TY - JOUR
T1 - Morphology and crystallography of α precipitates in β Ti-Mo binary alloys
AU - Furuhara, T.
AU - Makino, T.
AU - Idei, Y.
AU - Ishigaki, H.
AU - Takada, A.
AU - Maki, T.
PY - 1998/1
Y1 - 1998/1
N2 - The morphology and crystallography of α(hcp) precipitates formed in the α(bcc) matrix were examined in the Ti-Mo binary alloys with various Mo contents below the currently proposed monotectoid temperature by means of transmission electron microscopy. In the Ti-10, 20 and 30 mass%Mo alloys, a precipitates form on β grain boundaries and grow into the interior of β grains. An α precipitate_ formed intragranularly is lath-shaped, and has the Burgers orientation relationship, ((110)β//(0001)α, [111]β//[1120]α) with respect to its β matrix. The habit plane of α lath is near {111}β. In the Ti-40 mass%Mo alloy, a fine α phase distribution, probably due to the prior β phase separation, was observed below 823 K although non-uniform α precipitation on β grain boundaries and dislocations occurs above 873 K. An α precipitate has the near-Potter orientation relationship ((011)β//(1101)α, [111]β//[1120]α), and is plate-shaped with the {013}β habit plane. The validity of the Ti-Mo phase diagram currently proposed is discussed in terms of the coherent phase separation of β phase and the equilibrium volume fraction of α phase. It is concluded that the region where β phase separation occurs should be present in the much lower temperature range than the currently proposed Ti-Mo binary phase diagram.
AB - The morphology and crystallography of α(hcp) precipitates formed in the α(bcc) matrix were examined in the Ti-Mo binary alloys with various Mo contents below the currently proposed monotectoid temperature by means of transmission electron microscopy. In the Ti-10, 20 and 30 mass%Mo alloys, a precipitates form on β grain boundaries and grow into the interior of β grains. An α precipitate_ formed intragranularly is lath-shaped, and has the Burgers orientation relationship, ((110)β//(0001)α, [111]β//[1120]α) with respect to its β matrix. The habit plane of α lath is near {111}β. In the Ti-40 mass%Mo alloy, a fine α phase distribution, probably due to the prior β phase separation, was observed below 823 K although non-uniform α precipitation on β grain boundaries and dislocations occurs above 873 K. An α precipitate has the near-Potter orientation relationship ((011)β//(1101)α, [111]β//[1120]α), and is plate-shaped with the {013}β habit plane. The validity of the Ti-Mo phase diagram currently proposed is discussed in terms of the coherent phase separation of β phase and the equilibrium volume fraction of α phase. It is concluded that the region where β phase separation occurs should be present in the much lower temperature range than the currently proposed Ti-Mo binary phase diagram.
KW - Alpha phase
KW - Beta phase
KW - Binary phase diagram
KW - Crystallography
KW - Interfacial structure
KW - Phase separation
KW - Precipitation
KW - Titanium alloy
UR - http://www.scopus.com/inward/record.url?scp=0031651394&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0031651394&partnerID=8YFLogxK
U2 - 10.2320/matertrans1989.39.31
DO - 10.2320/matertrans1989.39.31
M3 - Article
AN - SCOPUS:0031651394
SN - 0916-1821
VL - 39
SP - 31
EP - 39
JO - materials transactions, jim
JF - materials transactions, jim
IS - 1
ER -