Population inversion

related topics
{math, energy, light}
{acid, form, water}
{rate, high, increase}
{county, mile, population}
{group, member, jewish}
{area, part, region}

In physics, specifically statistical mechanics, a population inversion occurs when a system (such as a group of atoms or molecules) exists in state with more members in an excited state than in lower energy states. The concept is of fundamental importance in laser science because the production of a population inversion is a necessary step in the workings of a standard laser.

Contents

Boltzmann distributions and thermal equilibrium

To understand the concept of a population inversion, it is necessary to understand some thermodynamics and the way that light interacts with matter. To do so, it is useful to consider a very simple assembly of atoms forming a laser medium.

Assume there are a group of N atoms, each of which is capable of being in one of two energy states, either

The number of these atoms which are in the ground state is given by N1, and the number in the excited state N2. Since there are N atoms in total,

The energy difference between the two states, given by

determines the characteristic frequency ν12 of light which will interact with the atoms; This is given by the relation

h being Planck's constant.

If the group of atoms is in thermal equilibrium, it can be shown from thermodynamics that the ratio of the number of atoms in each state is given by a Boltzmann distribution:

where T is the thermodynamic temperature of the group of atoms, and k is Boltzmann's constant.

We may calculate the ratio of the populations of the two states at room temperature (T ≈ 300 K) for an energy difference ΔE that corresponds to light of a frequency corresponding to visible light (ν ≈ 5×1014 Hz). In this case ΔE = E2 - E1 ≈ 2.07 eV, and kT ≈ 0.026 eV. Since E2 - E1kT, it follows that the argument of the exponential in the equation above is a large negative number, and as such N2/N1 is vanishingly small; i.e., there are almost no atoms in the excited state. When in thermal equilibrium, then, it is seen that the lower energy state is more populated than the higher energy state, and this is the normal state of the system. As T increases, the number of electrons in the high-energy state (N2) increases, but N2 never exceeds N1 for a system at thermal equilibrium; rather, at infinite temperature, the populations N2 and N1 become equal. In other words, a population inversion (N2/N1 > 1) can never exist for a system at thermal equilibrium. To achieve population inversion therefore requires pushing the system into a non-equilibrated state.

Full article ▸

related documents
Electrical resistance
Beer-Lambert law
Pauli exclusion principle
Ideal gas
Apparent magnitude
Equation of state
Crab Nebula
Shell model
DESY
Flux
Ellipse
Big Bang nucleosynthesis
Biot–Savart law
Tachyon
Luminosity
Angular velocity
Chandrasekhar limit
Refractive index
Degenerate matter
Wormhole
Auger electron spectroscopy
Soliton
Thermodynamics
Sphere
Bremsstrahlung
Sunspot
Aperture
Planetary science
Natural satellite
Sunlight