Stability of Grain Boundary Cavities in Copper
Stability of Grain Boundary Cavities in Copper
复制标题
铜晶界空洞的稳定性
作者:
A. Gittins
DURING both creep and fatigue at high temperatures cavities form on the grain boundaries of polycrystalline copper and cause a decrease in density. Under creep conditions cavity nuclei grow on those boundaries experiencing a normal tensile stress by the diffusion of vacancies from the grain boundary to the cavity surface1. For high temperature fatigue it has been proposed that an excess concentration of lattice vacancies is formed2; the vacancies then reach the cavity surface by lattice diffusion3. It is axiomatic that cavities formed by either high temperature creep or fatigue should shrink by losing vacancies when the stress is removed. The driving force to collapse a spherical cavity is 2γ/r where γ is the surface energy of the cavity and r is the cavity radius. In the absence of stress the time ts required to collapse a cavity of radius r is given by where kT has its usual significance, a is the cavity spacing (∼ 10−3 cm), Dg is the grain boundary atomic diffusion coefficient (∼10−8 cm2/sec for Cu at 400° C), δZ is the thickness of the grain boundary available for diffusion (∼ 10−7 cm) and Ω is the atomic volume (1.2 × 10−23 cm3). For copper γ ∼ 1,500 ergs/cm2. Thus a cavity of radius 5 × 10−5 cm in copper should collapse in about 5 h at 400° C.