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Single-Particle Electrodynamics - Assassination Science

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6.5.11 Final redshift expression<br />

Finally, from the definition (3.21), we have<br />

λ = 1 + 1 2 r d(n d· ˙v) + 1 2 r s(n s· ˙v). (6.66)<br />

6.5.12 Retarded field expressions<br />

We can now use the preceding expressions to compute the various retarded<br />

fields of the particle, generated by the sending constituent r ′ and received<br />

by the receiving constituent r.<br />

It will be noted that, in all cases, the “accelerative redshift” factor λ(r)—<br />

that relates the constituent proper-time derivatives to body proper-time<br />

derivatives—will be multiplied in as the final step of the self-interaction calculations.<br />

Most of these calculations will involve the self-generated electric<br />

and magnetic fields as a simple factor; for these calculations, it is convenient<br />

to compute λ times the electric or magnetic field from the outset.<br />

On the other hand, the self-interaction terms involving spatial gradients<br />

of the electromagnetic fields must be treated more carefully. Here, we must<br />

note that the operations of multiplying by λ(r), and that of taking the spatial<br />

derivative ∇ r in r-space, do not commute, because λ(r) of course has an<br />

explicit dependence on r. Thus, we may not compute (for example)<br />

(σ·∇)λ(r)E(r);<br />

we must, rather, compute<br />

λ(r)(σ·∇)E(r).<br />

The explicit expressions for the retarded self-fields of the particle are<br />

lengthy; we list them explicitly in Section G.6.19 of Appendix G.<br />

261

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