Progress of Non-ferrous Metallurgy in 1929

The American Institute of Mining, Metallurgical, and Petroleum Engineers
R. S. Dean
Organization:
The American Institute of Mining, Metallurgical, and Petroleum Engineers
Pages:
9
File Size:
951 KB
Publication Date:
Jan 1, 1930

Abstract

T HE theory of hardening by heat treatment was, as usual, the most actively discussed phase of metal working theory and in spite of the fact that it is now ten years since the dispersion theory was proposed by Messrs. Merica, Waltenberg, and Scott, it still retains a dominating influence. It is being increasingly recognized. however, that in its simplest form, that is, the purely mechanical effect of very fine crystallites distributed through a groundmass, it is distinctly in- adequate. To explain the observed facts we are obliged to assume some well-defined intermediate stage between supercooled solid solution and conglomerate, however fine be the particles of the latter. This intermediate has been inferred by Gaylor and Preston to be "the rejection of the atoms of the dissolved metal from the lattice of the solid solution accompanied by the possible formation of molecules."' Perhaps this may well be designated as the formation of supersaturated solid solution. Some very definite evidence of such an inter- mediate stage has been found in the hardening of steel where it appears that the very hard martensite may be considered as a supersaturated solution of carbon in a iron. The X-ray spectrometry of drastically quenched steel shows a tetragonal lattice whose parameter changes by tempering at 100" until it coincides with the cubic lattice of iron.? The same gradual change of the tetragonal to the cubic lattice has been observed by Sekito when esamining layers on increasing depth below the surface of a quenched carbon steel.
Citation

APA: R. S. Dean  (1930)  Progress of Non-ferrous Metallurgy in 1929

MLA: R. S. Dean Progress of Non-ferrous Metallurgy in 1929. The American Institute of Mining, Metallurgical, and Petroleum Engineers, 1930.

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