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HEINTZE, OLAF. A Computationally Efficient Free Energy Model for Shape Memory

Alloys - Experiments and Theory. (Under the direction of Dr. Stefan Seelecke.)

Shape memory alloys (SMA) belong to the class of active materials and have recently

been considered as novel actuation and damping mechanisms in micro- and macro-scale

applications. Combined with their advantageous lightweight and high work output

char-acteristics is a complex, highly non-linear and hysteretic material behavior, which is also

thermo-mechanically coupled. Due to this complexity, model development for SMA material

behavior is a challenging task, and experimental data in particular about the inner

hystere-sis loops is necessary to gain further understanding and successfully design applications. In

this thesis, a single crystal material model is presented and subsequently extended to the

more realistic polycrystalline case considering material inhomogeneities, grain impurities

and lattice imperfections. A first implementation, based on a stochastic homogenization procedure, provides a very accurate description of the observed phenomena, but also

re-quires very high computation times. A reformulation of the underlying concept leads to a

parameterization method, which preserves the advantages of the original method, but

dra-matically reduces the computation times. It is shown that the material behavior prediction

of both models are identical, and the parameterization method is compared extensively to

data from tensile experiments with a pseudoelastic SMA wire. Remarkably, the model is

able to capture all facets of the material behavior including rate-dependence and minor

loops. The versatility of the model also allows for the simulation of SMA actuator behavior

including the electrical resistance. Finally, a MEMS device using polycrystalline SMA thin

film actuators is experimentally investigated. As a first step, the material behavior of the SMA thinfilms is presented using strain-temperature and resistance-temperature measure-ments. Secondly, the performance of the MEMS device was determined for different driving

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FOR

SHAPE MEMORY ALLOYS - EXPERIMENTS AND THEORY

by Olaf Heintze

a dissertation submitted to the graduate faculty of north carolina state university

in partial fulfillment of the requirements for the degree of

doctor of philosophy

department of mechanical and aerospace engineering

raleigh December 2004

approved by:

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Peter

Ursula and Erich

In memoria

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Olaf Heintze saw the light of day after a breathtaking car chase on January 24, 1975 on the eastern side of the German Wall in the city of Dessau. As a son of two high school

teachers for the most beloved school subjects, namely mathematics, physics, chemistry

and astronomy, a future career in engineering seemed to be already unavoidable at this

point. He spent his childhood in Oranienbaum, Germany, whether behind the counter of

his grandparents hardware store or in the physics lab of his parents school. He learned

summating prices in the hardware store and setting up electrical circuitries in the physics

lab, which became handy later on during his time in school.

Guided by the roots of his childhood, he earned the degree Diplom-Ingenieur from

the Technical University in Berlin in Physical Engineering Science in 2001 and had been

generously offered to enroll in a Ph.D. program abroad. Following this offer, he became

a Ph.D. student at the Mechanical and Aerospace Engineering Department of NC State

University in the very same year.

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I would like to extend my deepest gratitude to my advisor and founder of my research

career Prof. Dr.-Ing. Stefan Seelecke. Since we started working together in Berlin in 1999,

I realized how much I still have to learn about profound, real-world engineering and that

he would be the one to learn it from. I sincerely thank you for the support and guidance

during all those years as well as for the generous offer to become your Ph.D. student and,

thus, allowing me to widen my experience enormously. Danke.

For being always helpful, encouraging and supportive, I would like to thank my

com-mittee members Dr. Mohammad Noori, Dr. Ralph C. Smith and Dr. Richard F. Keltie.

Although the air was often on fire and time always precious, you managed to be available for me. Thank you, Dr. Keltie, for your advise and engagement, when I needed it the

most.

I also would like to thank Dr. Gould for his fast and uncomplicated help during all my

time in the Ph.D. program.

Dr. Shaw. Thank you so much for providing me with access to your wonderful lab.

You even have colored screw drivers! I especially enjoyed your profound way of conducting

research combined with your great sense of humor. I also still miss the Fragles.

Many thanks to the staff of the MAE department, especially to Betty, who always

answered calmly my questions and to Mike and Skip, who always did their best to make

my experiments happen.

Although, they have left this university already, I need to thank my former fellow

stu-dents Jason and Jinghua for the scientific discussions we had and for introducing me to

their own cultures.

The NC State Water Polo Club. What had I done without you guys? You allowed me

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Yuriy for being my friends and for giving me the final boost, when I started to loose it. Another great ’thank you’ goes to the three T’s. Thanks Tim and Tim for the endless

discussions we had. Big thanks also to my room mate Tom. Chief, I’ll never forget your

help and encouragement.

The last and greatest Danke goes home to my family in Germany. You always

sup-ported me and made all this happen by your strong commitment to this little family and

to education. Although I can’t thank many of you in person anymore, I’m confident that

it reaches you.

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List of Figures viii

1 Introduction 1

1.1 Motivation and Background . . . 1

1.1.1 Applications . . . 1

1.1.2 Modeling . . . 2

1.2 Thesis Objective . . . 7

1.3 Thesis Outline . . . 8

2 Perfectly Homogeneous Single Crystal Model 10 2.1 Assumptions . . . 10

2.2 Free Energy as Central Quantity . . . 12

2.3 Stress-Strain Relation . . . 15

2.4 Kinetics of Phase Transformation . . . 16

2.5 Balance of Internal Energy . . . 20

2.6 Summary of Model Equations and Simulation of Hysteresis Loops . . . 21

3 Inhomogeneous Polycrystal Model - Direct Implementation 24 3.1 Concept of Stochastic Homogenization . . . 24

3.1.1 Stress vs. Strain Control . . . 27

3.1.2 Convergence Analysis . . . 30

3.1.3 Effects of Distribution Parameters . . . 34

4 Parameterization Method - Representative Single Crystal 37 4.1 Concept of Parameterization . . . 37

4.1.1 Parametrization Method for a Single Distribution . . . 38

4.1.2 Parametrization Method for Two Combined Distributions . . . 42

4.2 Implementation Details . . . 49

4.3 Evaluation of Parameterization Method . . . 52

4.3.1 Comparison with Direct Implementation . . . 53

4.3.2 Comparison with Experimental Data . . . 55

4.3.3 Simulation of Sensor and Actuator Behavior . . . 62

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5 SMA MEMS Actuator Experiments 67

5.1 Introduction . . . 67

5.2 Material Properties . . . 68

5.2.1 Setup and Procedure . . . 68

5.2.2 Mechanical and Sensor Properties . . . 70

5.2.3 Conclusions . . . 80

5.3 Actuator Performance . . . 80

5.3.1 Procedure and Setup . . . 80

5.3.2 Open Loop Results . . . 81

5.3.3 Conclusions . . . 83

6 Conclusions 85

List of References 87

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2.1 Lattice particle of a shape memory alloy in its possibel phases autenits A

and martensite M±. . . 10

2.2 Typical layer structure. . . 11

2.3 Layer model of a macroscopic material . . . 12

2.4 Free energy of a lattice layer for a fixed temperature without (left) and with external load (right). . . 13

2.5 Free energy of a lattice layer for different temperatures. . . 14

2.6 Free energy for a lattice layer forT = 328K and different loads. . . 15

2.7 Isothermal, mechanical response of a single crystal SMA for different temper-atures. Quasi-plastic (left, T = 280K), transition to pseudo-elastic (middle, T = 308K), and pseudo-elastic material behavior (right, T = 338K). . . 22

2.8 Strain vs. temperature behavior for two different loads. . . 23

3.1 Effect of distribution in barrier (left) and internal stress (right). . . 25

3.2 Comparison of strain and stress control for 9 integration points. . . 29

3.3 Comparison of strain and stress control for 9 integration points. Phase frac-tion evolufrac-tion. . . 31

3.4 Convergence behavior for isothermal tensile experiment. . . 32

3.5 Convergence behavior for non-isothermal experiment. . . 33

3.6 Pseudoelastic material behavior due to different distribution combinations, 1st order reversal . . . 35

3.7 Pseudoelastic material behavior due to different distribution combinations, 2nd order loops . . . 36

4.1 Gibbs free energy landscape during loading/unloading for elements with dif-ferent energy barriers. . . 40

4.2 Normal Distribution of barrier stresses and associated phase fraction change. 41 4.3 Gibbs free energy landscape during loading/unloading for elements with dif-ferent interaction stresses. . . 43

4.4 Gibbs free energy landscape during loading/unloading for elements with dif-ferent energy barriers and interaction stresses. . . 44

4.5 Contour and surface plots of double-distribution landscape during intial load-ing process. . . 47

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4.7 Numerical evaluation of double integral to calculate the phase fraction . . . 50

4.8 Phase transformation probabilities for single crystal SMA. . . 52

4.9 Phase transformation probabilites for parameterized SMA model. . . 53

4.10 Comparison of parameterized model and direct implementation, isothermal case. . . 54

4.11 Comparison of parameterized model and direct implementation, non-isothermal cases (strain rates 1e-4, 1e-3, 1e-2 1/s). . . 56

4.12 Isothermal case with barrier from data . . . 57

4.13 Strain rate effect - data and parameterized model . . . 58

4.14 Major loops - comparison with data for different strain rates. . . 59

4.15 Partial loading - comparison with experimental data for different strain rates. 60 4.16 Partial unloading - comparison with experimental data for different strain rates. . . 60

4.17 Minor loops - comparison with experimental data for different strain rates. 61 4.18 Relaxation - comparison with experimental data for different strain rates. . 62

4.19 Actuator properties for different loads - major loops . . . 64

4.20 Actuator properties for different load - partial heating. . . 65

4.21 Actuator properties for different loads - partial cooling . . . 65

4.22 Actuator properties for different loads - minor loops. . . 66

5.1 MEMS device; Schematic sketch (left), DMA7efixture (middle), 1-steel base, 2-stamp, 3-PC board, 4-lead wires, device after testing (right) . . . 69

5.2 Geometrical constraints due to MEMS principle of operation. . . 70

5.3 Major loops. Strain vs temperature (top), resistance vs temperature (bot-tom) for increasing load (left to right). . . 72

5.4 Partial heating, 1. type. Strain vs temperature (top), resistance vs temper-ature (bottom) for increasing load (left to right). . . 74

5.5 Partial heating, 2. type. Strain vs temperature (top), resistance vs temper-ature (bottom) for increasing load (left to right). . . 75

5.6 Partial heating. Temperature vs. time (left), strain vs. temperature (middle) and resistance vs. temperature (right). . . 76

5.7 Close up picture of MEMS device after testing with textured SMA actuators. In and out of plane deformations along SMA strips. . . 77

5.8 Partial cooling. Strain vs temperature (top), resistance vs temperature (bot-tom) for increasing load (left to right). . . 78

5.9 Minor Loops. Strain vs temperature (top), resistance vs temperature (bot-tom) for increasing load (left to right). . . 79

5.10 MEMS performance testing device . . . 81

5.11 MEMS actuator performance for 0.5Hz, 5Hz and 10Hz electric current input (rectangular pulse). . . 82

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Introduction

1.1

Motivation and Background

The shape memory phenomenon has been known for about seventy years now, but did not

receive much attention since its discovery by Ölander (see [64], [65]). It was rediscovered

by Bühler (see [22]) in the 1960’s, and technical applications are pursued since then.

After plastic deformation at low temperature, a shape memory alloy (SMA) restores its

initial configuration upon the supply of heat. This ’memory’ of the original shape provided

the name for the effect. At a higher temperature, the material exhibits another behavior.

Here the material can be reversibly deformed up to10%of its original length under a nearly constant load. This effect is called superelasticity. Both effects are a consequence of the

quasiplastic and pseudoelastic load-deformation behavior at low and high temperatures,

respectively. The underlying mechanism is a phase transformation between different

crys-tallographic structures, i.e. different variants of martensite and the austenite phase. Details

about the material behavior can be found in the textbooks of Funakubo [26] and Otsuka

and Wayman [67].

1.1.1

Applications

Some of the early applications were pipe couplings and electric circuit breakers acting

au-tonomously to changes in the environmental temperature. Due to their biocompatibilty,

they also found their way into medical applications. They cover the range from self-adjusting

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braces to tubular, self-expanding stents. Although they have also been used for energy

con-version purposes (see Glasauer and Müller [28]), two main application areas are damping

mechanism and actuation. Thefirst one is made possible by the non-linear hysteretic ma-terial behavior causing energy to dissipate. In particular, this is useful for the damping of

civil structures that need an efficient seismic isolation or a protection against wind

vibra-tion. For most recent applications see Wildeet al [82], Aizawaet al [5] and DesRoches and

Delemont [24]; for modeling of hysteresis-induced damping behavior see Seelecke [71] and

[72].

Since shape memory alloys provide the highest work output of all known actuation

mechanisms combined and are lightweight (see Hollerbachet al [38]), they are an attractive

choice for actuator applications. This ranges from macro-scale applications like adaptive

wing shape control (Bauer et al [6],Breitbach et al [19],Hanselka et al [35],Kudva et al

[53] and Campanile et al [23]). Campanile et al [23] use SMA actuators below the flexible surface of a trailing edge to control the position of transonic shocks. In addition to aerospace

related applications, SMAs are also used in robotics. Vaidyanathan creates a worm-like

robot (see [80]), and a controlled six-legged robot is presented by Heintze [36]. Other

robotic applications are, e.g., multifingered hands (Schleich [69])

The most promising area for SMA actuators is the field of micro-electro-mechanical systems (MEMS). Since the SMA actuation mechanism relies on passive cooling, their

effectiveness increases with decreasing dimensions. Micro-scale actuators have large surface

to volume ratio and, thus, effective cooling even when surrounded by still air. Hoet al [37]

report a thinfilm micropump operating at a frequency of300Hz. Such micropumps are used in microfluidics in, e.g., medical drug dosage systems and ink jet printers. A related area is

microvalves as presented by Kohl et al ([52], [50]). A US-based company, TiNi-Alloy, even

has a commercial product available, see Johnson [46], [48]. In [47] Johnson also explains in

the advantages of SMA MEMS actuators simultaneously claiming the lack of available data

and systematically conducted experiments, which provided one motivation for this work.

1.1.2

Modeling

If one wants to make an efficient use of these novel applications and successfully

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thermomechanically-coupled material behavior of shape memory alloys.

Early efforts go back to Tanaka and Nagaki [79], [77] and [78]. The model uses the

fraction of martensite as an internal variable and gives a phenomenological equation of

state for its dependence on stress and temperature in the form of an exponential function.

It provided the basis for a related model suggested by Liang and Rogers [55], who found

a cosine law for the martensite fraction to be more convenient. However, both versions

were only applicable to the high temperature case of pseudoelasticity, and it was only

after Brinson [20] introduced a decomposition of the martensite fraction into twinned and

detwinned martensite, that the quasiplastic behavior could be described as well. Due to

the phase diagram necessary to distinguish between the different branches of the martensite

fraction equation, these models are also called state-space models, see Bekker and Brinson

[7] for a generalization of the concept. All these models are purely mechanical in the sense

that temperature is considered as a parameter.

Boyd and Lagoudas [18] have developed a model that is derived from irreversible

thermo-dynamics. Based on the second law, an ansatz for the entropy production is made resulting

in an evolution law for the phase fractions which is thermodynamically admissible. The

model follows the guidelines of the classical theory of rate-independent plasticity with yield

conditions triggering the phase transformations and is formulated in a three-dimensional

setting. Closed form solutions for damping capacity and actuator efficiency are obtainable

from the model. A drawback, however, is the large number of material parameters to be

determined. Furthermore, due to its provenance from the classical theory of plasticity, the

dissipation potential is not chosen from physical reasoning but rather from mathematical

arguments like convexity properties.

Recently, a number of articles have been published, which attempt to combine the

framework of irreversible thermodynamics with a more detailed study of the underlying

microstructure. The main objective is to find a suitable expression for the free energy as composed of chemical and mechanical parts. The chemical part is temperature dependent

and is mainly determined by the entropies of austenite and martensite, whereas the

me-chanical contribution is due to the stress and strain fields from external loading and the interaction between the different phases. This interaction is due to the strains associated

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driving force for the transformation is calculated and set equal to dissipative terms from

interfacial energy contributions and so-called internal friction. Thus, an equation is derived

for the evolution of appropriate martensite phase fractions. Models of this type have been

proposed by several authors, among them Lu and Weng [56], who give a single crystal

for-mulation for oblate inclusions, which they extend to a self-consistent model for polycrystals

in a subsequent paper, [57]. A similar approach has been taken by Huang and Brinson [39],

who first illustrate the procedure for a fictitious two-variant material and later extend it to a typical 24 variant case. While in this paper the authors treat spheroidal inclusions,

they turn to the more realistic case of penny-shaped inclusions in Gao et al [27]. Here,

they also introduce a distinction between habit plane variants and correspondence variants,

accounting for the fact that habit plane variants may consist of smaller subunits leading

to an internal structure in the form of a certain stacking sequence. This model is further

generalized to polycrystalline behavior, see Gao Etal [40]. Bo and Lagoudas [13, 14, 15,

16] also present a paper on a polycrystalline model of such type, consisting of four parts.

Their main focus is on the introduction of plastic strains, which is an important mechanism

present in some SMAs under cyclic loading applications. It is shown to lead to a degradation

of performance when a non-stabilized material is used in an actuatoric application. The

authors use back and drag stress as internal variables and are able to simulate the two-way

shape memory effect, which is also related to the evolution of plastic strains. After a

the-oretical derivation of the three-dimensional formulation in part I, a material undergoing a

stable transformation cycle is treated in part II in a one-dimensional setting. This version

is also used for the full plastic model which is compared to experimental results in part

III. Part IV discusses the relationship to so-called Preisach models often used by hysteresis

researchers with a mathematical background. The model’s capabilities with respect to the

simulation of internal hysteresis loops are demonstrated.

Lagoudas and Entchev continued this work in [54] and further applied this model to

porous SMAs in [25]. Khanet al [49] present a Preisach model pseudoelastic response that

can model minor hysteresis loops, but does not consider the strain rate effect. Both models

are able to simulate polycrystalline material behavior.

Another recent model based on micromechanical considerations has been proposed by

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Lexcellent [81], who study the differences between tension and compression in

pseudoelas-ticity. Bouvetet al [17] present a model considering the same differences and incorporating

multiaxial proportional and nonproportional loading. It considers rate-independent

plastic-ity and minor loops due to yield surfaces for the phase transformation as a function of the

phase fraction.

Novak and Sittner present a micromechanical modeling approach for polycrystalline

SMA in [62],[63].

The authors in [21] propose a phenomenological model for polycrystalline SMA, based

on statically constrained micro-plane theory. Hereby, the macroscopic material behavior is

obtained by the evaluation of stresses and strains on differently oriented microplanes. The

paper presents simulations of polycrystalline material behavior based on 28 microplanes.

This approach can model minor hysteresis loops, and the ones shown for uniaxial loading

close after intensive cycling. It is expected from experiments and theory that minor loops

close only for the isothermal case. Since the model incorporates changes in temperature, a

discussion of the strain or stress rate effect would be desirable to explain the phenomenon

of non-closing minor loops.

The state-space models discussed above may be regarded as the beginning of SMA

modeling, and they are still nowadays widely used among engineers due to their conceptual

simplicity. Their suitability for the simulation of actuator applications, however, is very

limited. The same holds for the recent micromechanical models discussed above, which,

although possessing a high level of sophistication, are far too complex to be used for the

simulation of mostly one-dimensional SMA actuators. Here, in the present paper, the

major concern is a good one-dimensional description accounting for both, thermodynamic

and mechanical aspects, at the same time offering the possibility of implementation into

advanced control algorithms.

A noticeable model in this respect has been developed by Ivshin and Pence [44, 45].

The authors perform a detailed thermodynamic analysis to motivate their basic equations.

The potential of thermodynamic analysis, however, has not been fully exploited as it only

deals with the case of equilibrium thermodynamics based on integrability conditions derived

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description of the hysteretic shape memory behavior. They enter the model through

so-called envelope functions resulting in an ordinary differential equation of Duhem-Madelung

type for the austenite phase fraction. Despite a certain lack of physical reasoning, the

model appears to be quite powerful with respect to the simulation of actuatoric behavior.

It includes an energy balance with contributions from convective heat exchange, latent heats

and external heat sources, and a number of interesting simulations are displayed in [45].

Ikeda et al [43] introduce a macroscopic model for uniaxial loading derived from a

grain-based microscopic model. They have incorporated an energy balance and are able

to model inner hysteresis loops. The phase transformation occurs by exceeding a required

transformation energy, which is derived with arguments from the micromechanical model

in [61]. This transformation energy is a function of the phase fraction itself and its time

derivative to allow for a polycrystalline shape of the outer hysteresis. Additionally, it uses a

different energy for loading and unloading. The minor loop modeling is achieved by shifting

this energy to the appropriate reversal point in the energy and phase fraction space. As

a result closing minor hysteresis loops can be modeled and show good agreement with the

presented data, which is not the case for a partial loading or partial unloading scenario. The

strain rate effect is incorporated to a certain extent; the slope of only the outer hysteresis

loop changes with strain rate. A shortcoming in the presented implementation is that minor

loops still close for the non-isothermal case, which is not observed in the experiment.

Another model that has recently been applied to SMA actuator applications has

origi-nally been developed by Müller and Wilmanski [60], Achenbach and Müller [3, 4], Achenbach

et al [2], Achenbach [1] and Seelecke and Müller [73]. It uses ideas from statistical

ther-modynamics and describes the evolution of two martensite fractions based on the theory

of thermally activated processes. It has been shown that the model is able to

qualita-tively simulate the behavior of SMAs over the whole range of temperatures from

quasi-plasticity to pseudoelasticity. Through the introduction of the Helmholtz free energy as

the effective potential energy, Seelecke [74] has recently been able to make quantitative

predictions. The coupling with the balance of energy makes it possible to reproduce the

dependent length change of an electrically heated SMA wire under an arbitrary

time-dependent load. The attractiveness of the model is based on the fact that the complete

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function alone without any additional loading/unloading criteria. A very limited and clearly

interpretable number of parameters, which may be identified from only two tensile

experi-ments at different temperature levels, are necessary for the determination of the free energy.

Together with a convenient mathematical structure in the form of an ODE system, allowing

for robust numerical integration, these features make the model an attractive candidate for

the simulation of SMA actuators and their control behavior.

Before we proceed to discuss this model in more detail in the next chapter, we conclude

the present overview with another model that is based on thermal activation. Hall and

Govindjee [32] use locally defined phase fractions within the concept of mixture theory,

which they calculate from evolution laws very similar to the Müller-Achenbach model. They

particularly focus on numerical integration issues, and develop an improved method in [31].

In a further paper, [34], they extend the model to multiaxial loading conditions and also

discuss some aspects of polycrystals. The scope of all papers, however, is still isothermal.

1.2

Thesis Objective

The objective of this thesis consists of three major components:

1. Extension of the Müller-Achenbach-Seelecke model for perfect single crystal SMA to

polycrystalline material behavior

2. Presentation of a novel, but equivalent, modeling approach featuring high

computa-tional efficiency

3. Discussion of systematically conducted investigation of the material behavior and

performance of an SMA MEMS device.

First, we present the perfect single crystal material model for SMA and extend it to

a more realistic polycrystalline material behavior by incorporating the concept of

inhomo-geneities and effective stresses. This model results in a very accurate description of the

rate-dependent inner loop behavior, but requires high computation times.

The second and major part will present an alternative modeling approach, which is

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This allows for an implementation into other numerical codes, such as finite element or optimal control programs or a Matlab/Simulink environment. The method can reproduce

the experimentally observed behavior very accurately over a large range of strain rates

including the minor loop behavior.

Finally, we study the material behavior and performance of a SMA MEMS device

through a sequence of systematic experiments. From these experiments, it becomes

ob-vious that the presented models need to be extended to include an R-phase in addition to

the already considered martensite and austenite phases.

1.3

Thesis Outline

The thesis is divided into six chapters as follows:

Chapter 1 provides a motivation for the research along with a literature review of the

previous work on modeling of SMA behavior. This chapter also outlines the objectives and

structure of the thesis.

Chapter 2 details the perfect single crystal material model, which provides the basis for

all further extensions to polycrystalline material behavior. Its basis, the free energy, will

be discussed along with the derivation of the rate laws governing the phase transformation

and the energy balance.

Chapter 3 extends this single crystal material model to the more realistic polycrystalline

case considering material inhomogeneities, grain impurities and lattice imperfections. After

the introduction of the concept we focus on the two commonly encountered loading types,

stress control and strain control. A first implementation results in a very accurate but computationally highly inefficient model.

Chapter 4 proposes another modeling approach based on a representative single crystal

model, which requires only very small computation times. It is shown that this model can

reproduce experimental data accurately. To this purpose, model and experimental data

are compared for different loading scenarios incorporating minor loops and different strain

rates. We also show the versatility of the model and simulate typical actuator behavior

under a constant load along with the electrical resistance of the SMA, which is potentially

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In Chapter 5 a MEMS device using polycrystalline SMA thinfilm actuators is experimen-tally investigated. As a first step, the material behavior of the SMA thinfilms is presented using strain-temperature and resistance-temperature measurements. Secondly, the actuator

performance of the MEMS device was determined for different driving frequencies.

Finally, Chapter 6 will provide concluding remarks on the results and comments on

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Perfectly Homogeneous Single Crystal Model

The following chapter provides an overview of the modeling of the material behavior for

single crystal SMAs. We will describe the assumptions necessary for the model and discuss

the free energy as its central quantity. Following the discussion of the basic concepts, we

will present the main equations together with simulations of the typical material behavior.

2.1

Assumptions

The model considers a single crystal material under uniaxial loading, which allows for two

variants of martensite in addition to the austenite phase.

Figure 2.1 illustrates the schematic presentation of typical lattice particles in these three

configurations, where the austenite is highly symmetrical. The two martensite phases can

be understood as derived from it through a shear deformation. Their denotation M+ and

Figure 2.1: Lattice particle of a shape memory alloy in its possibel phases autenitsA and martensiteM±.

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Figure 2.2: Typical layer structure.

M is based on the direction of its shearing. This configuration results in a typical surface

texture (see Figure 2.2), often observed with specimen under tensile testing. Here, the

layers are formed of austenite and the martensite variant favorably oriented to the loading

direction. Motivated by this observation, the model considers a mesoscopic layer as the

basic element and assumes the macroscopic material as a stack of such layers.

Figure 2.3 illustrates this understanding of the mesoscopic material structure. The

single crystal is represented by the fact that all layers are aligned with the same angle to

the loading direction. In addition to the layer alignment, Figure 2.3 presents the mechanism

of the shape memory effect. At the very left, the material is in a load-free state at a low

temperature and consists of both martensite phasesM±. The orientation of one martensite

phase is favorable for tension and the other one for compression. In the second illustration

from the left, a tensile force is applied to the specimen, and the layers with the compression

orientation start to erect caused by the shear stress in the plane. Once a critical tensile force

is achieved, these layers flip in the other martensite phase (middle) and, thus, contribute to an extension in the specimen’s length. Most of this extension remains, when the load

is released from the specimen due to the fact that no reverse transformation occurs (2nd

from right). This residual deformation can be restored by heating. The specimen contracts

back to its original shape (right) due to a transformation from martensite to austenite. A

subsequent load-free cooling transforms this austenite into the twinned martensite structure

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Figure 2.3: Layer model of a macroscopic material

2.2

Free Energy as Central Quantity

Depending on its shear deformation ε and temperature T, the lattice layers have a

deter-mined free energy. We consider every layer as an ensemble of lattice particles being in

the same phase. The governing potential for the thermo-mechanical behavior of such an

ensemble is the Helmholtz free energyΨ=UT S consisting of the internal energyU and the entropyS. Figure 2.4 (left) shows a schematic sketch of a typical free energy at afixed temperature and without the action of an external load, where all three phases are stable.

It consists of a chain of parabolae; three of them are convex and two concave. The convex

parabolae belong to the three phase, whereas the two concave ones are energy barriers

sep-arating them. Figure 2.4 (right) illustrates the action of an external load σ. Its workσε needs to be added to the free energy.

We derive the Helmholtz free energy Ψwith arguments from statistical mechanics and refer the interested reader to [70] for details. Since the free energy is a function of the

temperature, we would like to discuss its influence using Figure 2.5 for a specimen made

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Figure 2.4: Free energy of a lattice layer for a fixed temperature without (left) and with external load (right).

An increase in temperature to T = 300K yields to the creation of a third minimum, which belongs to the austenite phase. Upon further heating to T = 305K the center minimum represents already a lower energy than the ones belonging to the martensite

phases, but the remaining energy barrier between the phases prevents a transformation

from happening. This occurred already atT = 328K since the austenite is the only stable phase at this temperature, and the energy barriers were eliminated. One identifies this

process as entropic stabilization of the austenite; the reversal is the formation of the

so-called temperature induced martensite.

Under the action of an external load σ the Gibbs free energy becomes the governing

thermodynamic potential for a lattice layer. We discuss the effect of an increasing load

using Figure 2.6 for a fixed temperatureT = 328K. The illustration at the top left shows the load-free state, where the Helmholtz and Gibbs free energy are identical, and, thus, is

the same plot as the last one in Figure 2.5.

An increasing load to σ = 50M P a lowers the minimum for M+ and raises the one for

M. We observe that the austenite is still stable with the lowest energy minimum. This

changes for σ = 150M P a, where the austenite remains stable, although the martensite M+ the same energy. Since both minima are still separated by an energy well, no phase

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(25)

Figure 2.6: Free energy for a lattice layer forT = 328K and different loads.

martensitic phase.

Along with this phase transformation goes a significant increase in the specimen’s strain.

Subsequent unloading of the specimen to σ= 150M P adoes not result in a phase mation, since Figure 2.6 shows a present energy barrier for this load. The reverse

transfor-mation to the martensite phase will occur at lower load, restoring the transfortransfor-mation strain

and, thus, creating a typical stress vs. strain hysteresis. We identify this as the pseudoelastic

material behavior of the shape memory typically occurring at high temperatures.

2.3

Stress-Strain Relation

The quantity of greatest interest is the resultant change in the specimen length caused by

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∆ denotes its actual deformation and l its original length in loading direction. Therefore the strain of the entire specimen

ε=xAεA+x+ε++x−ε− (2.1)

is determined as the sum of the strain of each phase weighted by its fraction, where

xA, x+, x− denote the phase fractions and εA, ε+, ε− the strain of each phase. Since there are three phases in the material considered, we know that the sum of all phase fractions

needs to equal one.

1 =xA+x++x− (2.2)

Caused by thermal activation, the layers fluctuate about its energy minimum. We assume that all layers of one phase are in a thermodynamic equilibrium among each other,

and the expected value for its strain can be calculated with argument from statistical

mechanics, e.g.

εA=

Z +wA(T)

−wA(T)

εexpG(ε, T, σ) kBT

R+wA(T)

−wA(T) exp−

G(ε,T,σ)

kBT dσ

(2.3)

In (2.3) T denotes the temperature, kB the Boltzmann constant and G(ε, T, σ) the

Gibbs free energy. The integration limits±wA(T)are the transition points with the concave

parabolae.

Since εA in (2.3) is a function of the stressσ, we call (2.1) the stress-strain relation for

the single crystal SMA, where the deformation also depends on the temperature and the

internal state of the specimen is determined by the phase fractions.

2.4

Kinetics of Phase Transformation

We determine the phase fractions by the integration of the ODE system

·

x+ = −x+p+A+xApA+ (2.4)

·

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The equations in (2.4) and (2.5) are kinetic rate laws for the phase fractions and describe

their evolution in time. They are derived with arguments from the theory of thermally

activated processes. The fraction of, e.g., martensiteM+can only be altered by an exchange

of particles with its neighboring phase. Hereby, this exchange consists of a loss proportional

to the number of layers in the M+ phase and a gain, which is proportional to the number

of layers in the austenite phase. The factors of proportionality are pαβ and the phase

transformation probabilities for the transformation from phaseαto the phase β.

They are derived with arguments from statistical mechanics andp+A, e.g., can be written as

p+A=

v u u

t kBT

2πmV 2 3

L

exp³G(σ,wm(T),T)

kBT ´

R+∞

wm(T)exp ³

−G(kσ,ε,TBT ) ´

(2.6)

Equation (2.6) describes the probability of a layer of martensite M+ to surpass the

energy barrier evaluated at the location wm(T) of the energy barrier. We introduced

VL as the activation volume of a lattice element, kB the Boltzman constant, and T the

temperature of the SMA.

In order to evaluate (2.6), we need to determine G(σ, ε, T) considering its definition

G(σ, ε, T) :=Ψ(ε, T)σε (2.7)

and a chain offive parabolae forΨ(ε, T)as shown in Figure 2.4. The following conditions and assumptions were used to determineΨ(ε, T) :

1. Smoothness for the transition points. The values and derivatives of the convex and

concave parabolae, evaluated at the transition points, must be equal. We denote the

transition points between the concave parabola and the austenite A and martensite

M± aswA,M(T) respectively.

2. We know for the stressσ=∂Ψ/∂εand, therefore, can evaluate the condition∂2Ψ/∂ε2 = ∂σ/∂εatwA,M(T) using µ

∂σ ∂ε

A,M

=EA,M (2.8)

3. The minima of the convex parabolae in the load-free case are located at zero strainε

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4. For a reference temperatureTR we assume Ψ(±εT, TR) = 0 and Ψ(0, TR) =∆β(TR),

where∆β(T) is unknown at this point.

The result is a system of equations, where we can solve the equations for the convex

parabolae immediately considering EA,M as to be known. Subsequently, the equations for

the concave parabolae were solved; they remain a function of wA,M and ∆β(T), and we

have

Ψ(ε, T) =                    1

2EM(ε+εT)

2 ε <

−wM

Aε2+Bε+C wM ≤ε <−wA

1 2EAε

2+β(T)

−wA≤ε < wA

Aε2Bε+C wA≤ε < wM

1

2EM(ε−εT)

2 w

M ≤ε

(2.9)

with

A = EM(εT −wM) +EAwA 2 (wA−wM)

(2.10)

B = wA[EM(εT −wM) +EAwM] wA−wM

(2.11)

C = 2∆β(T) (wA−wM) +w

2

A[EM(εT −wM) +EAwM]

2 (wA−wM)

(2.12)

Furthermore, we determine ∆β(T) as a function of wA,M from the set of equations

resulting from the conditions for Ψ(ε, T) as

∆β(T) = 1

2[EM(εT −wA) (εT −wM)−EAwAwM] (2.13) Finally, we introduce the stressesσAgoverning the austenite-martensite transformation

andσM governing its reversal. They both can be determined from two tensile experiments,

since they both depend on the temperature. It is a good assumption to assume their

temperature dependence as to be linear in the relevant temperature regime. This allows for

the determination of wA,M since we evalute σ =∂Ψ/∂ε at the transition points as shown

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σA = µ ∂Ψ ∂ε ¶ wA (2.14)

σM =

µ ∂Ψ ∂ε ¶ wM (2.15)

We finally solve (2.14) and (2.15) forwA and wM:

wA =

σA

EA

(2.16)

wM =

σM

EM

+εT (2.17)

We summarize that the Gibbs free energy can be uniquely identified knowing the

mate-rial parameters σA, σM, EA, EM.

Substituting (2.9)-(2.17) in (2.7) allows for the evalution of the phase probability

trans-formations, and we get for the martensite-austenite transformation

p±A= 2 τx

r

EM

EA

1 erfcx(αMzM)

(2.18)

where

αM : =

r

VS

2EMkBT

(2.19)

zM : =σM ∓σ (2.20)

Similarily, we derive the probabilities for the reverse transformation as

pA±= 2 τx

[erfcx(αAzA)−erfcx(2αAσA−αAzA) exp (4αAσA(αAzA−αAσA))]−1

(2.21)

where

αA : =

r

VS

2EAkBT

(2.22)

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2.5

Balance of Internal Energy

Since the stress-strain relation as well as the phase fractions are also temperature-dependent,

we need to include an equation for the temperature T and assume this temperature as to

be homogeneous. This equation is derived from the balance of the internal energyU

dU dt =

·

Q+σεV,· (2.24)

and we rewrite it using the enthalphy H:=U σεV as

dH dt =

·

QσεV· (2.25)

Hereby Q· is the heat input rate and σεV· the term representing the power of external

forces. We furthermore assume that the total enthalphy is the sum of the enthalpies of all

particles in one phase and have

H=X

α

(xαhα(σ, T))V (2.26)

whereV is the SMAs volume,xα denotes the volume phase fraction andhα the specific

enthalphy. We introduce (2.26) in (2.25) and consider the total differential for hα

dhα

dt = ∂hα

∂σ ·

σ+∂hα ∂T

·

T (2.27)

as well as

∂hα

∂σ = ∂g ∂σ −T

∂s ∂σ =

∂g

∂σ =−ε (2.28)

knowing that the specific entropy is independent of the stress and that g denotes the

specific Gibbs free energy.

The resulting equation for the temperature evolution in time

cT· = · Q V −

·

x+(h+−hA)−x·−(h−−hA) (2.29)

considers c = ∂hα

∂T , the specific heat of the SMA and hα the specific enthalphy of the

phases M+, M− and A respectively. The relevant heat supply terms for the SMA are

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electric current. Considering this and rearranging (2.29) leads the final form of the energy balance

ρcVT· =hAs(T −T0) +j(t)−x·+H+V −x·−H−V (2.30) This is a third ordinary differential equation (ODE) that needs to be solved

simultane-ously with the rate laws (2.4) and (2.5) for the phase fractions. Since the ODE system is

characterized by an extreme numerical stiffness, which is also varying with its non-linearity,

we use the Radau5 method for its integration. The method is described in [33] and considers

a 5th order Runge-Kutta scheme with step size control.

In (2.30) ρ denotes the density of the SMA, c its specific heat, V its Volume, h the

film coefficient, As the surface area and T0 the ambient temperature. The temperature of

a SMA can be changed by heat exchange with the environment, by Joule heatingj(t), and through the latent heats H± of the phase transformation, where we define

H± :=h±hA (2.31)

Since hα is a specific enthalpy, we can determineH±as the difference of the Helmholtz free energy for T = 0evaluated at the associated minima.

2.6

Summary of Model Equations and Simulation of

Hys-teresis Loops

In order to simulate the material behavior of the perfect single crystal SMA, we need to

integrate the rate laws for the phase fractions (2.4) and (2.5) as well as the balance of the

internal energy (2.30) simultaneously. The solution of this ODE sytem

·

x+ = −x+p+A+xApA+ (2.32)

·

x = xp−A+xApA− (2.33)

ρcVT· = hAs(T−T0) +j(t)−x·+H+V −x·−H−V (2.34)

allows to evaluate the stress-strain relation (2.1)

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Figure 2.7: Isothermal, mechanical response of a single crystal SMA for different temper-atures. Quasi-plastic (left, T = 280K), transition to pseudo-elastic (middle, T = 308K), and pseudo-elastic material behavior (right,T = 338K).

to determine the macroscopic mechanical material behavior.

Figure 2.7 exemplarily illustrates the stress-strain behavior for an isothermal, strain

con-trolled tensile experiment at different temperatures. The left picture in Figure 2.7 shows

the low temperature, the quasiplastic, material behavior. The hysteresis is located around

the origin, because there is no austenite stable atT = 280K and the phase transformations only occur between the two martensite phasesM+ and M−. With increasing temperature

the pseudoelastic material behavior develops and is fully pronounced at the highest

tem-perature T = 338K in the right picture of Figure 2.7. Phase transformations occur here between austeniteA and martensiteM±, where the stress level of the hysteresis shifts with

the temperature.

The strain vs. temperature relation shown in Figure 2.8 is typical for an experiment,

where the temperature of the SMA is cycled up and down under the action of afixed load. It is a direct consequence of the material behavior presented in Figure 2.7. Furthermore,

we observe that an increasing load shift this strain-temperature hysteresis to higher strains

and temperature levels. The diagram in 2.8 symbolizes the input-output relation for an

SMA actuator, where the output, its strain, is controlled by the temperature input.

We can summarize that the model is able to describe the temperature dependent

mate-rial behavior in the regime of quasiplasticity and pseudo elasticity. The hysteresis in both

regimes are characterized by sharp transitions and pronounced plateaus. The right picture

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Figure 2.8: Strain vs. temperature behavior for two different loads.

Upon unloading we observe a reversible unloading path through the hysteresis, which is not

typically observed in experiments. The data usually shows the formation of minor hysteresis

loops embedded in the major, outer hystersis.

Since, the model is based on the assumption of a perfectly homogeneous material, its

behavior is not typical and realistic. Therefore, in the next chapter we will focus on an

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Inhomogeneous Polycrystal Model - Direct

Implementation

The previous chapter described the basic structure of a model for single crystalline behavior

under the assumption of a perfectly homogeneous material. In regard to commercially

available SMA material, neither of the two is correct; and if we want to model the behavior

of "real life" engineering components like, e.g., stents, actuator wires or thinfilm devices in MEMS applications, we need to extend the above model. This section will develop a version,

which accounts for inhomogeneities and interaction between different phases and grains as

encountered in a typical polycrystalline material. After the introduction of the concept with

a focus on the two commonly encountered loading types, stress control and strain control,

we perform a convergence analysis for the isothermal and non-isothermal case. Finally, we

discuss the effects of different model parameters on the resulting hysteresis loops.

3.1

Concept of Stochastic Homogenization

The homogeneity assumptions made for the derivation of the perfect single crystal model in

the previous chapter certainly hold at best for small length scales only (micro- or meso-level).

For the description of the macroscopic behavior of SMA materials, we have to account for

effects like grain boundaries, or even within a single grain, lattice faults and impurities.

These effects have an impact in particular on the energy barrier separating two phases from

one another. In contrast to the perfect single crystal, where each mesoscopic lattice particle

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saw the same energy barrier, it will now be assumed that each lattice particle can

poten-tially have a barrier of its own, see Figure 3.1 (top left). Note that barriers are restricted to

unstable concave regions, which are also known as spinodal regions. The minimum barrier

is the one represented by the well known tangent construction from equilibrium

thermody-namics. Any barrier with a convex shape would actually not represent a barrier and destroy

the multi-phase character of the energy.

Figure 3.1: Effect of distribution in barrier (left) and internal stress (right). In addition to the aforementioned effects, inhomogeneity leads to another mechanism

that needs to be accounted for in order to describe the macroscopic behavior realistically.

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transforming particles, a particular lattice particle does not necessarily see the externally

applied stress σ only, but an additional interaction stress σi superimposed to it. This

leads to the concept of an effective stress σef f = σ+σi, which drives the actual material

response. This is similar to well known concepts in magnetics, see, e.g., [10]. In addition to

different barriers, lattice particles may thus also see differently distorted energy landscapes,

which biases the resulting barriers in one direction. This effect is illustrated in Figure 3.1

(top right). The center row of Figure 3.1 shows the stress-strain diagrams resulting from

the various energies in the top row. It can be seen that different energy barriers lead to

hysteresis loops with different thicknesses. The higher the energy barrier the thicker the

hysteresis, and the minimum barrier corresponds to a zero thickness hysteresis, indicating

a reversible transformation at the so-called Maxwell stress.

As we are interested in the resulting macroscopic behavior, we do not resolve the spatial

location of each lattice particle with its corresponding combination of energy barrier and

effective stress. We rather assume a certain distribution, characterized by a probability

density function, giving the fraction of particles with a particular combination, which

actu-ally exist in the control volume. We then apply a stochastic homogenization procedure to

compute the average strain in the control volume based on

εave=

Z +∞

σM axw

Z +∞

−∞

ε(σi, σA)fi(σi)fA(σA)dσidσA (3.1)

In Eq. (3.1),

ε(σi, σA) =

σ+σi

EM

·

x+(σi, σA) +x−(σi, σA) +

EM

EA

xA(σi, σA)

¸

(3.2)

+ [xA(σi, σA)−x−(σi, σA)]εT

denotes the strain contribution of a lattice particle with energy barrier and interaction stress

σA, σi,respectively, andfi(σi)andfA(σA)are the probabilities to encounter a particle with

these values. The distribution in energy barriers is best formulated in terms of the barrier

stresses σA and σM, representing the upper and lower plateau stresses of the hysteresis

loops in the center row of Figure 3.1. Because of the definition σ :=∂ψ/∂ε, these stresses are identified as the slopes of the Helmholtz free energy functionψat the connection points

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the Maxwell stressσMaxw,respectively, and their distributions are shown as clipped normal

distributions together with the normal distribution inσi in the bottom row of Figure 3.1.

3.1.1

Stress vs. Strain Control

A similar version of this model has already been presented in [58] and [59] for the case

of stress control using Equation (3.1). Typically however, experiments with SMAs are

conducted in strain control mode, in particular when the rate-dependent behavior is studied.

For this purpose we have to invert (3.1) such that the stress can be computed in response

to prescribed strain. Substitution ofε(σi, σA) in (3.1) using (3.2) results in

εave =σI1+I2+I3 (3.3)

where

I1 =

Z +∞

σM axw

Z +∞

−∞ 1 EM

·

x+(σi, σA) +x−(σi, σA) +

EM

EA

xA(σi, σA)

¸

(3.4)

×fi(σi)fA(σA)dσidσA

I2 =

Z +∞

σM axw

Z +∞

−∞ σi

EM

·

x+(σi, σA) +x−(σi, σA) +

EM

EA

xA(σi, σA)

¸

(3.5)

×fi(σi)fA(σA)dσidσA

I3 =

Z +∞

σM axw

Z +∞

−∞

εT[xA(σi, σA)−x−(σi, σA)] (3.6)

×fi(σi)fA(σA)dσidσA .

Inverting Eq. (3.3) and using (3.4) - (3.6), we can now easily determine the external

stress in the SMAσ as

σ = ε−I2−I3 I1

. (3.7)

All of the integrals can be solved numerically using a Gaussian quadrature method, e.g.,

εave= NA X m=1 Ni X n=1

wnmε(σi,n, σA,m)fi(σi,n)fA(σA,m) (3.8)

for Eq. (3.1).

When the strain is prescribed as a function of time, we proceed to solve for the stress

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1. Choose a suitable number of integration points. The Gauss method automatically

determines the abscissae pointsσi,n,andσA,m and the corresponding weightswnm.

2. For given initial valuesx±(0),wefirst compute the integralsI1−I3 from (3.4) - (3.6).

then

3. Determine the stress σ from (3.7).

4. Solve the system (2.4), (2.5), (2.30) for each single crystal with σef f =σ+σi,n, and

σA,m to compute new phase fractions at time t1.

5. Compute the new stress again from (3.7).

6. Repeat steps 2 - 5 until thefinal time is reached.

In Figure 3.4 we show results for both loading types for a very small number of

inte-gration points (3×3). It is clear that this number is not sufficient to represent smooth hysteresis curves, but it allows us to illustrate the underlying mechanisms and to highlight

the differences between the two loading types. Instead of the normal distribution shown in

Figure 3.1, we use the Laplace distribution, which for a number of observed hysteresis loops

gives a better description of the hysteresis shape. The Laplace distribution is defined as

fi(σi) =

1 2bi

exp

µ

−|σi−µi|

bi

, (3.9)

where µi denotes its mean value and bi its variance. In the above case of interaction

stress, we typically assume µi = 0, since positive and negative interaction stresses should be equally probable. For the barrier stresses, we assume

fA(σA) =

1 2bA

exp

µ

−|σAb−µA|

A

, (3.10)

with non-zero mean value µA.Note that this distribution is again clipped to begin at the Maxwell stress. The top row of Figure 3.4 shows the isothermal pseudoelastic behavior

resulting from a piecewise linear loading input ε(t) and σ(t), respectively (bottom row). The jagged behavior is the result of single crystals with corresponding effective barrier

transforming from austenite to martensite as the load increases. The width of the steps is

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results in only a small increase in strain when they transform, and a larger number causes a

larger increase in strain. In both cases, the probability distribution has a rather pronounced

maximum at about the stress value, where the plateau is largest.

Figure 3.2: Comparison of strain and stress control for 9 integration points. In comparison, both cases show a similar but not identical hysteresis loop, in fact, the

strain-controlled case predicts a somewhat thinner loop and a larger transformation strain.

Inspection of Figure 3.2, which shows the time evolution of the phase fractions of each of

the 9 lattice particles involved, reveals that the kinetics of the two processes differ as well.

The stress-controlled case is characterized by instantaneous complete transformations, once

it is triggered by the external stress reaching a suitable value, while the strain-controlled

case shows a linearly increasing phase fractions, of which the slope depends on the number

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a perfect single crystal with a box-shaped hysteresis loop as shown in Chapter 2, Figure 2.8

becomes unstable as soon as the stress level corresponding to the transformation plateau is

exceeded, while under strain-control it can be stabilized at each point along the plateau.

3.1.2

Convergence Analysis

Of course, the above plots do not give a reliable presentation of the stress-strain loop due to

the small number of integration points. It cannot be expected that the Gauss quadrature

has already converged for only (3×3) points, and in Figure 3.4, we study the evolution of the hysteresis loop as we increase the number of these integration points. The center

and the bottom row show the two distribution functions from Eqns. (4.14) and (4.13)

and the location of the Gauss points for a (3×3),(9×9),and (25×17)case. Comparing the first two cases, we find that the result of the "underintegration" had not only led to a non-smooth hysteresis shape, but also to a considerable underestimation of the total

transformation strain. The increase to(25×17)improves the smoothness of the hysteresis curve only, and we can consider this case to have sufficiently converged. If we inspect the

computation times shown in the header of the top row above each subfigure, however, we

see that this comes at a tremendous price. The increase in computation time from case 1

to case 2 is 226-fold, and from case 2 to case 3 is another 115 times. While the(3×3)case can be solved in 2.5 s,the total computation time for the most accurate case is thus more

than 18 hours on a typical 1 GHz PC.

The above case was solved for isothermal behavior. Subsequently, we study the

non-isothermal behavior caused by the rate-dependent release and absorption of latent heats.

For this purpose, we have to take the balance of internal energy into account as already

done for the single crystal case, see Eq. (2.30). We again assume heat conduction to

be very efficient within the material such that we can assume the temperature still to be

homogeneous, even though the latent heats are now being released and absorbed in an

in-homogeneous manner. If we average the energy balance (2.30) in the same way as we did

the strain in (3.1), we obtain:

ρcVT· =hAs(T−T0) +j(t)− D·

x+(σi, σA)H+(σi)

E

V

D·

x(σi, σA)H−(σi)

E

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Figure 3.4: Convergence behavior for isothermal tensile experiment. where

D·

x±(σi, σA)H±(σi)

E

=

Z +∞

σM axw

Z +∞

−∞

h·

x±(σi, σA)H±(σi)

i

(3.12)

×fi(σi)fA(σA)dσidσA

NA X

m=1

Ni X

n=1

wnm

h·

x±(σi,n, σA,m)H±(σi,n)

i

(3.13)

×fi(σi,n)fA(σA,m)

It appeared from Figure 3.4 that the large number of Gauss points had provided a

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at constant temperature, Figure 3.5 shows that this is not the case when we look at the

non-isothermal case. Even for (25×17) Gauss points, the temperature still exhibits a jagged behavior, see Figure 3.5 (center row). The reason can be identified from the bottom row of

the figure, which shows the production term due to the latent heats (3.13). Even though the mechanical aspects of the step-wise transformation have been smoothed out, the release

of latent heats is still discontinuous and leads to oscillations in the temperature. We did

not increase the number of Gauss points further to remove this behavior, however, as the

computation time was already unacceptably high.

3.1.3

E

ects of Distribution Parameters

Instead, in the final part of this chapter, we concentrate on the effect of the distribution parameters on the hysteresis shape. Figure 3.6, shows the variation of the hysteresis, when

we change the variance parametersbiandbA.The former increases along the axis denoted by

fs,while the latter increases along thefb-axis, essentially broadening the distributions. The

upper lefthand plot closely represents the single crystal case with very narrow distributions

about the means, and we see that the effect of broadening the range of the barrier stress

σA is to tilt the plateau and distort the outer hysteresis loop. However, we can also see

that it has an impact on paths in the interior of the hysteresis. It seems as if the inner

unloading paths are lifted against the outer one, and if we look carefully we realize that,

upon unloading, the material initially moves into the hysteresis on a reversible path as in

the single crystal case. No transformation takes place on this part until the Maxwell stress

is reached. This is to be expected as the particles corresponding to the Maxwell stress are

the ones with the lowest (no) energy barrier, and should be the ones to jump backfirst. Looking down the first row of the matrix, we can see that as the distribution in inter-action stress also tilts the outer loop, it does not have an impact on the inner hysteresis

behavior. As a wider range in these stresses helps to trigger the onset of the transformation

at a lower external stress level, there is no restriction to the Maxwell stress for this

distri-bution. In fact we see that by a suitable superposition of these parameters, we can realize

a considerable spectrum of inner hysteresis paths.

Figure 3.7 focuses on inner loops resulting from partial unloading and reloading, and we

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Figure 3.7: Pseudoelastic material behavior due to different distribution combinations, 2nd order loops

choices of the parameters is actually very close to what is observed experimentally.

However, as was already pointed out in the foregoing, the associated computation times

are extremely high. In particular if one were to think about potential implementations

into finite element or optimal control codes, they become prohibitive despite the good description of the material behavior. It will be the subject of the subsequent chapter to

develop a method, which preserves the positive aspects of the model, while considerably

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Parameterization Method - Representative Single

Crystal

The motivation for this chapter is to present a SMA model that combines the capabilities of

the version introduced in the preceding chapter with high computational efficiency. This is

necessary for a potential implementation into other numerical codes, such asfinite element or optimal control programs or a Matlab/Simulink environment. For this purpose we will

introduce a parameterization method leading to the concept of a representative single crystal

and illustrate it for the simple case of only one distribution in eitherσAorσi.Subsequently,

we will derive the method for the more complex case of the two combined distributions from

the previous chapter and show its equivalence with the model presented therein. Finally, we

show that the method does not even need the determination of distributions, rather, based

on direct experimental determination of the barriers, it can reproduce the experimentally

observed behavior very accurately over a large range of strain rates including the minor

loop behavior.

4.1

Concept of Parameterization

The major factor hampering the performance of the Gauss Quadrature method from the

previous chapter is the necessity to solveN ×M single crystal ODE systems, withN and

M representing the number of integration points for the two distributions in barrier stress

σAand interaction stressσi, respectively. This is based on the idea of an ensemble of single

crystals with independent combinations of these two quantities, and in order to make the

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evaluation of the problem more efficient, we are going to re-interpret the phase

transfor-mation process. Instead of considering the N ×M physical single crystals, we will now focus our attention on the one that is always the next in sequence to undergo the

transi-tion to the other phase. We will thus follow arepresentativesingle crystal, which means we actually switch focus from one physical crystal to the one with the next higher barrier

once it has transformed. As a consequence, this representative element sees a barrier which

changes during the process as the physical elements undergo transformations. The barrier

will increase during the loading part of the process and decrease during unloading. With

this process we have effectively parameterized the transformation by the phase fraction; and

the major advantage is that we only need to solve one ODE system as in the single crystal

case rather thanN ×M as in the previous chapter. The only formal difference is that the

barrier stress entering the transition probabilities, see Eq. (2.18,2.21) has now become a

function of the phase fraction σA(x),and this chapter will be devoted to the discussion of

the consequences of this difference.

4.1.1

Parametrization Method for a Single Distribution

We will start with the case of a single distribution in order to better illustrate the method.

Figure 4.1 shows three exemplary lattice elements with different energy barriers and thus

different barrier stresses σA for the pseudoelastic case. Here, austenite is the stable phase

and has the lowest minimum. The element at the bottom of each set represents the Maxwell

case with zero additional energy barrier, while the center and top elements have increasingly

higher barriers. During a loading process, the elements are initially all in the austenitic

phase. An applied positive stress lowers the energy barrier to the neighboring martensite

phase and favors the corresponding minimum. At a load level represented by external stress

σ2(coinciding with the Maxwell stressσM axw), the element with the lowest barrier performs

the transition to martensiteM+.Atσ3, the second one follows, and atσ4, all three elements

have transformed to M+. Unloading back to σ3, all of them remain martensitic, because

the barrier for the reverse jump back to austenite is still present (indicating a hysteresis).

Upon further unloading they consecutively transform back in the same order with the lowest

Figure

Figure 2.1: Lattice particle of a shape memory alloy in its possibel phases autenitsmartensite A and M±.
Figure 2.2: Typical layer structure.
Figure 2.5: Free energy of a lattice layer for different temperatures.
Figure 2.6: Free energy for a lattice layer for T = 328K and different loads.
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References

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