The problem of a finite-length simply supported rod hanging under gravity a
nd subject to a prescribed tangential twist Tw is studied using asymptotic
and numerical methods. A three-dimensional formulation of the problem is gi
ven in which a small parameter epsilon (2) measures the relative sizes of b
ending and gravitational forces. For small values of Tw, the rod shape is f
ound by singular perturbation methods and consists of an outer catenary-lik
e solution and an inner boundary layer solution. Large twist Tw = O(1/epsil
on) of an almost straight rod produces a torque on the order of the Greenhi
ll buckling level and is shown numerically to cause buckling into a modulat
ed helix-like spiral with period of O(epsilon) superimposed onto a paraboli
c sag across the spanned distance. Multiple scale methods are used in this
parameter regime to obtain an approximate description of the postbuckled so
lution. This analysis is found to capture all the broad features indicated
by the numerics. As Tw is further increased, the deformation may localise a
nd the rod jump into a self-intersecting writhed shape. (C) 2001 Elsevier S
cience Ltd. All rights reserved.