Motion in classical field theories and the foundations of the self-force problem
Abraham I. Harte

TL;DR
This paper provides a comprehensive, pedagogical overview of the self-force problem in classical field theories, deriving general laws for self-interaction effects across various theories including gravity and electromagnetism.
Contribution
It introduces a unified, non-perturbative framework for understanding self-force and self-torque in classical fields, extending previous work with new insights and interpretations.
Findings
Derivation of self-force laws for extended objects in multiple theories
Identification of structural similarities across different field theories
Discussion of renormalization and multipole moment shifts in self-interacting bodies
Abstract
This article serves as a pedagogical introduction to the problem of motion in classical field theories. The primary focus is on self-interaction: How does an object's own field affect its motion? General laws governing the self-force and self-torque are derived using simple, non-perturbative arguments. The relevant concepts are developed gradually by considering motion in a series of increasingly complicated theories. Newtonian gravity is discussed first, then Klein-Gordon theory, electromagnetism, and finally general relativity. Linear and angular momenta as well as centers of mass are defined in each of these cases. Multipole expansions for the force and torque are then derived to all orders for arbitrarily self-interacting extended objects. These expansions are found to be structurally identical to the laws of motion satisfied by extended test bodies, except that all relevant fields…
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