High-energy physicists already know that stable attractors ('solitons') can
exist in 3 + 1-dimensional conservative Lagrangian systems, so long as the
definition of an attractor is based on weak notions of stability and the f
ields admit topological charge. This paper explores the possibility of attr
actors in Lagrangian field theories without topological charge, using a new
, stronger concept of stability-Convective quantized Asymptotic Orbital Sta
bility (ChAOS). Under certain conditions, ChAOS is related to 'additive Lia
punov stability' or energetic stability. Russian physicists have argued tha
t such stability tends to require topological charge; however, this paper d
escribes systems which avoid those arguments, and suggests how numerical ex
amples might be constructed. 'Solitons' have been proposed to explain the e
xistence and nature of elementary particles within the Feynman version of q
uantum theory; Section 6 cites this literature, as well as new possibilitie
s for alternative versions with testable nuclear implications. (C) 1999 Pub
lished by Elsevier Science Ltd. All rights reserved.