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  2. Photon energy - Wikipedia

    en.wikipedia.org/wiki/Photon_energy

    Photon energy. Photon energy is the energy carried by a single photon. The amount of energy is directly proportional to the photon's electromagnetic frequency and thus, equivalently, is inversely proportional to the wavelength. The higher the photon's frequency, the higher its energy. Equivalently, the longer the photon's wavelength, the lower ...

  3. Electronvolt - Wikipedia

    en.wikipedia.org/wiki/Electronvolt

    1.602 176 634 × 10−19 J. [1] In physics, an electronvolt (symbol eV), also written electron-volt and electron volt, is the measure of an amount of kinetic energy gained by a single electron accelerating through an electric potential difference of one volt in vacuum. When used as a unit of energy, the numerical value of 1 eV in joules (symbol ...

  4. Photoelectric effect - Wikipedia

    en.wikipedia.org/wiki/Photoelectric_effect

    Photoemission of electrons from a metal plate accompanied by the absorption of light quanta – photons. The photoelectric effect is the emission of electrons from a material caused by electromagnetic radiation such as ultraviolet light. Electrons emitted in this manner are called photoelectrons. The phenomenon is studied in condensed matter ...

  5. Planck constant - Wikipedia

    en.wikipedia.org/wiki/Planck_constant

    The Planck constant, or Planck's constant, denoted by ,[1] is a fundamental physical constant [1] of foundational importance in quantum mechanics: a photon 's energy is equal to its frequency multiplied by the Planck constant, and the wavelength of a matter wave equals the Planck constant divided by the associated particle momentum.

  6. Wavenumber - Wikipedia

    en.wikipedia.org/wiki/Wavenumber

    A spectroscopic wavenumber can be converted into energy per photon E by Planck's relation: = ~. It can also be converted into wavelength of light: = ~, where n is the refractive index of the medium. Note that the wavelength of light changes as it passes through different media, however, the spectroscopic wavenumber (i.e., frequency) remains ...

  7. Photoemission spectroscopy - Wikipedia

    en.wikipedia.org/wiki/Photoemission_spectroscopy

    Typical PES (UPS) instruments use helium gas sources of UV light, with photon energy up to 52 eV (corresponding to wavelength 23.7 nm). The photoelectrons that actually escaped into the vacuum are collected, slightly retarded, energy resolved, and counted. This results in a spectrum of electron intensity as a function of the measured kinetic ...

  8. Band gap - Wikipedia

    en.wikipedia.org/wiki/Band_gap

    In solid-state physics and solid-state chemistry, a band gap, also called a bandgap or energy gap, is an energy range in a solid where no electronic states exist. In graphs of the electronic band structure of solids, the band gap refers to the energy difference (often expressed in electronvolts) between the top of the valence band and the ...

  9. Multi-junction solar cell - Wikipedia

    en.wikipedia.org/wiki/Multi-junction_solar_cell

    where E ph is photon energy, h is the Planck constant (h ≈ 6.626 × 10 −34 J⋅Hz −1), c is speed of light (c = 299 792 458 m⋅s −1), f is frequency, and λ is wavelength. Then the photon flux per photon energy, dn ph /dhν, with respect to certain irradiance E [W/m 2 ·eV] can be calculated as follows.