Power of the Radiative Friction Force for a Charged Particle Performing a Flyby Near a Rotating Black Hole

We analytically obtain a relativistic generalization of the classical Larmor formula for the power of the radiation friction force <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>P</mi><mo>=</mo><mi>m</mi><msup><mi>c</mi><mn>3</mn></msup><msub><mi>r</mi><mi>e</mi></msub><mrow><mo>(</mo><mo>−</mo><msub><mi>w</mi><mi>i</mi></msub><msup><mi>w</mi><mi>i</mi></msup><mo>)</mo></mrow></mrow></semantics></math></inline-formula> for the case where a relativistic charged particle moves in the vicinity of a rotating Kerr black hole.

Abstract licence: CC BY

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