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  2. Einstein coefficients - Wikipedia

    en.wikipedia.org/wiki/Einstein_coefficients

    In 1916, Albert Einstein proposed that there are three processes occurring in the formation of an atomic spectral line. The three processes are referred to as spontaneous emission, stimulated emission, and absorption. With each is associated an Einstein coefficient, which is a measure of the probability of that particular process occurring.

  3. Stimulated emission - Wikipedia

    en.wikipedia.org/wiki/Stimulated_emission

    In normal media at thermal equilibrium, absorption exceeds stimulated emission because there are more electrons in the lower energy states than in the higher energy states. However, when a population inversion is present, the rate of stimulated emission exceeds that of absorption, and a net optical amplification can be achieved.

  4. Spontaneous emission - Wikipedia

    en.wikipedia.org/wiki/Spontaneous_emission

    Spontaneous emission is the process in which a quantum mechanical system (such as a molecule, an atom or a subatomic particle) transits from an excited energy state to a lower energy state (e.g., its ground state) and emits a quantized amount of energy in the form of a photon. Spontaneous emission is ultimately responsible for most of the light ...

  5. Population inversion - Wikipedia

    en.wikipedia.org/wiki/Population_inversion

    The rate at which stimulated emission occurs is proportional to the number of atoms N 2 in the excited state, and the radiation density of the light. The base probability of a photon causing stimulated emission in a single excited atom was shown by Albert Einstein to be exactly equal to the probability of a photon being absorbed by an atom in ...

  6. Laser science - Wikipedia

    en.wikipedia.org/wiki/Laser_science

    Laser science predates the invention of the laser itself. Albert Einstein created the foundations for the laser and maser in 1917, via a paper in which he re-derived Max Planck’s law of radiation using a formalism based on probability coefficients (Einstein coefficients) for the absorption, spontaneous emission, and stimulated emission of electromagnetic radiation. [2]

  7. Two-photon absorption - Wikipedia

    en.wikipedia.org/wiki/Two-photon_absorption

    Schematic of energy levels involved in two photons absorption. In atomic physics, two-photon absorption (TPA or 2PA), also called two-photon excitation or non-linear absorption, is the simultaneous absorption of two photons of identical or different frequencies in order to excite an atom or a molecule from one state (usually the ground state), via a virtual energy level, to a higher energy ...

  8. McCumber relation - Wikipedia

    en.wikipedia.org/wiki/McCumber_relation

    Let be group velocity of light in the medium, the product () is spectral rate of stimulated emission, and () is that of absorption; () is spectral rate of spontaneous emission. (Note that in this approximation, there is no such thing as a spontaneous absorption) The balance of photons gives:

  9. Kramers–Heisenberg formula - Wikipedia

    en.wikipedia.org/wiki/Kramers–Heisenberg_formula

    The Kramers–Heisenberg formula was an important achievement when it was published, explaining the notion of "negative absorption" (stimulated emission), the Thomas–Reiche–Kuhn sum rule, and inelastic scattering — where the energy of the scattered photon may be larger or smaller than that of the incident photon — thereby anticipating ...