Elsevier

Acta Materialia

Volume 55, Issue 14, August 2007, Pages 4915-4923
Acta Materialia

Precipitation twinning

https://doi.org/10.1016/j.actamat.2007.05.007Get rights and content

Abstract

The paper describes the heterogeneous nucleation of mechanical twins in a TiAl alloy containing Ti3AlC perovskite precipitates. Examination of the deformation structure by high-resolution electron microscopy has revealed that overlapping planar faults were generated at the perovskite particles. These faults can apparently easily rearrange into embryonic twins and subsequently grow into large twins. The nucleation mechanism was found to be closely associated with the misfit character and stress state of the precipitates. The structural data serves as input for the modelling of the precipitation-induced twinning process. Based on these calculations, the thickness and length of the embryonic twins can be predicted, which agree well with the experimental observations.

Introduction

Precipitation hardening is a widely applied technique for improving the high-temperature performance of intermetallic alloys. In γ(TiAl) alloys precipitation reactions are often implemented by carbon additions because the optimum dispersion can be achieved by homogenization and ageing procedures [1], [2]. Suitable particle dispersions reduce the secondary creep rate over at least one order of magnitude, when compared with the homogenized reference state. However, the attributes that are desirable for high-temperature service might be counter to low-temperature ductility and damage tolerance. TiAl alloys suffer from brittle fracture that persists up to relatively high temperatures (700–800 °C). The brittleness is mainly associated with the existence of {1 1 1} cleavage planes [3], [4] and generally low dislocation mobility [5]. A significant toughening can only be obtained by the implementation of lamellar α2(Ti3Al) + γ(TiAl) microstructures [6]. Nevertheless, for crack propagation parallel to the lamellae, i.e. parallel to the {1 1 1} planes, the fracture toughness is extremely low [7]. As in γ(TiAl) the dislocations exclusively propagate on {1 1 1} planes, immobilization of glide processes may easily lead to fracture. Any further increase in the glide resistance by precipitation hardening can therefore be extremely harmful for the fabrication and handling of the material. As described in extensive reviews [3], [8], [9], [10], [11] and detailed experimental [4], [5] and theoretical [12], [13] studies, deformation of γ(TiAl) can also be supported by mechanical twinning along 1/6112¯]{111}. Thus, this mechanism provides auxiliary slip systems and plays an important role in γ(TiAl) alloy design strategies for mitigating the problems associated with the poor damage tolerance. As with other materials, in γ(TiAl) the spontaneous formation of a large twin is difficult to envisage. Thus, separate consideration is usually given to the nucleation of a small twinned region (embryonic twin) and to its subsequent growth into a large twin [9]. While the heterogeneous twin nucleation at dislocation structures [9], [10] and internal boundaries [4], [13] of γ(TiAl) alloys is well documented, there is little information on whether precipitates may act as nucleation centres.

The goal of the paper is to present both an experimental basis and a modelling frame-work for the understanding of precipitation (induced) twinning. In the experimental part a high-resolution electron microscope study of defect structures at precipitates is reported. Here, it is shown that the observed faults can easily be rearranged into embryonic twins. The modelling part consists of the kinematics of twinning, studying the twinning shear eigenstrain in a physically adequate coordinate system. Then the stress state due to the misfit of the precipitate is investigated with the current methods of micromechanics in the same coordinate system. Finally, the thermodynamics of precipitation twinning is analysed in a similar way to that in Ref. [13] for twinning induced by distinct dislocations.

Section snippets

Experimental setting

In a Ti–48.5Al–0.36C (at.%) alloy, Ti3AlC perovskite precipitates were formed by homogenisation at 1523 K and subsequent ageing at 1023 K (see e.g. [2]). The samples were deformed in compression at room temperature to strain ε = 3%, which produced a moderate density of dislocations, fault structures and fully developed mechanical twins. For the transmission electron microscopic observations slices were sectioned perpendicular to the sample axis, so that it was a simple matter to estimate the

Definition of a precipitation-induced twin

If one inspects the atomic arrangement in Fig. 2c, one finds planar faults forming sheared bands (e.g. the area between the fourth row from the bottom marked with C and the fifth row marked with B) alternating with unsheared bands (e.g. the area between the fifth row from the bottom marked with B and the sixth row marked with C). We define a precipitation (induced) twin as a sheared band (fault) with thickness h and length ℓ. In this specific case, the thickness h corresponds to the distance d

The twinning condition

Two approaches are possible to obtain a precipitation-induced twinning condition (PITC):

  • The energy stability criterion as outlined by Petryk et al. [12], [23].

  • The thermodynamic criterion considering the twinning process as a displacive transformation with no change in the chemical free energy of the system. Such a criterion has been derived by several researchers, e.g. Fischer et al. [24] and Levitas [25]. The corresponding transformation condition (in this case the PITC) can directly be

Discussion

We have developed a thermodynamically based relation providing a twin length ˜=/a from ˜/h˜ and fix h as the distance between two atomic planes, being h = d = 0.24 nm, h˜=h/a=0.24/1.65=0.145. We now use the data available to estimate ˜ as follows:

  • The Young’s modulus of the matrix at the temperature during a thermal treatment (750 °C) is taken from Schafrik [28] as E(m) = E = 145 GPa, giving with ν = 0.25 a shear modulus μ = 58 GPa.

  • The Young’s modulus of the Ti3AlC precipitate can be taken as Ep = 240 GPa from

Conclusions

  • Ti3AlC precipitates, present in γ(TiAl) alloys, serve as heterogeneous nucleation centres for mechanical “nano-twins”.

  • The twin nucleation is supported by the significant lattice misfit between the precipitates and the TiAl matrix, which, in part, is accommodated by misfit dislocations.

  • Recombination and reaction of these misfit dislocations leads to the emission of planar faults, which may be interpreted as “embryonic” twins or “nano-twins”. However, one must be careful with these denominations

Acknowledgements

H.C. and F.D.F. appreciate the helpful discussion with Mrs. Dr. Ch. Scheu and Prof. G. Dehm, both Montanuniversität Leoben.

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