Ch.8. Plasticity
CH.8. PLASTICITY
Multimedia Course on Continuum Mechanics Overview
Introduction Lecture 1 Previous Notions Lecture 2 Lecture 3 Principal Stress Space Lecture 4 Normal and Shear Octahedral Stresses Stress Invariants Lecture 5 Effective Stress Rheological Friction Models Elastic Element Frictional Element Elastic-Frictional Model
2 Overview (cont’d)
Rheological Friction Models (cont’d) Frictional Model with Hardening Elastic-Frictional Model with Hardening Phenomenological Behaviour Notion of Plastic Strain Notion of Hardening Lecture 6 Bauschinger Effect Elastoplastic Behaviour 1D Incremental Theory of Plasticity Additive Decomposition of Strain Lecture 7 Hardening Variable Yield Stress, Yield Function and Space of Admissible Stresses Lecture 8 Lecture 9 Constitutive Equation Lecture 9 Elastoplastic Tangent Modulus Lecture 10 Uniaxial Stress-Strain Curve
3 Overview (cont’d)
3D Incremental Theory of Plasticity Additive Decomposition of Strain Hardening Variable Lecture 11 Yield Function Loading - Unloading Conditions and Consistency Conditions Constitutive Equation Lecture 12 Elastoplastic Constitutive Tensor Yield Surfaces Lecture 13 Von Mises Criterion Tresca Criterion Mohr-Coulomb Criterion Lecture 14 Drucker-Prager Criterion
4 8.1 Introduction
Ch.8. Plasticity
5 Introduction
A material with plastic behavior is characterized by: A nonlinear stress-strain relationship. The existence of permanent (or plastic) strain during a loading/unloading cycle. Lack of unicity in the stress-strain relationship.
Plasticity is seen in most materials, after an initial elastic state.
6 Previous Notions
PRINCIPAL STRESSES Regardless of the state of stress, it is always possible to choose a special set of axes (principal axes of stress or principal stress directions) so that the shear stress components vanish when the stress components are referred to this system. The three planes perpendicular to the principle axes are the principal planes. The normal stress components in the principal planes are the principal σ stresses. σ 33 x 31 σ x 3 32 3 ′ σ x3 13 σ σ1 00 23 σ σ x′ σ σ = σ 11 12 σ 21 σ 1 3 [] 002 22 σ1 00σ 3 σ 2 x1 x1 x2 x2 x2′
7 Previous Notions
PRINCIPAL STRESSES The Cauchy stress tensor is a symmetric 2nd order tensor so it will diagonalize in an orthonormal basis and its eigenvalues are real numbers. Computing the eigenvalues λ and the corresponding eigenvectors v :
σσ⋅=vλλ v[] −1 ⋅= v0 σ11 − λσ12 σ13 not
det[]σσ−λ11= −= λ σ12 σ22 − λσ23 =0 σ σ σλ− INVARIANTS 13 23 33 σ σ 33 32 characteristic x 31 σ x λλ−I1 − II 23 λ −=0 3 32 3 equation x3′ σ13 σ 23
λσ≡ σ11 σ12 σ x1′ σ 11 21 σ 22 3 λσ≡ σ1 22 σ λσ33≡ 2 x1 x1 x2 x2 x2′ 8 Previous Notions
STRESS INVARIANTS Principal stresses are invariants of the stress state. They are invariant w.r.t. rotation of the coordinate axes to which the stresses are referred. The principal stresses are combined to form the stress invariants I : I= Tr σ =σ =++ σσσ 1 () ii 123 REMARK 1 2 The I invariants are obtained II2=()σσ: −=−+1 (σσ12 σσ 13 + σσ 23) 2 from the characteristic equation I3 = det ()σ of the eigenvalue problem. These invariants are combined, in turn, to obtain the invariants J:
JI11= = σ ii REMARK The J invariants can be 12 11 J2=() II 12 +=2:σσij ji =()σσ 2 22 expressed the unified form: 1 = σi ∈ 13 11Ji Tr() i {}1, 2, 3 J3=( I 1 +33 I 12 I + I 3) = Tr ()σσσ ⋅⋅ =σσij jk σ ki i 3 33 9 Previous Notions
SPHERICAL AND DEVIATORIC PARTS OF THE STRESS TENSOR Given the Cauchy stress tensor σ and its principal stresses, the following is defined: Mean stress 1 11 σ=Tr ()σ =σ =() σσσ ++ m 3 33ii 123 REMARK Mean pressure In a hydrostatic state of stress, the 1 p =−=−++σm () σσσ123 stress tensor is isotropic and, thus, 3 its components are the same in any Cartesian coordinate system. A spherical or hydrostatic As a consequence, any direction state of stress : σ 00 is a principal direction and the σσσ= = 123 σ ≡=00σσ1 stress state (traction vector) is the 00σ same in any plane.
10 Previous Notions
SPHERICAL AND DEVIATORIC PARTS OF THE STRESS TENSOR
The Cauchy stress tensor σ can be split into: σ=σsph + σ′ The spherical stress tensor: Also named mean hydrostatic stress tensor or volumetric stress tensor or mean normal stress tensor. Is an isotropic tensor and defines a hydrostatic state of stress. Tends to change the volume of the stressed body 11 σσ:=σσ1 =Tr () 11 = sph m 33ii The stress deviatoric tensor: Is an indicator of how far from a hydrostatic state of stress the state is. Tends to distort the volume of the stressed body
σ′ =dev σ = σ−σ m 1
11 Previous Notions
STRESS INVARIANTS OF THE STRESS DEVIATORIC TENSOR The stress invariants of the stress deviatoric tensor:
I1′′= Tr ()σ = 0 1 II′=σσ ′′: − 2 212 () 2221 I3′=det ()σ ′ =σσσ11 ′′′22 33 +2 σσσ 12 ′′′ 23 13 −−− σσ 12 ′′ 33 σσ 23′′ 11 σσ 13 ′′ 22 =() σσσij ′′′ jk ki 3 These correspond exactly with the invariants J of the same stress deviator tensor:
JI11′′= = 0 1 1 JI′′= 2 +==2:II′ ′()σσ ′′ 212 ()222
1 3 11 JI31′′= + 3II12′′+3I33′ = I ′ = Tr ()σσσ ′′′ ⋅⋅ =()σσij ′′′ jk σ ki 3 ( ) 33
12 Previous Notions
EFFECTIVE STRESS The effective stress or equivalent uniaxial stress σ is the scalar:
33 σ =3J ' = σσ′′ = σσ´: ´ 2 22ij ij
It is an invariant value which measures the “intensity” of a 3D stress state in a terms of an (equivalent) 1D tensile stress state. It should be “consistent”: when applied to a real 1D tensile stress, should return the intensity of this stress.
13 Example
Calculate the value of the equivalent uniaxial stress for an uniaxial state of stress defined by: E, ν y σ 00 uσ σ σ ≡ x x 0 00 σ u σ u 0 00 x
z
14 σ u 00 σ ≡ 0 00 Example - Solution 0 00
1 σ σ =σ )= u σ u Mean stress: m Tr( 00 33 3 σ m 00 σ σ ≡=0σ 00u 0 Spherical and deviatoric parts sph m 3 00σ of the stress tensor: m σ 00 u 3 2 σ 00 3 u σσum− 00 1 σ′ =−≡ σσ 0 −σσ 00 = − 0 sph m 3 u 00−σ m 1 00− σ 3 u 3 3 411 32 σσ= σσ′′ =2 () + + = σσσ= 2ij ij 2u 9 9 9 23 u u
15 8.2 Principal Stress Space
Ch.8. Plasticity
16 Principal Stress Space
The principal stress space or Haigh–Westergaard stress space is the space defined by a system of Cartesian axes where the three spatial axes represent the three principal stresses for a body subject to stress: σσσ123≥≥
17 Octahedral plane
Any of the planes perpendicular to the hydrostatic stress axis is a octahedral plane. 1 1 Its unit normal is n = 1 . 3 1 σσσ123≥≥
18 Normal and Shear Octahedral Stresses
Consider the principal stress space: The normal octahedral stress is defined as: 1/ 3 3σoct =OA = OP ⋅=n []σσσ123, , 1/ 3 = 1/ 3 3 =()σσσ ++ =3 σ 3 123 m
I σσ= = 1 oct m 3
19 Normal and Shear Octahedral Stresses
Consider the principal stress space: The shear or tangential octahedral stress is defined as:
3τ oct = AP
Where the AP is calculated from: 2 2 22222 3τoct =AP = OP − OA =(σσσ123 ++) − 1 2 ' −()σσσ123 ++ =2J 2 3 Alternative forms of τ oct : 1/2 112 τ= σσσ222 ++− σσσ ++ oct 1 2 3() 123 3 3 1/2 12 1 222 2 τ= σσ − +− σσ +− σσ τ = []J′ oct ()()()1 2 23 13 oct 3 2 33 20 Normal and Shear Octahedral Stresses
In a pure spherical stress state: 1 σ=σ11 →σ =3 σσ →σσ = = m 3 esf
σ′ =−= σσesf 0 J2′ = 0
τ = A pure spherical stress state is oct 0 located on the hydrostatic stress axis.
In a pure deviator stress state:
′ σ = σσ= σ m =Tr()σσ = Tr (′ ) = 0 oct 0
A pure deviator stress state is located on the octahedral plane containing the origin of the principal stress space
21 Stress Invariants
Any point in space is unambiguously defined by the three invariants:
The first stress invariant I 1 characterizes the distance from the origin to the octahedral plane containing the point.
The second deviator stress invariant J 2′ characterizes the radius of the cylinder containing the point and with the hydrostatic stress axis as axis.
The third deviator stress invariantJ 3′ characterizes the position of the point on the circle obtained from the intersection of the octahedral plane and the
cylinder. It defines an angle θ () J 3′ .
22 Projection on the Octahedral Plane
The projection of the principal stress space on the octahedral plane results in the division of the plane into six “sectors”: These are characterized by the different principal stress orders.
Election of a criterion, FEASIBLE
e.g.: σσσ123≥≥ WORK SPACE
23 8.4 Phenomenological Behaviour
Ch.8. Plasticity
38 Notion of Plastic Strain
PLASTIC STRAIN εε=ep + ε
elastic limit: σ e
LINEAR ELASTIC BEHAVIOUR σε= E e
39 Bauschinger Effect
Also known as kinematic hardening.
σ f σεe + K
K σ e
K
−+σεe K
K −σ e
41 Elastoplastic Behaviour
Considering the phenomenological behaviour observed, elastoplastic materials are characterized by:
Lack of unicity in the stress-strain relationship. The stress value depends on the actual strain and the previous loading history.
A nonlinear stress-strain relationship. There may be certain phases in the deformation process with incremental linearity.
The existence of permanent (or plastic) strain during a loading / unloading cycle.
42 8.5 1D Incremental Plasticity Theory
Ch.8. Plasticity
43 Introduction
The incremental plasticity theory is a mathematical model used to represent the evolution of the stress-strain curve in an elastoplastic material. Developed for 1D but it can be generalized for 3D problems.
REMARK This theory is developed under the hypothesis of infinitesimal strains.
44 Additive Decomposition of Strain
e Total strain can be split into an elastic (recoverable) part, ε , and an inelastic (unrecoverable) one, ε p :
ep σ εε= + ε where ε e = E elastic modulus or Young modulus
Also, dσ ddεε=ep + d εwhere dε e = E
45 Hardening Variable
The hardening variable, α , is defined as: REMARK p The sign () • function is: dα= sign() σε d
α ≥ α = Such that d 0 and ε p =0 0 .
Note that α is always positive and: p dα= d α = sign() σε d ddαε= p =1 Then, for a monotonously increasing plastic strain process, both variables coincide: εεpp dε p ≥ 0 αε=ddε p = ε p = p ∫∫00
46 Yield Stress and Hardening Law
Stress value, σ f , threshold for the material exhibiting plastic behaviour after elastic unloading + elastic loading It is considered a material property. p HARDENING LAW For εα = = 0 σσ fe =
σσfe= + H′ α σ= σαf ()
dσαf = Hd′ σ≤ σαf ()
H ′ is the hardening modulus
47 Yield Function
The yield function, F () σα , , characterizes the state of the material:
F ()σα, ≡− σ σf () α
F σα,0< σα = Space of () F (),0 admissible stresses ELASTIC STATE ELASTO-PLASTIC STATE
ERσ :=∈<{σF () σα ,0} ∂=∈ERσ :{σF () σα ,0 =} ELASTIC DOMAIN YIELD SURFACE
INITIAL ELASTIC 0 DOMAIN: ERσ :=∈{σF () σ,0 ≡−< σσe 0}
48 Space of Admissible Stresses
Any admissible stress state must belong to the space of
admissible stresses, E σ (postulate):
EEσσ= ∂= E σ =∈≤{σR F () σα,0}
F ()σα, ≡− σ σf () α
Space of admissible stresses REMARK
≡−σασα Eσ ff(), ()
49 Constitutive Equation
The following situations are defined: ELASTIC REGIME
σ ∈ Eσ dσε= Ed
ELASTOPLASTIC REGIME – UNLOADING
σ ∈∂Eσ dσε= Ed dF () σα,0<
ELASTOPLASTIC REGIME – PLASTIC LOADING REMARK σ ∈∂Eσ σ ∈∂Eσ The situation dσε= Edep dF ()σα,0= dF(,)σα > 0 is not possible because, by Elastoplastic definition, on the yield tangent modulus surface F () σα ,0 = . 50 Elastoplastic Tangent Modulus
Consider the elastoplastic regime in plastic loading,
σ ∈∂Eσ
F ()σα,≡− σ σf () α =0dF ()σα ,0= ∂ σ dF ()σα,0=d σ −= σ′f () α d α ∂σ =sign()σ =H′ 1 dα= sign() σσ d H′ Since the hardening variable is defined as: d α= sign() σε d p
dσαf = Hd′ p 1 ddε= σσfor ∈∂Eσ H′ HARDENING LAW 51 Elastoplastic Tangent Modulus
1 Elastic strain ddεσe = E 1 Plastic strain ddεσp = H′ Additive strain decomposition : 11 ddεε=+=+ep d ε() d σ EH′ 1 EH′ dσ= dd εε = 11 ′ + EH+ EH′ Eep
ELASTOPLASTIC ep EH′ dσε= Edep E = TANGENT MODULUS EH+ ′
52 Uniaxial Stress-Strain Curve
Following the constitutive equation defined
ELASTOPLASTIC REGIME dσε= Edep
ELASTIC REGIME dσε= Ed
REMARK Plastic strain is generated only during the plastic loading process.
53 Role of the Hardening Modulus
The value of the hardening modulus, H ′, determines the following situations: EH′ E ep = EH+ ′
H′ > 0 Linear elasticity Plasticity with strain hardening H′ < 0 Plasticity with strain softening
Perfect plasticity
55 Plasticity in Real Materials
In real materials, the stress-strain curve shows a combination of the three types of hardening modulus.
H′ < 0 H′ = 0 H′ > 0
56 8.6 3D Incremental Theory
Ch.8. Plasticity
57 Introduction
The 1D incremental plasticity theory can be generalized to a multiaxial stress state in 3D.
The same concepts are used: Additive decomposition of strain Hardening variable Yield function
Plus, additional ones are added: Loading - unloading conditions Consistency conditions
58 εε=ep + ε Additive Decomposition 1D → e σ ε = of Strain E
e Total strain can be split into an elastic (recoverable) part, ε , and an inelastic (unrecoverable) one, ε p :
ep e −1 εε= + ε where εσ= C :
constitutive elastic (constant) tensor Also,
e −1 ddεε=ep + d εwhere ddεσ= C :
59 p 1D→= dελ sign () σ Hardening Variable =dα
The hardening variable, α = f () σε , p , is a scalar:
dαλ= with α ∈∞[0, )
Where λ is known as the plastic multiplier.
The flow rule is defined as: ∂G ()σ ,α dε p = λ ∂σ
Where G () σα , is the plastic potential function
60 1,DF→()σα ≡− σ σ() α Yield Function f
The yield function, F () σ , α , is a scalar defined as: Equivalent uniaxial stress F ()()()σσ,α≡− φ σαf Yield stress
F ()σ ,0α < F ()σ ,0α = ELASTIC STATE ELASTOPLASTIC STATE
Eσ := {σσF () ,0α < } ∂=Eσ :{σσF () ,0α =} ELASTIC DOMAIN YIELD SURFACE Space of INITIAL ELASTIC 0 := σσF () ,0< 0 admissible EEσσ= ∂ E σ DOMAIN: Eσ { } stresses
61 Loading-Unloading Conditions and Consistency Condition
Loading/unloading conditions (also known as Karush-Kuhn- Tucker conditions): λ≥≤0;FF()σσ , α 0; λα() , = 0 Consistency conditions: For,0F ()σσα=→= λαdF () ,0
ELASTOPLASTIC p ∂G ()σ ,α F=<==0; dF 0λλ 0; dε =0 ELASTIC UNLOADING ∂σ
p ∂G ()σα, ELASTOPLASTIC λλ=0; dε = = 0 ∂σ NEUTRAL LOADING F=0; dF = 0 p ∂G ()σα, ELASTOPLASTIC λλ>=0; dε ≠0 ∂σ LOADING F=0; dF > 0 IMPOSSIBLE 62 Constitutive Equation
The following situations are defined: ELASTIC REGIME (F< 0)
σ ∈ Eσ ddσε= C :
ELASTOPLASTIC REGIME – ELASTIC UNLOADING (F= 0 and dF ()σ ,α < 0)
σ ∈∂Eσ ddσε= C : dF ()σ ,0α <
ELASTOPLASTIC REGIME – PLASTIC LOADING (F= 0 and dF ()σ ,α = 0)
σ ∈∂Eσ ddσε= Cep : dF ()σ ,0α = ELASTOPLASTIC CONSTITUTIVE TENSOR
63 MMC - ETSECCPB - UPC 26/04/2017 Elastoplastic Constitutive Tensor
The elastoplastic constitutive tensor is written as: REMARK ∂∂GF CC::⊗ When the plastic potential function ep ∂∂σσ and the yield function coincide, it is CC()σ,α = − ∂∂FGsaid that there is associated flow: H′ + ::C ∂∂σσ GF()()σσ,,αα=
∂∂GF CCijpq rskl ∂∂σσpq rs CCep =−∈i,,,,,,, jkl pqrs {} 1,2,3 ijkl ijkl ∂∂FG H′ + C pqrs ∂∂σσpq rs
64 8.7 Failure Criteria: Yield Surfaces
Ch.8. Plasticity
65 Introduction
0 The initial yield surface, ∂ E σ , is the external boundary of the initial 0 elastic domain E σ for the virgin material The state of stress inside the yield surface is elastic for the virgin material. When in a deformation process, the stress state reaches the yield surface, the virgin material looses elasticity for the first time: this is considered as a failure criterion for design. Subsequent stages in the deformation process are not considered.
66 MMC - ETSECCPB - UPC 26/04/2017 Yield (Failure) Criteria
The yield surface is usually expressed in terms of the following invariants to make it independent of the reference system (in the principal stress space):
F()()σ ≡F IJJ123,,′′ −=σ e 0 with σσσ123≥≥ φ(σ ) REMARK Where: Due to the adopted principal stress
I1= Tr ()σ =σii =++ σσσ123 criteria, the definition of yield surface only affects the first sector ′′1 2 ′ ′1 ′′ JI21= +==2:II22()σσ of the principal stress space. 2 () 2
1 3 11 JI31′′= + 3II12′′+3I33′ = I ′ = Tr ()σσσ ′′′ ⋅⋅ =()σσij ′′′ jk σ ki 3 ( ) 33
The elastoplastic behavior will be isotropic.
67 F ()σσ≡ φ( ) −σ = 0 Von Mises Criterion e
The yield surface is defined as: REMARK The Von Mises criterion σ ≡σσ −= F () () e 0 depends solely on the second deviator stress Where σ () σ = 3 J 2 ′ is the effective stress. invariant. (often termed the Von-Mises stress) 2 12 The shear octahedral stress is, by definition, τ oct = [] J 2 ′ . Thus, the effective stress is rewritten: 3
12 3 33 []J′ = τ σ()σ =3 ττoct = oct 2 2 oct 2 2
3 And the yield surface is given by: F()σ ≡τσoct −= e 0 2
68 3 F()σ ≡τσoct −= e 0 Von Mises Criterion 2
The octahedral stresses characterizes the radius of the cylinder containing the point and with the hydrostatic stress axis as axis. 22 τ= στ →=3 σ oct 33e oct e
FJ(σ) ≡−F ( 2′ ) σ e
REMARK The Von Mises Criterion is adequate for metals, where hydrostatic stress states have an elastic behavior and failure is typically due to deviatoric stress components.
69 Example
Consider a beam under a composed flexure state such that for a beam section the stress state takes the form,
στ 0 xσ xy σ σ = τ x x [] xy 00 0 00
Obtain the expression for Von Mises criterion.
70 Example - Solution
The mean stress is: 1 σ σ =Tr ()σ = x m 33 The deviator part of the stress tensor is:
σσ− τ2 σ τ x m xy 003 x xy 1 σ′ =−≡ σσ τσ −00 = τσ − esf xy m xy 3 x −−σσ1 0 0mx 00 3 The second deviator stress invariant is given by,
′1 ′′ 14112 2 22 2 1 22 J2 =σσ: =σx ++++=+ σ x στ x xy τ xy στx xy 2 29 9 9 3
71 Example - Solution
The uniaxial effective stress is: 22 σ()σ =33J2′ = στx + xy
Finally, the Von Mises yield surface is given by the expression:
στ22+= σ FJ()σ ≡ 3′ −=σ 0 x3 xy e 2 e co (comparison stress)
(Criterion in design codes for metal beams)
72 F ()σσ≡ φ( ) −σ = 0 Tresca Criterion e
Also known as the maximum shear stress criterion, it establishes that the elastic domain ends when: σσ− σ τ =13 = e F ()()σ ≡σσ − −= σ 0 max 22 13 e
Plane parallel to axis σ 2
′ It can be written univocally in terms of invariants J 2′ and J 3 :
F()σ ≡()()σσ1 − 3 −≡ σeeF JJ23′′, −σ
73 F ()()σ ≡σσ − −= σ 0 Tresca Criterion 13 e
F()()σ ≡F JJ23′′,0 −=σ e
REMARK The Tresca yield surface is appropriate for metals, which have an elastic behavior under hydrostatic stress states and basically have the same traction/compression behavior.
74 Example
Obtain the expression of the Tresca criterion for an uniaxial state of stress defined by: E, G y σ u 00 σ σ σ ≡ 0 00x x σ σ 0 00 u u x
z
76 σ u 00 σ ≡ 0 00 Example - Solution 0 00
Consider:
σσ1 = u σ ≥ F ()σ =()σσ13 − −= σe σ ue −= σ σ u − σ e u 0 σ 3 = 0 σu
σ = 0 σ < 1 u 0 F ()σ =()σσ13 − −=−−= σe σσ ue σ u − σ e σσ3 = u σu
The Tresca criterion is expressed as: Note that it coincides with σσ= F()σ ≡−σσe = 0 uethe Von Mises criterion for an uniaxial state of stress.
77 Example
Consider a beam under a composed flexure state such that for a beam section the stress state takes the form,
στ 0 xσ xy σ σ = τ x x [] xy 00 0 00
Obtain the expression for Tresca yield surface.
78 Example - Solution
The principal stresses are: 11 11 σ=++ σ στ22, σ =−+ σ στ22 1324x x xy 24x x xy
Taking the definition of the Tresca yield surface,
F ()()σ ≡σσ13 − −= σe 0 11 11 σσσ=−= σ + στ22 + − σ − στ22 + e 13 x x xy x x xy 24 24 στ22+=4 σ x xy e co (comparison stress) 79 Mohr-Coulomb Criterion
It is a generalization of the Tresca criterion, by including the influence of the first stress invariant. In the Mohr circle’s plane, the Mohr-Coulomb yield function takes the form, cohesion internal friction angle τ=c − σφtan REMARK The yield line cuts the normal stress axis at a positive value, limiting the materials tensile strength.
80 Mohr-Coulomb Criterion
Consider the stress state for which the yield point is reached:
τφA = R cos σσ+ σφ=13 + Rsin A 2
σσ− σσ +− σσ τσ+ φ −= 13φ+ 13 + 13φ φ−= AAtgcc 0 cos sin tg 0 2 22
()()σσ13−++ σσ 13sin φ − 2c cos φ = 0 REMARK
For φσ = 0 and c = e /2 , the Tresca criterion is Fc()()()σ ≡−++σσ13 σσ 13sin φ − 2 cos φ = 0 recovered.
81 Mohr-Coulomb Criterion
F()()σ ≡=F IJJ123,,′′ 0
REMARK The Mohr-Coulomb yield surface is appropriate for frictional cohesive materials, such as concrete, soils or rocks which have considerably different tensile and compressive values for the uniaxial elastic limit.
82 Drucker-Prager Criterion
It is a generalization of the Von Mises criterion, by including the influence of the first stress invariant.
The yield surface is given by the expression: REMARK 1/2 For φσ = 0 and c = /2 , FJσ ≡30ασ +′ −= β e () m []2 the Von Mises criterion is recovered. Where:
2sin φφ6c cos σσσ123++ I1 αβσ= ;;= m = = 3() 3 −− sinφφ3() 3 sin 33
It can be rewritten as: 1/2 3 FIJ()σ ≡α +[]′ −=β3, ασ + τ −= β ()IJ′′ 1 2 oct 2 oct 12
83 Drucker-Prager Criterion
F(σ) ≡F ( IJ12, ′ )
REMARK The Drucker-Prager yield surface, like the Mohr-Coulomb one, is appropriate for frictional cohesive materials, such as concrete, soils or rocks which have considerably different tensile and compressive values for the uniaxial elastic limit.
84 Chapter 8 Plasticity
8.1 Introduction The elastoplastic models (constitutive equations) are used in continuum mechan- ics to represent the mechanical behavior of materials whose behavior, once cer- tain limits in the values of the stresses (or strains) are exceeded, is no longer rep- resentable by means of simpler models such as the elastic ones. In this chapter, these models will be studied considering, in all cases, that strains are infinitesi- mal. Broadly speaking, plasticity introduces two important modifications with re- spect to the lineal elasticity seen in chapters 6 and 7: 1) The loss of linearity: stresses cease to be proportional to strains. 2) The concept of permanent or plastic strain: a portion of the strain generated during the loading process is not recovered during the unloading process.
8.2 Previous NotionsTheory and Problems The concepts in this section are a review of those already studied in Sec- tions 4.4.4Continuumto 4.4.7 of Chapter Mechanics4. for Engineers © X. Oliver and C. Agelet de Saracibar 8.2.1 Stress Invariants Consider the Cauchy stress tensor σ and its matrix of components in a base associated with the Cartesian axes {x,y,z} (see Figure 8.1), ⎡ ⎤ σ τ τ ⎢ x xy xz ⎥ [σ ] = ⎣ τ σ τ ⎦. xyz xy y yz (8.1) τxz τyz σz
369 370 CHAPTER 8. PLASTICITY
diagonalization
Figure 8.1: Diagonalization of the stress tensor.
Since σ is a symmetrical second-order tensor, it will diagonalize in an orthonor- mal base and all its eigenvalues will be real numbers. Then, consider a system of Cartesian axes {x ,y ,z } associated with a base in which σ diagonalizes. Its matrix of components in this base is ⎡ ⎤ σ 00 ⎢ 1 ⎥ [σ ] = ⎣ σ ⎦, x y z 0 2 0 (8.2) 00σ3 where σ1 ≥ σ2 ≥ σ3 , denoted as principal stresses, are the eigenvectors of σ and the directions associated with the axes {x ,y ,z } are named principal directions (see Figure 8.1). To obtain the stresses and the principal directions of σ , the corresponding eigenvalue and eigenvectorTheory problem must and be solved: Problems λ σ · = λ =⇒ (σ − λ ) · = , FindContinuumand v such that Mechanicsv v for Engineers1 v 0 (8.3) where λ corresponds to© the X. eigenvalues Oliver and and v C.to Agelet the eigenvectors. de Saracibar The necessary and sufficient condition for (8.3) to have a solution is det(σ − λ1)=σ − λ1 = 0 , (8.4) which, in component form, results in σ − λτ τ x xy xz τ σ − λτ = . xy y yz 0 (8.5) τxz τyz σz − λ
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Previous Notions 371
The algebraic development of (8.5), named characteristic equation, corre- sponds to a third-degree polynomial equation in λ, that can be written as
3 2 , λ − I1λ − I2λ − I3 = 0 (8.6) where the coefficients I1 (σij), I2 (σij) and I3 (σij) are certain functions of the components σij of the tensor σ expressed in the coordinate system {x,y,z}. Yet, the solutions to (8.6), which will be a function of its coefficients (I1, I2, I3), are the principal stresses that, on the other hand, are independent of the system of axes chosen to express σ . Consequently, said coefficients must be invariant with respect to any change of base. Therefore, the coefficients I1, I2 and I3 are denoted as I stress invariants or fundamental stress invariants and their expression (re- sulting from the computation of (8.5)) is ⎧ ⎪ I1 = Tr (σ )=σii = σ1 + σ2 + σ3 ⎨ I stress = 1 σ σ − 2 = −(σ σ + σ σ + σ σ ) ⎪ I2 : I1 1 2 1 3 2 3 (8.7) invariants ⎩⎪ 2 I3 = det(σ )=σ1 σ2 σ3
Obviously, any scalar function of the stress invariants will also be an invariant and, thus, new invariants can be defined based on the I stress invariants given in (8.7). In particular, the so-called J stress invariants are defined as ⎧ ⎪ ⎪ ⎪ = = σ = (σ ) ⎪ J1 I1 ii Tr ⎪ ⎪ ⎪ Theory1 and 1 Problems ⎪ J = I2 + 2I = σ σ = ⎨⎪ 2 2 1 2 2 ij ji J stress = 1 (σ σ )=1 (σ · σ ) (8.8) invariants ⎪ : Tr Continuum⎪ Mechanics2 2 for Engineers ⎪ © X. Oliver and C. Agelet de Saracibar ⎪ 1 1 ⎪ J = I3 + 3I I + 3I = σ σ σ = ⎪ 3 1 1 2 3 ij jk ki ⎪ 3 3 ⎪ 1 ⎩ = Tr (σ · σ · σ ) 3
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 372 CHAPTER 8. PLASTICITY
Remark 8.1. Note that I1 = 0 =⇒ Ji = Ii i ∈ {1,2,3} . Also, the invariants Ji , i ∈ {1,2,3} can be expressed in a unified and compact form by means of 1 J = Tr σ i i ∈ {1,2,3} . i i
8.2.2 Spherical and Deviatoric Components of the Stress Tensor
Given the stress tensor σ , the mean stress σm is defined as
I 1 1 1 σ = 1 = Tr (σ )= σ = (σ + σ + σ ) (8.9) m 3 3 3 ii 3 1 2 3 and the mean pressure p¯ as . p¯ = −σm (8.10) The Cauchy stress tensor can be decomposed into a spherical part (or com- σ σ ponent), σ sph, and a deviatoric one, σ , σ σ σ , σ = σ sph + σ (8.11) where the spherical part of the stress tensor is defined as Theory and Problems σ def 1 σ σ sph : = Tr (σ )1 = σm1 ⎡ 3 ⎤ σm 00 (8.12) Continuum Mechanics⎢ for⎥ Engineers ©σ X. Olivernot≡ and C. Agelet de Saracibar sph ⎣ 0 σm 0 ⎦
00σm and, from (8.11) and (8.12), the deviatoric part is given by
⎡ ⎤ σ − σ τ τ ⎢ x m xy xz ⎥ σ = σ − σ not≡ . sph ⎣ τxy σy − σm τyz ⎦ (8.13)
τxz τyz σz − σm
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Previous Notions 373
Finally, the I and J invariants of the deviatoric tensor σ , named I and J invari- ants, respectively, are derived from (8.7), (8.8), (8.9) and (8.13). ⎧ ⎪ ⎪ ⎪ J = I = 0 ⎪ 1 1 ⎨ J stress 1 1 ⎪ J = I = (σ : σ )= σ σ (8.14) invariants ⎪ 2 2 2 2 ij ji ⎪ ⎪ 1 ⎩ J = I = σ σ σ 3 3 3 ij jk ki
Remark 8.2. It is easily proven that the principal directions of σ co- incide with those of σ , that is, that both tensors diagonalize in the same base. In effect, working in the base associated with the princi- pal directions of σ , i.e., the base in which σ diagonalizes, and, given σ that σ sph is a hydrostatic tensor and, thus, is diagonal in any base, then σ also diagonalizes in the same base (see Figure 8.2).
Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 8.2: Diagonalization of the spherical and deviatoric parts of the stress tensor.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 374 CHAPTER 8. PLASTICITY
Remark 8.3. The effective stress or equivalent uniaxial stress σ¯ is the scalar 3 3 σ¯ = 3J = σ σ = σ : σ . 2 2 ij ji 2 The name of equivalent uniaxial stress is justified because its value for an uniaxial stress state coincides with said uniaxial stress (see Example 8.1).
Example 8.1 – Compute the value of the equivalent uniaxial stress (or effec- tive stress) σ¯ for an uniaxial stress state defined by ⎡ ⎤ σu 00 not ⎢ ⎥ σ ≡ ⎣ 000⎦ . 000
Solution The mean stress is 1 σ σ = Tr (σ )= u . m 3 3 Then, the spherical component of the stress tensor is ⎡ ⎤ ⎡ ⎤ σu 00 Theoryσm 00 and Problems⎢ 3 ⎥ ⎢ ⎥ ⎢ σ ⎥ σ not≡ = ⎢ u ⎥ sph ⎣ 0 σm 0 ⎦ ⎢ 0 0 ⎥ ⎣ 3 σ ⎦ Continuum Mechanics00σm for Engineersu © X. Oliver and C. Agelet00 de Saracibar 3 and the deviatoric component results in ⎡ ⎤ ⎡ ⎤ 2 σu 00 σu − σm 00 ⎢ 3 ⎥ ⎢ ⎥ ⎢ ⎥ σ σ σ not ⎢ 1 ⎥ σ = σ − σ sph ≡ ⎣ 0 −σ 0 ⎦ = ⎢ 0 − σ 0 ⎥ . m ⎣ 3 u ⎦ 00−σ 1 m 00− σ 3 u
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Principal Stress Space 375
Finally, the equivalent uniaxial stress (or effective stress) is obtained, 3 3 4 1 1 3 2 σ¯ = σ σ = σ 2 + + = |σ | = |σ | =⇒ 2 ij ji 2 u 9 9 9 2 3 u u
. σ¯ = |σu|
8.3 Principal Stress Space 3 Consider a system of Cartesian axes in R {x ≡ σ1, y ≡ σ2, z ≡ σ3} such that each stress state, characterized by the values of the three principal stresses σ1 ≥ σ2 ≥ σ3, corresponds to a point in this space, which is known as the prin- cipal stress space1(see Figure 8.3).
Definition 8.1. The hydrostatic stress axis is the locus of points in the principal stress space that verify the condition σ1 = σ2 = σ3 (see Figure 8.3). The points located on the hydrostatic stress axis repre- sent hydrostatic states of stress (see Chapter 4, Section 4.4.5).
Theory and Problemshydrostatic stress axis (σ1 = σ2 = σ3) Continuum Mechanics for Engineers= bisector of the 1st octant © X. Oliver and C. Agelet de Saracibar
Figure 8.3: The principal stress space.
1 The principal stress space is also known as the Haigh-Westergaard stress space.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 376 CHAPTER 8. PLASTICITY
hydrostatic stress axis (σ1 = σ2 = σ3)
Figure 8.4: The hydrostatic stress axis and the octahedral plane.
Definition 8.2. The octahedral plane Π is any of the planes that are perpendicular to the hydrostatic stress axis (see Figure 8.4). The equation of an octahedral plane is σ1 + σ2 + σ3 = const. and the unit normal vector of said plane is 1 n not≡ √ [1, 1, 1]T . 3
8.3.1 Normal and Shear Octahedral Stresses
Consider P is a point in theTheory principal stress and space Problems with coordinates (σ1,σ2,σ3). not T The position vector of this point is defined as OP ≡=[σ1,σ2,σ3] (see Fig- Π ure 8.5Continuum). Now, the octahedral Mechanics plane containing for point EngineersP is considered. The intersection of the hydrostatic© X. Oliver stress axis and with C. said Agelet plane de defines Saracibar point A.
Definition 8.3. Based on Figure 8.5, the normal octahedral stress is defined as √ OA = 3σoct and the shear or tangential octahedral stress is √ AP = 3τoct .
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Principal Stress Space 377
Figure 8.5: Definitions of the normal and shear octahedral stresses.
Remark 8.4. The normal octahedral stress σoct informs of the dis- tance between the origin O of the principal stress space and the oc- tahedral plane that contains point P. The locus of points in the prin- cipal stress space with√ the same value of σoct is the octahedral plane placed at a distance 3σoct of the origin. The shear octahedral stress τoct informs of the distance between point P and the hydrostatic stress axis. It is, thus, a measure of the distance that separates the stress state characterized by point P from a hydrostatic stress state. The locus of points in the principal stress space with the same value of τoct is a cylinder√ whose axis is the hy- drostatic stress axisTheory and whose radius and is Problems3τoct.
Continuum Mechanics for Engineers The distance OA can© be X. computed Oliver and as the C. projection Agelet deof the Saracibar vector OP on the unit normal vector of the octahedral plane, n, ⎡ √ ⎤ ⎫ / √ ⎪ 1 √3 √ ⎪ not ⎢ ⎥ 3 ⎬⎪ OA = OP · n ≡ σ1, σ2, σ3 ⎣ 1/ 3 ⎦ = (σ1 + σ2 + σ3)= 3σm √ 3 ⇒ 1/ 3 ⎪ √ ⎪ ⎭⎪ OA = 3σoct (8.15)
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 378 CHAPTER 8. PLASTICITY
I σ = σ = 1 (8.16) oct m 3 where the definition (8.9) of mean stress σm has been taken into account. The distance AP can be obtained solving for the right triangle OAP in Fig- ure 8.5, 2 2 2 1 AP = OP − OA = σ 2 + σ 2 + σ 2 − (σ + σ + σ )2 . (8.17) 1 2 3 3 1 2 3 By means of several algebraic operations, this distance can be expressed in terms of the second invariant of the deviatoric stress tensor in (8.14), J2,as √ ⎫ 2 = =⇒ = ( )1/2 ⎬ AP 2J2 AP 2 J2 √ =⇒ (8.18) ⎭ AP = 3τoct 2 / τ = (J )1 2 (8.19) oct 3 2
τ Alternative expressions of oct in terms of the value of J2 in (8.14) are 1/2 1 2 2 2 1 2 τoct = √ σ + σ + σ − (σ1 + σ2 + σ3) and 3 1 2 3 3 (8.20) 1/2 1 2 2 2 τoct = √ (σ1 − σ2) +(σ2 − σ3) +(σ1 − σ3) . 3 3
Remark 8.5. In a pureTheoryspherical stress and state Problems of σ ,