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  2. 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 ...

  3. Stopping power (particle radiation) - Wikipedia

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

    In nuclear and materials physics, stopping power is the retarding force acting on charged particles, typically alpha and beta particles, due to interaction with matter, resulting in loss of particle kinetic energy. [1] [2] Stopping power is also interpreted as the rate at which a material absorbs the kinetic energy of a charged particle.

  4. Beamstrahlung - Wikipedia

    en.wikipedia.org/wiki/Beamstrahlung

    Beamstrahlung (from beam + bremsstrahlung) is the radiation from one beam of charged particles in storage rings, linear or circular colliders, namely the synchrotron radiation emitted due to the electromagnetic field of the opposing beam. [1] [2] Coined by J. Rees in 1978. [3]

  5. Ionizing radiation - Wikipedia

    en.wikipedia.org/wiki/Ionizing_radiation

    This high-energy β − further interacts rapidly with other nuclei, emitting high-energy γ via Bremsstrahlung While not a favorable reaction, the 16 O (n,p) 16 N reaction is a major source of X-rays emitted from the cooling water of a pressurized water reactor and contributes enormously to the radiation generated by a water-cooled nuclear ...

  6. Bethe formula - Wikipedia

    en.wikipedia.org/wiki/Bethe_formula

    The interaction excites or ionizes the atoms, leading to an energy loss of the traveling particle. The non-relativistic version was found by Hans Bethe in 1930; the relativistic version (shown below) was found by him in 1932. [2] The most probable energy loss differs from the mean energy loss and is described by the Landau-Vavilov distribution. [3]

  7. Radiation length - Wikipedia

    en.wikipedia.org/wiki/Radiation_length

    In materials of high atomic number (e.g. tungsten, uranium, plutonium) the electrons of energies >~10 MeV predominantly lose energy by bremsstrahlung, and high-energy photons by e + e − pair production. The characteristic amount of matter traversed for these related interactions is called the radiation length X 0, usually measured in g·cm −2.

  8. Initial and final state radiation - Wikipedia

    en.wikipedia.org/wiki/Initial_and_final_state...

    In the case of initial-state radiation, one of the incoming particles emit radiation (such as a photon, wlog) before the interaction with the others, so reduces the beam energy prior to the momentum transfer; while for final-state radiation, the scattered particles emit radiation, and since the momentum transfer has already occurred, the ...

  9. External beam radiotherapy - Wikipedia

    en.wikipedia.org/wiki/External_beam_radiotherapy

    Bremsstrahlung X-rays are produced by bombarding energetic cathode rays onto a target made of a material with high atomic number, such as tungsten.The target acts as a sort of transducer, converting part of the electrons' kinetic energy into energetic photons.