Saha Equilibrium in Dense Sodium Vapor
Ionization fractions and the transition to a plasma state
The Saha equation governs the degree of ionization in a gas at thermal equilibrium. In dense sodium vapor, the low ionization potential of Na (5.14 eV) leads to significant partial ionization even at temperatures accessible in laboratory settings.
Saha Equilibrium in Dense Sodium Vapor
The degree of ionization in a thermalized vapor is determined by the balance between collisional ionization and three-body recombination. For a monatomic gas like sodium, this balance is expressed by the Saha equation:
$$\frac{n_e n_i}{n_n} = \frac{2}{\lambda_e^3} \frac{g_i}{g_n} \exp\left(-\frac{\epsilon_i}{k_B T}\right)$$
where $\lambda_e = \frac{h}{\sqrt{2\pi m_e k_B T}}$ is the thermal de Broglie wavelength of the electron.
Dense Vapor Context
In the context of 01-nlambda3-cooperative-threshold, we often consider the vapor as a collection of neutral emitters. For Na D₂ at 589 nm: - n_crit ≈ 3.13 × 10¹⁴ cm⁻³
However, as the temperature increases to reach this threshold, the population of free electrons $n_e$ grows. For sodium, the ionization energy $\epsilon_i$ is $5.139$ eV.
At $T = 1000$ K, the saturated number density $n_{total} \approx 3.0 \times 10^{16}$ cm⁻³ is well above the cooperative threshold. The presence of free electrons can significantly alter the 04-voigt-profile via Stark broadening and influence the transition from 02-holstein-radiation-trapping to collective states.
Regimes of Ionization
While 03-dicke-superradiance focuses on the coherent internal states of the atoms, the Saha equilibrium reminds us that the "atomic" nature of the medium is itself a function of the local thermodynamic state. In extreme density regimes, pressure ionization may further lower the effective $\epsilon_i$.
## See also - 01-nlambda3-cooperative-threshold - 02-holstein-radiation-trapping - 03-dicke-superradiance - 04-voigt-profile
Explorables
Drag T: saturated Na vapor density n(T) climbs the Nesmeyanov curve and crosses the cooperative threshold n_crit = 64/λ³. Watch the regime flip from Holstein-trapped to cooperative to superradiant.