When.com Web Search

Search results

  1. Results From The WOW.Com Content Network
  2. Photon energy - Wikipedia

    en.wikipedia.org/wiki/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 its energy.

  3. Photon - Wikipedia

    en.wikipedia.org/wiki/Photon

    Planck's energy formula = is often used by engineers and chemists in design, both to compute the change in energy resulting from a photon absorption and to determine the frequency of the light emitted from a given photon emission.

  4. Compton wavelength - Wikipedia

    en.wikipedia.org/wiki/Compton_wavelength

    The corresponding frequency f is given by =, and the angular frequency ω is given by =. The CODATA 2022 value for the Compton wavelength of the electron is 2.426 310 235 38 (76) × 10 −12 m. [1] Other particles have different Compton wavelengths.

  5. Planck relation - Wikipedia

    en.wikipedia.org/wiki/Planck_relation

    The Planck relation [1] [2] [3] (referred to as Planck's energy–frequency relation, [4] the Planck–Einstein relation, [5] Planck equation, [6] and Planck formula, [7] though the latter might also refer to Planck's law [8] [9]) is a fundamental equation in quantum mechanics which states that the energy E of a photon, known as photon energy, is proportional to its frequency ν: =.

  6. Wavenumber - Wikipedia

    en.wikipedia.org/wiki/Wavenumber

    where ν is the frequency of the wave, λ is the wavelength, ω = 2πν is the angular frequency of the wave, and v p is the phase velocity of the wave. The dependence of the wavenumber on the frequency (or more commonly the frequency on the wavenumber) is known as a dispersion relation.

  7. Rydberg formula - Wikipedia

    en.wikipedia.org/wiki/Rydberg_formula

    A frequency (or spectral energy) emitted in a transition from n 1 to n 2 therefore represents the photon energy emitted or absorbed when an electron makes a jump from orbital 1 to orbital 2. Later models found that the values for n 1 and n 2 corresponded to the principal quantum numbers of the two orbitals.

  8. 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.

  9. Template:SI photon units - Wikipedia

    en.wikipedia.org/wiki/Template:SI_photon_units

    photon energy: n: 1: count of photons n with energy Q p = h c/λ. [nb 2] photon flux: Φ q: count per second: s −1: T −1: photons per unit time, dn/dt with n = photon number. also called photon power: photon intensity: I: count per steradian per second sr −1 ⋅s −1: T −1: dn/dω: photon radiance: L q: count per square metre per ...