LASER Physics and Optical Amplification
Einstein coefficients, detailed balance, 3-level vs 4-level systems, population inversion, threshold gain, longitudinal modes, TEM modes, and survey of practical lasers.
§6.1 Radiation-Matter Interaction and Einstein’s A and B Coefficients
1. The Three Fundamental Radiative Transitions
Consider an atomic system with two discrete energy levels $E_1$ (lower state) and $E_2$ (upper state), separated by energy $h\nu = E_2 - E_1$, immersed in an electromagnetic radiation field of spectral energy density $\rho(\nu)$:- Induced (Stimulated) Absorption: An atom in level 1 absorbs a photon of energy $h\nu$ and transitions to level 2. The rate of absorption is: $$R_{\text{abs}} = B_{12} N_1 \rho(\nu)$$ where $B_{12}$ is Einstein's coefficient of stimulated absorption.
- Spontaneous Emission: An atom in level 2 spontaneously drops to level 1 without any external trigger, emitting a photon of energy $h\nu$ in a random direction and phase. The transition rate is: $$R_{\text{spont}} = A_{21} N_2$$ where $A_{21}$ is Einstein's coefficient of spontaneous emission (equal to the inverse spontaneous lifetime $1/\tau_{\text{sp}}$).
- Stimulated (Induced) Emission: An incident photon of energy $h\nu$ perturbs an atom in excited level 2, inducing it to drop to level 1 and emit a second photon that is an **identical clone** of the incident photon (identical frequency, wavevector $\mathbf{k}$, phase, and polarization state). The rate is: $$R_{\text{stim}} = B_{21} N_2 \rho(\nu)$$
2. Thermodynamic Derivation of Einstein Relations
In thermodynamic equilibrium at absolute temperature $T$, the rate of upward transitions must equal the rate of downward transitions (principle of detailed balance): $$R_{\text{abs}} = R_{\text{spont}} + R_{\text{stim}} \implies B_{12} N_1 \rho(\nu) = A_{21} N_2 + B_{21} N_2 \rho(\nu)$$ Solving for the spectral radiation density: $$\rho(\nu) = \frac{A_{21} N_2}{B_{12} N_1 - B_{21} N_2} = \frac{A_{21} / B_{21}}{\left(\frac{B_{12}}{B_{21}}\right) \frac{N_1}{N_2} - 1}$$ From Maxwell-Boltzmann statistics, the equilibrium population ratio of non-degenerate states is: $$\frac{N_1}{N_2} = \frac{g_1 e^{-E_1/k_B T}}{g_2 e^{-E_2/k_B T}} = \frac{g_1}{g_2} e^{(E_2 - E_1)/k_B T} = \frac{g_1}{g_2} e^{h\nu / k_B T}$$ Substituting into $\rho(\nu)$: $$\rho(\nu) = \frac{A_{21} / B_{21}}{\left(\frac{B_{12} g_1}{B_{21} g_2}\right) e^{h\nu / k_B T} - 1}$$ Comparing this directly with Planck’s Blackbody Radiation Formula: $$\rho(\nu) = \frac{8\pi h \nu^3}{c^3} \frac{1}{e^{h\nu / k_B T} - 1}$$ Equating corresponding terms yields the fundamental **Einstein Relations**: $$g_1 B_{12} = g_2 B_{21} \quad \implies \quad B_{12} = B_{21} \quad (\text{for } g_1 = g_2)$$ $$\frac{A_{21}}{B_{21}} = \frac{8\pi h \nu^3}{c^3}$$3. Physical Consequence
The probability of stimulated emission is strictly identical to the probability of stimulated absorption ($B_{21} = B_{12}$). The ratio of spontaneous to stimulated emission scales as $\nu^3$, explaining why optical and UV lasers are vastly harder to construct than microwave masers.§6.2 Population Inversion, Pumping Schemes and Laser Cavity Threshold Condition
1. 3-Level vs 4-Level Pumping Schemes
- 3-Level Laser (e.g., Ruby Laser): Pumping excites ground state atoms ($E_1$) into a broad pump band ($E_3$). Fast non-radiative decay transfers atoms to a metastable laser level ($E_2$). Laser action occurs between $E_2 \to E_1$. Disadvantage: Because the lower laser level $E_1$ is the ground state containing nearly all atoms, more than $50\%$ of the total atomic population must be excited just to reach transparency ($N_2 = N_1$). This requires immense pump threshold power.
- 4-Level Laser (e.g., Nd:YAG, He-Ne): Laser action occurs between metastable state $E_3$ and an excited lower laser level $E_2$ situated well above the ground state ($E_2 - E_1 \gg k_B T$). Advantage: In thermal equilibrium, level $E_2$ is essentially empty ($N_2 \approx 0$). Thus, even a very weak pump creates population inversion ($N_3 > N_2$), resulting in orders-of-magnitude lower threshold pump power and enabling continuous-wave (CW) operation.
2. The Laser Cavity Threshold Gain Condition
An active gain medium of length $L$ with small-signal gain coefficient $\gamma_0$ is placed inside an optical resonator bounded by two mirrors of reflectances $R_1$ and $R_2$. For a beam of intensity $I$ completing one full round-trip of length $2L$:- Amplification through gain medium: $e^{2 \gamma_0 L}$
- Internal scattering and absorption losses: $e^{-2 \alpha_s L}$
- Mirror reflections: $R_1 R_2$
§6.3 Optical Resonator Modes and Survey of Practical Laser Systems
1. Longitudinal (Axial) Cavity Modes
For constructive interference of waves reflecting back and forth between two flat parallel mirrors separated by cavity length $L$, the cavity must support an integral number $m$ of half-wavelengths: $$2 L = m \lambda_m = m \frac{c}{n \nu_m} \implies \nu_m = m \frac{c}{2 n L}, \quad m \in \mathbb{Z}$$ The frequency spacing between two adjacent longitudinal modes is constant: $$\Delta \nu = \nu_{m+1} - \nu_m = \frac{c}{2 n L}$$ For a He-Ne laser with $L = 30\text{ cm}$, $\Delta \nu = \frac{3 \times 10^8 \text{ m/s}}{2(0.30 \text{ m})} = 500\text{ MHz}$.2. Transverse Electromagnetic Modes ($\text{TEM}_{mn}$)
Diffraction at mirror apertures and beam divergence create transverse intensity variations described by Hermite-Gaussian modes: $$I_{mn}(x, y) = I_0 \left[ H_m\left(\frac{\sqrt{2}x}{w}\right) \right]^2 \left[ H_n\left(\frac{\sqrt{2}y}{w}\right) \right]^2 e^{-2(x^2 + y^2)/w^2}$$ The fundamental mode $\text{TEM}_{00}$ has a purely Gaussian profile ($H_0(\xi) = 1$) with zero null lines, providing diffraction-limited beam divergence.3. Survey of Practical Laser Systems
| Laser Type | Active Medium | Wavelength | Pumping | Operation |
|---|---|---|---|---|
| Helium-Neon (He-Ne) | Neutral He + Ne gas mixture (10:1) | $632.8\text{ nm}$ (Red) | Electric DC discharge | Continuous Wave (CW) |
| Ruby Laser | $\text{Cr}^{3+}$ in $\text{Al}_2\text{O}_3$ crystal | $694.3\text{ nm}$ (Deep Red) | Xenon flashtube | Pulsed (Q-switched) |
| Nd:YAG | $\text{Nd}^{3+}$ in Yttrium Aluminum Garnet | $1064\text{ nm}$ (IR) / $532\text{ nm}$ | Laser diode arrays / Flashlamp | CW / High-power pulsed |
| Carbon Dioxide ($\text{CO}_2$) | Molecular $\text{CO}_2 + \text{N}_2 + \text{He}$ | $10.6 \ \mu\text{m}$ (Far IR) | RF / Electrical discharge | High power industrial (kW) |
| Semiconductor Diode | GaAs / InGaAsP p-n junction | $405 - 1550\text{ nm}$ | Direct electrical current injection | High efficiency ($>50\%$) CW |
📝 Chapter Worked Examples & Exercises
Complete derivations & analytical proofsA Helium-Neon laser operating at $\lambda = 632.8 ext{ nm}$ has an active discharge tube length of $L = 25.0 ext{ cm}$. The cavity mirrors have reflectances $R_1 = 1.00$ (high reflector) and $R_2 = 0.98$ (output coupler). The internal scattering and diffraction loss coefficient is $alpha_s = 0.010 ext{ m}^{-1}$. Calculate: (a) the threshold gain coefficient $\gamma_{ ext{th}}$ in $ ext{m}^{-1}$, and (b) the frequency separation between adjacent longitudinal cavity modes.
The gain medium must provide at least $0.0504\text{ m}^{-1}$ ($5.04\%\text{ per meter}$) to overcome cavity losses.
Cavity longitudinal modes are separated by $600\text{ MHz}$.