The dynamics of defects with linear dimensions from approximate to 1 to app
roximate to 100 nm on a Au surface under load have been studied by means of
tunnelling microscopy. It is found that the origin, growth, and resorption
of the defects is caused by displacements of bands of material from 5 to 5
0 nm wide, parallel to the {111} slip planes. The defects can be separated
into two groups: nonsteady-state defects, whose lifetime does not exceed 15
min, while the depth is less than or equal to 20 nm, and quasi-steady-stat
e defects, with a lifetime three orders of magnitude greater than the first
. It is assumed that the nonsteady-state defects are formed when the ensemb
le of dislocations is being reconstructed, while the quasi-steady-state def
ects are formed at the instant of formation of dislocation substructures du
ring the creep of the loaded metal. (C) 1998 American Institute of Physics.
[S1063-7834(98)00912-5].