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Journal of the Mechanics and Physics of Solids
journalhomepage:www.elsevier.com/locate/jmps
Modeling of surface effects in crystalline materials within the framework of gradient crystal plasticity
Xiang-Long Peng
a,b, Edgar Husser
c, Gan-Yun Huang
a,∗, Swantje Bargmann
b,∗aDepartment of Mechanics, School of Mechanical Engineering, Tianjin University, Tianjin 300350, PR China
bChair of Solid Mechanics, School of Mechanical Engineering and Safety Engineering, University of Wuppertal, Wuppertal 42119, Germany
cInstitute of Continuum Mechanics and Material Mechanics, Hamburg University of Technology, Hamburg 21073, Germany
a rt i c l e i n f o
Article history:
Received 20 September 2017 Revised 5 December 2017 Accepted 12 January 2018 Available online 12 January 2018 Keywords:
Strain gradient Crystal plasticity Size effect Surface effects Surface yielding
a b s t ra c t
Afinite-deformationgradient crystalplasticitytheoryisdeveloped,whichtakesintoac- count theinteractionbetweendislocations andsurfaces. Themodelcaptures bothener- geticand dissipativeeffectsfor surfacespenetrableby dislocations.By takingadvantage oftheprincipleofvirtualpower,thesurfacemicroscopicboundaryequationsareobtained naturally.Surfaceequationsgovernsurfaceyieldingandhardening.Athinfilmundershear deformation servesas abenchmarkproblemforvalidation oftheproposed model.It is foundthatbothenergeticanddissipativesurfaceeffectssignificantlyaffecttheplasticbe- havior.
© 2018TheAuthors.PublishedbyElsevierLtd.
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1. Introduction
In the last two to three decades, many efforts have been devoted to studying the mechanical properties of small- scaledand/orfine-grainedcrystallinematerialswidelyusedinsmall-scaledengineeringsuchasmicroelectronicsandmicro- electromechanicalsystemstoensuretheirperformanceandreliabilityinpracticalapplications.Ithasbeenfoundinvarious experiments(seee.g.,Flecketal.,1994;Guetal.,2012;McElhaneyetal.,1998;Swadeneretal.,2002)thatcrystallinema- terialsatsmallscalesusuallypossessplasticbehaviorsquitedifferentfromthoseoftheirbulkcounterparts,amongwhichis thesize-dependenceoftheyieldstressandstrain hardeningbehavior.Sinceconventionalplasticitytheoriesareessentially size-independent,thesesizeeffectsarebeyondtheir predictability.Asiswell known,themacroscopicplasticdeformation incrystalsmainlyresultsfromthemicroscopicdislocationglidingontheindividualcrystallographicslipplanes,thusthose unusualplastic behaviorsare closelyrelevantto thedistinctive dislocationactivities insmall-scaled crystals.Accordingto Ashby (1970),dislocations incrystals can be classifiedinto two types,namely statisticallystoreddislocations (SSDs) and geometricallynecessarydislocations(GNDs).Thelatterisstoredincrystalstoaccommodatelatticecurvature.Asdiscussed byNixandGao(1998),GNDsmayberesponsibleforsizeeffectsduetostraingradientssincetheyaremorelikelytoaccu- mulatewheninhomogeneousplasticdeformationtakesplace.Furthermore,withthedecreaseofgrainsizeand/orgeometry sizeofcrystals,thevolumetograin boundary(GB)/surfaceratioincreasesdramatically,whichmaypromptdislocationsto reachandtheninteractwiththeGB/surface.Forinstance,asdemonstratedbyatomisticsimulations(seee.g.,Spearotetal.,
∗ Corresponding authors.
E-mail addresses: gyhuang@tju.edu.cn (G.-Y. Huang), bargmann@uni-wuppertal.de (S. Bargmann).
https://doi.org/10.1016/j.jmps.2018.01.007
0022-5096/© 2018 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY license.
( http://creativecommons.org/licenses/by/4.0/ )
2005;VanSwygenhovenetal.,2002;Yuasaetal.,2010),grainboundariesactassourcesandsinks,emittingandabsorbing dislocations.Insinglecrystals,dislocationsareobservedtoescapetowardsandnucleateatthesurface,whichdramatically changesthestrainhardeningbehavior(Ohetal.,2009;Shanetal.,2008;Wangetal.,2012).Inordertoconstructpredictive theoriesfortheplasticbehaviorinsmall-scaledcrystallinematerials,thedislocation-relevantmechanismsbothinthebulk andattheGB/surfaceneedtobeproperlyconsideredonthecontinuumlevel.
Sofar,sincethepioneeringworkbyAifantis(1984),numerousstraingradientplasticitytheorieshavebeenproposedby incorporatingtheplasticstraingradientortheGNDdensity,andhavesuccessfullypredictedexperimentallyobservedsize- effects(seee.g.,ChenandWang,2000;Flecketal.,1994).AsdiscussedinKurodaandTvergaard(2008),theexistingstrain gradienttheoriescanbeclassifiedintotwotypesnamelythelower-ordertheories(seee.g.,AcharyaandBassani,2000;Chen andWang,2000;Eversetal., 2002)andthehigher-ordertheories(seee.g.,Bargmannetal.,2011;Evers, 2004;Fleckand Hutchinson,1993;1997;Gromaetal.,2003;Gurtin,2000;2002;Yefimovetal.,2004)basedonhowtheeffectsofGNDsare considered.Ofparticularinterestarehigher-ordertheories,inwhichinadditiontothetraditionalforcebalanceequationand thetractionboundarycondition,themicroscopicgoverningequationsandthecorrespondingmicroscopicboundarycondi- tionsareinvolved.1Thehigher-ordertheoriesprovidethepossibilitytomodeldislocationactivitiesataGB/surfacethrough properlychoosingmicroscopicboundaryconditions.Forsimplicity,themicrohardandmicrofreeconditionsrepresentingtwo extremecasesareusuallyimposed,andtheunderlyingassumptionisthattheGB/surfaceiscompletelyimpenetrableresp.
freelypenetrabletodislocations.However,thesetwoextremeGB/surfacemodelsarenotsufficienttocapturedislocationac- tivitiesattheGB/surface.Todate,afewintermediateGB/surfacemodelshavebeenproposed.CermelliandGurtin(2002)de- velopedadissipativegrainboundarymodelwhereavisco-plasticrelationforgrainboundarymicrotractionisassumed.By consideringtheinterfaceenergycontributedbytheinteractionbetweendislocationsandgrainboundaries,otherresearchers proposedenergeticgrainboundarymodels(seee.g.,Aifantisetal.,2006;FredrikssonandGudmundson,2005;Gudmundson, 2004).Thesemodelsarepurelyphenomenological.Gurtin(2008)constructedagrainboundarymodelwheretheeffectsof grainmisorientationandgrainboundaryorientationareconsideredthroughtheexactlyderivedgrainboundaryBurgersten- sor.InvanBeersetal.(2013),agrainboundarymodelsimilartothatofGurtin(2008)wasputforward,inwhichavectorial measureofthedensityofgrainboundarydefectwasintroduced.AsillustratedbyGottschalketal.(2016),thesetwomod- elsareessentiallyidenticalifconsideringplanarproblems.vanBeersetal.(2015)extendedthepreviousmodel(vanBeers etal.,2013) byfurtheraccountingfortheredistributionofthegrainboundarydefects.Ekhetal.(2011)suggestedamicro- flexibleboundaryconditionbywhichthecrystallographicmisorientationbetweenadjacentgrainsistakenintoaccount.The thermaleffectsonthemodelarefurtherconsideredby BargmannandEkh(2013).Inthegrainboundarymodelproposed byWulfinghoff etal.(2013),acriterionforinterfaceyieldingisintroducedtoaccountfortheresistanceofgrainboundaries againstslipoccurrence.Kuroda(2017)proposedastrategyformodelingvariousmicroscopicinterfaceboundaryconditions byintroducingascalarquantitytocontroltheslippingrateattheinterface,basedonwhichanorientation-dependentgrain boundarymodelisproposedandthenimplementednumericallytostudytheplasticbehaviorofbicrystalmicropillars.
Somemodelsstudydislocation-surfaceinteractionsinsinglecrystals.HuangandSvendsen(2010)proposedanenergetic surfacemodelbyconsideringthechangeofsurfaceenergycontributedbysurfacestepsduetodislocationabsorptionbysur- faces.Similarly,HurtadoandOrtiz(2012)derivedanexplicitexpressionforthedensityofsurfaceenergybyconsideringthe relativeorientationbetweenslipsystemsandsurfaces.Inbothmodels,thedensityofsurfaceenergydependslinearlyonthe plasticslipsatthesurface.Byfurtherconsideringtheinteractionenergybetweensurfacesteps,PengandHuang(2015)con- structedaphysicallybasedenergeticsurfacemodelwithintheframeworkofwork-conjugatedhigher-ordergradientcrystal plasticity.Inthismodel,asurfaceyieldingconditionisderivednaturally,andinteractionsbetweenslipsystemsareconsid- ered.Recently, Husseretal.(2017) suggestedaflexible surfaceboundarymodelby establishinga directrelationbetween thesurfacesliprateandthemicroforcevectorprojectedontotheboundary.Usingasurfaceyieldcriterion,anon-idealized surfacebehaviorwasaddressedincludingdissipativeeffectsofsize-dependentsurfaceyielding.
Asreviewedabove,modelingGB/surfaceeffectshasrecentlybeentheforefrontinthefieldofcrystalplasticityatsmall scales.Yet,intheexisting GB/surfacemodels,lessattentionhasbeenpaidontheunderlyingphysicalmechanisms.Toin- corporatetheunderlyingphysicalmechanisms relevanttointeractions betweendislocationsandsurfacesasillustratedby insituexperiments intothecontinuum model, werevisit modeling dislocation absorption bysurfaces.On theone hand, afterdislocationabsorptionbysurfaces,surfacestepsform(seee.g.,Shanetal.,2008;Wangetal.,2012;Zhongetal.,2017), whichresultsinthechangeofsurfaceenergy. Thus,suchsurface-drivenchangeinthefree energymustbeproperlycon- sidered.Ontheotherhand,asisobservedinOhetal.(2009),dislocationsstopforawhilenearasurfacecontaminatedby anoxidelayerbefore theyareabsorbed.Thisisstrongevidenceforthe existenceofanincreasedresistanceagainstdislo- cationabsorptionatsurfacesaffectedbyoxidelayers,coatingsorinitialdefects.Furthermore,accordingtotheexperiment byZhongetal.(2017),dislocationabsorptionbysurfacesmaybeviewedasadissipativeprocess.Allthoseindicatethedis- sipativenatureofdislocationabsorptionby surfaces.Inaddition,modelsconfinedtosmalldeformationareinadequatefor situationswithsevereplasticdeformation.Consequently,anadvancedsurfacemodelwithenergeticanddissipativesurface effectsisproposed intheframework offinitedeformationgradientcrystalplasticity.Energeticsurfaceeffectsaremodeled byextendingthephysicallymotivatedsurfacemodelproposedinPengandHuang(2015).Toconsiderdissipativesurfaceef- fects,arate-dependentconstitutiverelationforthedissipativesurfacemicroforceisproposedwithinthenewsurfacemodel.
1For a unified formulation and comparison of higher-order theories, see ( Svendsen and Bargmann, 2010 ).
Thetheoryisnumericallyimplementedbyusinganin-housefiniteelementcodebasedonadual-mixedfiniteelementso- lutionstrategytostudyabenchmarkproblem.
2. Modelframework
2.1. Basickinematicsoffinitedeformationcrystalplasticity
Infinitedeformationcrystalplasticity,thebasicassumptionisthatthedeformationgradienttensorFismultiplicatively decomposedintoanelasticpartFeandaplasticpartFp asfollows
F=Fe·Fp. (1)
Theplastic partFp describestheplasticdeformation fromthereferenceconfigurationtothestress-freeintermediatecon- figuration resultingfromdislocation glidingon thecrystallographic planes.Theelastic partFe by whichthe intermediate configurationisdeformedtothecurrentconfigurationcomprisesthelatticedistortionandrotation.Itisassumedthatthe plasticdeformationdoesnotchangethevolumesuchthatdetFp=1withdetdenotingthedeterminantofatensor.Inthe following,ifnecessary,thesubscriptsiandcareusedtoidentifyquantitiesintheintermediateandthecurrentconfigura- tion,respectively.
Basedonrelation(1),thevelocitygradienttensorLisdecomposedas
L=
∇
cu˙ =F˙·F−1=Le+Fe·Lp·Fe−1, (2)withtheelasticvelocitygradientLeandtheplasticvelocitygradientLp definedas
Le=F˙e·Fe−1 (3)
and
Lp=F˙p·Fp−1, (4)
where[
∇
a]i j=ai,jdenotesthegradientofavectora,thesuperposeddotdenotesthematerial-timederivative,thesuper- script −1 denotesthe inverseof a tensor,andu isthe displacement vector. Letusconsider a crystalinwhich each slip systemα
isidentifiedbyaslipdirections(α)andaslipplanenormalm(α)attachedtothelatticespaceintheintermediate configuration.Theisoclinicassumption isadoptedsuchthat s(α) andm(α) remainunalteredfromthereferenceconfigura- tiontotheintermediateconfiguration.Then,bydenotingthesliprateintheintermediateconfigurationasγ
˙(α),theplastic velocitygradienttensorisexpressedasthesumoverthecontributionsfromallslipsystemsLp= α
γ
˙(α)s(α)m(α). (5)Therelevantstrain measures,namelytheGreen–Lagrangestrain tensor,andtherightCauchy–Green stretchtensorand theirelasticpartsarerespectivelydefinedas
E=1
2[C−I], C=FT·F (6)
and
Ee=1
2[Ce−I], Ce=FeT·Fe, (7)
wherethesuperscriptTdenotesthetransposeofatensorandIistheidentitytensor.
TheevolutionofedgeandscrewGNDdensities
ρ
ige(α)andρ
igs(α)areputdownasρ
˙ige(α)=−1b
∇
iγ
˙(α)·s(α) (8)and
ρ
˙igs(α)=1b
∇
iγ
˙(α)·p(α), (9)whereb is themagnitudeofthe Burgersvector, andp(α)=s(α)×m(α).Theinitial conditionsare
ρ
ige(α)|
t=0=ρ
0ige(α) andρ
igs(α)|
t=0=ρ
0igs(α)withρ
ge0i(α)andρ
0igs(α)beingtheinitialGNDdensities.2.2. Balanceequationsandboundaryconditions
Inthefollowing,themacroscopicandthemicroscopicbalanceequationsarederived viatheprincipleofvirtualpower.
FollowingGurtin(2002),intheintermediateconfiguration,theinternalpowerinthebulkisassumedtobeexpendedbythe second Piola–Kirchhofstress tensorSe power-conjugatetotherateoftheGreen–Lagrange straintensorE˙e,themicroforce
π
i(α) power-conjugate to the slip rate ˙γ
(α) and the microstressξ
i(α) power-conjugateto theslip rategradient∇
iγ
˙(α) foreachslipsystem
α
.Inthepresentwork,anadditionalcontributiontotheinternalpowerexpendedbythemicroforceη
(α)ipower-conjugate to the sliprate
γ
˙(α) at the surfaceSi is introduced to consider the effect of dislocation absorption by surfaces.Thus,thetotalinternalpowerPintisexpressedintheintermediateconfigurationasPint=
Vi
Se:E˙edVi+ α
Vi
π
i(α)γ
˙(α)+ξ
(α)i ·∇
iγ
˙(α)dVi+ α
Si
η
i(α)γ
˙(α)dSi, (10)wherethesecond Piola–Kirchholfstress tensorSe isdefinedasSe=Fe−1·J
σ
·Fe−T withσ
beingthe Cauchystress tensor.Accordingly,theexternalpowerPextintheabsenceofbodyforcesiswrittenas Pext=
Si
Ti·u˙dSi+ α
Si
(α)i
γ
˙(α)dSi, (11)whereTiistheprescribedtractionand(α)i isthemicrotractiondefinedintheintermediateconfiguration.Accordingtothe principleofvirtualpower,the variationoftheinternalpowerwithrespecttothevelocityu˙ andthesliprate
γ
˙(α) equals thatoftheexternalpower,whichgives
Vi
Se:
δ
E˙edVi+ α
Vi
π
i(α)δ γ
˙(α)+ξ
(α)i ·∇
iδ γ
˙(α)dVi
+
α
Si
η
i(α)δ γ
˙(α)dSi=Si
Ti·
δ
u˙dSi+ α
Si
(α)i
δ γ
˙(α)dSi. (12) FromEqs.(2),(3),(5)and(7),thevariationofE˙eisexpressedasδ
E˙e=12FeT·
∇
iδ
u˙ −α
Ce·s(α)m(α)
δ γ
˙(α)+1 2
FeT·
∇
iδ
u˙ −α
Ce·s(α)m(α)
δ γ
˙(α) T. (13)
Then,by substituting Eq.(13)intoEq.(12) andusingthe divergencetheorem,theprinciple ofvirtual power isrewritten
as
Vi
Divi(Fe·Se)·
δ
u˙dVi− α
Vi
Diviξ
(iα)+s(α)·M·m(α)−π
i(α)δ γ
˙(α)dVi+
α
Si
ξ
i(α)·Ni+η
(iα)−(iα)
δ γ
˙(α)dSi+Si
[[Fe·Se]·Ni−Ti]·
δ
u˙dSi=0, (14)whereNi is the surfaceoutward normal vector, Div denotes thedivergence operator, andthe Mandelstress tensor M is expressedas
M=Ce·Se. (15)
First, considering the special case without plastic slip (
δ γ
˙(α)=0), the requirementthat Eq. (14)should be satisfied for arbitraryδ
u˙ results in the macroscopicforce balance equation andthe corresponding standard traction conditionin the intermediateconfiguration,i.e.,0=Divi
(
Fe·Se)
(16)and
[Fe·Se]·Ni=Ti (17)
atthepartofsurfaceSTi withprescribedtraction.Then,giventhevalidityofEq.(14)forarbitrary
δ γ
˙(α)inthecasewithoutmacroscopicdisplacement (
δ
u˙ =0), the microscopicbalance equation andtheassociated microscopic boundarycondition foreachslipsystemα
areobtainedasfollowsDivi
ξ
i(α)+τ
i(α)−π
i(α)=0, (18)with
τ
i(α)=s(α)·M·m(α)beingtheSchmidstress,andξ
i(α)·Ni+η
i(α)−(α)i =0. (19)
2.3.Constitutiverelations:theorywithsurfaceeffects
Theelasticbehavior ofthe crystalisassumedtobe compressibleneo-Hookeansuchthat thestrainenergydensity
ψ
iehasthefollowingform
ψ
ie(
Ee)
=μ
Ee:I+λ
2[ln
(
J)
]2−μ
ln(
J)
(20)withJ=
det(2Ee+I),and
λ
andμ
beingtheLamé constants.Then,thehyperelasticconstitutiverelationforSeisderived asSe=
∂ψ
ie(
Ee)
∂
Ee =μ
I+[λ
ln(
J)
−μ
]Ce−1. (21)Generally,the microstress
ξ
(α)i maycomprise anenergetic partanda dissipativepart(Bargmannet al.,2014;Gurtin and Anand, 2005).Here, forsimplicity,ξ
i(α) isassumedtobepurely energetic.AccordingtoKuroda andTvergaard(2008)andErtürk etal. (2009),the energetic microstress
ξ
(α)i inthe work-conjugate theories can be essentially relatedto the back stressτ
ib(α)inthenon-work-conjugatetheories(seee.g.,Bayleyetal.,2006)asfollowsτ
ib(α)=−Diviξ
i(α). (22)In Ertürk et al. (2009), based on relation (22) and the expression of the back stress
τ
ib(α) derived byBayley et al. (2006) through considering the elastic interactions between GNDs within the same slipsystem and those fromdifferentslipsystems,theconstitutiverelationfor
ξ
i(α)isgiven.Here,wedirectlyadopttherelationtherein,thusξ
i(α)isexpressedas
ξ
i(α)=μ
bl28[1−
ν
]
β
ρ
ige(β)Be(αβ)+μ
bl24
β
ρ
igs(β)Bs(αβ) (23)with
Be(αβ) =
3
s(α)·s(β)
m(α)·s(β)
+
s(α)·m(β)
m(α)·m(β)
+4
ν
s(α)·p(β)
m(α)·p(β)
m(β)
−
s(α)·s(β)
m(α)·m(β)
+
s(α)·m(β)
m(α)·s(β)
s(β), Bs(αβ) =−
s(α)·p(β)
m(α)·s(β)
+
s(α)·s(β)
m(α)·p(β)
m(β) +
s(α)·s(β)
m(α)·m(β)
+
s(α)·m(β)
m(α)·s(β)
p(β), (24)
where
ν
isPoisson’s ratioandldenotes theradiusof thedomainwithin whichtheinteraction betweenGNDsis consid- ered.Alternatively,theinteractionbetweendifferentslipsystemscanbeaccountedforintherelationforGNDdensitiesin Eqs.(8)and(9)asdoneinBargmannetal.(2011)andHusser&Bargmann(2017),butthiswayisnotpursuedhere.Thescalarmicroforce
π
i(α)beingdissipativeinnatureisassumedtofollowavisco-plasticpower-law,i.e.,π
i(α)=Rbi(α)γ
˙(α)γ
˙0b mbsgn
γ
˙(α), (25)
wheresgn()denotesthesignfunction,mb istherate-sensitivityexponentinthebulk,and
γ
˙0bisthereferencesliprate.The slipresistanceRbi(α)resultingfromtherandomtrappingprocessesbetweenSSDshasthefollowinglinearhardeningform,Rbi(α)=Rb0(α)+ β
Hb(αβ)
γ
acc(β), (26)where
γ
acc(β)=γ
˙(β)dt is the accumulated plastic slip. The initial slip resistance Rb0(α) may depend on the initial SSD density,andHb(αβ) isthelocalhardeningmodulus.BysubstitutingEq.(25)intoEq.(18),themicroscopicbalanceequation isrewrittenastheevolutionequationofplasticsliprate,i.e.,γ
˙(α)=γ
˙0bDivi
ξ
i(α)+τ
i(α)Rbi(α)
m1b
sgn Divi
ξ
i(α)+τ
i(α) , (27)The microforce
η
i(α) atthe surfaceisdivided intoan energetic partη
eni (α) anda dissipativepartη
disi (α).According toPengand Huang(2015),the powerexpended by the energeticmicroforce
η
eni (α) atthesurface equals thechange ofthesurfaceenergyresultingfromsurfacestepsformedafterdislocationabsorption,
α
Si
η
ien(α)γ
˙(α)dSi−Si
ψ
˙iSdSi=0, (28)where
ψ
˙iS is the rate of the surface energy densityresulting from surface steps formed after dislocation absorption. In PengandHuang(2015),theexpressionforthedensityofsurfaceenergyinthesmalldeformationcasewasstrictlyderived by considering both the surfaceenergy change due to the increase of surfacearea andthe interaction energy between surfacesteps. Following the ideatherein andconsidering the effectof finitedeformations, theexpression forψ
˙iS can be readilyderived,andwithoutgoingintothedetails,theresultisdirectlygivenhere,i.e.,ψ
˙iS=α
1(α)
γ
˙(α)s(α)·Nisgnγ
(α)+ α,β
2(αβ)s(α)·Nim(α)×Nis(β)·Nim(β)×Ni
γ
˙(α)γ
(β). (29)Thefirstandsecondtermsrepresentcontributionsfromtheincreaseofsurfaceareaandtheinteractionbetweensurface steps,respectively.(α)1 denotes the surface freeenergy per unit surface step area and(αβ)2 is the surface hardening mod- ulusmeasuringtheinteractionstrengthbetweensurfacestepsfromslipsystems
α
andβ
.InEq.(29),thesurfaceoutwardnormalvectorNiintheintermediateconfigurationdependsondeformation,and,hence,theexplicitexpressionfortheden- sityofsurfaceenergyisnotavailable,whichisdifferentfromthesmalldeformationcasewherethesurfaceoutwardnormal vectorremainsunaltered.Then,fromEq.(28),
η
ien(α)isexpressedasη
ien(α)=(α)1 s(α)·Nisgn
γ
(α)+ β
2(αβ)s(α)·Nim(α)×Nis(β)·Nim(β)×Ni
γ
(β). (30)Thedissipativesurfacemicroforce
η
disi (α)isintroducedtoconsiderthedissipativenatureofdislocationabsorptionbysur- facesasindicatedbyinsituexperiments(Ohetal.,2009;Zhongetal.,2017).Toconstructaconstitutiverelationforη
disi (α)physically,detailedinformationontheprocess fora dislocationabsorbedby asurfaceisnecessary, whichneverthelessis notyetavailableintheliterature.Asan estimate,theresistanceforce againstdislocationabsorptionisproportional tothe rateofdislocationabsorption(measuredbytheplasticsliprateatthesurface).Moreover,theresistanceforceincreaseswith theaccumulateddensityofsurfacesteps.Thesecan beaccountedforinthe followingrate-dependentpower-lawrelation for
η
idis(α),η
idis(α)=Rsi(α)γ
˙(α)γ
˙0s mssgn
γ
˙(α). (31)
γ
˙0s isthereferencesliprateatthesurfaceandms isthesurfacerate-sensitivityexponent.ThesurfaceslipresistanceRsi(α) isexpressedasRsi(α)=Rs0(α)+ β
Hs(αβ)
γ
accs(β), (32)where
γ
accs(β)=γ
˙(β)dt istheaccumulatedslipatthesurface,Rs0(α) denotestheinitialsurfaceslipresistance,andHs(αβ) isthe dissipativesurfacehardening modulus. Forimperfect surfaceswith surfacecoatings,oxide layers orinitial defects, thesurfaceparametersdependontheinitialsurfacestate.Itisworthmentioningthatinsomegrainboundarymodels(van Beers etal., 2013), a similar formfor dissipativegrain boundary microforce is adopted, butthe slipresistance is simply assumedtobeconstant,bywhichthedissipativehardeningisignored.Neglectingthemicrotractioni(α),themicroscopicboundaryconditionEq.(19)isrewrittenas
γ
˙(α)=γ
˙0s−
ξ
i(α)·Ni−η
eni (α)Rsi(α)
m1ssgn −
ξ
(α)i ·Ni−η
eni (α) (33)whichconstitutesthegoverningequationfordislocation absorptionby surfaces.Bothenergeticanddissipativesurfaceef- fectsareaccountedfor.
3. Finiteelementimplementation
Forthe rate-dependentinitial boundary value problemfromthe presentrate-dependentmodel to be solved forarbi- trarygeometriesandboundaryconditions,adual-mixedfiniteelementformulation(Ekhetal.,2007)isadopted.Theforce balanceEq.(16) andtheevolutionEqs. (8)and(9)forthe GNDdensities arechosen asgoverningequations,and, hence, thedisplacement u andthe GNDdensities
ρ
ge(α) andρ
gs(α) are considered as primary variables. The plasticslipγ
(α) isevaluated locallyat the integrationpoints. The treatment for thebalance of momentum (16)is straightforward, butdue tothesurfaceeffects,thedicretizationandimplementationoftheGNDevolutionequationsdeservesomeattention. Since theevolution equationsfor thetwo kinds ofdislocationsare similar, it isonly explainedfor edgeGND densities forthe sakeof brevity.Toobtain theweak formsofthegoverning equations,theyare multipliedby weighting functions
δ
uandδ ρ
˙ge(α), whichvanishat thepartof thesurfacewithnaturalboundary conditions,andthen integratedoverthe volume.Next,applyingthedivergencetheorem,weobtain
Fig. 1. Sketch of thin film benchmark problem.
Vi
[Fe·Se]:
∇
iδ
udVi−STi
δ
u·TidSTi =0, (34)
Vi
δ ρ
˙ige(α)ρ
˙ige(α)−1bs(α)·
∇
iδ ρ
˙ige(α)γ
˙(α)dVi+
STi
1
bs(α)·Ni
δ ρ
˙ige(α)γ
˙(α)dSTi =0, (35) where the surface traction boundary condition(17) has been substituted into Eq.(34). The plastic slip rateγ
˙(α) atthe surfaceinEq.(35)isevaluated locallyvia themicroscopicsurfaceboundary condition(33),andtheinitial GNDdensities areneglected(butarestraightforwardtoincorporate).Forthespatialdiscretization,thevolumeofthebodyisdividedinto finite elementsineach ofwhich, followingthe standard Galerkinapproach,the unknown fieldsofthe displacement and GNDdensitiesandtheweightingfunctionsareapproximatedbytheirnodalvaluesmultipliedbyshapefunctions.Fortime integrationwithinatimeincrement[tn,tn+1],theimplicitbackwardEulerschemeisadoptedsuchthatγ
˙n(α)+1=γ
(α)t ,
ρ
˙nge+(α)1 =ρ
ge(α)t , Fpn−+11=Fpn−1·
I−
α
γ
(α)s(α)m(α), (36)
where
γ
(α)=γ
n(α)+1−γ
n(α),ρ
ge(α)=ρ
gen+(α)1 −ρ
nge(α), t=tn+1−tn andthe subscript n identifies the quantities atthe nthtime step.Then, theweak forms(34)and(35)reduce toa highlynonlinear, stronglycoupledsystemofequations at eachtimestepwhicharesolvedbytheNewton–Raphsonmethod.Fortheincorporationofthesurfacemodelintothefiniteelementformulation,theevaluationofsliprateatthesurface involvedinthesurfaceintegrationinEq.(35)isrequired.Tothisend,theincrementofplasticslip
γ
(α) atthesurfaceisdeterminedbythemicroscopicboundarycondition(33)as
γ
(α)=t
γ
˙0s−
ξ
i(α)·Ni−η
eni (α)Rsi(α)
m1ssgn −
ξ
(α)i ·Ni−η
eni (α), (37)
whereplasticslipsrequiredtoevaluatethetermsattherighthandsideareextrapolatedfromthebulk.Particularly,ifthe surfacedissipativemicroforceisignored,theincrementofplasticslip
γ
(α) atthesurfaceisevaluatedby−
ξ
i(α)·Ni=(α)1 s(α)·Nisgn
γ
(α)+γ
n(α)+
β
(αβ)2 s(α)·Nim(α)×Nis(β)·Nim(β)×Ni
γ
(β)+γ
n(β) , (38)whichconstitutesthemicroscopicboundaryconditionsforapurelyenergeticsurface.
4. Numericalexample
Aplane strain benchmarkproblemofplaneconstrainedshearofa singlecrystallinethinfilmisstudied.As illustrated inFig.1,thefilmwiththicknesshinthex2-directionisassumedtobeinfinitelylonginthex1-direction,andwithoutloss ofgenerality, two active slipsystemswitheach ofthem definedby aslip directions(α)=[cos
θ
α,sinθ
α] anda slipplane normalm(α)=[−sinθ
α,cosθ
α]areconsidered.Forthepresentplanestrainproblem,onlyedgeGNDsareinvolved.Thethinfilm suffersa homogeneous external shear rate
γ
˙ext with its lower surfacebeingconstrained such that the macroscopic boundaryconditionsreadu1
(
x1,0)
=u2
(
x1,0)
=u2
(
x1,h)
=0,u1
(
x1,h)
=γ
˙extht, (39) whereu1 andu2 denotethedisplacementincrementsaftertime incrementt.Microscopically,thesinglecrystalthin film isfree-standing, andthereforethe governing Eq.(33) fordislocation absorption by surfaces actsas the microscopic surfaceboundarycondition.Inaddition,tomodeltheinfiniteextensionofthefilminthex1-direction,arepresentativepart ofthethinfilmwithlengthLisconsidered andperiodicboundaryconditionsare imposedforboththedisplacementand theGNDdensities
u1
(
0,x2)
=u1(
L,x2)
, u2(
0,x2)
=u2(
L,x2)
,ρ
ge(1)(
0,x2)
=ρ
ge(1)(
L,x2)
,ρ
ge(2)(
0,x2)
=ρ
ge(2)(
L,x2)
, (40)wheretheperiodiclength Lcan bearbitrarily chosen withoutaffectingthesolution.Forthespatialdiscretization,4-node bilinear quadrilateralelements with2×2full integrationare chosen forboth thedisplacements andthe GND densities.
Tonumericallyevaluatethesurfaceintegral,twoadditionalintegrationpointsareplacedonthesurfaceedges ofelements locatedatthesurface.
The elastic parameters and the magnitude of the Burgers vector representative of aluminium are taken here, i.e.,
μ
=26.3GPa,ν
=0.33andb=0.286nm.Some ofthe plastic material parameters are takenasRb0(α)=20MPa, Hb(αβ)= 200MPa,γ
˙0b=γ
˙0s=0.001s−1,mb=ms=0.05.The characteristic length scale isassumed to be constant, i.e., l=0.5μ
m.The magnitudeofthe loading shearrate
γ
˙ext is 0.001s−1.To illustrate theinfluence ofenergetic anddissipativesurface effects,differentvalueswill be takenfortheremaining parameters involvedin thesurfacemodel,i.e., Rs0(α),Hs(αβ),(α)1 and2(αβ)inthefollowingsimulations.Forsimplicity,thesurfaceparametersfromdifferentslipsystemsareassumedtobe thesame,i.e.,Rs0(α)=Rs0,Hs(αβ)=Hs,1(α)=1 and(αβ)2 =2.4.1. ValidationoftheFEMsolution
First,tovalidatethefiniteelement implementationsummarizedinSection3,theFEMsolutioniscomparedtothean- alyticalsolution of (Peng andHuang, 2017). The analytical solution in Pengand Huang(2017) only applies to the small deformationcasewithoutdissipativeeffects.However, ifthe appliedloadissmallanddissipativemicroforcesboth inthe bulk and the surfaceare ignored, the solution of the presentproblem should approach the analytical one. Thus, in the followingcomparison,thedissipativeforces
π
i(α) andη
disi (α) aretemporarilyignored.Toavoidrepetition,theresultsfrom theanalyticalsolutionaredirectlygivenherewithoutpresentingthedetailedformulationwhichcanbefoundinPengand Huang(2017).Forboththenumericalandanalyticalcases,theassociatedparametersotherthanthosegivenabovearetaken ash=1μ
m,θ
1=π
/12,θ
2=5π
/12,1=10N/mand2=100N/m.InFig.2a,theshearstressσ
12,whichishomogeneous alongthex2-direction,isplottedasafunction oftheexternally appliedshearγ
ext.Thenumericalresultscorrespondverywelltotheanalyticalresultsfor
γ
ext<0.005.Ifγ
extincreases,aslightdifferenceisnoticeablewhichisattributedtothefi-nitedeformationframeworkappliedhere.Thestress-straincurvesaredividedintothreestagesbytwoyieldingpointswhich denotetheonsetofdislocationabsorptionbysurfacesforthetwoslipsystems.Asdissipativeresistancesareignoredatthis stage,plasticdeformationoccursimmediatelyafterloading,and, hence,thereisnobulkyieldingpointonthestress-strain curve.InFig.2bandc,thedistributionsofplastic slipsandGNDdensities alongthex2-direction areshown, wherethree valuesof
γ
extnamely0.001,0.002and0.005representingthethreestagesrespectivelyaretaken.Forbothplasticslipsand GNDdensities,theFEMcurvescoincidealmostperfectlywiththeanalyticalcurves,indicatingtheexcellentmatchbetween theFEMandanalyticalsolutions.4.2.Influenceofenergeticanddissipativesurfaceeffects
Inthepresentsurfacemodel,bothenergeticanddissipativesurfaceeffectsareinvolved.Here,toillustratetheirinfluence separately,two specific cases, i.e., the casewithonly energetic surfaceeffects and theone withonly dissipativesurface effectsareconsidered,respectively.Inbothcases,
θ
1=π
/3andθ
2=2π
/3aretaken.First,weconsiderthecasewithonlyenergeticsurfaceeffects.Fordifferentvaluesof1 and2,thestress-straincurve, theevolutionofthetotalaverageGNDdensity
ρ
¯ge=h0
ρ
ge(1)+ρ
ge(2)dx2/h,theevolutionofsliprateγ
˙satthesur- face,andthedistributionofplasticslipγ
forγ
ext=0.01areplottedinFig.3a–d,respectively.Sincetheresultsforthetwo slipsystemsaresimilarduetosymmetry,onlythoseforslipsystem1aredisplayed.InFig.3a,thestress-straincurvesfor theenergeticsurfacemodelare generallydivided intothreestagesby two pointsrespectively denotingmacroscopicbulk yieldingandtheonsetofdislocationabsorptionbysurfaces(oralternatelysurfaceyielding).Similarstress-straincurveswith bothbulkandsurface/interfaceyieldingpointsarealsopredictedbysomeother modelswithsurface/interfaceeffects(see e.g.,Aifantisetal.,2006;vanBeersetal.,2013;FredrikssonandGudmundson,2005;Husseretal.,2017).Afterbulkyielding, thesurfaceinitiallyremainsimpenetrableduetothelackofdrivingforcefordislocationabsorption,andthehardeningrate isthesameasthatpredictedbymicrohardboundarycondition.Iftheexternallyappliedshearreachesacriticalvalue,the drivingforce issufficient to overcomethe energeticsurfaceresistance fordislocation absorption, surfaceyielding occurs,Fig. 2. Comparison between FEM and analytical solutions: (a) stress-strain curve; (b) distribution of plastic slips; (c) distribution of GND densities. The FEM results correspond very well with the analytical results except the slight difference in stress-strain curve if γextis larger than 0.005 due to the finite-deformation framework in contrast to the small deformation theory employed in the analytical solution.
resultinginaconsiderabledecreaseinthehardeningrate.FromFig.3b,aftersurfaceyielding duetotheabsorptionofdis- locationsbythesurface,theaccumulationrateofthetotalaverageGNDdensitydecreasesinaccordancewiththedecrease ofhardeningrate.Comparingtheresultsfordifferentvaluesof1and2revealsthatthecriticalpointforsurfaceyielding onlydependsonthesurfaceenergyparameter1.Alarger1resultsinsurfaceyieldingatalarger
γ
ext.ThehardeningrateandtheaccumulationrateofGNDdensityaftersurfaceyieldingaregovernedbytheenergetichardeningmodulus2ina waythatalarger2 yieldsalarger hardeningrate.AsshowninFig.3c,aftersurfaceyielding,thesliprateatthesurface (measuringtherateofdislocationabsorptionbysurface)increasesimmediatelyfromzerotoaconstantleveldependingon thechosen magnitudeof2.Moreover,the surfaceresistanceagainst dislocationabsorption increaseswithincreasing 2. FromFig.3d,forsmaller1 and2,plasticslipsareeasiertodevelopanddistributemorehomogeneously.Thecurvespre- dictedbytheenergeticsurfacemodelareboundedbythoseformicrohardandmicrofreemodels,andtheenergeticsurface modelcanreadilyreduce tothemicrohard caseorthemicrofree caseby increasingthesurfaceparameters 1 and2 to infinityordecreasingthemtozero.
FromFig.3a,strainhardeningaftersurfaceyielding isinsignificantunlesstheenergetichardeningmodulusisimpracti- callylarge.2AsimilarconclusionwasdrawnfortheenergeticsurfacecontributioninthemodelofHurtadoandOrtiz(2012). There,animpracticallylargesurfaceparameterwasrequiredinorderforthemodeltocapturesize-dependentstrainhard- eningof micropillarsunder compression.Thecurrentresults implythat theenergetic surfaceeffectsare not sufficientto account forthe size-dependenthardeninginsmall-sizedsinglecrystals.Forthatreason, therole ofdissipativesurfaceef- fectsneedstobeinvestigated.Thus,weconsidernextthecasewithonlydissipativesurfaceeffects.Tothisend,theenergetic surfacemicroforcesareignoredbysetting1and2tozero.TheinitialsurfaceslipresistanceRs0andthedissipativesurface
2As estimated by Peng and Huang (2015) , the physically based energetic hardening modulus 2should be smaller than 100 N/m.
Fig. 3. Purely energetic surface model: (a) stress-strain curves; (b) evolution of the total average GND density; (c) evolution of slip rate at the surface; (d) distribution of plastic slip for γext= 0 . 01 . Surface yielding depends on 1. Surface hardening, the accumulation rate of the total average GND density after surface yielding, and the slip rate at the surface at the steady-state are governed by the energetic surface hardening modulus 2. For smaller 1and 2, plastic slips develop faster and distribute more homogeneously after surface yielding. The results of the energetic surface model are bounded by those of microhard and microfree models.
hardeningmodulusHsarevaried. InFig.4a–d,thestress-straincurve,theevolutionofthetotalaverageGNDdensity
ρ
¯ge, theevolutionofsliprateγ
˙s atthesurface,andthedistributionofplasticslipγ
forγ
ext=0.01 fordifferentvaluesofRs0 andHsaredisplayed,respectively.Thepurelydissipativesurfacemodelpredictsplasticbehaviorquitesimilartothatofthe purelyenergetic one.Particularly, thesurfaceyielding dependsonthe initialslipresistance Rs0,while thehardeningrate, theaccumulation rateofthetotal GNDdensityafter surfaceyielding, andthesliprateat thesurfaceatsteady-state are governedbythedissipativesurfacehardeningmodulusHs.Inviewofreversibilityassociatedwithsurfacestepformation,weexploretheinfluenceofsurfaceeffectsontheplastic behavior duringunloading. Tothisend, the stress-straincurve, the evolution ofsliprate atthe surfaceduringa loading andunloading cycle predictedby the purely energetic surface model,the purely dissipative surfacemodel andthe gen- eralsurfacemodel withboth energetic anddissipativesurface effectsare displayed inFig. 5a andb,respectively, where 1=10N/m,2=100N/m,Rs0=5N/mandHs=200N/m.The loading isapplied up to
γ
ext=0.01,followed by full un- loading.Fromthefigures,thecurvespredictedbythetwomodelsaresimilarduringloading.Forunloading,thesituationis different.Forthepurelyenergeticsurfacemodel,duringunloading,theenergeticsurfacemicroforce,whichcanberegarded asasurfaceback-stress,actsasthedrivingforcefortherecovery ofsurfacesteps(inversetodislocationabsorptionduring loading).Hence,bulkyieldingandsurfaceyieldingoccuratthesametime.Thehardeningrateandthesliprateatthesur- faceimmediatelyafteryielding (thesecondunloadingstage)areidenticaltothatofthethirdloadingstagewithbothbulk andsurfacehardening.Ifγ
extdecreasestoacriticalvalue,theenergeticmicroforcesdecreasetozero,thesurfacebecomes impenetrableagain. After that the hardening rate remains the same asthat ofthe second loading stage with onlybulk hardening,andthe sliprateat thesurfacedecreases to zero.Forthe purely dissipativesurfacemodel,during unloading, duetotheexistenceofthedissipativesurfacemicroforce,therecoveryofsurfacestepsdoesnottakeplaceuntilthedrivingFig. 4. Purely dissipative surface model: (a) stress-strain curves; (b) evolution of the total average GND density; (c) evolution of slip rate at the surface;
(d) distribution of plastic slip for γext= 0 . 01 . Surface yielding depends on initial surface resistance R s0. Surface hardening, the accumulation rate of the total average GND density after surface yielding, and the slip rate at the surface at the steady-state are governed by dissipative surface hardening modulus H s. For smaller R s0and H s, plastic slips develop faster and distribute more homogeneously after surface yielding. The results of the dissipative surface are bounded by those of the microhard and microfree models.
force (the net contributionofbulk andsurfaceenergetic microforces)is sufficient toovercomethe dissipativeresistance.
Hence,thebulkyieldsfirstand,subsequently,thesurfaceyieldingoccursonlyifthedrivingforceovercomestheresistance.
Thehardeningrateandthesliprateatthesurfaceforthesecondandthirdunloadingstagesareidenticaltothoseforthe correspondingloadingstages.Forthegeneralsurfacemodelwithbothdissipativeandenergeticsurfaceeffects,theloading andunloadingbehaviorsaresimilartothoseofthepurelydissipativesurfacemodel.Inaddition,apronouncedBauschinger effectisalsoobservedinFig.5a.
4.3. Influencesoffilmthicknessandorientationofslipsystems
Toexploretheinfluencesofthefilmthicknessh,fordifferentvaluesofh,thestress-straincurve,theevolutionofthetotal averageGNDdensity
ρ
ge ,theevolutionofsliprateγ
˙ atthesurface, andthedistributionofplasticslipγ
forγ
ext=0.01 are plottedin Fig.6a–d, whereθ
1=π
/3 andθ
2=2π
/3,1=5N/m,2=100N/m,Rs0=5N/mand Hs=200N/m. The resultsdisplayedinFig.6clearlydepict asize-dependentmaterialresponse.Inthinnerfilms,theflowstress andthetotal averageGNDdensityataspecificγ
extare larger,whichindicatesthat “smallerisstronger”.AsshowninFig.6aandc,inthinnerfilms, surfaceyieldingoccursatasmallerapplied shear
γ
ext,andthesliprateatthesurface(measuringtherateof dislocation absorption)atthe steady state islarger, which impliesthat surface yielding occursmore easily atsmaller scales.Infact,intheexperimentsby Gruberetal.(2008),itisfoundthat forsingle-crystallineAuthinfilms withsmaller thickness,afterbulkyielding,thestrainhardeningratesdecreasesuddenlyataspecificpointwhichissuspectedtobethe surfaceyieldingpoint,whileforfilms withlargerthickness, nosuchphenomenonoccurs, whichisqualitativelyconsistent withthepredictedresultshere.
Fig. 5. Purely dissipative surface model versus purely energetic surface model: (a) stress-strain curves; (b) evolution of slip rate at the surface. A pro- nounced Bauschinger effect of earlier re-yielding is observed. The results predicted by the purely energetic and dissipative surface models are similar during loading but differ during unloading.
Fig. 6. Size effect: (a) stress-strain curves; (b) evolution of the total average GND density; (c) evolution of slip rate at the surface; (d) distribution of plastic slip for γext= 0 . 01 . In thinner films, surface yielding occurs earlier. A smaller thickness results in a larger flow stress and a larger total average GND density at a specific load, and a larger surface slip rate at the steady-state. In the middle of the film, a smaller thickness yields a smaller plastic slip. Near the surface, a smaller thickness gives a larger plastic slip.