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  2. Bethe formula - Wikipedia

    en.wikipedia.org/wiki/Bethe_formula

    At low energy, the energy loss according to the Bethe formula therefore decreases approximately as v −2 with increasing energy. It reaches a minimum for approximately E = 3Mc 2, where M is the mass of the particle (for protons, this would be about at 3000 MeV).

  3. Electron energy loss spectroscopy - Wikipedia

    en.wikipedia.org/wiki/Electron_energy_loss...

    Electron energy loss spectroscopy (EELS) is a form of electron microscopy in which a material is exposed to a beam of electrons with a known, narrow range of kinetic energies. Some of the electrons will undergo inelastic scattering , which means that they lose energy and have their paths slightly and randomly deflected.

  4. Free electron model - Wikipedia

    en.wikipedia.org/wiki/Free_electron_model

    In solid-state physics, the free electron model is a quantum mechanical model for the behaviour of charge carriers in a metallic solid. It was developed in 1927, [1] principally by Arnold Sommerfeld, who combined the classical Drude model with quantum mechanical Fermi–Dirac statistics and hence it is also known as the Drude–Sommerfeld model.

  5. Bremsstrahlung - Wikipedia

    en.wikipedia.org/wiki/Bremsstrahlung

    Bremsstrahlung produced by a high-energy electron deflected in the electric field of an atomic nucleus. In particle physics, bremsstrahlung / ˈ b r ɛ m ʃ t r ɑː l ə ŋ / [1] (German pronunciation: [ˈbʁɛms.ʃtʁaːlʊŋ] ⓘ; from German bremsen ' to brake ' and Strahlung ' radiation ') is electromagnetic radiation produced by the deceleration of a charged particle when deflected by ...

  6. Binding energy - Wikipedia

    en.wikipedia.org/wiki/Binding_energy

    Electron binding energy; Ionization energy Electron binding energy, more commonly known as ionization energy, [3] is a measure of the energy required to free an electron from its atomic orbital or from a solid. The electron binding energy derives from the electromagnetic interaction of the electron with the nucleus and the other electrons of ...

  7. Free carrier absorption - Wikipedia

    en.wikipedia.org/wiki/Free_carrier_absorption

    The energy of free carriers is proportional to the square of momentum (). Using the band gap energy E g {\displaystyle E_{g}} and the electron-hole distribution function, we can obtain the absorption coefficient with some mathematical calculation.

  8. Inelastic mean free path - Wikipedia

    en.wikipedia.org/wiki/Inelastic_mean_free_path

    The inelastic mean free path (IMFP) is an index of how far an electron on average travels through a solid before losing energy. Universal curve for the electron inelastic mean free path in elements based on equation (5) in. [ 1 ]

  9. Stopping power (particle radiation) - Wikipedia

    en.wikipedia.org/wiki/Stopping_power_(particle...

    The stopping power of the material is numerically equal to the loss of energy E per unit path length, x: = / The minus sign makes S positive. Bragg curve of 5.49 MeV alpha particles in air. The force usually increases toward the end of range and reaches a maximum, the Bragg peak, shortly before the energy drops to zero.