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We address some questions related to radiation and energy conservation inclassical electromagnetism. We first treat the well-known problem of energyaccounting during radiation from a uniformly accelerating particle. We presentthe problem in the form of a paradox, and then answer it using a moderntreatment of radiation reaction and self-force, as it appears in the expressiondue to Eliezer and Ford and O'Connell. We clarify the influence of the Schottforce and the total radiated power, which differs from Larmor's formula.Finally, we present a simple and highly visual argument which enables one totrack the radiated energy without the need to appeal to the far field in thedistant future (the 'wave zone').

Tracking the radiation reaction energy when charged bodies accelerate