Existing slender body theories for the dynamics of a thin tube in a Stokes flow differ
in the way the asymptotic errors depend on a small parameter defined as the radius
of the body over its length. Examples are the theory of Lighthill, that of Keller and
Rubinow, and that of Johnson. Slender body theory is revisited here in the more
general setting of forces which are localized but smoothly varying within a small
neighborhood of the filament centerline, rather than delta distributions along the
centerline. Physically, this means that the forces are smoothly distributed over the
cross-section of the body. The regularity in the forces produces a final expression that
has built-in smoothing which helps eliminate instabilities encountered in
computations with unsmoothed formulas. Consistency with standard theories is
verified in the limit as the smoothing parameter vanishes, where the original
expressions are recovered. In addition, an expression for the fluid velocity at
locations off the slender body is derived and used to compute the flow around a
filament.