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Single-Particle Electrodynamics - Assassination Science

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particle in the CACS—and hence is independent of any particular coördinate<br />

frame we choose to use to evaluate components of quantities. On the other<br />

hand, the naïve proper-time derivative of the four-vector Σ α actually furnishes<br />

us with the quantities [ Σ ˙ α ]:<br />

d τ [Σ α ] ≡ [ ˙ Σ α ],<br />

because we generally evaluate the components Σ α in a Lorentz frame, and<br />

then take the derivatives of these components. Thus, the quantity<br />

˙ Σ α + U α ˙U β Σ β<br />

that one frequently sees in the literature should, in the author’s notation, be<br />

surrounded by square brakets—and is indeed simply the right-hand side of<br />

(2.68).<br />

We now turn to the question of finding appropriate names for the quantities<br />

( Σ ˙ ) and [ Σ ˙ ], so that they shall not be confused in the remainder of<br />

this thesis. If one looks, for example, in Jackson’s textbook [113, Sec. 11.11],<br />

one finds that he has, indeed, recognised the fundamental importance of<br />

( ˙ Σ ): he has given it a new symbol F α in his equation (11.166) (to which<br />

we shall return shortly). However, he simply refers to it as “the terms with<br />

coefficient (ge/2mc) in (11.162)”.<br />

Now, it may be acceptable to refer to<br />

this quantity as “the terms with coefficient (ge/2mc) in (11.162)” on one,<br />

or perhaps two, occasions; but if one were to read about “the terms with<br />

coefficient (ge/2mc) in (11.162)” repeatedly, one would no doubt appreciate<br />

the need for a simpler name. Furthermore, we shall shortly have need to consider<br />

proper-time derivatives, similar in nature to “the terms with coefficient<br />

(ge/2mc) in (11.162)”, but for completely different quantities altogether.<br />

We shall therefore refer to ( Σ ˙ ) as the covariant proper-time derivative of<br />

Σ ; and the quantity [ Σ ˙ ] as the partial proper-time derivative of Σ . The justification<br />

for this nomenclature is that it is of course that which is commonly<br />

used in General Relativity (see, e.g., [153]). Although our description above<br />

75

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