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    The Physics of Deformation and Fracture of Polymers

    Demonstrating through examples, this book presents a mechanism-based

    perspective on the broad range of deformation and fracture responses of solidpolymers. It draws on the results of probing experiments and considers the similar

    mechanical responses of amorphous metals and inorganic compounds to develop

    advanced methodology for generating more precise forms of modeling. This, in

    turn, provides better fundamental understanding of deformation and fracture

    phenomena in solid polymers. Such mechanism-based constitutive response forms

    have far-reaching application potential in the prediction of structural responses

    and in tailoring special microstructures for tough behavior. Moreover, they can

    guide the development of computational codes for deformation processing of 

    polymers at any level. Applications can range from large-strain industrial deform-ation texturing to production of precision micro-fluidic devices, making this book

    of interest both to advanced graduate students and to practicing professionals.

    A li S . A rg on   is Quentin Berg Professor Emeritus in the Department of 

    Mechanical Engineering at Massachusetts Institute of Technology (MIT). He is

    recognized world-wide as an authority on the mechanical behavior of engineering

    solids, has published over 300 papers and three books, and is one of the inter-

    nationally most widely cited authors in materials science. He has received a

    number of honors and awards, including membership of the US National Acad-

    emy of Engineering, Fellowship of the American Physical Society, DistinguishedLife Membership of the Alpha Sigma Mu (International Professional Society

    of Materials and Engineering), the Nadai Medal of the American Society of 

    Mechanical Engineers, the Heyn Medal of the German Society for Materials

    Science, and a US Senior Scientist Award of the Alexander von Humboldt

    Foundation for research in Germany.

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    The Physics of Deformation

    and Fracture of Polymers

     A . S . A R G O N

    Massachusetts Institute of Technology

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    c a m b r i d g e u n i v e r s i t y p r e s s

    Cambridge, New York, Melbourne, Madrid, Cape Town,

    Singapore, Sa ˜o Paulo, Delhi, Mexico City

    Cambridge University PressThe Edinburgh Building, Cambridge CB2 8RU, UK

    Published in the United States of America by

    Cambridge University Press, New York

    www.cambridge.org

    Information on this title:  www.cambridge.org/9780521821841

    © A. S. Argon 2013

    This publication is in copyright. Subject to statutory exception

    and to the provisions of relevant collective licensing agreements,

    no reproduction of any part may take place without

    the written permission of Cambridge University Press.

    First published 2013

    Printed and bound in the United Kingdom by the MPG Books Group

     A catalog record for this publication is available from the British Library

     Library of Congress Cataloging-in-Publication Data

    Argon, Ali S.

    The physics of deformation and fracture of polymers / A. S. Argon, Massachusetts Institute of 

    Technology.

    pages cm

    Includes bibliographical references and indexes.

    ISBN 978-0-521-82184-1

    1. Polymers–Fracture. 2. Polymers–Plastic properties. 3. Plastics. I. Title.

    TA455.P58A74 2013

    620.10920413–dc23

    2012025871

    ISBN 978-0-521-82184-1 Hardback

    Cambridge University Press has no responsibility for the persistence or

    accuracy of URLs for external or third-party internet websites referred toin this publication, and does not guarantee that any content on such

    websites is, or will remain, accurate or appropriate.

    http://www.cambridge.org/http://www.cambridge.org/9780521821841http://www.cambridge.org/http://www.cambridge.org/9780521821841http://www.cambridge.org/9780521821841http://www.cambridge.org/

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    This book is dedicated to

    Ian M. Ward of Leeds University for his long-term friendship

    and tomy wife Xenia for her enduring support

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    “An insightful exposition from one of the most influential material scientists

    of our time. A must read for anybody wishing to gain a mechanician’s

    (not a chemist’s!) perspective on the physics and mechanics of polymers.”Vasily Bulatov, Lawrence Livermore National Laboratory 

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    Contents

     Preface page xv

    Symbols   xviii

     Frequently used abbreviations   xxii

    1 Structure of non-polymeric glasses   1

    1.1 Overview   1

    1.2 Glass formability in metallic alloys   3

    1.3 Atomic packing in disordered metallic solids   3

    1.4 Energetic characterization of the structure of metallic glasses   7

    1.4.1 The atomic site stress tensor   7

    1.4.2 Calorimetry   9

    1.5 Free volume   10

    1.6 Viscosity of glass-forming liquids   14

    1.7 Structural relaxations   16

    1.7.1 A computational model   16

    1.7.2 Kinetic models of structural relaxations in metallic glasses   20

    1.8 The distributed character of structural relaxations and the

    glass transition   21

    1.9 The dependence of the glass-transition temperature on cooling rate   25

    1.10 Crystallization in bulk metallic glasses   26

    1.11 Deformation-induced alterations of atomic structure in sub-cooled

    liquids and glasses   271.12 The range of metallic alloys that have been obtained as bulk

    metallic glasses   30

    1.13 The structure of amorphous silicon   30

    1.14 Characterization of the structure of amorphous silicon   32

    Suggested further reading on structure of non-polymeric glasses   36

    References   37

    2 Structure of solid polymers   40

    2.1 Overview   402.2 Structure of polymers   41

    2.3 Molecular architecture   46

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    2.4 Molecular weight   47

    2.5 Structure of amorphous polymers   49

    2.5.1 Molecular-structure models of amorphous polymers   49

    2.5.2 Chemically specific molecular-structure models of amorphous polymers   49

    2.5.3 Chemically non-specific models of amorphous polymer

    structure   53

    2.5.4 Experimental means of characterization of the structure

    of glassy polymers   54

    2.6 Crystalline polymers   54

    2.6.1 The fringed-micelle model of semi-crystalline polymers   54

    2.6.2 Spherulites   55

    2.6.3 Hedrites   58

    2.6.4 Polymer single crystals   58

    2.6.5 Crystallization from the melt and growth of spherulites   61

    2.7 Defects in polymer crystals   66

    2.7.1 Overview   66

    2.7.2 Chain defects   67

    2.7.3 Lattice defects   71

    2.8 Chain-extended polymers   71

    Suggested further reading on structure of solid polymers   72

    References   73

    3 Constitutive connections between stress and strain in polymers   77

    3.1 Overview   77

    3.2 Stresses and strains   77

    3.2.1 Stresses   77

    3.2.2 Strains   78

    3.3 Linear elasticity of polymers   81

    3.4 Plasticity of polymers   83

    3.4.1 Generalized yield conditions   83

    3.4.2 The associated-flow rule   853.5 Thermally activated deformation   87

    References   89

    4 Small-strain elastic response   90

    4.1 Overview   90

    4.2 Small-strain elasticity in crystals   91

    4.2.1 The generalized Hooke’s law   91

    4.2.2 Orthorhombic crystals or orthotropic solids   93

    4.2.3 Hexagonal crystals   934.2.4 Cubic crystals   93

    4.2.5 Isotropic materials   93

    viii   Contents

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    4.2.6 Temperature and strain dependence of elastic response   95

    4.3 Theoretical determination of elastic constants of polymers   96

    4.3.1 Glassy polymers   96

    4.3.2 Crystalline polymers   974.4 Elastic response of textured anisotropic polymers   102

    4.5 Elastic properties of heterogeneous polymers   104

    4.5.1 Methods of estimating the elastic properties of 

    heterogeneous polymers   104

    4.5.2 The self-consistent method   105

    4.5.3 The Eshelby inclusion method   106

    References   109

    5 Linear viscoelasticity of polymers   112

    5.1 Introduction   112

    5.2 Phenomenological formalisms of viscoelasticity   112

    5.2.1 Uniaxial creep or stress-relaxation response   112

    5.2.2 Dynamic relaxation response   116

    5.2.3 Temperature dependence of viscoelastic relaxations   118

    5.3 Viscoelastic relaxations in amorphous polymers   120

    5.3.1 The  α-relaxation   120

    5.3.2 The free-volume model of the  α-relaxation   122

    5.3.3 Dependence of the α-relaxation on the chemical structure

    of molecules   126

    5.3.4 Secondary relaxations in the glassy regime   127

    5.3.5 Effect of physical aging on the relaxation spectra of polymers   130

    5.3.6 Secondary relaxations in polycarbonate of bisphenol-A   132

    5.4 Shear relaxations in partially crystalline polymers   139

    5.5 Some problems of viscoelastic-stress analysis   143

    5.6 Non-linear viscoelasticity   145

    Suggested further reading on linear viscoelasticity of polymers   146

    References   146

    6 Rubber elasticity   148

    6.1 Overview   148

    6.2 Molecular characteristics of rubbers   149

    6.2.1 Distinctive features of rubbers   149

    6.2.2 The chemical constitution of rubbers   151

    6.3 Thermodynamics of rubbery behavior   151

    6.4 The Gaussian statistical model of rubber elasticity   155

    6.5 The non-Gaussian statistical model of rubber elasticity   159

    6.5.1 The freely jointed single chain   1596.5.2 Langevin networks   161

    6.5.3 Comparison of the Langevin-network model with experiments   164

    ixContents

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    6.6 Modes of deformation in rubber elasticity   167

    6.6.1 Conditions for general response   167

    6.6.2 Uniaxial tension or compression   167

    6.6.3 Equi-biaxial stretch   1686.6.4 Plane-strain tension and pure shear   168

    6.6.5 Simple shear   169

    6.6.6 Plane-strain compression flow in a channel die   171

    6.7 Gaussian rubbery-type response in glassy polymers   172

    References   172

    7 Inelastic behavior of non-polymeric glasses   174

    7.1 Overview   174

    7.2 The mechanism of plasticity in non-polymeric glasses   1757.3 The kinematics of plasticity in glassy solids by shear transformations   176

    7.4 Nucleation of shear transformations under stress   179

    7.4.1 The elastic strain energy of a shear transformation in the

    unstressed solid   179

    7.4.2 The Gibbs free energy of nucleation of the shear

    transformation under stress   180

    7.4.3 Stages in the nucleation of the shear transformation   181

    7.5 Yielding in metallic glasses   185

    7.5.1 Behavior at low temperatures (T   T g)   185

    7.5.2 Temperature dependence of the yield stress (T   T g)   187

    7.5.3 Analysis of the experimental results on yield behavior of 

    metallic glasses at low temperatures   188

    7.5.4 Yielding in metallic glasses at temperatures close to T g   189

    7.5.5 Changing kinetics of plasticity near T g   193

    7.6 Post-yield large-strain plastic response of glassy solids: strain

    softening and strain hardening   199

    7.6.1 Features of large-strain plastic flow of glassy solids   199

    7.6.2 Plastic-flow-induced increase in the liquid-like

    material fraction,  φ   2007.6.3 Plastic-strain-induced changes in structure and the kinetics

    of associated evolutions of  φ   203

    7.6.4 Kinetics of large-strain plastic flow of glasses at T   T g   205

    7.6.5 Kinetics of large-strain plastic flow of glasses at  T  close to  T g   207

    7.6.6 Multi-axial deformation: correspondences of shear, tension,

    and compression at low temperatures   210

    7.7 The strength-differential effect in disordered solids   213

    7.8 Shear localization   216

    7.8.1 The phenomenology of shear localization in metallic glasses   216

    7.8.2 The mechanics of shear localization   217

    x   Contents

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    7.8.3 Temperature rises associated with shear localization   220

    7.8.4 The flow state   221

    Appendix. Plastic-floor-induced structural alterations: the relation

    between flow dilatations of free volume and liquid-like material   222References   224

    8 Plasticity of glassy polymers   228

    8.1 Overview   228

    8.2 The rheology of glassy polymers   229

    8.2.1 Important provisos   229

    8.2.2 The phenomenology of plastic flow in glassy polymers   230

    8.3 The mechanism of plastic flow in glassy polymers   234

    8.3.1 Computer simulation of plastic flow   2348.3.2 Simulation results in polypropylene   236

    8.3.3 Simulation results in polycarbonate   238

    8.4 Temperature dependence of yield stresses of glassy polymers   243

    8.5 The kinetic model of plastic yield in glassy polymers   243

    8.5.1 Temperature dependence of the plastic resistance   243

    8.5.2 The thermal activation parameters   247

    8.5.3 A kinetic model of flow of linear-chain glassy polymers   248

    8.6 Large-strain plastic flow in glassy polymers   249

    8.6.1 Development of post-yield large-strain plastic flow   249

    8.6.2 A model for post-yield plastic flow of glassy polymers   254

    8.6.3 Stored energy and Bauschinger back strains   258

    8.6.4 The strength-differential effect and the multi-axial

    yield condition   259

    8.7 Strain hardening in glassy polymers   262

    8.8 Comparison of experiments and simulations on the yielding and

    large-strain plastic flow of glassy polymers   264

    References   270

    9 Plasticity of semi-crystalline polymers   273

    9.1 Overview   273

    9.2 Mechanisms of plastic deformation   274

    9.3 Plasticity of two semi-crystalline polymers: high-density polyethylene

    (HDPE) and polyamide-6 (Nylon-6)   276

    9.3.1 Methodology of deformation   276

    9.3.2 Plastic strain-induced alterations of spherulite morphology in

    Nylon-6 in uniaxial tension   277

    9.3.3 Large-strain plastic flow in HDPE in plane-strain compression   280

    9.3.4 Large-strain plastic flow in monoclinic Nylon-6 by plane-straincompression   291

    xiContents

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    9.3.5 Measurement of critical resolved shear stresses in textured

    HDPE and Nylon-6 and their normal-stress dependence   292

    9.4 The kinetics of plastic flow in semi-crystalline polymers   295

    9.4.1 Modes of dislocation nucleation in lamellae   2989.4.2 The strain-rate expression   301

    9.4.3 The dominant nucleation mode   303

    9.4.4 Activation volumes   304

    9.4.5 Temperature dependence of the plastic resistance   307

    9.5 Simulation of plastic-strain-induced texture development in HDPE   309

    9.5.1 Characteristics of the simulation   309

    9.5.2 Basic assumptions of the model   309

    9.5.3 Constitutive relations   311

    9.5.4 Composite inclusion   315

    9.5.5 Interaction law and solution procedure   315

    9.5.6 Parameter selection in the model   316

    9.5.7 Predicted results of the composite model and comparison

    with experiments   317

    Suggested further reading on plasticity of semi-crystalline polymers   321

    References   321

    10 Deformation instabilities in extensional plastic flow of polymers   325

    10.1 Overview   325

    10.2 Deformation instabilities in extensional plastic flow of polymers   325

    10.3 Conditions for impending localization in extensional deformation   326

    10.3.1 Basic shear response   326

    10.3.2 Basic extensional response   328

    10.4 Stability of extensional plastic flow   331

    10.5 The effect of strain-rate sensitivity on stability in extensional

    plastic flow   333

    10.5.1 In the onset of necking   333

    10.5.2 In the post-necking behavior   335

    10.6 Plastic drawing of polymers   336References   341

    11 Crazing in glassy homo- and hetero-polymers   342

    11.1 Overview   342

    11.2 The phenomenology of crazing in glassy homo-polymers   343

    11.3 Simulation of cavitation in a glassy polymer at the atomic level   345

    11.4 Craze initiation   347

    11.4.1 Experimental observations   347

    11.4.2 Intrinsic crazing   34911.4.3 Tension–torsion experiments   349

    11.5 A craze-initiation model   353

    xii   Contents

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    11.6 Comparison of the predictions of the craze-initiation model with

    experiments   356

    11.7 Craze growth   359

    11.7.1 Craze stresses   35911.7.2 Craze microstructure   364

    11.7.3 Craze-growth experiments   366

    11.8 A craze-growth model   368

    11.9 Comparison of the craze-growth model with experiments   374

    11.10 Crazing in block copolymers   376

    11.10.1 Morphology of diblock copolymers   376

    11.10.2 Crazing experiments in PS/PB diblock copolymers   378

    11.10.3 A model of craze growth in a PS/PB diblock copolymer

    with spherical PB domains   381

    11.10.4 Comparison of the predictions of the craze-growth model

    in PS/PB diblock copolymers with experiments   385

    References   387

    12 Fracture of polymers   391

    12.1 Overview   391

    12.2 Cracks and fracture   391

    12.2.1 Two complementary perspectives in crack mechanics   391

    12.2.2 Cracks in LEFM   392

    12.2.3 The energy-release rate GI  in LEFM with crack extension   396

    12.3 Cracks with plastic zones   398

    12.3.1 Pervasiveness of plasticity at the crack tip   398

    12.3.2 Cracks with small-scale yielding (SSY)   399

    12.3.3 Crack-tip fields with contained plasticity   404

    12.3.4 Crack fields in fully developed plasticity   407

    12.4 Stability of crack advance   414

    12.5 Intrinsic brittleness of polymers   416

    12.6 Brittle-to-ductile transitions in fracture   418

    12.7 Mechanisms and forms of fracture in polymers   41912.7.1 The crack-tip process zone   419

    12.7.2 The role of chain scission in polymer fracture   419

    12.7.3 Fracture of unoriented polymers   420

    12.7.4 Cohesive separation   420

    12.7.5 Fracture in glassy polymers involving crazing   422

    12.7.6 Molecular-scission-controlled fracture of oriented

    semi-crystalline polymers   425

    12.7.7 Fracture toughnesses of a selection of polymers   428

    12.8 Impact fracture of polymers   429

    12.8.1 Application of fracture mechanics to impact fracture   429

    12.8.2 Fracture of polymers at high strain rate   431

    xiiiContents

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    Suggested further reading on fracture of polymers   432

    References   433

    13 Toughening of polymers   435

    13.1 Overview   435

    13.2 Strategies of toughening of polymers   436

    13.3 Different manifestations of toughness in polymers   437

    13.4 The generic fracture response of polymers in uniaxial tension   438

    13.5 Toughening of crazable glassy polymers by compliant particles   440

    13.5.1 Types of compliant composite particles   440

    13.5.2 Brittleness of glassy homo-polymers and alleviating it

    through craze plasticity   443

    13.5.3 The mechanism of toughening in particle-modified crazableglassy polymers   445

    13.5.4 Elasticity of compliant particles   447

    13.5.5 Craze initiation from compliant particles and the craze-flow

    stress   449

    13.5.6 The role of compliant-particle size in toughening

    glassy polymers   449

    13.5.7 A model for the craze-flow stress of particle-toughened

    polystyrene   452

    13.5.8 Special HIPS blends prepared to evaluate the

    toughening model   454

    13.5.9 Comparison of the behavior of special HIPS blends

    with model predictions   457

    13.6 Diluent-induced toughening of glassy polymers   459

    13.6.1 Different manifestations of toughening with diluents   459

    13.6.2 Factors affecting diluent toughening of PS   462

    13.6.3 A model of diluent-induced toughening of glassy polymers   465

    13.6.4 Comparison of the diluent-induced-toughening model with

    experiments   472

    13.7 Toughening of semi-crystalline polymers   47513.7.1 Toughness of unmodified HDPE and polyamides of 

    Nylon-6 and -66   475

    13.7.2 Toughening semi-crystalline polymers by particle

    modification   477

    13.8 Toughening of brittle thermosetting polymers   492

    References   497

     Author index   501

    Subject index   507

    xiv   Contents

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    Preface

    The chemistry and physics of polymers, and their molecular microstructure,

    morphology, and larger-scale organization have been extensively studied and

    described in many treatises.

    In comparison the plastic deformation and fracture processes, both in the

    laboratory and in industrial practice, have largely been dealt with at a phenom-

    enological level, and often separately for different polymers and blends, rather

    than from a unified and comprehensive mechanistic perspective. This has left the

    mechanisms governing the deformation and fracture resistance of polymers far

    less well understood.

    On the other hand, fundamental developments in polymer physics and polymer

    materials science in the recent past are now making it possible to consider broad

    ranges of their deformation and fracture from a mechanistic point of view at an

    appropriate molecular and morphological level. Moreover, insight gained fromstudies of corresponding responses of amorphous metals and semiconductors,

    reinforced by computational simulations and mechanistic modeling, has also

    broadened the perspective.

    The purpose of this book is to present a coherent picture of the inelastic

    deformation and fracture of polymers from a mechanistic point of view, addressed

    to graduate students of material science and mechanical engineering and to

    professional practitioners in the field.

    The book concentrates heavily on research conducted at the Massachusetts

    Institute of Technology from the mid 1980s to the mid 2000s by the author and

    a group of collaborators. It reports on extensive experimental studies and related

    computational simulations. In the latter there is much emphasis on development

    of mechanistic models ranging from unit plastic relaxation events to the evolution

    of deformation textures in channel die compression flow to large plastic strains. At

    every level the experimental results are compared in detail with predictions from

    the models.

    The core of the book is devoted to subjects starting with anelastic behavior of 

    polymers and rubber elasticity, but proceeds with greater emphasis in following

    chapters to mechanisms of plastic relaxations in glassy polymers and semi-

    crystalline polymers with initial spherulitic morphology. Other chapters concen-trate on craze plasticity in homo-polymers and block copolymers, culminating

    with a chapter on toughening mechanisms in brittle polymers. To make the

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    main chapters on plastic flow and toughening tractable to the reader, the book

    starts with a brief tutorial chapter devoted to the structure of polymers from the

    chain molecular levels to morphological aggregation of crystalline lamellae and

    their further aggregation into spherulites. Since unit plastic relaxations arecomplex phenomena in glassy polymers, which, however, exhibit parallel phe-

    nomena that can be followed more transparently in amorphous metals and

    amorphous silicon, a chapter is also included at the start on the atomic structure

    of such simpler elemental glasses. Finally, since fracture involves propagation of 

    cracks emanating from notches, with crack tips being modified by plastic zones

    of various levels of pervasiveness, a relatively comprehensive chapter on fracture

    mechanisms and mechanics is included to precede the chapter on toughening

    mechanisms.

    Each chapter starts with an overview laying out the topics to be presented to

    give an overall perspective. Copious references are provided at the ends of chap-

    ters, often supplemented with lists of additional references that develop some

    topics in greater depth.

    It is assumed that the reader has had an introductory course on materials

    science and perhaps on polymers such as e.g.   An Introduction to the Mechanical

     Properties of Solid Polymers  by I. M. Ward and J. Sweeney, John Wiley & Sons,

    second edition 2004.

    Clearly, the present book covers in depth only a narrow subject area on the

    mechanical response of polymers; thus, as such, it is not intended as a review. The

    informed reader will note that much work of other investigators falling outsidethe main scope has not been included. This omission is intentional, in order to

    preserve a coherent central perspective.

    Many colleagues at various levels contributed significantly to the conduct of 

    the research discussed in the book and the overall development of the subject of 

    this book, either in experimentation or in computational modeling. These

    include, in order of depth of involvement, R. Cohen, U. Suter, A. Gałęski,

    Z. Bartczak, E. Pio ´ rkowska, H. Brown, D. Parks, O. Gebizlioglu, S. Ahzi,

    M. Hutnik, P. Mott, O. Muratoglu, B. Lee, J. Vancso, J. Qin, and G. Dagli.

    In private discussions on many aspects of polymer research, G. Rutledge con-

    tributed some important perspective. M. Weinberg of DuPont supplied specially

    pedigreed polymer samples and blends for the experimental studies. P. Geil,

    B. Wunderlich, E. Kramer, and E. Ma generously furnished electronic files of 

    some key micrographs and computer-generated images. The text was prepared,

    and numerous modifications were implemented, always cheerfully, by Doris

    Elsemiller. The illustrations were ably produced by Andrew Standeven. All this

    would not have been possible without funds provided by Deans T. Magnanti

    and S. Suresh and Department Heads R. Abeyaratne and M. Boyce. Finally,

    the very thorough copy-editing by Dr. Steven Holt on behalf of Cambridge

    University Press that uncovered a number of inconsistencies in referencingbetween the text and the lists of references at the ends of chapters is also

    gratefully acknowledged.

    xvi   Preface

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    The serious entry of the author into the field of deformation and fracture of 

    polymers started in 1971 during a sabbatical leave at Leeds University in Britain

    with Professor Ian Ward. The friendly association with Ward has continued until

    the present. For this reason the book is dedicated first of all to him in appreciationof his long-term friendship. Secondly, however, the book is dedicated in equal

    measure to my wife Xenia for her enduring support.

    xviiPreface

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    Symbols

    All mathematical symbols are fully defined in the text where they are introduced.

    Some material parameters have been referred to by different symbols, preserving

    their usage in the literature.

     A   area of bar A0   area of perfect bar B(v, β ) energy factor in STC   proportionality factor

     D   diameter of craze fibril; diameter of particle Dc   critical particle diameter for craze initiation D0   mean spacing of craze fibrils E   Young’s modulus F   Helmholtz free energy

     F0   self Helmholtz free energy of ST Fint   interaction (Helmholtz) energy with σ m of STΔ F0   ¼ F0þ FintΔ Fv   activation free energy for viscous flowFe   edge-dislocation line energyFs   screw-dislocation line energyGI   mode I energy-release rateGIC   critical mode I energy-release rate for crack advanceΔG* Gibbs free energy of activationΔ H * activation enthalpy

     I n   normalization factor for stresses in J   integral field J I   J  integral non-linear crack-tip energy-release rate J IC   critical  J  integral crack driving force J U   unrelaxed creep compliance J R   relaxed creep compliance K I   mode I stress intensity factor K IC   critical mode I stress intensity factor for crack growth in plane strain K S   critical mode I stress intensity factor for crack growth for plane stress K C   mode I stress intensity factor for growth of cracks between plane stress

    and plane strain:  K S> K C> K IC L   load on deforming barL    Langevin function

     M e   entanglement molecular weight in rubbers

     M n   number-average molecular weight M w   weight-average molecular weight M w/ M n   polydispersity ratio

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     N    strain exponentQ   Heat; dQ, heat increment

     R   rate; universal gas constant

     RSD   strength differential ratioS   entropy; dS, change in entropyT    temperatureT 0   (¼ΔG

    */k )T BD   brittle-to-ductile transition temperatureT g   glass-transition temperatureT m   melting temperatureU    internal energy; dU , change in internal energyV    volumeW p plastic work; dW p, increment of plastic workY    tensile uniaxial yield strength

    Y c   intrinsic craze yield stressY 0   athermal tensile yield strengthY C   yield strength in compressionY T   yield strength in tensiona   crack length; Cartesian coordinate axisa0   molecular diameteraT    viscoelastic shift factorb   Burgers vector; Cartesian coordinate axisc   Cartesian coordinate axis; volume fractioncf    fraction; free-volume fractioncij    Voigt elastic constant elementcijkl   tensor elastic constant elementeij    Voigt deviatoric strain element

     f    fraction f a   amorphous fraction f c   crystalline fractiong( λ) (¼ λ2 1/ λ) Gaussian orientation hardening functionk    Boltzmann’s constant; yield strength in sheark r   rate constantl   monomer link length; generic lengthl_   elongation ratem   (¼ dln  γ_/dln  σ ) phenomenological stress exponentmT   Taylor factor in polycrystalline aggregates

     p   pressureq   cooling rater    radial coordinates   applied simple shear stress, deviatoric shear stresss0   athermal shear resistancesij    Voigt elastic compliancesijkl   tensor compliance elementt    timet f    time to fractureur   radial displacementuθ    angular displacement

    uz   axial displacementvf    volume fractionz   polar coordinate axis

    xixSymbols

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     x,  y,  z   Cartesian axesF   fluidityΔ   process-zone length

     χ    interface energy, crystallinityΛ   matrix ligament thicknessΛc   critical matrix ligament thickness where a toughness jump occursO   atomic volumeOf    volume of ST clusterOmon   monomer volumeα   proportionality constantα   (¼ τ ̂/ μ(0)) normalized threshold shear resistanceαb   (¼ vcb/vc) proportionality factor between craze-border velocity and

    craze-tip velocity β    (¼ ε T/γT) activation dilatancy

     β    level of porosity, secondary relaxation β e   activation-energy attenuation factorγ   tangential shear strainγp plastic shear strain (deviatoric)γT transformation shear strain_γ   shear strain rate_γp plastic shear strain rate_γe elastic shear strain rate_γ0   frequency factor in thermal activationδ   crack-tip opening displacementδij    Kronecker deltaε    normal strainε T free-standing transformation strain tensor

    ε C constrained transformation strain tensorε T activation dilatation (¼ βγT)ε    equivalent total normal straindε 

    pij    plastic normal strain increment

    dε    equivalent total strain incrementε TC   craze strain as dilatational transformation strainε _   nominal strain rateε e   equivalent strain (deviatoric)ε 

    pf    plastic strain at fractureε y   normal strain at yield (¼ σ y/ E)

    φ   fraction, liquid-like-material fractionφs   liquid-like-material fraction at the flow state λ1,  λ2, λ3   principal extension ratios in a rubber λc   chain-extension ratio in Langevin rubbery response λL   locking stretch λe   stress-attenuation factor in activation energy λn   natural draw ratio between onset of instability and regaining of stabil-

    ity in fiber drawing, also in craze matter fibril strain μ   shear modulus μ0 storage modulus in viscoelasticity μ00 loss modulus in viscoelasticity

     μu   unrelaxed modulus in viscoelasticity μr   relaxed modulus in viscoelasticity, friction factorn   Poisson’s ratio

    xx   Symbols

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    vD   Debye frequencyvG   pre-exponential frequency factor, an eigenfrequency ρ   material density

     ρm   mobile dislocation densityσ    generally an applied shear stress, sometimes normal stress (deviatoric)σ B   brittle strengthσ 1,  σ 2,  σ 3   principal normal stressesσ c   craze-border tractionσ C   flow stress in compressionσ e   uniaxial Mises equivalent axial stressσ S   flow stress in shearσ T   flow stress in tensionσ m   mean normal stress (¼ σ n)σ TH   thermal misfit negative pressure in particle

    σ y   (¼

    Y ) uniaxial yield strengthσ    von Mises equivalent stress (¼ σ e)σ ̂   ideal cavitation strength in UBER modelσ ∞

      applied tensile stress promoting craze growthθ    angular coordinateθ    (¼ σ / μ(T )) reduced shear stress normalized with shear modulusθ    (¼ T /T g) reduced temperature normalized with the glass transition

    temperatureτ    stress tensorτ    time periodτ a   shear resistance of amorphous component in HDPEτ c   shear resistance of a crystalline component in HDPEτ ̂   threshold plastic shear resistance at T ¼ 0 Kτ ̂C   threshold uniaxial plastic resistance in compression

    xxiSymbols

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    Frequently used abbreviations

    CD constraint directionCN center-notchedCR compression ratio

    DAM dry as moldedDEN double-edge-notchedDGEBA diglycidyl ether of bisphenol-A, a common epoxy resinFD free directionHDPE high-density polyethyleneHRR Hutchinson–Rice–Rosengren (model)KRO-1 a diblock resinLD loading directionPB polybutadienePMMA polymethyl methacrylatePS polystyrene

    QSC quasi-single-crystalline (deformation texture)RH relative humidityRVE representative volume elementSANS small-angle neutron scatteringSAXS small-angle X-ray scatteringSEN single-edge-notchedST shear transformationTEM transmission electron microscopyWAXS wide-angle X-ray scattering

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    1   Structure of non-polymeric glasses

    1.1 Overview

    The principal assignment of this book is to present the physics of inelastic

    deformation and fracture of polymers, incorporating microstructural forms

    ranging from fully disordered glassy polymers to semi-crystalline morphologies

    of quite considerable crystalline perfection. While the semi-crystalline polymers

    have few, if any, parallels in morphology among other solids, the glassy polymers

    have such parallels in their atomic packing forms and morphologies in metallic

    glasses and space-network glasses, which exhibit most of the forms of structural

    relaxation, inelastic response, and fracture behavior of glassy polymers, albeit

    often in modified forms and on somewhat different scales. Since these non-

    polymeric glasses are free of the severe molecular-segmental-level topological

    constraints, they exhibit the corresponding forms of mechanical response in afar simpler context, which is amenable to more precise analysis. For this reason we

    start our assignment in this chapter by considering in some depth the hierarchical

    details of atomic-packing forms of metallic glasses and those of amorphous silicon

    as a surrogate for a space-network glass before we deal with the molecular

    structure of glassy polymers and semi-crystalline polymers in   Chapter 2. The

    atomic structure of amorphous silicon, in particular, makes contact with other

    directionally bonded covalent glasses and acts as a bridge between the densely

    packed amorphous metals with close-to-isotropic atomic interaction and high

    levels of atomic coordination and the structures of randomly snaking chain

    molecules of polymer glasses.

    In both cases, namely for amorphous metals and for space-network glasses, in

    this chapter we develop important concepts such as free volume or liquid-like

    atomic environments that both serve to promote structural rearrangements and

    also play crucial roles in triggering shear relaxations under stress that can range

    from few-atom clusters to far-reaching avalanches of plastic events. In every case,

    however, the presentation of the quantitative details of the topology and kinetics

    of such relaxations will be deferred to later chapters, where they are discussed

    together with the corresponding phenomena in glassy polymers, using the simpler

    processes in amorphous metals as guides to the more complex processes inpolymers. For metallic glasses, in which crystallization is suppressed and replaced

    by disorder, or at best only by some short-to-medium-range order, the

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    characteristic atomic packing can be reached operationally in a variety of ways.

    These include, e.g., direct condensation from a vapor into a solid and irradiation

    of a crystalline solid by energetic particles at relatively high fluences at low

    temperatures at which reordering of knock-on atoms is largely suppressed. How-ever, the most widely used route for obtaining a metallic glass is by rapid cooling

    of a complex alloy melt that is fast enough to override crystallization. It is this

    route that will be of exclusive interest to us.

    The first report of a metallic glass was that by Duwez and co-workers concern-

    ing an Au–Si alloy (Klement  et al. 1960). Since that time the science and technol-

    ogy of the production of the metallic glasses has progressed from a scientific

    curiosity to a very active area of materials science, leading to the development

    of a myriad of increasingly more stable glasses with wide-ranging potential for

    product applications.

    To understand the thermodynamics and kinetics of formation of metallic

    glasses through rapid cooling of an alloy melt of complex composition by overrid-

    ing crystallization, a number of interrelated subjects need to be understood in

    considerable detail. These include the evolving changes in atomic packing in sub-

    cooled melts, the kinetics of inter-diffusion of the constituent atom species that are

    part of the kinetics of atomic relaxations in the sub-cooled melts entering the glass

    transition range, and the kinetics of the competing crystallization processes.

    In the following sections we discuss first the atomic packing in sub-cooled alloy

    melts near a glass transition, referring to results obtained from recent combin-

    ations of modeling studies and associated experiments for some successful alloycompositions of metallic glasses. We follow this by considering the kinetics of 

    structural relaxations in some metallic glass compositions supported by actual

    inter-diffusion experiments on constituent atom species. We contrast these

    observations with competing forms and kinetics of polymorphic crystallization

    processes in these compositions to arrive at classical time–temperature– 

    transformation (TTT) diagrams. Following these considerations of the structure

    of sub-cooled alloy melts, we consider the all-important process of glass transition

    from a point of view of cessation of percolation of unit structural relaxation

    elements of atomic clusters possessing liquid-like character. Finally, employing

    mechanistic considerations and their kinetics, we examine some very successful

    metallic glass compositions that now permit one to obtain metallic glasses in

    relatively bulky form with sufficient stability in the sub-cooled melt to permit

    increasingly complex processing paths.

    We follow the discussion of metallic glass alloys with a brief parallel consider-

    ation of the behavior of amorphous silicon that is based primarily on computer

    simulations that have not only introduced the corresponding behavior of space-

    network glasses but also permitted a much deeper mechanistic understanding

    both of structural relaxations, and, more importantly, of the nature of plastic

    shear relaxations by ubiquitous shear transformations in glassy solids of alltypes, particularly in glassy polymers. These are developed in detail later in

    Chapters 7 and 8.

    2   Structure of non-polymeric glasses

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    1.2 Glass formability in metallic alloys

    The requirements for glass formability in metallic alloy melts by rapid quenching

    have received much attention since the first report by Duwez and co-workers in

    1960 on obtaining a metallic glass in an Au–Si alloy composition. Both laboratory

    experiments and computer studies have established that melts of pure metals tend

    to crystallize at such high rates that they cannot be quenched rapidly enough to

    obtain a glass. Thus, obtaining an alloy glass requires satisfying a number of 

    interrelated conditions that stifle crystallization. Success in the early investigations

    with binary metal–metalloid compositions of, e.g., Au–Si, Pd–Si, Fe–B, etc. with

    atom number ratios of 4:1 between metal and metalloid ions of substantial atomic-

    size difference already demonstrated the importance of atomic-size difference

    between constituents to stabilize the melt and retard crystallization. Other relatedfactors that emerged as essential for glass formability include the presence of a

    deep eutectic in the alloy composition that is beneficial in shortening the path

    between the melt and the glass; a high viscosity of the sub-cooled alloy melt at the

    liquidus range; and well-chosen alloy constituents requiring complex polymorphic

    crystallization involving coupled, sluggish diffusive atom fluxes among alloy

    constituents. Such fluxes produce topological and chemical short-range order that

    minimizes free-energy differences between the sub-cooled melt and the crystalline

    phase, and results in low levels of free volume in the sub-cooled melt at the glass-

    transition range. These have all proved to be important factors for glass form-

    ability. Detailed studies up to the present have demonstrated that many of these

    requirements are not independent but emanate from a need for efficient atomic

    packing in the sub-cooled melt, in which an important factor is the atomic-size

    mismatch among the alloy constituents.

    1.3 Atomic packing in disordered metallic solids

    The atomic packing in disordered solids was investigated first by Bernal (1964),

    who considered the problem in the context of a model of a simple liquid that

    consisted of randomly close-packed hard spheres of uniform size and described

    the structure as a distribution of five different canonical polyhedra with well-

    defined volume fractions.

    A more realistic computer model of a disordered solid considering both attract-

    ive and repulsive atom interactions, carried out by Finney (1970), gave very

    similar results, establishing that the hard-sphere repulsive interactions did indeed

    play a dominant role in the dense random packing of atoms. While these pioneer-

    ing models for liquids transforming into disordered solids gave reasonable agree-

    ment between the structure of the models and the radial distribution functions(RDFs) of atom positions of simple liquids (Bernal  1964), they severely under-

    predicted the densities of liquids at melting (or by extension, the densities of 

    31.3 Atomic packing

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    glasses) in comparison with face-centered cubic (fcc) crystals, at a level of a density

    reduction of around 13.5% (Miracle   et al.   2003). In comparison the density

    reduction of fcc crystals upon melting is only, on average, 4.5% (Brandes  1983).

    To explain the large density difference between the models of dense randomly

    packed uniform-sized spheres and the actual density of metallic glasses a number

    of factors for more efficient packing of spheres were considered. Since the early

    metallic-glass compositions were of metal–metalloid type such as Au–Si, Pd–Si,

    and Fe–B with number ratios of 4:1 between metal and metalloid atoms at a size

    ratio   R   of around 0.7, Polk (1972) proposed that the smaller solute metalloid

    atoms might more nearly fit into the interstitial spaces of the metal ions, thereby

    achieving a higher density. However, it was soon recognized that the interstitial

    volumes between metal atoms in the glass are far too small to accommodate the

    metalloid atoms without a large misfit strain. A number of more complete packing

    exercises for spheres of different size ratios   R   between solute (metalloid) and

    solvent (metal) atoms in binary systems (Visscher and Bolsterli   1972; Zheng

    et al.   1995; Lee   et al.   2003) showed conclusively that atomic-size differences

    between constituents in the framework of dense random packing of hard spheres

    could not by themselves account for the larger density difference between actualmetallic glasses and models. This is well demonstrated in Fig. 1.1, showing that the

    packing density of 0.64 of the models of dense randomly packed uniform-sized

    fcc structure

    98% of fcc structure

    Number Fraction of Smaller Spheres

       P  a  c   k   i  n  g   D  e  n  s   i   t  y

    00.60

    0.65

    0.70

    0.80

    0.75

    0.2 0.4

    R  = 0.60

    R  = 0.40

    R  = 0.20

    R  = 0.80

    0.80.6 1

    Fig. 1.1  Relative atomic packing density of a binary mixture of spheres with radius

    ratios  R  ranging from 0.2 to 0.8, based on developments of Zheng  et al. (1995)

    (from Miracle  et al. (2003): courtesy of Taylor and Francis).

    4   Structure of non-polymeric glasses

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    spheres remains well below the density of 0.74 of an fcc crystal, for all reasonable

    number fractions of smaller solute atoms in binary alloys for all atom ratios   R

    down to 0.4 (Miracle  et al.  2003). In a comprehensive study Egami and Waseda(1984) calculated critical solute-concentration limits that were based on determin-

    ation of excess enthalpies of binary systems through evaluation of the elastic misfit

    interactions between solute and solvent atoms before phase separation occurs.

    However, this led to no further improvement in accounting for the density

    disparity. The failure of these considerations resulted, in time, in a recognition

    that the dense random-packing models of spheres do not represent the atom

    packing in metallic glasses even when actual flexibility of atoms is considered

    and that there must be quite considerable short-to-medium-range packing order of 

    atoms that results in the relatively high actual densities of metallic glasses. Thus,

    from combined modeling and experimental structural studies of Miracle   et al.

    (2003), Miracle (2004a, 2004b, 2006), and Ma and co-workers (Sheng et al. 2006),

    among others, it has emerged that a high degree of short-to-medium-range atomic

    order exists in metallic-glass alloys. In alloys with a primary solvent component

    and one or more solute components the principal packing order is in the form of 

    solute-centered polyhedra for all solute-to-solvent radius ratios   R   in the range

    0.7–1.3. An excellent example of this is shown in   Fig. 1.2, namely an Ni80P20binary glass where the principal solute (P) appears as the small black spheres

    surrounded by solvent Ni atoms (dark gray) in the first icosahedral-type shells.

    The light-gray spheres represent, in turn, Ni atoms shared by neighboring soluteatoms lying in shells outside those depicted in the figure (Sheng   et al.   2006).

    In alloys with other solute components, the latter also either form additional

    Fig. 1.2  Model of solute-centered icosahedral type atom packing in an Ni80P20 binary glass

    obtained through Monte Carlo modeling (from Sheng  et al. (2006): courtesy of  Nature).

    51.3 Atomic packing

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    polyhedral shells in which these solutes are surrounded by other solvent Ni atoms,

    or the additional solute atoms are preferentially accommodated in the interstitial

    spaces of the solute-centered polyhedral shells (Miracle 2006). While there is very

    good evidence for this icosahedral-type packing order (Sheng  et al. 2006), it is not

    based only on purely geometrical effects of fit of atoms of different size ratios  R

    but also arises because the free energy of the alloy is governed importantly by the

    concentrations of the misfit-produced elastic strain energies of atoms in the

    ordered polyhedral shells. The latter effects have been considered by Egami and

    Waseda (1984) to lead to estimates of limits to the composition of glasses provided

    by specific constituents. It is clear that the short-to-medium-range order that is

    present in the sub-cooled melt is accentuated with decreasing temperature as the

    elastic misfits are systematically reduced as much as possible by diffusional

    exchanges of atoms. The existing evidence suggests that, e.g., in the most stable

    Zr-based bulk metallic glass alloys the atomic ordering results in an increase in

    density and a decrease in free volume in the alloy to a fractional concentration of a

    mere 1%–2% just prior to reaching the glass transition where the kinetics of 

    atomic ordering decreases below a critical low level (Busch  2000). It is this form

    of ordering that results in the very significant decrease in atomic mobility and

    increase in viscosity of the sub-cooled melt that suppress crystallization in thesealloys. This is demonstrated well in Fig. 1.3 with the classical TTT diagram of the

    Zr-based alloy Vitreloy-1 (Zr41.2Ti13.8Cu12.5Ni10Be22.5).   Figure 1.3   introduces a

    glass

    supercooledliquid

    crystalline

    Log time (s)

    600

    700

    800

    900

    1000

    1100

    T g

    T liq

    1 2 3 4

       T  e  m  p  e  r  a   t  u  r  e ,   K

    Fig. 1.3  A time–temperature–transformation diagram for the Vitreloy 1 glass-forming

    liquid (▴, obtained using electrostatic levitation;  , obtained using carbon crucibles) (fromBusch (2000): courtesy of TMS).

    6   Structure of non-polymeric glasses

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    number of important kinetic concepts, which we develop further in more detail in

    subsequent sections. These include the equilibrium   liquidus temperature T liqbelow which, depending on time or cooling rate, a number of different scen-

    arios can develop. For short periods of time or higher cooling rates a   super-cooled liquid   is maintained in which the viscosity increases monotonically as

    the temperature decreases. For longer periods of time or lower cooling rates

    polymorphic  crystallization   sets in. The border between the supercooled liquid

    and initiation of crystallization is given by the characteristic “C”-shaped curve

    which has a   critical nose  at a location of 895 K and 60 s. Cooling rates faster

    than those that merely graze the nose of the curve maintain the supercooled

    liquid to lower temperatures, albeit with continued monotonic increase in

    viscosity. Finally, depending on the cooling rate, the atomic mobility in the

    supercooled liquid becomes too low to permit further structural relaxation

    and atomic compaction at the given rate of cooling. Then, the supercooled

    liquid undergoes a   glass transition   at   T g   that is higher the higher the cooling

    rate, below which the excess volume per atom, the   free volume, decreases only

    very sluggishly. The rather long transformation time window of 60 s at the nose

    permits comfortable cooling rates in the range of 1.0 K/s to avoid incipient

    crystallization for many processing histories for such stable glasses. The tempera-

    ture dependence of the viscosity of this alloy in its supercooled liquid region is

    shown in Fig. 1.4 (Masuhr  et al.  1999). The figure also shows the viscosities of 

    many pure metals at their melting points near the bottom. These viscosities are

    typically three orders of magnitude lower than that of the Vitreloy 1 alloy,demonstrating why crystallization is extremely rapid in pure metals upon quench-

    ing and the extreme difficulty for them to undergo a successful glass transition.

    The vertical, upward-directed arrow in Fig. 1.4 shows where the glass transition

    occurs, at a viscosity of 1012 Pa s, but that some fluid-like behavior still persists at

    lower temperatures and higher viscosities.

    1.4 Energetic characterization of the structure of metallic glasses

    1.4.1 The atomic site stress tensor

    A very important form of characterization of the structural state of disorder in a

    glass is through the atomic site stress tensor introduced by Egami and Vitek

    (1983). While all atoms in a crystal are in mechanical equilibrium in their orderly

    arrangement that results in a low internal energy, in a glass all atoms are also in

    mechanical equilibrium but experience very large misfit-induced forces of inter-

    action with their neighbors. This permits one to define an atomic site stress tensor

    τ  resulting from the very substantial local interaction forces between atoms. Two

    scalar invariants of this stress tensor, defined for every atomic site, namely theatomic site pressure, p, and the atomic site deviatoric stress, σ , are of most interest.

    They are defined as

    71.4 Energetic characterization

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     p   τ ð Þ ¼   1=3ð Þtr   τ ð Þ ð1:1Þ

    and

    σ τ ð Þ ¼jτ     1=3ð Þtr   τ ð Þ I j ð1:2Þ

    where tr stands for the trace of the tensor   τ  and   Ι  stands for the identity tensor

    (Demkowicz and Argon 2005a). These two quantities furnish directionless scalar

    measures of the size misfit and distortional misfit, respectively, of atomic sites.

    Figures 1.5(a) and (b) show the distributions of the atomic site pressure and

    deviatoric stress calculated by Egami and Vitek (1983) from a three-dimensional

    (3D) computational model of a well-relaxed glass. The pressure distribution is

    nearly symmetric by virtue of overall traction equilibrium since there are both

    dilated and compacted domains. However, the overall volume fraction of the

    dilatation somewhat dominates over the compaction because of the unsymmet-

    rical character of the atomic binding potential around zero stress. The deviatoric

    stress distribution, however, is always positive by definition and by virtue of non-directionality. We note that the tail end of the pressure distribution on the

    negative side (i.e., positive mean normal stress) borders on levels of de-cohesion,

    Temperature, K

    1000/ T  (1/K)

    T  (K)   V   i  s  c  o  s   i   t  y   (   P  a  s   )   v

       f   /    v  m   (   %   )

    Ti   NiZr

    Be   Cu

    T g

    T liq

    0.5 1.0

    500 1000

    0.5

    0.0

    1.0

    4000 2000 1000 600

    10 –2

    100

    102

    104

    106

    108

    1010

    1012

    1014

    1016

    10 –41.5

    Fig. 1.4  The temperature dependence of the thermal equilibrium viscosity of liquid Vitreloy1 compared with experimental data from viscosity experiments (○), and beam-bending

    experiments (□). The inset gives the temperature dependence of the free volume of this

    alloy. The viscosities of many pure metals (▵), including Zr, Ti, Ni, Be, and Cu, are shown

    close to the temperature axis (from Masuhr  et al. (1999): courtesy of the APS).

    8   Structure of non-polymeric glasses

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    albeit over only atomic dimensions, while the high-end tail of the deviatoric stress

    distribution is a large fraction of the shear modulus. These characteristics of 

    atomic sites in glasses emphasize the very important fact that glassy solids store

    a very substantial excess enthalpy of disorder, which has its origin in the elastic

    strain energies associated with the atomic site structural misfit.

    1.4.2 Calorimetry

    A precise way of monitoring the thermodynamic properties of a glassy metal is

    accomplished through differential scanning calorimetry (DSC), in which the

    amount of heat required to increase the temperature of a sample is measured in

    comparison with that of a reference sample with well-known heat capacity. The

    technique supplies very useful information on the onset of property changes such

    as the glass transition and phase changes such as crystallization or melting as well

    as distinguishing thermodynamic-property differences such as levels of excess

    enthalpy of disorder and specific heat associated with different thermal and

    mechanical treatments. For example,   Fig. 1.6   shows three DSC scans for a

    Pd40Ni40P20   metallic-glass alloy heated at a rate of 20 K/min. The solid line

    represents the gradually increasing heat flow into an initially quenched sample

    as it transitions from a glassy solid into an under-cooled liquid at a glass-transition

    temperature of around 585 K. The dotted and dashed lines, on the other hand,

    show the similar endothermic transitions in samples pre-annealed at 540 K for

    1.0 h and 50 h, respectively. Clearly, the much more stabilized sample with the 50 h

    of annealing required considerably more heat input before undergoing the transi-

    tion. If crystallization had set in above the glass transition with a strong negative

    heat flow, as an exothermic process, a significant dip would have occurred in thescan. Alternatively, the occurrence of melting would produce a substantial upward

    peak (Duine  et al. 1992).

     –20 20   20 301000

    100

    200

    100

    200

    300

    0.0

    p  (GPa)

    N (p )(a) (b)

    N (s /√3)

    s /√3 (GPa)

    Fig. 1.5  Histogram of smoothed Gaussian distributions of (a) atomic site pressure  p  and

    (b) atomic site deviatoric stress  σ , calculated from a model of amorphous Fe (from Egami

    and Vitek (1983): courtesy of the Metallurgical Society of AIME).

    91.4 Energetic characterization

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    1.5 Free volume

    A concept of critical importance in understanding atomic mobility in glass-

    forming liquids and even glasses, that is referred to as free volume, was introduced

    by Fox and Flory (1950), and all subsequent theoretical developments on atomic

    mobility in disordered structures and their structural relaxation processes have

    been based on this concept. In a disordered structure like a dense liquid, for an

    atom to migrate, room must be provided in its immediate neighborhood for it tomove into. In such structures atoms occupy, on average, volumes   v  equal to or

    larger than   v0, the van der Waals volume of the atom, or its size in an ordered

    reference structure. When the actual size of the volume the atom occupies in the

    structure exceeds a critical value vc (vc> v0 ), locally the excess can be considered as

     free volume. Then atomic transport occurs only when momentary voids of some

    critical size   v* approximately equal to the atomic volume   v0  appear by redistri-

    bution of the local free volume as a result of fluctuations. In a liquid such

    redistribution of free volume is considered not to require overcoming an energy

    barrier. Fox and Flory (1950) defined the local free volume as

    vf  ¼  v  v0   ð1:3Þ

    using v0 rather than vc, which needs a more precise definition that will be given below.

    600 625575550525 –1

    Temperature, K

       H  e  a   t   f   l  o  w   (  m   W   )

    0

    1

    2

    3

    4

    Fig. 1.6  DSC scans of thermal effects in Pd40Ni40P20  with a heating rate of 20 K/min: the

    solid line is for a quenched sample; the dotted line and dashed lines are for samples

    pre-annealed at 540 K for 1.0 h and 50 h, respectively (from Duine et al. (1992): courtesy

    of Pergamon Press).

    10   Structure of non-polymeric glasses

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    Using the above ideas, Doolittle (1951) proposed an expression for the viscosity

    η  of a liquid given by

    η ¼  η0

      exp   bv0=vf ð Þ ð1:4Þ

    where both  η0  and  b  were considered adjustable parameters and  vf   represents the

    volume-average free volume. This equation was quite successful in representing

    the viscosities of simple hydrocarbon fluids. Earlier Vogel (1921), Fulcher (1925),

    and Tamman and Hesse (1926) quite independently proposed a different-

    appearing expression for the viscosity of molten-oxide glasses that had the form

    ln  η ¼  A þ  B

    T   T 0ð1:5Þ

    with   A,   B, and   T 0   being often considered as adjustable constants, but having

    distinct physical meanings. The constant  B, e.g., having the dimension of tempera-

    ture, is the reciprocal of the difference between the volumetric coefficient of 

    thermal expansion of the liquid and that of the solid below the glass-transition

    temperature. This so-called Vogel–Fulcher–Tamman (or VFT) equation, which

    was arrived at entirely empirically, has proved to be very successful in representing

    the equilibrium viscosities of many sub-cooled liquids, including metal alloys and

    some molten-oxide glasses at high temperature in the melt region. A quick exam-

    ination shows that the VFT equation is identical with the Doolittle equation if it is

    recognized that

     A ¼  ln  η0   ð1:6aÞ

    and

    vf  ¼  v0   b= Bð Þ   T   T 0ð Þ ð1:6bÞ

    where the ratio   b/ B   must be a constant having the dimension of reciprocal

    temperature. With this comparison, the free volume is seen to be linearly

    temperature-dependent, representing a form of thermal expansion of the liquid

    that is always substantially larger than that of its solid form. We note that on this

    comparison the free volume vanishes at  T ¼ T 0 and that the viscosity according to

    Eq. (1.4) becomes unbounded, being based on trends having no experimental

    support, requiring further refinement of the concept.

    Cohen and Turnbull (1959) clarified the physical significance of the Doolittle

    equation by demonstrating that the probability P(v*) of finding a hole of size v* or

    larger in a field of free volume can be expressed as

     P vð Þ ¼ exp   γv

    vf 

      ð1:7Þ

    and that, following the arguments of Fox and Flory, this would lead to a diffusion

    constant

     D ¼  gau exp  γv=vf ð Þ ð1:8Þ

    111.5 Free volume

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    where a* is the molecular diameter, g  a geometrical constant of order unity, and  u

    the gas kinetic velocity. Moreover, since the Stokes–Einstein relation for dilute

    systems, which gives

     D ¼   kT =   3pað Þð ÞF   ð1:9Þ

    that relates the fluidity,  F ¼  1/η, to the diffusion constant  D  for dilute systems, is

    also largely applicable to the liquids of interest here, an expression for the shear

    viscosity η  follows directly as

    η ¼  η0   exp  γv

    vf 

      ð1:10Þ

    which is the Doolittle equation, where η0  ¼  kT =3pðaÞ2u

    and has the dimensions

    of Pa s, if  g  is taken as 1.0.

    Finally, the average free volume, given by

    vf  ¼  αv0   T   T 0ð Þ ð1:11Þ

    where  α  is the volumetric thermal coefficient of expansion, provides the physical

    basis of the VFT relation for the shear viscosity. The form of eq. ( 1.11) with

    T 0   vc, in which atoms are more weakly bound to

    12   Structure of non-polymeric glasses

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    their neighbors and are surrounded by an excess of volume, were referred to as liquid-

    like (LL). In this picture the local free volume,  vf , is redefined more precisely as

    vf  ¼ v  vc   ð1:12Þ

    Since the volume per atom  v  is temperature-dependent and will vary with fluctu-

    ations, the free volume will also fluctuate and in a liquid will wander around, not

    necessarily being associated with specific atoms. In the Cohen and Grest model

    the probability distribution of   v,   P(v), and the local free-energy function,   f (v),sketched in Figs. 1.7(a) and (b) permit the determination of a specific expression

    for the average free volume  vf  and its temperature dependence given by

    0

    v 0   v c   v 

    f (v )

    (b)

    0

    v 0   v 1

    (a)f (v )

    Fig. 1.7  A schematic representation of the free-energy function  f (v), which is dependent

    primarily on the atomic volume at an atom site: (a) the binding-energy plot showing

    equilibrium volume  v0 and inflexion point  v1; (b) division of  f (v) into two parts, consisting

    of a central, strongly bonded harmonic part with  v < vc and a linear part with v > vc used todefine solid-like, SL, and liquid-like, LL, atomic environments (from Cohen and Grest

    (1979): courtesy of the APS).

    131.5 Free volume

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    vf  ¼ k 

     A  T   T 0ð Þ þ   T   T 0ð Þ

    2 þ 2 AvaT 

    1=2( )  ð1:13Þ

    where  k  is Boltzmann’s constant and other parameters, such as  A   representing ashape parameter of the free-energy function having the dimensions of modulus

    (Pa), and va and  T 0, with dimensions of volume and temperature, respectively, are

    all derived from the free-volume model and have similar meanings to those used

    above, but can be treated as adjustable. Unlike the free-volume expression of 

    eq. (1.3) or eq. (1.11), which vanishes at   T ¼ T 0, the expression of eq. (1.13)

    vanishes only when   T → 0 and removes a critical flaw in eqs. (1.6b) and (1.11).

    When used in the Doolittle equation, the free-volume expression of eq. (1.13)

    provides the best fit to the thermal-equilibrium viscosity of sub-cooled melts and

    dense liquids over the widest range of temperature. In  Fig. 1.4  it gives the solid

    curve capturing the entire range of experimental measurements of the viscosity of 

    Vitreloy 1, while the temperature dependence of the free-volume expression  vf  of 

    eq. (1.13) is shown in the inset of this figure, as normalized by  vm(¼v0), the van der

    Waals volume in the alloy melt (Masuhr  et al. 1999).

    1.6 Viscosity of glass-forming liquids

    To better understand the viscosity of sub-cooled liquids, the formation of metallicglasses, and the kinetics of their glass transition, as well as the kinetics of the

    competing processes of crystallization, it is useful to view their viscosity in the

    context of a broader collection of other potentially glass-forming liquids. Angell

    (1995), who has considered this comparison in quite considerable detail, has

    introduced an insightful classification grading liquids in a range from   strong   to

     fragile   depending on the form of the temperature dependence of their viscosity.

    Figure 1.8 shows an Angell plot of a limited set of glass-forming liquids chosen for

    the purpose of a comparison of the alloys that form bulk metallic glasses (BMGs)

    with some other liquids. Since these liquids have vastly different relaxation pro-

    cesses, the temperature scale is normalized with the glass-transition temperature

    T g  of the liquids considered. For this purpose the glass transition is defined as

    occurring when the viscosity of the liquid reaches 1012 Pas.

    At one limit, that of the strong liquids, are liquids of covalent and strongly

    directionally bonded types such as SiO2, GeO2, and molten Si, all of which

    maintain their directionally bonded character in the liquid state. The temperature

    dependence of these liquids is of Arrhenius type, which, in the context of the VFT

    framework of viscosities represented by eq. (1.5), means that   T 0   vanishes and

     B ¼Δ Fv/ R, where Δ Fv is the activation energy of viscous flow and R is the universal

    gas constant. The Arrhenius dependence is shown by the straight line for SiO 2 inFig. 1.8. In the context of distributed structural relaxation processes, rather than

    mono-energetic types, which we discuss in Section 1.8,  Δ Fv  refers to the terminal

    14   Structure of non-polymeric glasses

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    activation energy of a characteristic spectrum of activation energies for flow of a

    disordered medium, in which the low end of the spectrum represents those relax-

    ations of low volume fraction that are readily accomplished, while  Δ Fv represents

    the most sluggish background relaxation that governs global flow. In these strong

    liquids diffusion and structural relaxations are thermally assisted directly rather

    than being governed indirectly by free-volume fluctuations as in the VFT model of 

    diffusion and fluidity that reflects the behavior of liquids bound by non-directional

    metallic bonds or by van der Waals interactions.

    At the other limit of the gradation of fluidity response are the fragile liquids that

    exhibit viscosities with a VFT type of temperature dependence reflecting atomic

    mobility governed indirectly by the volume fluctuation as discussed in Section 1.5.

    In Fig. 1.8, glycerol and KCa(NO3) are two such fragile liquids. To account for

    the differences in behavior of fragile liquids in the VFT framework, Angell (1995)

    introduced a so-called fragility constant  D   into the VFT viscosity relation, giving

    η ¼  η0   exp   DB=   T   T 0ð Þð Þ ð1:14Þ

    where  D  is of the order of unity, i.e., 1–3, etc., for the fragile liquids, whereas for

    the behavior of strong liquids  D   is in the range of 100 or so. Clearly, apart from

    the presence of   T 0, the increasing fragility constant reflects an increase of theactivation energy for flow for strong liquids. In   Fig. 1.8   the behaviors of 

    the BMG-forming liquids of Vitreloy 1 and 4 and the metallic alloy melt of 

    fragile

    strong

    glycerol

    T g* / T 

    T gSiO2 = 1410 K

    T gV1 = 606 K

    T mV1 = 1030 K

    K+Ca2+(NO3)3– 

    Na2O2˙SiO2

    Zr41.2Ti13.8 Cu12.8Ni10Be22.5(V1)

    Zr46.75Ti8.25Cu7.5Ni10Be27.5(V4)

    Mg65

    Cu25

    Y10

    103

    107

    1011

    10 –5

    10 –1

    0.4 0.6 0.8 1.0

       V   i  s  c  o  s   i   t  y   (   P  a  s   )

    SiO2

    Fig 1.8  An Angell plot of the dependences of the viscosities of a series of liquids on their

    reduced temperature  T =T g, defining strong (Arrhenian) and fragile (VFT) liquids (fromBusch (2000): courtesy of TMS).

    151.6 Viscosity of glass-forming liquids

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    Mg65Cu25Y10  are intermediate between those of fragile and strong liquids and

    demonstrate their success in retarding crystallization.

    1.7 Structural relaxations

    1.7.1 A computational model

    The free-energy function sketched out in   Fig. 1.7, from which free volume is

    defined, indicates that only LL cells with  v> vc  possess free volume, while those

    with   v< vc  that are SL cells provide negligible free volume. In this characteriza-

    tion, the SL cells are expected to be stiff, whereas LL cells are much more

    compliant both to dilatation and to distortion. Thus, clusters of cells with large

    LL fractions of atom environments would be expected to play a dominant role in

    structural relaxations. It would then follow that in a liquid or sub-cooled melt that

    readily changes shape LL environments must percolate through the structure at all

    times on the average. This condition that exists at the melting point of an alloy

    must then continue to hold also in the sub-cooled melt region. As the temperature

    decreases and structural relaxations continue steadily, albeit at a lower rate, the

    LL material fraction must decrease systematically, resulting in progressive, large

    increases in viscosity as, e.g., the trend in Fig. 1.4 shows. In all cases, however, the

    LL fraction of atom environments must continue to percolate through the struc-

    ture to maintain fluid behavior. At a certain temperature  T g  at which the percola-tion of the LL environments ceases for a characteristic period of observation, the

    SL fraction will form a topologically continuous stiff background and the alloy

    begins to exhibit solid behavior. This represents a glass transition at   T g, below

    which some LL environments may still be present but in frozen-in and isolated

    form. The systematic decrease of the LL environments in the sub-cooled melt

    between the melting point and the glass-transition temperature has been studied in

    computer simulations. For example, in a two-dimensional (2D) molecular-

    dynamics simulation of the structure of a generic Cu50Zr50   alloy melt and sub-

    cooled liquid Deng et al. (1989a), using a 4–8 Lennard-Jones-type atomic potential

    to represent the interactions of the Cu and Zr atoms, carried out limited studies of 

    melting and quenching in small mats of atoms under periodic boundary condi-

    tions. With such models they explored both the topological features and the

    kinetics of structural relaxations (Deng   et al.   1989b,   1989c).   Figure 1.9   shows

    the dimensionless volume per atom v* as a function of dimensionless temperature

    T * in the melting and quenching simulation, the details of which, including the

    definitions of dimensionless quantities, can be found in Deng   et al.  (1989a). On

    tessellating the 2D field of atoms in the melt and the sub-cooled liquid between T mand T g by Voronoi polygons they noted first that the field contained primarily two

    distinct families of atom environments. One family was in the form of distortedhexagons of roughly similar size. These environments were labeled as solid-like,

    SL. While the second family of environments consisted primarily of pentagons

    16   Structure of non-polymeric glasses

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    and heptagons, also occasionally present were a few squares and octagons. The

    average area of these different types of polygons increased monotonically with

    increasing number of sides as shown in Fig. 1.10. Of the non-hexagonal family of 

    polygons, the pentagons and heptagons showed a strong association into 5–7-

    sided structural dipoles. Figure 1.10 demonstrates that the area (volume) of each

    structural dipole was, on average, 7% larger than that of an average pair of 

    hexagons. These dipolar environments were labeled as liquid-like, LL, and were

    considered as principal carriers of free volume. Separate simulations of plastic

    deformation in such 2D mats demonstrated that the LL atom environments did

    indeed act as the principal facilitator of plastic flow, confirming their anticipated

    role in providing atomic mobility (Deng   et al.  1989d).   Figures 1.11(a) –(c) show

    three 2D atom mats with a Voronoi tessellation at temperatures of (a)  T  ¼ 1:2T m,

    (b)   T g 

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    showed that LL environments moved over atom sites rapidly without muchdiscernible actual exchange of atoms, indicating that in general environments

    are transient and are not necessarily locked onto specific atoms.

    It is useful to consider the fluctuating disorder in the liquid in  Fig. 1.11(a) as a

    graphical representation of the configurational entropy,   Sc, attributable to the

    presence of the LL component. This can be defined along conventional lines as

    Sc ¼  k   ln   N =2ð Þ!=   N =2  nð Þ!n!½ ð1:15Þ

    where  n  is the number of dipolar LL sites and  N  represents the total number of 

    sites, or N /2 the total number of pairs of either 5–7-sided LL polygons or the 6–6-

    sided SL environments. The maximum of  Sc  occurs at  n ¼ N /4, or when   n  repre-

    sents half of the total of pair sites or an LL site concentration  φ ¼ 0.5. We take this

    as a characteristic of the flow state.

    The graphical representation of percolation of LL environments above  T g  and

    the absence of such percolation below  T g  are in broad agreement with the Cohen

    and Grest (1979) model of the structure of simple atomic liquids and glasses

    discussed in Section 1.5. Two-dimensional simulations of the type discussed above

    have been carried out also by others and have largely supported the picture

    sketched above (Perrera and Harrowell  1999; Hentschel  et al. 2007).

    The relatively simple simulations of the topology of structural disorder andassociated atom mobility hav