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  2. Larmor formula - Wikipedia

    en.wikipedia.org/wiki/Larmor_formula

    For a particle whose velocity is small relative to the speed of light (i.e., nonrelativistic), the total power that the particle radiates (when considered as a point charge) can be calculated by the Larmor formula: = (˙) = = = = where ˙ or is the proper acceleration, is the charge, and is the speed of light. [2]

  3. Paradox of radiation of charged particles in a gravitational ...

    en.wikipedia.org/wiki/Paradox_of_radiation_of...

    This radiation electric field has an accompanying magnetic field, and the whole oscillating electromagnetic radiation field propagates independently of the accelerated charge, carrying away momentum and energy. The energy in the radiation is provided by the work that accelerates the charge.

  4. Abraham–Lorentz force - Wikipedia

    en.wikipedia.org/wiki/Abraham–Lorentz_force

    Physically, an accelerating charge emits radiation (according to the Larmor formula), which carries momentum away from the charge. Since momentum is conserved, the charge is pushed in the direction opposite the direction of the emitted radiation. In fact the formula above for radiation force can be derived from the Larmor formula, as shown below.

  5. Synchrotron radiation - Wikipedia

    en.wikipedia.org/wiki/Synchrotron_radiation

    Pictorial representation of the radiation emission process by a source moving around a Schwarzschild black hole in a de Sitter universe. Electromagnetic field observed far from the source (in arbitrary unit) of a positive accelerated point charge. When the velocity increase, the radiation concentrates along the trajectory.

  6. 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 ...

  7. Jefimenko's equations - Wikipedia

    en.wikipedia.org/wiki/Jefimenko's_equations

    As it decreases only as / ′ with distance compared to the standard / ′ Coulombic behavior, this term is responsible for the long-range electromagnetic radiation caused by the accelerating charge. The Heaviside–Feynman formula can be derived from Maxwell's equations using the technique of the retarded potential .

  8. Nonradiation condition - Wikipedia

    en.wikipedia.org/wiki/Nonradiation_condition

    In some classical electron models a distribution of charges can however be accelerated so that no radiation is emitted. [1] The modern derivation of these nonradiation conditions by Hermann A. Haus is based on the Fourier components of the current produced by a moving point charge.

  9. Liénard–Wiechert potential - Wikipedia

    en.wikipedia.org/wiki/Liénard–Wiechert_potential

    [5] [6] Electromagnetic field (arbitrary unit) of a positive accelerated point charge (far from the source). Acceleration is parallel to velocity. When the particle decelerates, this leads to braking radiations which can be strong when particles collide. Electromagnetic field (arbitrary unit) of a positive accelerated point charge (far from the ...