Abstract

This paper is devoted to a consideration of the following problem: An incompressible fluid sphere, in which the density and the viscosity are functions of the distance r from the centre only, is subject to a radial acceleration -γr, where γ is a function of r: to determine the manner of initial development of an infinitesimal disturbance. By analysing the disturbance in spherical harmonics, the mathematical problem is reduced to one in characteristic values in a fourth-order differential equation and a variational principle characterizing the solution is enunciated. The particular case of a sphere of radius R and density p 1 embedded in a medium of a different density p 2 (but of the same kinematic viscosity v) is considered in some detail; and it is shown that the character of the equilibrium depends on the sign of γR(p 2 -p 1 ) and the magnitude of = γ R R 4 /v 2 . If γ R (p 2 -p 1 ) > 0, the situation is unstable and the mode of maximum instability is l = 1 for all R (p 2 -p 1 ) > 0 the results of both an exact calculation and an approximate calculation (based on the variational principle) are given and contrasted. In the case γ R (p 2 -p 1 ) < 0 when the situation is stable, the manner of decay of the disturbance is briefly discussed in terms of an approximate theory only.

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call