A micromechanics-inspired constitutive model
for shape-memory alloys that accounts for initiation
and saturation of phase transformation
Alex Kelly
a
, Aaron P. Stebner
b
, Kaushik Bhattacharya
a
,
n
a
Division of Engineering and Applied Science, California Institute of Technology, Pasadena, CA 91125, USA
b
Mechanical Engineering, Colorado School of Mines, Golden, CO 80401, USA
article info
Article history:
Received 29 May 2015
Received in revised form
2 February 2016
Accepted 17 February 2016
Available online 18 February 2016
Keywords:
Shape-memory alloys
Constitutive model
Phase transformation
abstract
A constitutive model to describe macroscopic elastic and transformation behaviors of
polycrystalline shape-memory alloys is formulated using an internal variable thermo-
dynamic framework. In a departure from prior phenomenological models, the proposed
model treats initiation, growth kinetics, and saturation of transformation distinctly, con-
sistent with physics revealed by recent multi-scale experiments and theoretical studies.
Specifically, the proposed approach captures the macroscopic manifestations of three
micromechanial facts, even though microstructures are not explicitly modeled: (1) In-
dividual grains with favorable orientations and stresses for transformation are the first to
nucleate martensite, and the local nucleation strain is relatively large. (2) Then, trans-
formation interfaces propagate according to growth kinetics to traverse networks of
grains, while previously formed martensite may reorient. (3) Ultimately, transformation
saturates prior to 100% completion as some unfavorably-oriented grains do not transform;
thus the total transformation strain of a polycrystal is modest relative to the initial, local
nucleation strain. The proposed formulation also accounts for tension
–
compression
asymmetry, processing anisotropy, and the distinction between stress-induced and tem-
perature-induced transformations. Consequently, the model describes thermoelastic re-
sponses of shape-memory alloys subject to complex, multi-axial thermo-mechanical
loadings. These abilities are demonstrated through detailed comparisons of simulations
with experiments.
&
2016 Elsevier Ltd. All rights reserved.
1. Introduction
Shape-memory alloys (SMAs) exhibit unusual macroscopic phenomena including superelasticity, the shape-memory effect,
and actuation. Through these behaviors, inelastic strains on the order of several percent are recovered because they are
accommodated through diffusionless, reversible microstructure rearrangement instead of slip, glide, climb, and other irre-
coverable, plastic mechanisms. These remarkable phenomena are enabled by solid-to-solid phase transformation between a
high symmetry
austenite
phase that is stable at high temperatures, and a low symmetry
martensite
phase that is stable at low
temperatures. The symmetry disparity between the phases allows multiple
variants
of the martensite phase
–
martensite
Contents lists available at
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Journal of the Mechanics and Physics of Solids
http://dx.doi.org/10.1016/j.jmps.2016.02.007
0022-5096/
&
2016 Elsevier Ltd. All rights reserved.
n
Corresponding author.
E-mail address:
bhatta@caltech.edu (K. Bhattacharya)
.
Journal of the Mechanics and Physics of Solids 97 (2016) 197
–
224
structures that are identical up to their orientation
–
to form from each austenite structure during transformation. The ability
to form variants or patterns of variants manifests an infinite number of possibilities for macroscopic strains, or shape changes,
during transformation of a polycrystal. As for a liquid
–
solid or liquid
–
gas transformation, a Clausius
–
Clapeyron relation
governs the solid-state phase transformation of SMAs. Thus, the transformation may be induced by changing temperature or
stress. The state of thermo-mechanical loading during transformation will also dictate the shape change. Furthermore, while in
the martensitic state, one variant may switch to another
–
i.e.
,
reorient
–
in response to applied forces, also resulting in
macroscopic shape changes.
Regardless of whether a given martensite structure was formed directly during transformation or via post-transfor-
mation deformation, upon reverse transformation, all variants of martensite revert back to the same initial austenite
structure, resulting in full shape recovery, or
“
shape-memory.
”
Superelasticity
describes a constant ambient temperature
event in which elastic and transformation strains induced by mechanical loading are completely recovered upon unloading.
Analogously, via
the shape-memory effect
, a SMA mechanically deformed, then unloaded below the critical transformation
temperature, while in the martensite phase, returns to its original shape upon heating to austenite.
Actuation
is achieved by
maintaining an applied load while heating and cooling through transformation; the SMA recovers transformation strain
against the load thereby producing mechanical work.
The unusual properties of SMAs have led to their use in a variety of engineering applications ranging from implantable
medical devices to actuators. We refer the reader to
Otsuka and Wayman (1998)
for a detailed introduction. The increasingly
sophisticated applications of these materials calls for a model that is capable of faithfully describing complex phenomena,
while being simple enough to be used in the engineering design process. This demand has motivated a number of models.
Some of these, like the widely used models of
Auricchio et al. (1997)
,
Auricchio and Petrini (2004)
and
Lexcellent et al.
(2002),
are phenomenological and adapt frameworks from other subjects like plasticity. Others, like the models of
Qidwai
and Lagoudas (2000)
,
Panico and Brinson (2007)
,
Sadjadpour and Bhattacharya (2007b
,
a)
, and
Chemisky et al. (2011)
in-
troduce internal variables to incorporate some microscopic information. Yet other models like those of
Zaki and Moumni
(2007)
focus on thermomechanical interactions and cyclic loadings. We refer the reader to
Chemisky et al. (2011)
for a
comprehensive survey of the literature. Despite significant advances, a phenomenological model that accurately describes
transformation initiation, growth, and saturation during multiaxial proportional and non-proportional loading remains a
work in progress, and motivates the proposed model.
We now consider superelasticity in some detail to describe the ideas of the current model. To understand the underlying
mechanisms behind this phenomenon, we first consider an ideal
single crystal
at a temperature just above its transformation
temperature. At this temperature, austenite is the stable phase and martensite the metastable phase. As the crystal is
subjected to stress, it initially responds elastically as in loading prior to point A in
Fig. 1
a. However, at some critical stress,
the martensite is stabilized (
Burkart and Read, 1953
;
James, 1986
) and the material begins to transform from austenite to
martensite. This event results in a macroscopic inelastic yield event that appears similar to perfect plasticity (A). Once the
material is fully martensite, the martensite now responds elastically on further loading to some maximum load below the
stress required for detwinning and/or plastic flow (B to C). Upon unloading, the martensite remains the stabilized phase as
long as the stress remains high and unloads elastically (C
–
E). However, at some critical stress, it becomes unstable and
begins to transform to the austenite, and this reverse transformation gives rise to the lower plateau (E to F). Once the
transformation is complete, the austenite unloads elastically.
Hysteresis results from energy dissipated during transformation. For superelasticity, it is often characterized by the
differences between the critical stresses for forward and reverse transformation. Single crystal transformation responses
differ with differing loading directions due to crystallographic anisotropy (
Miyazaki et al., 1984
;
Shield, 1995
). Specifically, a
Fig. 1.
A schematic representation of superelasticity in (a) single crystal and (a) polycrystalline specimens.
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
198
critically resolved stress criterion adequately describes the single crystal anisotropy of transformation (
Miyazaki et al., 1984
;
Shield, 1995
). Asymmetries with respect to loading mode (
e.g.
, tension vs. compression) and the deformation mechanisms
are broadly explained by considering the Gibbs energy, and more specifically the Clausius
–
Clapeyron relation between the
critical stress for transformation, the strain of transformation, and temperature (
Burkart and Read, 1953
;
James, 1986
).
The situation is considerably more complicated in a
polycrystal
. The transformation strains, microstructures, and re-
sponses to the applied stress of the grains all depend on their orientation. Thus unique grains attempt to deform uniquely.
However, they are not free to do so due to intergranular constraints. Therefore transformation is a complex composite
process in a polycrystal; the subject of many recent experimental and theoretical investigations (see for example,
Sitter
et al., 2010
;
Stebner et al., 2013
). Furthermore, the quantified characteristics of superelastic responses vary significantly with
material, processing, and loading mode. Non-proportional loading provides further complexities (
Thamburaja and Anand,
2002
;
McNaney et al., 2003
;
Richards et al., 2013
). The models we previously mentioned each focus on certain aspects of
these phenomena with varying levels of complexity and fidelity, but an engineering demand for a simple, unified framework
that describes all of these observations still exists.
To understand how the present model aims to address this demand, we now consider a polycrystal completely in the
austenite state, above its transformation temperature, subjected to increasing tensile stress. A characteristic polycrystal su-
perelastic stress
–
strain curve in this circumstance is shown in
Fig. 1
b. The material initially loads elastically, then yields to
transformation at the point marked A, macroscopically similar to the single crystal case. The stress in the polycrystal is largely
uniform during elastic loading except as a result of the elastic anisotropy of the austenite. Thus, if we were to ignore the latter,
the first grains that will transform are those most favorably oriented for transformation according to a resolved stress criterion,
as observed in recent neutron diffraction experiments by
Stebner et al. (2015)
. Using in-situ optical microscopy,
Brinson et al.
(2004)
have also observed that the first appearance of the martensite occurs in isolated regions in well-oriented grains. This
finding is also supported by the mesoscale observations of
Daly et al. (2008)
that deviations in linearity of the stress
–
strain
curve occurs well before the formation of macroscopic transformed regions.
Bhattacharya and Schlömerkemper (2010)
have
recently proved in an idealized setting with uniform modulus that the transformation begins in isolated grains, while Richards
et al. have made the same observation using a full-field micromechanical model (
Richards et al., 2013
). Finally,
Sittner and
Novak (2000)
have noted that the constant stress Sachs or Ruess bound accurately describes the initiation of the transformation
in polycrystals. In summary, transformation
initiation
is governed by well-oriented grains.
Transformation growth kinetics, however, are not. As the best oriented grains begin to transform, whole grains cannot
due to the constraints of the neighbors and the transformation proceeds in isolated regions (
Richards et al., 2013
). Thus, the
internal stress distribution amongst grains becomes extremely heterogeneous as stress is redistributed from ideally oriented
grains where transformation has nucleated to slightly misoriented grains, which subsequently nucleate (
Richards et al.,
2013
;
Paranjape and Anderson, 2014
). These events cause a rapid progression of the transformation within the polycrystal.
This progression is further accelerated by the fact that once transformation has nucleated in a grain, little additional driving
force is needed for martensite growth. Additionally, stress redistribution may change the stress orientation within trans-
formed grains, and these events will cause martensite variants other than those initially formed to be preferred (
Stebner
et al., 2015
). The activity of these mechanisms in tandem gives rise to the stress
–
strain plateau AB.
Macroscopically, single and polycrystal superelasticity have appeared very similar up to point B. However, in loading
beyond the plateau (BC), polycrystals exhibit pronounced hardening (
Fig. 1
b) where most single crystals do not (
Fig. 1
a). In
polycrystals loaded to point B (
Fig. 1
b), transformation is incomplete or non-existent in some of the most poorly oriented
grains. Further transformation in these grains requires increased stress, while grains that have completed transformation
begin to elastically load again. Twinning events are also incited that reorient martensite to a greater extent than in the
plateau region (
Stebner et al., 2015
). All of these mechanisms in combination give rise to the observed hardening BC. As a
result, the transformation of the polycrystal is quite heterogeneous (
Brinson et al., 2004
;
Daly et al., 2008
;
Richards et al.,
2013
;
Stebner et al., 2015
;
Paranjape and Anderson, 2014
), as is the state of internal stress (
Pelton et al., 2015
). As trans-
formation and reorientation proceed, the poorly oriented grains exhibit smaller transformation strain in the direction of
loading, and thus they begin to saturate and lock together eventually leading to a network of fully transformed grains
surrounded by partially transformed and untransformed grains at C (
Brinson et al., 2004
). Thus, the
saturation
of the
transformation is governed by the poorly oriented grains. This phenomenon is also the reason why the constant strain Taylor
or Voigt bound gives a good description of the macroscopic transformation strains (
Bhattacharya and Kohn, 1997
;
Shu and
Bhattacharya, 1998
;
Bhattacharya and Suquet, 2005
).
Forward loading is continued until some maximum load is reached at point C; further loading evokes plasticity, which is
beyond the scope of the current model. Upon unloading, the material initially unloads elastically. However, at some point,
marked D, the material begins to recover its inelastic strain, initially with some softening and then (point E) perfectly. Upon
the recovery of all inelastic strain, at point F, the material unloads elastically.
An interesting consequence of the fact that the initiation and saturation of the martensitic transformation in polycrystals
are governed by two separate mechanisms is that the critically resolved shear stress criterion or the stress
–
strain aspect of
the Clausius
–
Clapeyron relation fails in a polycrystal after the very first initiation(s) of transformation (
Daly et al., 2007
). The
key heuristic and the point of departure
for the current work is the explicit recognition that the mechanics of initiation and
saturation of the martensitic transformation in polycrystals are two essentially different processes. Therefore, we differ-
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
199
entiate between two separate kinematic quantities, the nominal transformation strain in the martensite and the effective
transformation strain of the polycrystal. The former heuristically represents the macroscopic transformation strain one
would see if the grains were allowed to transform independently. This quantity governs the initiation of transformation. The
latter heuristically represents the transformation strain one actually sees limited by intergranular constraints. This quantity
governs the saturation of the transformation. We will see that the reorientation of both stress-induced and thermally
stabilized martensite arises naturally due to competition between these mechanisms. While, for simplicity, the introduction
above focused on superelasticity and stress-induced martensite, the model we present is thermomechanical and also
capable of describing thermal transformations and the resulting shape-memory effect and actuation phenomena.
The present model builds on the framework developed by
Sadjadpour and Bhattacharya (2007b
,
a)
. Their work, like other
internal variable models in the literature, did not distinguish between initiation and saturation mechanisms. The current
work does, and also differs by adopting a new formulation for transformation surfaces that follows from a formula in-
troduced by
Cazacu et al. (2006)
to describe anisotropic and asymmetric plastic yield surfaces; this change improves the
ability to capture transformation asymmetry and processing-induced material anisotropy of SMAs. The present model has
similarities to those of
Panico and Brinson (2007)
and
Chemisky et al. (2011)
. Those models make a distinction between self-
accommodated and oriented martensite, hence they capture some of the features describe above. However, they do not
completely describe the difference between initiation and saturation.
The kinetics of transformation and reorientation in the model we present are rate-independent. Relative to the slow
loading rates of typical engineering applications (10
2
s
1
and below), these kinetics are largely rate independent
(
Abeyaratne et al., 1996
). Macroscopic rate effects are often seen, but these are often the consequence of the release of latent
heat, which is not inherent to the kinetics. In the present model, apparent rate effects due to thermal energy enter naturally
via the energy balance. On occasion, rate effects are also introduced due to grips, work hardened alloys, etc., but these are
small and are the result of particular circumstances that we do not address in this work. We note, however, that inherent
rate effects are important in dynamic situations, and the model can easily be modified to account for these if necessary (for
example as in
Sadjadpour and Bhattacharya, 2007b
,
a
).
Finally, some (highly worked) specimens of nickel
–
titanium based SMAs (a.k.a.
“
Nitinol
”
) display R-phase, an inter-
mediate phase that forms in between the austenite and martensite phases during thermal cycling (
Otsuka and Wayman,
1998
,
Duerig and Bhattacharya, 2015
). This phase has a small transformation strain and only appears in engineering ap-
plications with very particular processing and thermomechanical loading conditions. We ignore the R-phase in this model.
We proceed to introduce the model in
Section 2
, analytically demonstrate some features of the model in simplified
settings in
Section 3
, discuss our numerical implementation in
Section 4
, and conduct a parameter study while also
demonstrating the model relative to experimental data in
Section 5
. We conclude with a discussion of desirable future work
with the framework in
Section 6
.
2. Continuum model
2.1. Kinematics
Consider a macroscopic polycrystalline specimen of a shape-memory alloy, so that each material point corresponds to a
representative volume of material with numerous austenite grains, with possible fine-scale martensite microstructure
within each grain. We denote the macroscopic strain as
ε
and the (absolute) temperature as
θ
.Asin
Sadjadpour and
Bhattacharya (2007b)
, we introduce two additional internal variables that describe the state of transformation. The first is
the
volume fraction
of the martensite
λ
. By definition, this variable satisfies the constraint
λ
≤≤
()
01.
1
The second is the
nominal transformation strain
of the martensite
ε
m
, which we define as the average transformation strain
of every region of martensite in every grain in the representative volume. We will assume that
ε
∈
()
2
mi
.
where
i
.
describes the set of all possible nominal transformation strains that may occur. This set could be computed by
taking averages of local martensite strains over all variants in the representative volume, however we prescribe this phe-
nomenologically in the next section. In subsequent sections of the model formulation,
ε
m
will dictate the driving force on
transformation and the set
i
.
will define initiation events. The overall or
effective transformation strain
is obtained by
multiplying the nominal transformation strain with the volume fraction,
λ
ε
m
. This overall transformation strain drives
macroscopic behaviors governed by inter-granular compatibility; thus
λ
ε
m
will play a critical role in saturation. We define a
set
s
.
that describes the set of effective transformation strains that may be achieved without hardening/softening influence
from poorly oriented grains in forward/reverse transformation events. The effective transformation strain may take on
values outside of this set with some energy penalty, as mathematically prescribed in the next section.
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
200
2.2. Energy
The Helmholtz free energy density of the system is postulated to be of the form
⎛
⎝
⎜
⎞
⎠
⎟
( )()()
()
εελθελελελελ
θθ
θ
λθ
θ
θ
λελελ
=−
()− +
(− )
−()
+ ()+
+()
()
λ
WLcGGG
,,,
1
2
:C :
ln
.
3
mmm
c
c
p
c
im
s m
The first term is the elastic energy density, which depends quadratically on the elastic strain, i.e., the difference between the
total strain and the effective transformation strain. The second term represents the excess chemical energy density of
martensite which depends on temperature. Note that we have chosen to restrict the model to a moderate range of tem-
peratures close to the thermodynamic transformation temperature
θ
c
where this relation may be taken as linear, scaling
with the latent heat of transformation,
L
, relative to the difference between the absolute temperature and the thermo-
dynamic transformation temperature. The third term is the contribution of heat capacity
c
p
. Each phase of the material may
exhibit a unique heat capacity as well as a unique tensor of bulk elastic constants,
C
, thus we adopt a rule of mixtures
approach in defining the composite responses of the two phases at a material point
1
λλλ
()=
+( − )
()
CC1C,
4
MA
λλλ
()=
+( − )
()
cc
c
1,
5
pp
M
p
A
where the superscripts
A
and
M
denote austenite and martensite phase properties, respectively.
The last three terms in the energy
G
i
,
G
s
,and
λ
G
describe the energy densities for initiation, saturation, and growth of
transformation, respectively. Specifically,
λ
G
reflects internal stored energy related to i
ncompatibility between variants and across
grains; i.e., the barrier to transformation growth. Thus, in a manner analogous to hardening in plasticity, we postulate that
2
⎧
⎨
⎪
⎩
⎪
ξ
ξξξ
()=
()=
+
∈[
]
+∞
()
λ
λ
λλ
λλ
+
λλ
G
g
f
n
1
0, 1
else
6
n
1
where
>>
λλ
λλ
fn
0,
0
are constitutive constants. The first line accounts for the fact that the amount of stored energy in the
system can increase with increasing volume fraction due to
the development of internal
stresses, thus for choices of
≠
λλ
f
0
,
λ
experiences some hardening within the set [0,1]. The second line enforces the hard constraint
(1)
.
The functions
α
G
for
α
=
is
,
are defined over symmetric matrices. To prescribe the sets of nominal and effective trans-
formation strains, we introduce functions of the form
α
g
following
Cazacu et al. (2006)
:
⎛
⎝
⎜
⎜
⎞
⎠
⎟
⎟
()
∑
ξμξμξ
()=
(
) −
(
)
−
()
α
αααα
=
α
α
gab
::
7
n
nn
a
a
1
3
1
2
2
**
where
ξ
is any symmetric matrix,
μ
ξ
(
̃
)=
n
,1,2,
3
n
denote the principal values of the matrix argument
ξ
̃
,
α
*
are 4th order
tensors satisfying minor and major symmetries and reflecting the anisotropy of the material (choosing
=
α
*
0
where
0
is the
4th order identity tensor results in isotropy) and
ααα
aab
,,
12
are constitutive constants to be prescribed. We assume that
−<
<
>
>
ααα
aab
11,1,
0
12
to ensure the convexity and coercivity of
α
g
.
We postulate
⎧
⎨
⎩
ξ
ξ
()=
∈
+∞
()
G
0
else.
8
i
i
.
where the set of allowable initiation strains is taken as
3
ξξξ
={
( )=
( )≤ }
()
g
:tr 0,
0 .
9
i
i
.
Eq.
(8)
enforces the constraint
(2)
. The martensite strain may evolve freely with no energy cost within the set
i
.
, but
evolution outside of this set is not allowed. We can also give physical meaning to the coefficients in
(7)
. The coefficient
b
i
denotes some radius of the set
i
.
while the constants
a
i
1
and
a
i
2
control asymmetry in the same way the coefficients
k
and
a
do in the formulation of Cazacu et al. (see Fig. 4 of
Cazacu et al., 2006
).
We note that the expressions
(7)
are different from the polynomials of the invariants
J
2
and
J
3
used in
Sadjadpour and
Bhattacharya (2007a)
. We found that these formulae restricted the amount of asymmetry that one could prescribe before
1
We assume that the bulk moduli of the phases (under hydrostatic stress) are equal consistent with experimental observations of SMAs (
Patel and
Cohen, 1953
).
2
We introduce a notation where
ξ
is generically used to represent the argument of the functions; i.e., it is a placeholder for the internal variables of the
model defined in
(3)
.
3
We clarify that the colon in
ξ
ξ
(
)
:tr
reads
“
ξ
such that the trace of
ξ
,
”
where in
(7)
the colon denotes the contraction of the fourth and second order
tensors. Despite the ambiguity, both uses of the colon are obvious in their context.
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
201
the sets of allowable strains became non-convex, especially in anisotropic media. This limitation proved unsatisfactory for
highly textured SMA polycrystals. In contrast,
(7)
enabled greater asymmetries of convex sets, especially for anisotropic
media (
Cazacu et al., 2006
).
Recall that for saturation, the effect of incompatibility between variants and grains means that continued transformation
strain requires internal stresses and additional stored energy. Thus, unlike the previous hard constraints on the allowable
values of volume fraction and martensite strains, we postulate a soft constraint for saturation such that kinematic hardening
occurs once the allowable set of effective transformation saturation strains is exceeded:
⎧
⎨
⎪
⎪
⎩
⎪
⎪
⎛
⎝
⎜
⎜
⎛
⎝
⎜
⎞
⎠
⎟
⎞
⎠
⎟
⎟
ξ
ξξ
ξ
ξξ
ξ
()=
()≤
()=
()
()>
()=
+∞
( ) ≠
()
G
g
k
g
b
g
00,tr0
ln
0, tr
0
tr
0
10
s
s
s
s
s
a
m
s
s
s
2
where
k
s
and
m
s
are the saturation hardening coefficient and exponent, respectively. The function
G
s
¼
0 on the set
ξξξ
={
( )=
( )≤ }⊂
()
g
:tr 0,
0
11
s
s
i
..
where the final inequality is enforced by the choice of constants
b
a
,
ss
1
, and
a
s
2
, which have analogous interpretation as their
initiation counterparts.
Finally, we assume the usual Fourier law for heat conduction, which is a linear relation between heat flux
q
and tem-
perature gradient according to the thermal conductivity,
K
θ
=− ∇
()
qK
.
12
2.3. Balance laws, driving forces and kinetics
We postulate the usual balance laws for equilibrium and energy as well as the second law of thermodynamics (Clausius
–
Duhem inequality)
σσσ
+=
=
()
b
div
0,
,
13
T
σε
ε
̇
=
̇
−∇· +
()
qr
:,
14
⎜⎟
⎛
⎝
⎞
⎠
η
θθ
̇
≥∇· −
+
()
qr
15
where
s
is the stress,
b
is the body force,
ε
is the internal energy density,
η
is the entropy density,
θ
is the absolute
temperature,
q
is the heat flux and
r
is the radiative heating.
With the free energy density specified in
(3)
, we can use the balance laws and arguments following
Coleman and Noll
(1963)
to obtain constitutive relations for the stress (
s
) and entropy (
η
):
σ
ε
λελε
=
∂
∂
=()(− )
()
W
C:
,
16
m
⎛
⎝
⎜
⎜
⎛
⎝
⎜
⎞
⎠
⎟
⎞
⎠
⎟
⎟
η
θ
λ
θ
θ
θ
=−
∂
∂
=−
+
+
()
WL
c
1ln .
17
c
p
0
We also obtain the following driving forces as the thermodynamic conjugates to the internal variables
λ
and
ε
m
. This is a
little tricky since the function
G
α
are not smooth. However, it is first instructive to assume that the functions
λ
G
is
,,
are
smooth. In such situations,
⎛
⎝
⎜
⎞
⎠
⎟
λ
ελε
λ
ελε
λ
θ
θ
θ
σε
θθ
θ
εε
ξξ
=−
∂
∂
=− ( −
)
∂
∂
(−
)+
+
−
(− )
−()−
∂
∂
−
∂
∂
()
λ
λε
λ
λ
d
W
dc
d
LG
GG
1
2
:
C
:ln:
:,
18
mm
p
c
m
c
c
im
m
s
m
ε
λσλ
ξ
λ
ξ
=−
∂
∂
=−
∂
∂
−
∂
∂
()
ε
ελε
d
W
GG
.
19
m
is
m
mm
In the non-smooth situation, we interpret these equations using usual methods of convex analysis (
Ekeland and Témam,
1999
) as follows
⎛
⎝
⎜
⎞
⎠
⎟
ελε
λ
ελε
λ
θ
θ
θ
σε
θθ
θ
εελελ
−−(− )
∂
∂
(−
)+
+
−
(− )
−()∈ ∂( )+∂()
()
λ
λ
d
dc
d
LG
GG
1
2
:
C
:ln:
:,
20
mm
p
c
m
c
c
im
m s m
λσλελλε
− +
∈∂( )+∂ ( )
()
ε
dGG
21
dev
im
s m
m
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
202
where
σσ
=−
σ
I
dev
tr
3
and
∂
α
G
denotes the sub-differential of the
G
α
.
To close the system, we relate the driving forces to the relevant rates using kinetic relations. In the rate-dependent
smooth setting, we postulate
λε
̇
=()
̇
=()
()
λλε
Kd
K d
,
22
mm
m
for given functions
K
m
and
K
λ
. However, in this paper, we are interested in the rate-independent case where
λ
and
ε
m
evolve
freely if and only if the corresponding driving forces reach a critical value. Therefore, the functions
λ
K
and
K
m
are neither
smooth or invertible. So, we specify them in the form of Kuhn
–
Tucker conditions. The rate of change of the internal variables
are constitutive functions of the driving forces such that transformation evolves according to:
λλλ
̇
=||<
̇
≥||≤
≤≤
()
λλλλλ
dd d
dd
0for
,
0,
if0
1
23
cc
and martensite strain:
ε
λλ
ε
λ
ε
̇
=<
̇
≥≤∈
()
dd d
dd
0for
1
,
1
:0,
1
if
;
24
mmm
c
mm
m
m
c
mi
.
ελθ
==≥
()
A
Reset
0 when 0,
25
mf
where
λ
d
c
is the critical driving force for transformation and
d
m
c
is the critical driving force for martensite variant reor-
ientation. We may rewrite these conditions by introducing a dissipation potential
λελλελε
(
̇
̇
)= |
̇
|+
|
̇
|= (
̇
)+
(
̇
)
()
λλ
DddDD
,.
26
m
c
m
c
mmm
Now kinetic equations may be rewritten as
∈∂
∈∂
()
λλε
dDd D
,
27
m
m
subject to the reset condition
(25)
.
Combining
(27)
with
(20)
and
(21)
, we can write the evolution equations for
λ
,
ε
m
as
⎛
⎝
⎜
⎞
⎠
⎟
ελε
λ
ελε
λ
θ
θ
θ
σε
θθ
θ
εελελε
∈(− )
∂
∂
(−
)+
−
+
(− )
+
( )+
∂ (
)+∂ ( )+∂ (
̇
)
()
λ
dc
d
LG GGD
0
1
2
:
C
:ln:
:
,
28
mm
p
c
m
c
c
im
m s m
mm
λσλελλελ
∈−
+∂( )+∂ ( )+∂ (
̇
)
()
λ
GGD
0
29
dev
im
s m
subject to the reset condition
(25)
.
We will further discuss the interpretation of these conditions through specific analytic examples of shape memory
behaviors in
Section 3
, and their numerical implementation in
Section 4
. For now, we note that these equations are con-
sistent with the variational structure
∈∂ +∂
WD
0
(
Mielke, 2005
;
Yang et al., 2006
).
Finally, since
θ
η
ε=
+
W
we can use
(3)
,
(12)
, and
(17)
to rewrite the energy balance
(14)
as
θθ
θ
θ
λλε
̇
=∇· ∇ + +
̇
+
̇
+
̇
()
λε
cKr
L
dd
:.
30
p
c
m
m
In summary, the model specifies that the behavior of SMAs is governed by the equilibrium equation
(13)
, the heat
equation
(30)
and the evolution equations
(28)
and
(29)
.
3. Some features of the model
We now demonstrate some of the relationships between the parameters and mechanisms of the model through analytic
calculations. To enable these analyses, we make a number of assumptions: we assume that the elastic moduli of the two
phases
==
C
C
C
AM
are equal and isotropic and the specific heat of the two phases
==
cc c
p
A
p
M
p
are equal. We also assume
that the exponent
m
s
in the definition of
G
s
is infinite so that it becomes the hard constraint
⎧
⎨
⎩
ξ
ξξξξ
()=
∈={ ()=
()≤}
+∞
()
G
g
0:tr0,0.
else.
31
s
i
s
.
We also ignore the critical driving force for martensite reorientation (
=
d
0
m
c
). Finally, except for actuation in Section 3.1.3,
we assume that
=
λλ
f
0
in
(6)
so that
λ
may evolve freely within the interval [0, 1].
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
203
3.1. One dimension
It is instructive to specialize the model to one dimension. We can derive this one-dimensional model from the three
dimensional formulation by assuming uniaxial loading; we reserve this formal derivation for
Section 3.3
. For now, we simply
assume
⎛
⎝
⎜
⎞
⎠
⎟
()
()
()
εελθελελωθθ
θ
θ
λελελ
=−+ −
+()+ +()
()
WcGGG
,,,
1
2
Eln
,
32
mmpimsm
2
0
where
ωθ
θθ
θ
()=
(− )
()
L
33
c
c
and the sets
i
s
,
.
reduce to the scalar intervals
εεεεεε
=[]≤≤≤
()
,,
.
34
is
is
c
is
t
i
c
s
c
s
t
i
t
,,,
.
The constraints that these choices impose on the kinematic variables
λ
and
ε
m
are shown in
Fig. 2
(a).
3.1.1. Superelasticity
Consider an isothermal strain-controlled experiment where the temperature is held constant at a value significantly
higher than the transformation temperature so that
ωθ
()>
>
λ
d
0
c
. Consider the specimen at rest at zero stress so that it is in
the austenite state with
λ
=
0
and
ε
=
0
m
. Now subject the specimen to a monotonically increasing overall tensile strain
ε
(
)
t
.
For very small times, the stress is given by
σε
()= (
)
tt
E
. Since this stress is positive, the nominal transformation strain
ε
m
takes its maximal tensile value
ε
i
t
. This is marked as the point
+
0
in
Fig. 2
a. Following
(18)
, the driving force for transfor-
mation in one-dimension is given by
εεω
=−
λ
d
E
i
t
, and is initially negative. However, since
λ
is already zero, it can not
decrease any further. Thus the volume-fraction remains zero and the stress increases proportional to the imposed strain
according to E, and we begin to traverse from 0
þ
/0 toward the points marked 1 in
Fig. 2
a/b.
As the applied strain increases, so do the stress and the driving force
d
λ
till the latter becomes positive and eventually
reaches the value
λ
d
c
(i.e.,
εεω
−=
λ
d
E
i
t
c
) at the points marked 1 in the figure. At this point, the strain and stress are given as
ε
ω
ε
σ
ω
ε
=
+
=
+
()
λλ
dd
E
,.
35
MS
t
c
i
t
MS
t
c
i
t
Now transformation begins and proceeds in such a manner to keep
d
λ
constant and consequently the stress
s
constant so
that the material traverses from the points marked 1 towards 2 with increasing applied strain. As
λ
increases, the overall
transformation strain
λ
ε
m
increases and eventually saturates the constraint
λ
εε
≤
ms
t
at the value
Fig. 2.
The kinematic variables and stress-induced martensite in one dimension. (a) The volume fraction and nominal transformation strain are constrained
to lie in the shaded region. (b) The stress
–
strain curve.
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
204
λ
ε
ε
=
()
.
36
t
s
t
i
t
This is indicated by the points 2 in the figure, where
ε
ω
ε
εσ
ω
ε
=
+
+=
+
()
λλ
dd
E
,.
37
MF
t
c
i
t
s
t
MF
t
c
i
t
The transformation is now saturated, and further loading does not lead to any further transformation. Thus, the stress
increases in an affine manner with applied strain and the material traverses towards the points 3 in the figure.
The specimen is then unloaded by monotonically decreasing the applied tensile strain. The transformation is initially
constant, with no change, and the material unloads elastically, traversing towards the points 4 in the figure. The stress and
the driving force decrease monotonically, till the latter becomes negative and eventually reaches the value
−
λ
d
c
at points 4.
Here,
ε
ω
ε
εσ
ω
ε
=
−+
+=
−+
()
λλ
dd
E
,.
38
AS
t
c
i
t
s
t
AS
t
c
i
t
Reverse transformation now begins at points 4 and
λ
decreases as unloading proceeds. The driving force and stress remain
constant from points 4 to 5. The reverse transformation is complete at points 5 when
λ
=
0
, and
ε
ω
ε
σ
ω
ε
=
−+
=
−+
()
λλ
dd
E
,.
39
AF
t
c
i
t
AF
t
c
i
t
The material subsequently unloads elastically and the material returns to the origins.
We have an analogous situation in a compressive loading cycle with the analogous quantities obtained by replacing the
superscripts
t
with
c
in the formulae
(35)
–
(39)
above.
A series of comments are in order. First note that the material parameters
ε
i
t
c
,
associated with the set of nominal
transformation strains determine the initiation of transformation (c.f.
(35)
) while the material parameters
ε
s
t
c
,
associated
with the set of effective transformation strains determine the extent of transformation (c.f.
(37)
). This justifies the subscript
i
for initiation for the former and the subscript
s
for saturation for the latter. More importantly, the parameters determining
initiation and saturation are independently prescribed in this model.
Second and related, we can infer the values of transformation strain, the stress hysteresis and mean-value of stress to be
εεεεεε
σσσσσ
ε
σσσσσ
ω
ε
≔( −
+
− )=
≔( +
−
− )=
≔( +
+
+ )=
()
λ
d
1
2
,
1
2
2
,
1
4
.
40
trans
tc
MF
tc
MS
tc
AS
tc
AF
tc
s
tc
hyst
tc
MS
tc
MF
tc
AF
tc
AS
tc
c
i
tc
tc
MS
tc
MF
tc
AF
tc
AS
tc
i
tc
,,,,,,
,
,,,,
,
, ,,,,
,
Note that each of them can be independently constitutively prescribed
–
the transformation strains are determined by the
parameters
ε
s
t
c
,
, the hysteresis by the parameter
λ
d
c
and the mean-value of the stress by
ε
i
t
c
,
, and there is no universal relation
amongst them.
Third, tension and compression are different due to the difference in parameters with superscript
t
and superscript
c
.
This tension-compression asymmetry is consistent with various observations going back to
Burkart and Read (1953)
.
Fourth, note that the transformation from austenite to martensite does not go to completion, but saturates at a maximum
volume fraction of
λ
εε
=
/
tc
i
tc
s
t
c
,
,
,
. This is consistent with surface observations of
Brinson et al. (2004)
, which have been
recently affirmed to be a bulk phenomena by
Stebner et al. (2015)
.
Fifth, the value of stress at which the transformation begins and completes or the reverse transformation begins and
completes depend on temperature through
ω
.If
ω
depends linearly in temperature as in
(33)
, then these stresses depend
linearly on temperature consistent with the Clausius
–
Clapeyron relation (
Otsuka and Wayman, 1998
). Further, we can invert
these relations to obtain the values of temperature where the transformation begins at zero stress:
θθ
==−
==+
()
λλ
MM
d
L
AA
d
L
,.
41
sfc
c
sfc
c
Sixth, we see above that
σσ
=
MS
tc
MF
tc
,,
,
σσ
=
AS
tc
AF
t
c
,,
and
M
s
¼
M
f
. These are all manifestations of the aforementioned assumptions.
There is no reorientation of martensite because we have assumed one dimension. We shall see in
Section 3.2
that reor-
ientation of martensite can give rise to a situation where
σσσσ
<>
,
MS
tc
MF
tc
AS
tc
AF
t
c
,,,,
. Here, we have also assumed hard constraints
on the sets
(34)
and that
=
λλ
f
0
. The more general assumption or soft constraint
(10)
on
G
s
allows the transformation to
continue to evolve to higher volume fractions with increasing stress so that
σσσσ
<>
,
MS
tc
MF
tc
AS
tc
AF
t
c
,,,,
. Setting
>
λλ
f
0
violates all
three equalities
(40)
. We will study these other choices extensively in Section
5
. We also assume rate-independent kinetics
(23)
and
(24)
. Rate-dependent kinetics would also violate all three inequalities
(40)
, as was examined by
Sadjadpour and
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
205
Bhattacharya (2007b)
. Finally, we have assumed isothermal conditions. Most experiments are not isothermal since the
transformation from austenite to martensite is exothermic through the release of the latent heat. We can estimate the
hardening in the other extremity of adiabatic conditions (
==
qr
0
) following
Sadjadpour and Bhattacharya (2007b)
. Under
our constitutive assumption and the additional assumption that the dissipation due to kinetics is small compared to latent
heat,
(30)
reduces to
θ
θ
θλ
̇
=
̇
()
c
L
.
42
p
c
We can integrate this from time
t
1
to
t
2
to obtain
⎛
⎝
⎜
⎜
⎞
⎠
⎟
⎟
θ
θ
λλ
θ
()
()
=
(( )− ( ))
()
t
t
Lt
t
c
exp
,
43
pc
2
1
21
or the temperature increases with advancing transformation. Returning now to the loading-unloading cycle under tension,
the volume fraction is initially zero and the temperature is
θ
0
. As we begin loading from the austenite, the temperature
remains constant and things remain unchanged from before till we begin transformation. Thus, as before,
σ
ε
θθ
θε
=+
(−)
()
λ
dL
.
44
MS
t
c
i
t
c
ci
t
0
As transformation proceeds, the temperature rises. However, the driving force has to remain at the critical value
d
c
λ
, and
thus,
⎛
⎝
⎜
⎜
⎛
⎝
⎜
⎜
⎞
⎠
⎟
⎟
⎞
⎠
⎟
⎟
σε
θ
θθσ
εε
θ
θ
λ
() − ( ()− )=
⇒ ()=
+
()
−
λ
λ
t
L
tdt
d
LLt
c
exp
1 .
i
t
c
c
c
c
i
t
i
t
cp
0
The transformation saturates at
λ
λ
=
t
c
,
given in
(36)
; here,
⎛
⎝
⎜
⎜
⎛
⎝
⎜
⎜
⎞
⎠
⎟
⎟
⎞
⎠
⎟
⎟
σ
εε
θ
θ
λ
θ
=+
−
()
λ
d
LL
c
exp
1 .
45
MF
t
c
i
t
i
t
c
t
cp
0
Thus, hardening due to latent heat of transformation that would occur under adiabatic conditions is given by
⎛
⎝
⎜
⎜
⎛
⎝
⎜
⎜
⎞
⎠
⎟
⎟
⎞
⎠
⎟
⎟
σσ
θ
θε
λ
θ
−=
−
()
L
L
c
exp
1 .
46
MF
tc
MS
tc
c
i
tc
tc
cp
,,
0
,
,
3.1.2. Shape-memory effect
We now subject our one dimensional specimen to a controlled (infinitely slow) temperature-load cycle to explore the
shape-memory effect. We begin as before with an unloaded specimen at a temperature above
A
f
with
λ
=
0
and
ε
=
0
m
. This
Fig. 3.
Shape-memory effect in one dimension. (a) Stress
–
strain
–
temperature curve and (b) the volume fraction-nominal transformation strain space.
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
206
is marked as the points 1 in
Fig. 3
. We lower the temperature below
M
s
and
M
f
so that the material transforms to martensite
and
λ
=
1
at points 2. We now keep the temperature constant and subject the material to a strain controlled loading un-
loading cycle. The moment that strain, and consequently the stress becomes positive, the nominal transformation strain
ε
m
takes the value
ε
i
t
to optimize the energy and the material traverses from points 2 to points 3 in the figure. Now, the effective
transformation strain is the saturation transformation strain
ε
t
s
. Note that in
Fig. 3
, this event happens at a value of stress
equal to
=
d
0
m
c
; non-zero values would raise the stress of the martensite reorientation plateau. Further loading takes the
material to points 4, and unloading brings it to 5 (which coincides with 3 in the stress
–
strain
–
temperature space). We now
keep the stress zero and heat the specimen. There is no change in strain or transformation as the material traverses from
points 5 to 6. At points 6, the temperature has reached
A
s
so that
ω
==
λλ
−
dd
and the reverse transformation begins. As the
material traverses from points 6 to points 7, the volume fraction goes from
λ
=
1
to
λ
]
=
0
. Once it reaches zero, the
ε
m
resets
to 0 and the material is in the state indicated by points 8 in the figure. Further heating brings the material back to the
starting points 1.
Note that in the thermal cycle, there is no restriction on the amount of transformation, and the specimen is able to
transform fully to martensite. Further, rate and heat transfer effects would make the curves rounded.
3.1.3. Actuation
We now examine the behavior of the model for actuation by studying a constant stress, temperature cycle. In this
subsection, we assume
>
d
0
m
c
and
>
λλ
f
0
. This changes the transformation temperatures to
θ
θ
=−
()
λ
M
d
L
,
47
sc
c
c
θ
θ
=−
(+ )
()
λ
λλ
M
df
L
,
48
fc
c
c
θ
θ
=+
(− )
()
λ
λλ
A
df
L
,
49
sc
c
c
θ
θ
=+
()
λ
A
d
L
.
50
fc
c
c
instead of
(41)
.
Consider a material at a temperature
θ
0
well below
M
f
with self-accommodated martensite at the points marked 0 in
Fig. 4
. We begin to apply a uniaxial stress to the material. As soon as it reaches the value
σσ
==
()
d
,
51
mm
c
the martensite reorients and the martensite strain
ε
m
jumps from zero to the value
ε
s
t
, i.e., to the points 1 in the figure. Since
λ
=
1
, this is also the value of the effective transformation strain. We continue to increase the stress and
ε
m
remains at
ε
s
t
until the material reaches a final stress
s
at points 2 in the figure. The value of the strain at this point is
Fig. 4.
Actuation effect in one dimension. (a) The volume fraction-nominal transformation strain space. (b) Strain (black solid) and volume fraction (red d
ashed)
as a function of temperature. (For interpretation of the references to color in this figure caption, the reader is referred to the web version of this pa
per.)
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
207
εεε
σ
==+
()
E
52
s
t
hi
We now begin to heat the material. The driving force for transformation
(19)
is given by
σε
θθ
θ
=−
(− )
−
()
λ
λλ
dL f
.
53
s
t
c
c
This force is initially positive but eventually becomes negative and reaches the critical value
−
λ
d
c
when the temperature
reaches
()
σθ
θ
σε
()= +
−
+
()
λ
λλ
A
L
df
54
sc
c
c
ms
t
and the material reaches points 3 in
Fig. 4
. The martensite now begins to convert to austenite,
λ
begins to decrease as
temperature increases and the material traverses from points 3 to 4 in the figure. Note that since the stress is still above
s
m
,
the nominal transformation strain
ε
m
increases to maintain the constraint
λ
εε
=
ms
t
. However, notice that the strain remains
at the value
ε
h
i
in
(52)
.
4
The driving force is
σε
λ
θθ
θ
λ
=−
(− )
−
()
λ
λλ
λλ
dL f
.
55
s
t
c
c
n
In particular, the temperature continues to increase during reverse transformation to maintain a driving force value of
−
λ
d
c
.
The material reaches points 4 when the nominal transformation strain is
ε
i
t
and the volume fraction is
λ
t
given in
(36)
at a
temperature
⎛
⎝
⎜
⎜
⎛
⎝
⎜
⎞
⎠
⎟
⎞
⎠
⎟
⎟
σθ
θε
ε
σε
()= +
−
+
()
λ
λλ
λλ
A
L
df
.
56
ic
c
c
s
t
i
t
n
mi
t
Further heating causes further reverse transformation as the material traverses from points 4 to 5 in
Fig. 4
. The nominal
transformation strain remains at
ε
i
t
, but the effective transformation strain is
λ
ε
i
t
so that the total strain
ε
λεσ
=+
E
/
i
t
begins
to decrease with
λ
. The driving force is now
σε
θθ
θ
λ
=−
(− )
−
()
λ
λλ
λλ
dL f
,
57
i
t
c
c
n
and the material needs further heating to sustain reverse transformation. It reaches points 5 when
λ
=
0
, the temperature
()
σθ
θ
σε
()= +
+
()
λ
A
L
d
58
fc
c
c
i
t
and strain
ε
σ
=
()
E
59
lo
Further heating does not change the state or the strain.
The material reaches the maximum temperature at points 6, and then begins to cool. The driving force
σε
=−
λ
θθ
θ
(− )
dL
i
t
c
c
is negative; however since
λ
=
0
, further reverse transformation does not occur. As the temperature decreases, the driving
force becomes positive and eventually reaches the value
λ
d
c
at temperature
()
σθ
θ
σε
()= +
−
+
()
λ
M
L
d
60
sc
c
c
mi
t
indicated as points 7. The transformation from austenite to martensite now begins and
λ
begins to increase along with the
strain as the material traverses from points 7 to 8 with decreasing temperature. The driving force now is given by the
expression
(57)
, thus the material needs continued cooling to sustain transformation. It finally reaches the points 8 when
the volume fraction reaches the value
λ
t
given in
(36)
and the temperature reaches the value
⎛
⎝
⎜
⎜
⎛
⎝
⎜
⎞
⎠
⎟
⎞
⎠
⎟
⎟
σθ
θε
ε
σε
()= +
−
−
+
()
λ
λλ
λλ
M
L
df
.
61
ic
c
c
s
t
i
t
n
mi
t
The strain has now reached the value
ε
h
i
in
(52)
.
Further heating continues transformation;
λ
increases and the driving force is given by
(55)
. The nominal transformation
4
This decoupling between phase fraction and strain is a result of the simplifying assumptions in this analytic section including
==
∞
λλ
mn
s
.
A. Kelly et al. / J. Mech. Phys. Solids 97 (2016) 197
–
224
208