Phase stability of martensitic structures

被引:11
作者
Ahlers, M [1 ]
机构
[1] COMIS NACL ENERGIA ATOM,INST BALSEIRO,RA-8400 SAN CARLOS BARILO,RIO NEGRO,ARGENTINA
来源
JOURNAL DE PHYSIQUE IV | 1995年 / 5卷 / C8期
关键词
D O I
10.1051/jp4:1995808
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In the first part of the paper the relative stabilities of the different martensitic phases, mainly in Cu-Zn-Al, are compared. It is shown that the differences in enthalpy of formation between the fee type 3R or 6R and the 9R, 18R or 2H structures are above all due to a lattice distortion which reduces the energy per stacking fault, considering 9R, 18R and 2H as a basic face centered lattice into which faults are introduced on each third or second plane. In the second part the factors are discussed which are important in the relative stabilities not only between the matrix and martensite phases, but also for the equilibrium phases in the noble metal alloys. These are: i) the vibrational entropy difference Delta S, which is a functi sn mainly of electron concentration e/a. It depends little, if at all, on the special alloy system, on the deg-ree of long range order, or on temperature; ii) the stability of the average periodic lattice which is a smooth function of e/a,without any indication of nesting effects at intermediate e/a; iii) the pair interchange energies which depend strongl:y on the alloy system. They are a function of the pair distance but otherwise are structure independent. They determine most of the enthalpy of formation and simultaneously account for the long range order contribution.
引用
收藏
页码:71 / 80
页数:10
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