(\lambda a)\\ -F \kappa e^{-\kappa a} &= \lambda C \cos(\lambda a) - \lambda D \sin(\lambda a)\\ \end{aligned} \qquad \frac{d\psi(x)}{dx} \textrm{ continuous in } x = -a, a \]
Now subtract the first two equations and add the others:
\[ \begin{aligned} (B - F) e^{-\kappa a} &= -2 C \sin{\lambda a}\\ (B - F) \frac{\kappa}{\lambda} e^{-\kappa a} &= 2 C \cos{\lambda a}\\ \end{aligned} \]
And divide them \(\Leftrightarrow B \neq F\)
\[ \begin{aligned} \frac{\kappa}{\lambda} &= -\cot{\lambda a} \qquad \textrm{ if } B \neq F\\ \frac{\kappa}{\lambda} &= \tan{\lambda a} \qquad \textrm{ if } B \neq -F \textrm{ from before} \\ \end{aligned} \]
\[ \begin{aligned} \frac{\kappa}{\lambda} &= -\cot{\lambda a} \qquad \textrm{ if } B \neq F\\ \frac{\kappa}{\lambda} &= \tan{\lambda a} \qquad \textrm{ if } B \neq -F \textrm{ from before} \\ \end{aligned} \]
\[ B = F \quad \Rightarrow \quad \begin{aligned} (B - F) e^{-\kappa a} &= -2 C \sin{\lambda a}\\ (B - F) \frac{\kappa}{\lambda} e^{-\kappa a} &= 2 C \cos{\lambda a}\\ \end{aligned} \quad \Rightarrow C = 0, \psi(x) = D \cos(\lambda x) \]
\[ B = -F \quad \Rightarrow \quad \begin{aligned} (B + F) e^{-\kappa a} &= 2 D \cos{\lambda a}\\ (B + F) \frac{\kappa}{\lambda} e^{-\kappa a} &= 2 D \sin{\lambda a}\\ \end{aligned} \quad \Rightarrow D = 0, \psi(x) = C \sin(\lambda x) \]
Symmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= D \cos(\lambda x)\\ \psi(x > a) &= B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = B \quad \& \quad \kappa = \lambda \tan \lambda a\)
Asymmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= C \sin(\lambda x)\\ \psi(x > a) &= -B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = -B \quad \& \quad \kappa = -\lambda \cot \lambda a\)
Symmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= D \cos(\lambda x)\\ \psi(x > a) &= B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = B \quad \& \quad \kappa = \lambda \tan \lambda a\)
Asymmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= C \sin(\lambda x)\\ \psi(x > a) &= -B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = -B \quad \& \quad \kappa = -\lambda \cot \lambda a\)
Let’s first obtain the energy from \(\kappa\) and \(\lambda\):
\[ \kappa^2 = \frac{2m}{\hbar^2}(V_0 - E), \qquad \lambda^2 = \frac{2m}{\hbar^2}(E) \]
Define \(z = \lambda \, a\) and \(z_0 = a\, \frac{\sqrt{2mV_0}}{\hbar}\)
\[ \Longrightarrow \quad \kappa^2 + \lambda^2 = \frac{2m}{\hbar^2}(V_0) = z_0^2/a^2 \quad \Longrightarrow \quad \kappa^2 a^2 = z_0^2 - z^2 \]
Symmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= D \cos(\lambda x)\\ \psi(x > a) &= B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = B \quad \& \quad \kappa = \lambda \tan \lambda a\)
\[ \Longrightarrow \tan z = \sqrt{\frac{z_0^2}{z^2} - 1} \]
Asymmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= C \sin(\lambda x)\\ \psi(x > a) &= -B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = -B \quad \& \quad \kappa = -\lambda \cot \lambda a\)
\[ \Longrightarrow -\cot z = \sqrt{\frac{z_0^2}{z^2} - 1} \]
where we made use of:
\[ \kappa^2 a^2 = z_0^2 - z^2 \Longrightarrow \kappa/\lambda = \sqrt{z_0^2/z^2 - 1} \]
Symmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= D \cos(\lambda x)\\ \psi(x > a) &= B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = B \quad \& \quad \kappa = \lambda \tan \lambda a\)
\[ \Longrightarrow \tan z = \sqrt{\frac{z_0^2}{z^2} - 1} \]
Asymmetric solutions
\[ \left\{ \begin{aligned} \psi(x < -a) &= B e^{\kappa x}\\ \psi(-a < x < a) &= C \sin(\lambda x)\\ \psi(x > a) &= -B e^{-\kappa x}\\ \end{aligned} \right. \]
with \(F = -B \quad \& \quad \kappa = -\lambda \cot \lambda a\)
\[ \Longrightarrow -\cot z = \sqrt{\frac{z_0^2}{z^2} - 1} \]
Asymmetric energies approximately “shifted” to the right
\[ E_n = \frac{\hbar^2 z^2}{2m a^2} \lessapprox E^\infty_n = \frac{\hbar^2}{2m}\frac{n^2\pi^2}{(2a)^2} \]
Numerically solving for \(z\):
\[ \begin{aligned} \tan z &= \sqrt{z_0^2/z^2 - 1},\\ -\cot z &= \sqrt{z_0^2/z^2 - 1}\\ \end{aligned} \]
Gives us:
\[ \begin{aligned} B &= D \cos(\lambda a) e^{\kappa a}\\ B &= -C \sin(\lambda a) e^{\kappa a}\\ \end{aligned} \]
Lecture 05: Free particles, bound states, and scattering