(Shear) Stress Acting on the Plane Perpendicular to the A-Axis in the Direction of the B-Axis
CH.4. STRESS
Multimedia Course on Continuum Mechanics Overview
Forces Acting on a Continuum Body Lecture 1 Cauchy’s Postulates Lecture 2 Stress Tensor Lecture 3 Lecture 4 Stress Tensor Components Scientific Notation Lecture 5 Engineering Notation Sign Criterion Properties of the Cauchy Stress Tensor Cauchy’s Equation of Motion Lecture 6 Principal Stresses and Principal Stress Directions Mean Stress and Mean Pressure Lecture 7 Spherical and Deviatoric Parts of a Stress Tensor Stress Invariants
2 Overview (cont’d)
Stress Tensor in Different Coordinate Systems Cylindrical Coordinate System Lecture 8 Spherical Coordinate System Mohr’s Circle Lecture 9 Mohr’s Circle for a 3D State of Stress Lecture 10 Determination of the Mohr’s Circle Mohr’s Circle for a 2D State of Stress 2D State of Stress Lecture 11 Stresses in Oblique Plane Direct Problem Lecture 12 Inverse Problem Mohr´s Circle for a 2D State of Stress Lecture 13
3 Overview (cont’d)
Mohr’s Circle a 2D State of Stress (cont’d) Construction of Mohr’s Circle Mohr´s Circle Properties Lecture 14 The Pole or the Origin of Planes Lecture 15 Sign Convention in Soil Mechanics Lecture 16 Particular Cases of Mohr’s Circle Lecture 17
4 4.1. Forces on a Continuum Body
Ch.4. Stress
5 Forces Acting on a Continuum Body
Forces acting on a continuum body: Body forces. Act on the elements of volume or mass inside the body. “Action-at-a-distance” force. E.g.: gravity, electrostatic forces, magnetic forces
f= ρ bx(),t dV body force per unit V ∫V mass Surface forces. (specific body forces) Contact forces acting on the body at its boundary surface. E.g.: contact forces between bodies, applied point or distributed loads on the surface of a body fx= t (),t dS surface force S ∫∂ (traction vector) V per unit surface
6 4.2. Cauchy’s Postulates
Ch.4. Stress
7 Cauchy’s Postulates
st 1. Cauchy’s 1 postulate. REMARK The traction vector t remains unchanged The traction vector (generalized to for all surfaces passing through the point P internal points) is not influenced by and having the same normal vector n at P . the curvature of the internal surfaces. tt= ()P, n
2. Cauchy’s fundamental lemma (Cauchy reciprocal theorem) The traction vectors acting at point P on opposite sides of the same surface are equal in magnitude and opposite in direction. tn()()PP,,=−− t n REMARK Cauchy’s fundamental lemma is equivalent to Newton's 3rd law (action and reaction).
8 4.3. Stress Tensor
Ch.4. Stress
9 Stress Tensor
The areas of the faces of the tetrahedron are: S11= nS T S22= nS with n ≡ {}n123 ,n ,n
S33= nS
The “mean” stress vectors acting on these faces are ** ()1* * ()2* * ()3* * t= tx(SS , n ), −= t tx ( , − eˆˆˆ123 ), −= t tx ( S , − e ), −= t tx ( S , − e ) 12 3 ** xx∈Si =1, 2, 3 ; ∈→S mean value theorem Sii S
The surface normal vectors of the planes perpendicular to the axes are =−=−=−ˆˆˆ ne11;; ne 2 2 ne 33 REMARK Following Cauchy’s fundamental lemma: The asterisk indicates an not ()i mean value over the area. tx()(),,−=− eˆˆii txe =− t(){} x i ∈ 1, 2, 3
10 Mean Value Theorem
Let f : [] a,b → R be a continuous function on the closed interval [] a,b , and differentiable on the open interval () a,b , where ab < . Then, there exists some x * in () a,b such that:
1 fx()* = ∫ fx()dΩ Ω Ω
I.e.: f : [] a,b → R gets its “mean value” fx () * at the interior of [] a,b
11 Stress Tensor
From equilibrium of forces, i.e. Newton’s 2nd law of motion: Rf ==m aρ b dV+= t dS aρρ dV = a dV ∑∑i ii ∫ ∫∫ ∫ ii V∂ VV V resultant dm body forces ∫ρρ bt dV+ ∫∫ dS +− t()12 dS +− ∫ t() dS +− ∫ t() 3 dS = ∫ a dV V SS S S V 12 3 resultant Considering the mean value theorem, surface forces **()()()12 * * 3 * * (ρρb )V+− tt S S123 − t S − t S = ( a )V
1 Introducing S = nS i ∈ {} 1, 2, 3 and V = Sh , ii 3 11 ()ρρb*h S+− tt ** S()()12 n S − t * n S − t() 3 * n S = () a * hS 33123
12 Stress Tensor
If the tetrahedron shrinks to point O,
* ()ii** () xS→= xO lim t xeSi , ˆˆ t(){}O, ei i∈ 1, 2, 3 iih0→ () * ** xSS→= xO lim t() xn , t()O , n h0→
11** lim (ρρ b ) h = lim ( a0 ) h = h0→→33 h0
The limit of the expression for the equilibrium of forces becomes,
()2 3 = t()1 = t = t() 11()()()12 3 i ()ρρb**h+− tt * nnn − t * − t * =() a * h t()On, nt−=() 0 33123 i = tn()O,
13 Stress Tensor
Considering the traction vector’s Cartesian components : ()i ()i ()i t()P= tPj() eeˆˆ j =σ ij j t()Pn, nt= ⇒ ij,∈ 1, 2, 3 i ()i {} σ = ()i ij ()PtPj () t()P, nt= nn = σ j j i i ij σij Cauchy’s Stress Tensor t()()PP, nn= ⋅σ σ =σ eeˆˆ ⊗ ij i j P In the matrix form: ()1 ()2 ()3 t1 t1 t1 T tnj= iσσ ij = ji n i j ∈{1, 2, 3} T [][][]tn= σ
()1 t t()2 t()3 14 Stress Tensor
REMARK 1 The expression t ()() PP , nn = ⋅ σ is consistent with Cauchy’s postulates: t()P, nn= ⋅σ tn()()PP,,=−− t n t()P,− nn =−⋅σ
REMARK 2 The Cauchy stress tensor is constructed from the traction vectors on three coordinate planes passing through point P.
σ11 σσ 12 13 ≡ σ σσ σ 21 22 23
σ31 σσ32 33
Yet, this tensor contains information on the traction vectors acting on any plane (identified by its normal n) which passes through point P.
15 4.4.Stress Tensor Components
Ch.4. Stress
16 Scientific Notation
Cauchy’s stress tensor in scientific notation
σσσ11 12 13 σ ≡ σσσ 21 22 23
σσσ31 32 33
Each component σ ij is characterized by its sub-indices: Index i designates the coordinate plane on which the component acts. Index j identifies the coordinate direction in which the component acts.
17 Engineering Notation
Cauchy’s stress tensor in engineering notation
στ τ x xy xz σ ≡ τ στ yx y yz ττσ zx zy z
Where: σ a is the normal stress acting on plane a. τ ab is the tangential (shear) stress acting on the plane perpendicular to the a-axis in the direction of the b-axis.
18 Tension and compression
The stress vector acting on point P of an arbitrary plane may be resolved into:
a vector normal to the plane ()σ n = σ n an in-plane (shear) component which acts on the plane.
(;ττnn=τ )
The sense of σ n with respect to n defines the normal stress character: >0 tensile stress (tension) σ =σ ⋅n n <0 compressive stress (compression) The sign criterion for the stress components is: positive (+) tensile stress σσor ij a negative (−) compressive stress positive (+) positive direction of the b-axis τ ab negative (−) negative direction of the b-axis
19 4.5.Properties of the Cauchy Stress Tensor Ch.4. Stress
20 Cauchy’s Equation of Motion
Consider an arbitrary material volume, Cauchy’s equation of motion is: ∇⋅ σ+ρρ ba = ∀∈ x V ∂σ ij +=ρρ ∈ bjj aj{}1, 2, 3 ∂xi
In engineering notation: bx(),t x∈ V ∂∂στ∂τ tx* (),t x∈∂ V x +yx +zx +=ρρba ∂∂∂xyz xx ∂∂∂τ στ xy y zy REMARK + + +=ρρbayy ∂∂∂xyz Cauchy’s equation of motion is derived ∂τ ∂τ ∂σ from the principle of balance of linear xz +yz +z +=ρρba ∂∂∂xyz zz momentum.
21 Equilibrium Equations
For a body in equilibrium a0 = , Cauchy’s equation of motion becomes ∇ ⋅σ+ρ b0 = ∀∈ x V ∂σ ij internal equilibrium +=∈ρbj0{} 1, 2, 3 ∂x j equation i The traction vector is now known at the boundary nx()()(),,tt⋅σ x = t* x , t ∀ x ∈∂ Vequilibrium equation ntσ=* j ∈{}1, 2, 3 at the boundary i ij j The stress tensor symmetry is derived from the principle of balance of angular momentum: σσ= T σσ= ∈ ij ji ij,{} 1, 2, 3
22 Cauchy’s Equation of Motion
Taking into account the symmetry of the Cauchy Stress Tensor, Cauchy’s equation of motion ∇⋅ σ+=ρ b σ⋅∇ += ρρ ba ∀∈ x V ∂∂σσ ij +=ρji += ρρ ∈ bj ba jj j{}1, 2, 3 ∂∂ xxii bx(),t x∈ V Boundary conditions tx* (),t x∈∂ V * n⋅σσ = ⋅ n = tx(,)tV∀x ∈∂ σ =σ = * ∀ ∈∂ ∈ ni ij ji ni t j ()xx, t V ij,{} 1, 2, 3
23 Principal Stresses and Principal Stress Directions
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 principal axes are the principal planes. The normal stress components in the principal planes are the σ principal stresses. 33 σ 31 x3 σ 32 x3 x3′ σ13 σ 23 σ1 00 σ11 σ12 σ x1′ σ σ = σ 21 σ 22 3 [ ] 002 σ1 00σ 3 σ 2 x1 x1 x2 x2 x2′ 24 Principal Stresses and Principal Stress Directions
The Cauchy stress tensor is a symmetric 2nd order tensor so it will diagonalize in an orthonormal basis and its eigenvalues are real numbers. For the eigenvalue λ and its corresponding eigenvector v :
σ ⋅=vvλ []σ −λ1 ⋅=v0 INVARIANTS not 32 characteristic det[]σσ−λλ11 =−=0 λλ−I1()σ − II 23 () σσ λ −= () 0 equation
σ 33 λσ11≡ σ 31 x3 σ 32 x3 x3′ σ13 λσ22≡ σ 23 σ11 σ12 σ x1′ σ λσ33≡ 21 σ 22 3 σ1 σ REMARK 2 x1 x1 The invariants associated with a x x 2 ′ 2 tensor are values which do not change x2 25 with the coordinate system being used. Mean Stress and Mean Pressure
Given the Cauchy stress tensor σ and its principal stresses, the following is defined: σσσ Mean stress 11 12 13 σ ≡ σσσ 1 11 21 22 23 σ=Tr ()σ =σ =() σσσ ++ σσσ m 3 33ii 123 31 32 33 Mean pressure REMARK 1 p =−=−++σ() σσσ In a hydrostatic state of stress, the m 3 123 stress tensor is isotropic and, thus, its components are the same in A spherical or hydrostatic any Cartesian coordinate system. state of stress : σ 00 As a consequence, any direction is a principal direction and the σσσ= = σ ≡=00σσ1 123 stress state (traction vector) is the 00σ same in any plane.
26 Spherical and Deviatoric Parts of a 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 σσsph:=σσ m1 =Tr () 11 = ii REMARK 33The principal directions of a stress tensor The stress deviator tensor: and its deviator stress component coincide. 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 m1
27 Stress Invariants
Principal stresses are invariants of the stress state: 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 : =σ =σ =++ σσσ I1 Tr () ii 123 REMARK 1 2 The I invariants are obtained II2=()σσ: −=−+1(σσ 12 σσ13 + 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
12 11 The J invariants can be J2=() II 12 +=2:σσij ji =()σσ 2 22 expressed in the unified form: 1 13 11 = σi ∈ J3=( I 1 +33 I 12 I + I 3) = Tr ()σσσ ⋅⋅ =σσij jk σ ki Ji Tr() i {}1, 2, 3 3 33 i
28 Stress Invariants of the Stress Deviator Tensor
The stress invariants of the stress deviator tensor:
I1′′= Tr ()σ = 0 1 II′=σσ ′′: − 2 =++σσ′′ σσ ′′ σσ ′′ 212 () 12 12 13 13 23 23 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
29 4.6. Stress Tensor in Different Coordinate Systems Ch.4. Stress
30 Stress Tensor in a Cylindrical Coordinate System
The cylindrical coordinate system is defined by:
dV= r dθ dr dz
xr= cosθ x(r ,θθ , z )≡= yr sin zz= The components of the stress tensor are then:
σ τ τ στθ τ x´ x ´´ y x ´´ z r r rz στ= σ τ= τ στ xy´′ y ´ yz ´´ rθ θθz τ τ σ ττ σ x´´ z y ´´ z z ´ rzθ z z
31 Stress Tensor in a Spherical Coordinate System
dV= r2 senθ dr d θϕ d The cylindrical coordinate system is defined by:
xr= senθφ cos x()r,θϕ ,≡= yr senθ sen φ The components of the stress tensor are then: zr= cosθ
σx´ τ xy ´´ τ xz ´´ στ r rθφ τ r σ ≡=τ σ τ τ στ xy´′ y ´ yz ´´ rθ θ θφ τ τ σ ττσ xz´´ yz ´´ z ´ rφ φθ φ
32 4.7. Mohr´s Circle
Ch.4. Stress
33 Mohr’s Circle
Introduced by Otto Mohr in 1882. Mohr´s Circle is a two-dimensional graphical representation of the state of stress at a point that: will differ in form for a state of stress in 2D or 3D. illustrates principal stresses and maximum shear stresses as well as stress transformations. is a useful tool to rapidly grasp the relation between stresses for a given state of stress.
34 4.8. Mohr´s Circle for a 3D State of Stress Ch.4. Stress
35 Determination of Mohr’s Circle
Consider the system of Cartesian axes linked to the principal directions of the stress tensor at an arbitrary point P of a continuous medium: x3 eˆ3 The components of the stress tensor are eˆ1 σ 3 x σ1 00 1 σ ≡ σ σ 2 002 with eˆ 00σ 3 2 x2 The components of the traction vector are
σσ1 00 nn1 11 =⋅=σ σσ = tn002 nn 2 22
00σσ3 nn 3 33
where n is the unit normal to the base associated to the principal directions
36 Determination of Mohr’s Circle
The normal component of stress σ is
n1 222 σ=⋅= tn [ σσn,, n σ nn] = σσσ n + n + n 11 2 2 33 2 11 2 2 33 T n t 3 σn =σ ⋅n n The squared modulus of the traction vector is
2 =⋅=σσσ22 + 22 + 22 t tt 11nnn 22 33 22 22 22 2 2 σσσστ11nnn++=+ 22 33 2 22 t =+=στ:: τ τn Mohr's 3D problem half - space The unit vector n must satisfy = 222 n 1 nnn1++= 231
Locus of all possible () στ , points?
37 Determination of Mohr’s Circle
The previous system of equations can be written as a matrix equation which can be solved for any couple σσσ222 n 2 στ 22+ 1 23 1 σσσ 2 = σ 1 23 n 2 2 111 n3 1 x A b ≤≤2 T 01n1 222 A feasible solution for x ≡ nnn 1 ,, 23 requires that 2 for the 01≤≤n2 222 expression nnn ++= 1 to hold true. ≤≤2 1 23 01n3 Every couple of numbers () στ , which leads to a solution x , will be considered a feasible point of the half-space. The feasible point is representative of the traction vector () στ , on a T ≡ plane of normal n nnn 1 ,, 23 which passes through point P. The locus of all feasible points is called the feasible region.
38 Determination of Mohr’s Circle
The system σσσ222 n 2 στ 22+ 1 23 1 σσσ2 = σ 1 23 n 2 2 111 n3 1 A x b can be re-written as
22 A 2 ()In→σ +− τ() σ1 + σ 3 σ + σσ 13 −1 =0 ()σσ13− 22 A 2 ()II →σ +− τ() σ2 + σ 3 σ + σσ 23 −n2 =0 ()σσ23− 22 A 2 ()III →σ +− τ() σ1 + σ 2 σ + σσ 12 −n3 =0 ()σσ12−
with A =−−−()()()σσ1 2 σσ 23 σσ 13
39 Determination of Mohr’s Circle
Consider now equation () III : 22 A 2 with A =−−−σσ σσ σσ σ+− τ() σ1 + σ 2 σ + σσ 12 −n3 =0 ()()()1 2 23 13 ()σσ12− It can be written as: 1 a =()σσ12 + 2 2 () στ−aR +=22with 1 2 2 Rn=()()()σσ1 − 2 +− σσ 2 3 σσ 1 − 33 4
which is the equation of a semicircle of center C 3 and radius R 3 : 1 C3=()σσ 12 + ,0 2 REMARK
1 2 2 A set of concentric semi-circles is Rn3=()()()σσ 1 − 2 +− σσσσ 2 3 1 − 33 4 obtained with the different values of
n 3 with center C 3 and radius Rn 33 () : 2 min 1 n = 0 R3=()σσ 12 − 3 2 n2 =1 max 1 3 R3=()σσ 12 +− σ 3 2
40 Determination of Mohr’s Circle
Following a similar procedure with () I and () II , a total of three semi-annuli with the following centers and radii are obtained:
min 1 1 R1 =(σσ23 − ) C1= [(σσ 23 + ) ,0] 2 2 Rmax =σ − a a1 1 11
1 1 Rmax =σσ − C= [(σσ + ) ,0] 2 ( 13) 22 13 2 min a2 R2 =σ 22 − a
1 min 1 C3= [(σσ 12 + ) ,0] R3 =(σσ12 − ) 2 2 a3 max R3 =σ 33 − a
41 Determination of Mohr’s Circle
Superposing the three annuli,
The final feasible region must be the intersection of these semi-annuli Every point of the feasible region in the Mohr’s space, corresponds to the stress (traction vector) state on a certain plane at the considered point 44 4.9. Mohr´s Circle for a 2D State of Stress Ch.4. Stress
45 2D State of Stress
3D general state of stress 2D state of stress
στ στx xy τ xz x xy 0 σ ≡ τ στ σ ≡ τσ0 yx y yz yx y ττσ 00σ zx zy z z
3D problem
στ REMARK σ ≡ x xy τσ In 2D state of stress problems, the yx y principal stress in the disregarded direction is known (or assumed) a priori. 2D (plane) problem
46 Stresses in a oblique plane
Given a plane whose unit normal n forms an angle θ with the x axis, Traction vector σ τcosθ σcos θτ+ sin θ t =⋅= σn x xy = x xy τ σ τ θσ+ θ xy y sinθ xy cosy sin n σ Normal stress σσ+− σσ σ=⋅= tn xy + xycos()() 2θτ+ sin 2 θ cosθ sinθ θ 22 xy n = m = sinθ −cosθ Shear stress σσ− τ=⋅=tm xysin()() 2θτ− cos 2 θ θ 2 xy
Tangential stress τ θ is now endowed with sign (ττθθ≥< 0or 0) Pay attention to the “positive” senses given in the figure 47 Direct and Inverse Problems
Direct Problem: Find the principal stresses and principal stress directions given σ in a certain set of axes. equivalent stresses Inverse Problem: Find the stress state on any plane, given the principal σ stresses and principal stress directions.
48 Direct Problem
In the x ´ and y ´axes, τ α = 0 then, σσ− τ=xysin()() 2ατ −= cos 2 α 0 α 2 xy τ tan() 2α = xy σσxy− 2 Using known trigonometric relations, 1 τ sin() 2α =±=±xy 2 This equation has two solutions: 1 σσ− 1+ xy 2 2 +τ α + tg() 2α xy 1 (sign " ") 2 1. π 2. αα 21=+−(sign " ") σσxy− 2 1 cos() 2α =±=±2 These define the principal stress 1+ tg2 () 2α 2 σσxy− 2 directions. +τ xy 2 (The third direction is perpendicular to the plane of analysis.) 49 Direct Problem
The angles θα = 1 and θα = 2 are then introduced into the equation σσ+− σσ σ=++xy xycos()() 2θτ sin 2 θ θ 22 xy to obtain the principal stresses (orthogonal to the plane of analysis):
2 σσ+− σσ xy xy 2 στ1 =++xy 22 σα → 2 σσxy+− σσ xy 2 στ2 =−+xy 22 θα≡
50 Inverse Problem
Given the directions and principal stresses σ 1 and σ 2, to find the stresses in a plane characterized by the angle β : Take the equations
Replace , , and θβ ≡ to obtain: σσ+− σσ σβ=12 + 12cos() 2 β 22 σσ− τβ= 12sin() 2 β 2
51 Mohr’s Circle for a 2D State of Stress
Considering a reference system xy ´´ − and characterizing the inclination of a plane by , From the inverse problem equations: σσ+− σσ σβ−=12 12cos() 2 22 σσ− τβ= 12 sin() 2 σσ− 2 R = 12 2 Squaring both equations and adding them: σσ+ C = 12,0 22REMARK 2 σσ+− 2 σσ στ−12 +=12 22 This expression is valid for any Eq. of a circle with value of . center C and radius R . Mohr’s Circle
52 Mohr’s Circle for a 2D State of Stress
The locus of the points representative of the state of stress on any of the planes passing through a given point P is a circle. (Mohr’s Circle) The inverse is also true: Given a point () στ , in Mohr’s Circle, there is a plane passing through P whose normal and tangential stresses are and τ , respectively.
σσ+ σσ12− σ − 12 Mohr's 2D problemspace R = 2 σ − a 2 cos() 2β = = σσ− R 12 2 ττ sin() 2β = = σσ− R σσ+ 12 C = 12,0 2 2
53 Construction of Mohr’s Circle
Interactive applets and animations: by M. Bergdorf: http://www.zfm.ethz.ch/meca/applets/mohr/Mohrcircle.htm
from MIT OpenCourseware: http://ocw.mit.edu/ans7870/3/3.11/tools/mohrscircleapplet.html
from Virginia Tech: http://web.njit.edu/~ala/keith/JAVA/Mohr.html
From Pennsilvania State University: http://www.esm.psu.edu/courses/emch13d/design/animation/animation.htm
54 Mohr’s Circle’s Properties
A. To obtain the point in Mohr’s Circle representative of the state of stress on a plane which forms an angle β with the principal stress
direction σ 1:
1. Begin at the point on the circle (representative of the plane where σ 1 acts).
2. Rotate twice the angle in the sense σσ 1 → β . 3. This point represents the shear and normal stresses at the desired plane (representative of the stress state at the plane where acts).
3.
2. 1.
55 Mohr’s Circle’s Properties
B. The representative points of the state of stress on two orthogonal planes are aligned with the centre of Mohr’s Circle: π This is a consequence of property A as ββ = + . 212
56 Mohr’s Circle’s Properties
C. If the state of stress on two orthogonal planes is known, Mohr’s Circle can be easily drawn: 1. Following property B, the two points representative of these planes will be aligned with the centre of Mohr’s Circle. 2. Joining the points, the intersection with the σ axis will give the centre of Mohr’s Circle. 3. Mohr’s Circle can be drawn. 3. 1. 2.
57 Mohr’s Circle’s Properties
D. Given the components of the stress tensor in a particular orthonormal base, Mohr’s Circle can be easily drawn: This is a particular case of property C in which the points representative of the state of stress on the Cartesian planes is known. 1. Following property B, the two points representative of these planes will be aligned with the centre of Mohr’s Circle. 2. Joining the points, the intersection with the σ axis will give the centre of Mohr’s Circle. 3. Mohr’s Circle can be drawn. 3. 1. 2.
στ σ = x xy τσ xy y
58 Mohr’s Circle’s Properties
The radius and the diametric points of the circle can be obtained:
στ σ = x xy τσ xy y
2 σσxy− 2 R = +τ xy 2
59 Mohr’s Circle’s Properties
Note that the application of property A for the point representative of the vertical plane implies rotating in the sense contrary to angle.
στ σ = x xy τσ xy y
60 The Pole or the Origin of Planes
The point called pole or origin of planes in Mohr’s circle has the following characteristics: Any straight line drawn from the pole will intersect the Mohr circle at a point that represents the state of stress on a plane parallel in space to that line. 2.
1.
61 The Pole or the Origin of Planes
The point called pole or origin of planes in Mohr’s circle has the following characteristics: If a straight line, parallel to a given plane, is drawn from the pole, the intersection point represents the state of stress on this particular plane.
1.
2.
62 Sign Convention in Soil Mechanics
The sign criterion used in soil mechanics, is the inverse of the one used in continuum mechanics: In soil mechanics, negative (−) tensile stress σ β positive (+) compressive stress
positive (+) counterclockwise rotation continuum mechanics τ β negative (-) clockwise rotation
But the sign criterion for angles is the same: positive angles are measured counterclockwise
* ττββ= − σσ* = − ββsoil mechanics
63 Sign Convention in Soil Mechanics
For the same stress state, the principal stresses will be inverted.
* σσ12= − * ττββ= − * σσ21= − σσ* = − π ββββ* = + 2 continuum mechanics soil mechanics The expressions for the normal and shear stresses are ** ** **−−σσ21 −+ σσ 21 −=σβ + cos() 2βπ+ 22 ** ** σσ12+− σσ 12 **σ1+ σ 2 σσ 1 − 2 σβ=+= * σ+ β ββcos() 2 −cos 2β cos() 2 22 2 2 →→ σσ− −+σσ** σσ**− τβ= 12 **21 *1 2 * β sin() 2 −=τββsin() 2βπ+ τ= sin() 2β 2 22 * −sin 2β like in continuum mechanics The Mohr’s circle construction and properties are the same in both cases 64 4.10. Particular Cases of Mohr’s Circle
Ch.4. Stress
65 Particular Cases of Mohr’s Circles
Hydrostatic state of stress
Mohr’s circles of a stress tensor and its deviator
()σ sph= σ m1 σσ1= m1 + σ′ ′ σσ= sph + σ′ σσσ2= m2 +
σσσ3= m3 + ′
Pure shear state of stress
66 Chapter 4 Stress
4.1 Forces Acting on a Continuum Body Two types of forces that can act on a continuous medium will be considered: body forces and surface forces.
4.1.1 Body Forces
Definition 4.1. The body forces are the forces that act at a distance on the internal particles of a continuous medium. Examples of this kind of forces are the gravitational, inertial or magnetic attraction forces.
Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.1: Body forces on a continuous medium.
127 128 CHAPTER 4. STRESS
Consider b(x,t) is the spatial description of the vector field of body forces per unit of mass. Multiplying the vector of body forces b(x,t) by the density ρ, the vector of body forces per unit of volume ρb(x,t) (density of body forces)is obtained. The total resultant, fV , of the body forces on the material volume V in Figure 4.1 is
fV = ρb(x,t)dV . (4.1) V
Remark 4.1. In the definition of body forces given in (4.1), the exis- tence of the vector density of body forces ρb(x,t) is implicitly ac- cepted. This means that, given an arbitrary sequence of volumes ΔVi that contain the particle P, and the corresponding sequence of body
forces fΔVi , there exists the limit fΔ ρb(x,t)= lim Vi ΔVi ΔVi→0 and, in addition, it is independent of the sequence of volumes con- sidered.
Example 4.1 – Given a continuous medium with volume V placed on the Earth’s surface, obtain the value of the total resultant of the body forces in terms of the gravitational constant g.
Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar Solution
Assuming a system of Cartesian axes (see figure above) such that the x3- axis is in the direction of the vertical from the center of the Earth, the vector field b(x,t) of gravitational force per unit of mass is b(x,t) not≡ [0 , 0 , −g]T and, finally, the vector of body forces is not T fV = ρb(x,t)dV ≡ 0 , 0 , − ρgdV . V V
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4.1.2 Surface Forces
Definition 4.2. The surface forces are the forces that act on the boundary of the material volume considered. They can be regarded as produced by the contact actions of the particles located in the boundary of the medium with the exterior of this medium.
Consider the spatial description of the vector field of surface forces per unit of surface t(x,t) on the continuous medium shown in Figure 4.2. The resultant force on a differential surface element dS is tdS and the total resultant of the surface forces acting on the boundary ∂V of volume V can be written as
fS = t(x,t)dS . (4.2) ∂V
Remark 4.2. In the definition of surface forces given in (4.2), the ex- istence of the vector of surface forces per unit of surface t(x,t) (trac- tion vector1) is implicitly accepted. In other words, if a sequence of surfaces ΔSi, each containing point P, and the corresponding surface
forces fΔSi are considered (see Figure 4.3), there exists the limit fΔ t(x,t)= lim Si ΔSi ΔSi→0 and it is independent of the chosen sequence of surfaces. Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.2: Surface forces on a continuous medium.
1 In literature, the vector of surface forces per unit of surface t(x,t) is often termed traction vector, although this concept can be extended to points in the interior of the continuous medium.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 130 CHAPTER 4. STRESS
Figure 4.3: Traction vector.
4.2 Cauchy’s Postulates Consider a continuous medium on which body and surface forces are acting (see Figure 4.4). Consider also a particle P in the interior of the continuous medium and an arbitrary surface containing point P and with a unit normal vector n at this point, which divides the continuous medium into two parts (material vol- umes). The surface forces due to the contact between volumes will act on the imaginary separating surface, considered now a part of the boundary of each of these material volumes. Consider the traction vector t that acts at the chosen point P as part of the boundary of the first material volume. In principle, this traction vector (de- fined now at a material point belonging to the interior of the original continuous medium) will depend on 1) the particle being considered, 2) the orientation of the surface (defined by means of the normal n) and 3) the separating surface itself. Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.4: Cauchy’s postulates.
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The following postulate2 makes it independent of this last condition.
Definition 4.3. Cauchy’s 1st postulate establishes that the traction vector that acts at a material point P of a continuous medium ac- cording to a plane with unit normal vector n depends only on the point P and the normal n.
t = t(P,n)
Remark 4.3. Consider a particle P of a continuous medium and dif- ferent surfaces that contain this point P such that they all have the same unit normal vector n at said point. In accordance with Cauchy’s postulate, the traction vectors at point P, according to each of these surfaces, coincide. On the contrary, if the normal to the surfaces at P is different, the corresponding traction vectors will not coincide (see Figure 4.5).
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Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.5: Traction vector at a point according to different surfaces.
2 A postulate is a fundamental ingredient of a theory that is formulated as a principle of this theory and, as such, does not need proof.
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Definition 4.4. Cauchy’s 2nd postulate - action and reaction law es- tablishes the traction vector at point P of a continuous medium, ac- cording to a plane with unit normal vector n, has the same magnitude and opposite direction to the traction vector at the same point P ac- cording to a plane with unit normal vector −n at the same point (see Figure 4.4). t(P,n)=−t(P,−n)
4.3 Stress Tensor 4.3.1 Application of Newton’s 2nd Law to a Continuous Medium Consider a discrete system of particles in motion such that a generic particle i of this system has mass mi, velocity vi and acceleration ai = dvi/dt. In addition, a force fi acts on each particle i, which is related to the particle’s acceleration through Newton’s second law3,
fi = miai . (4.3) Then, the resultant R of the forces that act on all the particles of the system is
R = ∑fi = ∑miai . (4.4) i i The previous concepts can be generalized for the case of continuous mediums when these are understood as discrete systems constituted by an infinite number of particles. In this case,Theory the application and of Newton’s Problems second law to a continu- ous medium with total mass M, on which external forces characterized by the vector density of body forces ρb(x,t) and the traction vector t(x,t) are acting, Continuum Mechanics( , ) for Engineers whose particles have an© acceleration X. Olivera andx t ,C. and Agelet that occupies de Saracibar at time t the space volume Vt results in R = ρb dV + t dS = a dm = ρa dV . (4.5) V ∂ M V t Vt ρdV t Resultant of Resultant of the body the surface forces forces
3 The Einstein notation introduced in (1.1) is not used here.
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4.3.2 Stress Tensor Consider now the particular case of a material volume constituted by an ele- mental tetrahedron placed in the neighborhood of an arbitrary particle P of the interior of the continuous medium and oriented according to the scheme in Fig- ure 4.6. Without loss of generality, the origin of coordinates can be placed at P. The tetrahedron has a vertex at P and its faces are completely defined by T means of a plane with normal n =[n1,n2,n3] that intersects with the coordi- nate planes, defining a generic surface with area S (the base of the tetrahedron) at a distance h (the height of the tetrahedron) of point P. In turn, the coordinate planes define the other faces of the tetrahedron with areas S1, S2 and S3, and (outward) normals −eˆ1, −eˆ2 and −eˆ3, respectively. Through geometric consid- erations, the relations
S1 = n1SS2 = n2SS3 = n3S (4.6) can be established. The notation for the traction vectors on each of the faces of the tetrahedron is introduced in Figure 4.7 as well as the corresponding normals with which they are associated. According to Cauchy’s second postulate (see Definition 4.4), the traction vec- tor on a generic point x belonging to one of the surfaces Si (with outward nor- mal −eˆi) can be written as
not (i) t(x,−eˆi)=−t(x,eˆi) = −t (x) i ∈ {1,2,3} . (4.7)
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Figure 4.6: Elemental tetrahedron in the neighborhood of a material point P.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 134 CHAPTER 4. STRESS
Figure 4.7: Traction vectors on an elemental tetrahedron.
Remark 4.4. The mean value theorem establishes that, given a (scalar, vectorial o tensorial) function that is continuous in the in- terior of a (compact) domain, the function reaches its mean value in the interior of said domain. In mathematical terms, given f (x) continuous in Ω, ∗ ∗ ∃ x ∈ Ω | f (x) dΩ = Ω · f (x ) Ω
where f (x∗) is the mean value of f in Ω. Figure 4.8 shows the graphical interpretation of the mean value theorem in one dimen- sion. Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.8: Mean value theorem.
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In virtue of the mean value theorem, the vector field t(i) (x), assumed to be continuous in the domain Si, attains its mean value in the interior of this∗ domain. ∗ ∈ (i) = (i) ∗ Let xsI Si be the point where the mean value is reached and t t xsI ∗ = ∗ ρ∗ ∗ = ρ ( ∗ ) ( ∗ ) this mean value. Analogously, the vectors t t xS , b xV b xV ρ∗ ∗ = ρ ( ∗ ) ( ∗ ) and a xV a xV are the mean values corresponding to the vector fields: traction vector t(x) in S, density of body forces ρb(x) and inertial forces ρa(x), respectively. These mean values are attained, again according to the mean value ∗ ∈ ∗ ∈ theorem, at points xs S and xV V of the interior of the corresponding do- mains. Therefore, one can write ∗ (i) (i) ∗ t (x)dS = t Si i ∈ {1,2,3} , t(x)dS = t S ,
Si S (4.8) ∗ ∗ ∗ ∗ ρ (x)b(x)dV = ρ b V and ρ (x)a(x)dV = ρ a V . V V Applying now (4.5) on the tetrahedron considered, results in ρbdV + tdS+ tdS+ tdS+ tdS = V S S S S 1 2 3 (4.9) ( ) ( ) ( ) = ρbdV + tdS+ −t 1 dS+ −t 2 dS+ −t 3 dS = ρadV,
V S S1 S2 S3 V where (4.7) has been taken into account. Replacing (4.8)in(4.9), the latter can be written in terms of the mean values as ∗ ∗ ∗ ρ∗ ∗ + ∗ − (1) − (2) − (3) = ρ∗ ∗ . b V tTheoryS t S1 andt S2 Problemst S3 a V (4.10) Introducing now (4.6) and expressing the total volume of the tetrahedron as = / V ShContinuum3, the equation above Mechanics becomes for Engineers ©∗ X. Oliver∗ and C.∗ Agelet de Saracibar 1 ∗ ∗ ∗ (1) (2) (3) 1 ∗ ∗ ρ b hS+ t S − t n1 S − t n2 S − t n3 S = ρ a hS =⇒ 3 3 (4.11) 1 ∗ ∗ ∗ 1 ρ∗ b∗ h + t∗ − t(1) n − t(2) n − t(3) n = ρ∗ a∗ h . 3 1 2 3 3 Expression (4.11) is valid for any tetrahedron defined by a plane with unit normal vector n placed at a distance h of point P. Consider now an infinites- imal tetrahedron, also in the neighborhood of point P, by making the value of PP = h tend to zero but maintaining the orientation of the plane constant (n=constant). Then, the domains Si, S and V in (4.11) collapse into point P (see Figure 4.7). Therefore, the points of the corresponding domains in which the
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 136 CHAPTER 4. STRESS mean values are obtained also tend to point P,
∗ ∗ → =⇒ (i) ∗ = (i) ( ) ∈ { , , } , xS xP lim t xS t P i 1 2 3 i h→0 i (4.12) ∗ → =⇒ ∗ ( ∗, )= ( , ) , xS xP lim t xS n t P n h→0 and, in addition, 1 ∗ ∗ 1 ∗ ∗ lim ρ b h = lim ρ a h = 0 . (4.13) h→0 3 h→0 3 Taking the limit of (4.11) and replacing expressions (4.12) and (4.13)init leads to
(1) (2) (3) (i) t(P,n) − t n1 − t n2 − t n3 = 0 =⇒ t(P,n) − t ni = 0 . (4.14)
The traction vector t(1) can be written in terms of its corresponding Cartesian components (see Figure 4.9)as
(1) t = σ11eˆ1 + σ12eˆ2 + σ13eˆ3 = σ1ieˆi . (4.15)
Operating in an analogous manner on traction vectors t(2) and t(3) (see Fig- ure 4.10) results in
(2) t = σ21eˆ1 + σ22eˆ2 + σ23eˆ3 = σ2ieˆi (4.16)
(3) t = σ31eˆ1 + σ32eˆ2 + σ33eˆ3 = σ3ieˆi (4.17) and, for the general case,
(i) t Theory(P)=σijeˆ j andi, j ∈ Problems{1,2,3} . (4.18)
σ ( )= (i) ( ) , ∈ { , , } Continuumij P Mechanicst j P i j for1 2 Engineers3 (4.19) © X. Oliver and C. Agelet de Saracibar
Remark 4.5. Note that in expression (4.19) the functions σij are (i) ( ) functions of (the components of) the traction vectors t j P on the surfaces specifically oriented at point P. Thus, it is emphasized that these functions depend on point P but not on the unit normal vec- tor n. σij = σij(P)
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Stress Tensor 137
Figure 4.9: Decomposition of the traction vector t(1) into its components.
Figure 4.10: Traction vectors t(2) and t(3) .
Replacing (4.19)in(4.14) yields
( , )= (i) =⇒ ( , )= (i) ( )= σ ( ) , ∈ { , , } =⇒ t P n ni t t j P n ni t j P ni ij P i j 1 2 3
( , )= · σ ( ) Theoryt P n andn ProblemsP (4.20) where the Cauchy stress tensor σ is defined as Continuum Mechanicsσ = σ eˆ ⊗ eˆ for. Engineers (4.21) © X. Oliverij andi C.j Agelet de Saracibar
Remark 4.6. Note that expression (4.20) is consistent with Cauchy’s first postulate (see Definition 4.3) and that the second postulate (see Definition 4.4) is satisfied from ⎫ ⎬ t(P,n)=n · σ =⇒ ( , )=− ( ,− ) . ⎭ t P n t P n t(P,−n)=−n · σ
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Figure 4.11: Traction vectors for the construction of the Cauchy stress tensor.
Remark 4.7. In accordance with (4.18) and (4.21), the Cauchy stress tensor is constructed from the traction vectors according to three co- ordinate planes that include point P (see Figure 4.11). However, by means of (4.20), the stress tensor σ (P) is seen to contain informa- tion on the traction vectors corresponding to any plane (identified by its normal n) that contains this point.
4.3.3 Graphical Representation of the Stress State in a Point It is common to resort to graphical representations of the stress tensor based on elemental parallelepipeds in the neighborhood of the particle considered, with faces oriented in accordance to the Cartesian planes and in which the corre- sponding traction vectors are decomposed into their normal and tangent compo- nents following expressionsTheory (4.15) through and (4.20 Problems) (see Figure 4.12). 4.3.3.1 Scientific Notation The representationContinuum in Figure Mechanics4.12 corresponds for to what Engineers is known as scientific notation. In this notation,© the X. matrix Oliver ofand components C. Agelet of the de stress Saracibar tensor is written as ⎡ ⎤ σ σ σ ⎢ 11 12 13 ⎥ σ not≡ ⎣ σ21 σ22 σ23 ⎦ (4.22)
σ31 σ32 σ33 and each component σij can be characterized in terms of its indices: − Index i indicates the plane on which the stress acts (plane perpendicular to the xi-axis). − Index j indicates the direction of the stress (direction of the x j-axis).
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Stress Tensor 139
Figure 4.12: Graphical representation of the stress tensor (scientific notation).
4.3.3.2 Engineering Notation In engineering notation, the components of the Cauchy stress tensor (see Fig- ure 4.13) are written as ⎡ ⎤ σ τ τ ⎢ x xy xz ⎥ σ not≡ ⎣ τyx σy τyz ⎦ (4.23)
τzx τyz σz and each component can be characterized as follows:
− The component σa is the normal stress acting on the plane perpendicular to the a-axis. − The component τab is the tangential (shear) stress acting on the plane per- pendicular to the a-axis in the direction of the b-axis. Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.13: Graphical representation of the stress tensor (engineering notation).
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4.3.3.3 Sign Criterion Consider a particle P of the continuous medium and a plane with unit normal vector n that contains this particle (see Figure 4.14). The corresponding traction vector t can be decomposed into its normal component σ n and its tangential component τ n. The sign of the projection of t on n (σ = t · n) defines the tensile (σ n tends to pull on the plane ) or compressive (σ n tends to compress the plane) character of the normal component. This concept can be used to define the sign of the components of the stress tensor. For this purpose, in the elemental parallelepiped of Figure 4.12, the dis- tinction is made between the positive or visible faces (its outward normal has the same direction as the positive base vector and the faces can be seen in the figure) and the negative or hidden faces. The sign criterion for the visible faces is positive (+) ⇒ tension Normal stresses σ or σ and ij a negative (−) ⇒ compression positive (+) ⇒ direction of b-axis Tangential stresses τ ab negative (−) ⇒ opposite direction to b-axis
In accordance with this criterion, the directions of the stresses represented in Figure 4.13 (on the visible faces of the parallelepiped) correspond to positive values of the respective components of the stress tensor4. In virtue of the action and reaction law (see Definition 4.4) and for the hidden faces of the parallelepiped, the aforementioned positive values of the compo- nents of the stress tensor correspond to opposite directions in their graphical representation (see Figure 4.15). Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Ageletσ n = σn de Saracibar > 0 tension σ = t · n < 0 compression
Figure 4.14: Decomposition of the traction vector.
4 It is obvious that the negative values of the components of the stress tensor will result in graphical representations of opposite direction to the positive values indicated in the figures.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Properties of the Stress Tensor 141
Figure 4.15: Positive stresses in the hidden faces.
4.4 Properties of the Stress Tensor Consider an arbitrary material volume V in a continuous medium and its bound- ary ∂V. The body forces b(x,t) act on V and the prescribed traction vector t∗ (x,t) acts on ∂V. The acceleration vector field of the particles is a(x,t) and the Cauchy stress tensor field is σ (x,t) (see Figure 4.16).
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Figure 4.16: Forces acting on a continuous medium. Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
4.4.1 Cauchy Equation. Internal Equilibrium Equation The stress tensor, the body forces and the accelerations are related through Cauchy’s equation, ⎧ ⎪ ⎨ ∇ · σ + ρb = ρa ∀x ∈ V Cauchy’s ∂σ (4.24) equation ⎪ ij ⎩ + ρb j = ρa j j ∈ {1,2,3} ∂xi
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 142 CHAPTER 4. STRESS whose explicit expression in engineering notation is ⎧ ⎪ ∂σ ∂τ ∂τ ⎪ x + yx + zx + ρb = ρa , ⎪ ∂ ∂ ∂ x x ⎨⎪ x y z ∂τ ∂σ ∂τ xy + y + zy + ρ = ρ , ⎪ by ay (4.25) ⎪ ∂x ∂y ∂z ⎪ ⎪ ∂τ ∂τ ∂σ ⎩ xz + yz + z + ρb = ρa . ∂x ∂y ∂z z z If the system is in equilibrium, the acceleration is null (a = 0), and (4.24)is reduced to ⎧ Internal ⎨ ∇ · σ + ρb = 0 ∀x ∈ V equilibrium ∂σ (4.26) ⎩ ij + ρ = ∈ { , , } equation b j 0 j 1 2 3 ∂xi which is known as the internal equilibrium equation of the continuous medium. Cauchy’s equation of motion is derived from the principle of balance of linear momentum, which will be studied in Chapter 5.
4.4.2 Equilibrium Equation at the Boundary Equation (4.20) is applied on the boundary points taking into account that the traction vector is now known in said points (t = t∗). The result is denoted as equilibrium equation at the boundary. Equilibrium n(x,t) · σ (x,t)=t∗ (x,t) ∀x ∈ ∂V equation at (4.27) Theoryσ = ∗ and Problems∈ { , , } the boundary ni ij t j j 1 2 3 Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar 4.4.3 Symmetry of the Cauchy Stress Tensor The Cauchy stress tensor is proven to be symmetric by applying the principle of balance of angular momentum (see Chapter 5). σ = σ T (4.28) σij = σ ji i, j ∈ {1,2,3}
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Properties of the Stress Tensor 143
Remark 4.8. The symmetry of the stress tensor allows the Cauchy’s equation (4.24) and the equilibrium equation at the boundary (4.27) to be written, respectively, as ⎧ ⎨ ∇ · σ + ρb = σ · ∇ + ρb = ρa ∀x ∈ V ∂σ ∂σ ⎩ ij ji + ρb j = + ρb j = ρa j j ∈ {1,2,3} ∂xi ∂xi n · σ = σ · n = t∗ (x,t) ∀x ∈ ∂V σ = σ = ∗ ∈ { , , } ni ij ji ni t j j 1 2 3
Example 4.2 – A continuous medium moves with a velocity field whose spa- tial description is v(x,t) not≡ [z, x, y]T . The Cauchy stress tensor is ⎡ ⎤ yg(x,z,t) 0 not ⎢ ⎥ σ ≡ ⎣ h(y) z(1 +t) 0 ⎦ . 000
Determine the functions g, h and the spatial form of the body forces b(x,t) that generate the motion.
Solution The stress tensor is symmetric,Theory therefore and Problems h(y)=C , σ = σ T =⇒ h(y)=g(x,z,t)=⇒ Continuum Mechanics for Engineersg(x,z,t)=C , © X. Oliver and C. Agelet de Saracibar where C is a constant. In addition, the divergence of the tensor is null, ⎡ ⎤ yC 0 not ∂ ∂ ∂ ⎢ ⎥ ∇ · σ ≡ , , ⎣Cz(1 +t) 0 ⎦ =[0, 0, 0] . ∂x ∂y ∂z 00 0
Thus, Cauchy’s equation is reduced to ∇ · σ + ρb = ρa =⇒ b = a . ∇ · σ = 0
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Applying the expression for the material derivative of velocity, dv ∂v a = = + v · ∇v with dt ∂t ⎡ ⎤ ∂ ⎢ ⎥ ⎢ ∂ ⎥ ⎡ ⎤ ⎢ x ⎥ 010 ∂v ⎢ ∂ ⎥ = 0 and ∇v = ∇ ⊗ v not≡ ⎢ ⎥[z, x, y]=⎣ 001⎦ . ∂t ⎢ ∂ ⎥ ⎢ y ⎥ 100 ⎣ ∂ ⎦ ∂z the acceleration ⎡ ⎤ 010 a = v · ∇v not≡ [z, x, y]⎣ 001⎦ =[y, z, x] 100
is obtained. Finally, the body forces are
b(x,t)=a(x,t) not≡ [y, z, x]T .
4.4.4 Diagonalization. Principal Stresses and Directions Consider the stress tensor σ . Since it is a symmetric second-order tensor, it diagonalizes5 in an orthonormal basis and its eigenvalues are real. Consider, then, its matrix of componentsTheory in the Cartesian and Problems basis {x, y, z} (see Figure 4.17), ⎡ ⎤ σ τ τ ⎢ x xy xz ⎥ Continuumσ Mechanicsnot≡ ⎣ τ σ τ ⎦ for. Engineers (4.29) © X. Oliveryx andy yz C. Agelet de Saracibar τ τ σ zx yz z {x, y, z}
In the Cartesian system {x, y, z} in which σ diagonalizes, its matrix of com- ponents will be ⎡ ⎤ σ 00 ⎢ 1 ⎥ σ not≡ . ⎣ 0 σ2 0 ⎦ (4.30) 00σ 3 {x, y, z}
5 A theorem of tensor algebra guarantees that all symmetric second-order tensor diagonalizes in an orthonormal basis and its eigenvalues are real.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Properties of the Stress Tensor 145
Figure 4.17: Diagonalization of the stress tensor.
Definition 4.5. The principal stress directions are the directions, as- sociated with the axes {x, y, z}, in which the stress tensor diago- nalizes. The principal stresses are the eigenvalues of the stress tensor (σ1, σ2, σ3). In general, they will be assumed to be arranged in the form σ1 ≥ σ2 ≥ σ3.
To obtain the principal stress directions and the principal stresses, the eigen- value problem associated with tensor σ must be posed. That is, if λ and v are an eigenvalue and its corresponding eigenvector, respectively, then σ · = λ =⇒ (σ − λ ) · = . vTheoryv and Problems1 v 0 (4.31) The solution to this system will not be trivial (will be different to v = 0) when the determinant of (4.31) is equal to zero, that is Continuum Mechanics for Engineers ©det X.(σ Oliver− λ1) not= and|σ C.− λ Agelet1| = 0 . de Saracibar (4.32) Equation (4.32) is a third-grade polynomial equation in λ. Since tensor σ is symmetric, its three solutions (λ1 ≡ σ1, λ2 ≡ σ2, λ3 ≡ σ3) are real. Once the eigenvalues have been found and ordered according to the criterion σ1 ≥ σ2 ≥ σ3, (i) the eigenvector v can be obtained for each stress σi by resolving the system in (4.31), (i) (σ − σi1) · v = 0 i ∈ {1,2,3} . (4.33) This equation provides a non-trivial solution of the eigenvectors v(i), orthogo- nal between themselves, which, once it has been normalized, defines the three elements of the base corresponding to the three principal directions.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 146 CHAPTER 4. STRESS
Remark 4.9. In accordance with the graphical interpretation of the components of the stress tensor in Section 4.3.3, only normal stresses act on the faces of the elemental parallelepiped associated with the principal stress directions, which are, precisely, the principal stresses (see Figure 4.17).
4.4.5 Mean Stress and Mean Pressure
Definition 4.6. The mean stress is the mean value of the principal stresses. σ = 1 (σ + σ + σ ) m 3 1 2 3
Considering the matrix of components of the stress tensor in the principal stress directions (4.30), results in 1 1 σ = (σ + σ + σ )= Tr (σ ) . (4.34) m 3 1 2 3 3
Definition 4.7. The mean pressure is the mean stress with its sign changed. 1 mean pressureTheorynot= p¯ = − andσ = − Problems(σ + σ + σ ) m 3 1 2 3 Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Definition 4.8. A spherical or hydrostatic stress state is a state in which all three principal stress directions have the same value. ⎡ ⎤ σ 00 not ⎣ ⎦ not σ1 = σ2 = σ3 =⇒ σ ≡ 0 σ 0 ≡ σ1 00σ
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Properties of the Stress Tensor 147
Remark 4.10. In a hydrostatic stress state, the stress tensor is isotropic6 and, thus, its components are the same in every Cartesian coordinate system. As a consequence, any direction is a principal stress direction and the stress state (traction vector) is the same in any plane.
4.4.6 Decomposition of the Stress Tensor into its Spherical and Deviatoric Parts σ 7 σ The stress tensor σ can be split into a spherical part (or component) σ sph and a deviatoric part σ , σ = σ + σ . (4.35) sph spherical deviatoric part part The spherical part is defined as ⎡ ⎤ σm 00 def 1 not ⎢ ⎥ σ : = Tr (σ )1 = σ 1 ≡ ⎣ 0 σ 0 ⎦ , (4.36) sph 3 m m 00σm where σm is the mean stress defined in (4.34). According to definition (4.35), the deviatoric part of the stress tensor is ⎡ ⎤ ⎡ ⎤ Theoryσx τ andxy τxz Problemsσm 00 ⎢ ⎥ ⎢ ⎥ σ = σ − σ not≡ − sph ⎣ τxy σy τyz ⎦ ⎣ 0 σm 0 ⎦ (4.37) τ τ σ σ Continuum Mechanicsxz yz z for00 Engineersm © X. Oliver and C. Agelet de Saracibar resulting in ⎡ ⎤ ⎡ ⎤ σ − σ τ τ σ τ τ ⎢ x m xy xz ⎥ ⎢ x xy xz ⎥ σ not≡ = . ⎣ τxy σy − σm τyz ⎦ ⎣ τxy σy τyz ⎦ (4.38) τxz τyz σz − σm τxz τyz σz
6 A tensor is defined as isotropic when it remains invariant under any change of orthogonal basis. The general expression of an isotropic second-order tensor is T = α1 where α can be any scalar. 7 This type of decomposition can be applied to any second-order tensor.
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σ Remark 4.11. The spherical part of the stress tensor σ sph is an isotropic tensor (and defines a hydrostatic stress state), therefore, it remains invariant under any change of orthogonal basis.
Remark 4.12. The deviatoric component of the tensor is an indica- tor of how far from a hydrostatic stress state the present state is (see (4.37) and Remark 4.11).
Remark 4.13. The principal directions of the stress tensor and of its deviatoric tensor coincide. Proof is trivial considering that, from Re- σ mark 4.11, the spherical part σ sph is diagonal in any coordinate sys- tem. Consequently, if σ diagonalizes for a certain basis in (4.37), σ will also diagonalize for that basis.
Remark 4.14. The trace of the deviatoric (component) tensor is null. Taking into account (4.34) and (4.37), σ σ σ σ σ Tr σ = Tr σ − σ sph = Tr (σ ) − Tr σ sph = 3σm − 3σm = 0 . Theory and Problems
Continuum Mechanics for Engineers 4.4.7 Tensor Invariants© X. Oliver and C. Agelet de Saracibar The three fundamental invariants of the stress tensor8(or I invariants) are
I1 = Tr (σ )=σii = σ1 + σ2 + σ3 , (4.39) 1 I = σ : σ − I2 = −(σ σ + σ σ + σ σ ) , (4.40) 2 2 1 1 2 1 3 2 3 I3 = det(σ ) . (4.41)
8 The tensor invariants are scalar algebraic combinations of the components of a tensor that do not vary when the basis changes.
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Any combination of the I invariants is, in turn, another invariant. In this manner, the J invariants J1 = I1 = σii , (4.42) 1 1 1 J = I2 + 2I = σ σ = (σ : σ ) , (4.43) 2 2 1 2 2 ij ji 2 1 1 1 J = I3 + 3I I + 3I = Tr (σ · σ · σ )= σ σ σ , (4.44) 3 3 1 1 2 3 3 3 ij jk ki are defined.
Remark 4.15. For a purely deviatoric tensor σ , the corresponding J invariants are (see Remark 4.14 and equations (4.39)to(4.44)) ⎧ ⎪ ⎫ ⎪ = = ⎪ J1 I1 0 J1 = I1 = 0 ⎬⎪ ⎨⎪ 1 1 J = I =⇒ σ =⇒ = = (σ σ )= σ σ 2 2 ⎭⎪ ⎪ J2 I2 : ij ji = ⎪ 2 2 J3 I3 ⎪ 1 ⎩ J = I = σ σ σ 3 3 3 ij jk ki
4.5 Stress Tensor in Curvilinear Orthogonal Coordinates 4.5.1 Cylindrical Coordinates Consider a point in space defined by the cylindrical coordinates {r,θ,z} (see Figure 4.18). A physicalTheory (orthonormal) and basis { Problemseˆr,eˆθ ,eˆz} and a Cartesian system of local axes {x,y,z} defined as dextrorotatory are considered at this point. The components of the stress tensor in this basis are Continuum⎡ Mechanics⎤ ⎡ for Engineers⎤ ©σ X. Oliverτ τ and C.σ Ageletτ τ de Saracibar x x y x z r rθ rz not ⎢ ⎥ ⎢ ⎥ σ ≡ τ σ τ = τ σ τ . ⎣ x y y y z ⎦ ⎣ rθ θ θz ⎦ (4.45) τ τ σ τ τ σ x z y z z rz θz z
The graphical representation on an elemental parallelepiped is shown in Fig- ure 4.19, where the components of the stress tensor have been drawn on the visible faces. Note that, here, the visible faces of the figure do not coincide with the positive faces, defined (in the same direction as in Section 4.3.3.3) as those whose unit normal vector has the same direction as a vector of the physical basis.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 150 CHAPTER 4. STRESS
⎡ ⎤ x = r cosθ x(r,θ,z) not≡ ⎣ y = r sinθ ⎦ z = z
Figure 4.18: Cylindrical coordinates.
Figure 4.19: Differential element in cylindrical coordinates.
4.5.2 Spherical CoordinatesTheory and Problems A point in space is defined by the spherical coordinates {r,θ,φ} (see Fig- ure 4.20). A physical (orthonormal) basis eˆr,eˆθ ,eˆφ and a Cartesian system Continuum Mechanics for Engineers of local axes {x ,y ,z } defined© X. Oliver as dextrorotatory and C. Agelet are considered de Saracibar at this point. The components of the stress tensor in this basis are ⎡ ⎤ ⎡ ⎤ σ τ τ σ τ τ x x y x z r rθ rφ not ⎢ ⎥ ⎢ ⎥ σ ≡ τ σ τ = τ σ τ . ⎣ x y y y z ⎦ ⎣ rθ θ θφ ⎦ (4.46) τ τ σ τ τ σ x z y z z rφ θφ φ
The graphical representation on an elemental parallelepiped is shown in Fig- ure 4.21, where the components of the stress tensor have been drawn on the visible faces.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Mohr’s Circle in 3 Dimensions 151
⎡ ⎤ x = r sinθ cosφ x(r,θ,φ) not≡ ⎣ y = r sinθ sinφ ⎦ z = z cosθ
Figure 4.20: Spherical coordinates.
Figure 4.21:Theory Differential element and in Problems spherical coordinates. Continuum Mechanics for Engineers 4.6 Mohr’s Circle© in X. 3 Oliver Dimensions and C. Agelet de Saracibar 4.6.1 Graphical Interpretation of the Stress States The stress tensor plays such a crucial role in engineering that, traditionally, sev- eral procedures have been developed, essentially graphical ones, to visualize and interpret it. The most common are the so-called Mohr’s circles. Consider an arbitrary point in the continuous medium P and the stress tensor σ (P) at this point. Consider also an arbitrary plane, with unit normal vector n, that contains P (see Figure 4.22). The traction vector acting on point P corre- sponding to this plane is t = σ · n. This vector can now be decomposed into its components σ n, normal to the plane considered, and τ n, tangent to said plane.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 152 CHAPTER 4. STRESS
Figure 4.22: Decomposition of the traction vector.
Consider now the normal component σ n = σ n, where σ is the normal com- ponent of the stress on the plane, defined in accordance with the sign criterion detailed in Section 4.3.3.3, σ > 0 tension , σ = σ · n (4.47) n σ < 0 compression .
Consider now the tangential component τ n, of which only its module is of inter- est, τ n = t − σ n |τ n| = τ ≥ 0 . (4.48) The stress state on the plane with unit normal vector n at the point considered can be characterized by means of the pair σ ∈ R (σ,τ) → τ ∈ R+ (4.49) which, in turn, determine a point of the half-plane (x ≡ σ,y ≡ τ) ∈ R × R+ in Figure 4.23. If the infiniteTheory number ofand planes thatProblems contain point P are now con- sidered (characterized by all the possible unit normal vectors n(i)) and the corre- sponding values of the normal stress σi and tangential stress τi are obtained and, finally,Continuum are represented in the Mechanics half-space mentioned for above, Engineers a point cloud is ob- tained. One can then wonder© X. whether Oliver the and point C. cloud Agelet occupies de Saracibar all the half-space or is limited to a specific locus. The answer to this question is provided by the following analysis.
n1 → (σ 1,τ 1)
n2 → (σ 2,τ 2) ···
ni → (σ i,τ i)
Figure 4.23: Locus of points (σ,τ).
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Mohr’s Circle in 3 Dimensions 153
4.6.2 Determination of the Mohr’s Circles Consider the system of Cartesian axes associated with the principal directions of the stress tensor. In this basis, the components of the stress tensor are ⎡ ⎤ σ 00 ⎢ 1 ⎥ σ not≡ σ ≥ σ ≥ σ ⎣ 0 σ2 0 ⎦ with 1 2 3 (4.50)
00σ3 and the components of the traction vector are ⎡ ⎤⎡ ⎤ ⎡ ⎤ σ 00 n σ n ⎢ 1 ⎥⎢ 1 ⎥ ⎢ 1 1 ⎥ = σ · not≡ = , t n ⎣ 0 σ2 0 ⎦⎣ n2 ⎦ ⎣ σ2 n2 ⎦ (4.51)
00σ3 n3 σ3 n3 where n1,n2,n3 are the components of the unit normal vector n in the basis as- sociated with the principal stress directions. In view of (4.51), the normal com- ponent of the stress (σ), defined in (4.47), is ⎡ ⎤ n ⎢ 1 ⎥ · not≡ [σ , σ , σ ] = σ 2 + σ 2 + σ 2 = σ t n 1 n1 2 n2 3 n3 ⎣ n2 ⎦ 1 n1 2 n2 3 n3 (4.52)
n3 and the module of the traction vector is | |2 = · = σ 2 2 + σ 2 2 + σ 2 2 . t t t 1 n1 2 n2 3 n3 (4.53) The modules of the traction vector and of its normal and tangential components can also be related through | |2 =Theoryσ 2 2 + σ 2 and2 + σ 2 Problems2 = σ 2 + τ2 , t 1 n1 2 n2 3 n3 (4.54) where (Continuum4.53) has been taken Mechanics into account. Finally, for the Engineers condition that n is a unit normal vector can be expressed© X. Oliver in terms and of its C. components Agelet de as Saracibar | | = =⇒ 2 + 2 + 2 = . n 1 n1 n2 n3 1 (4.55)
Equations (4.54), (4.52) and (4.55) can be summarized in the following ma- trix equation. ⎡ ⎤⎡ ⎤ ⎡ ⎤ σ 2 σ 2 σ 2 n2 σ 2 + τ2 ⎢ 1 2 3 ⎥⎢ 1 ⎥ ⎢ ⎥ ⎣ σ σ σ ⎦⎣ 2 ⎦ = ⎣ σ ⎦ =⇒ · = 1 2 3 n2 A x b (4.56) 111 n2 1 3 A x b
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System (4.56) can be interpreted as a linear system with: a) A matrix of coefficients, A(σ ), defined by the stress tensor at point P (by means of the principal stresses). b) An independent term, b, defined by the coordinates of a certain point in the half-space σ − τ (representative, in turn, of the stress state on a certain plane). c) A vector of unknowns x that determines (by means of the components of the unit normal vector n) in which plane the values of the selected σ and τ correspond.
Remark 4.16. Only the solutions of system (4.56) whose compo- not≡ 2, 2, 2 T nents x n1 n2 n3 are positive and smaller than 1 will be fea- sible (see (4.55)), i.e., ≤ 2 ≤ , ≤ 2 ≤ ≤ 2 ≤ . 0 n1 1 0 n2 1 and 0 n3 1 Every pair (σ,τ) that leads to a solution x that satisfies this require- ment will be considered a feasible point of the half-space σ − τ, which is representative of the stress state on a plane that contains P. The locus of feasible points (σ,τ) is named feasible zone of the half- space σ − τ.
Consider now the goal of finding the feasible region. Through some algebraic operations,⎧ system (4.56) can be rewritten as ⎪ A ⎪ σ 2 + τ2 − (σ + σ )σ + σ σ − 2 = ( ) ⎪ 1 3 1 3 (σ − σ )n1 0 I ⎨⎪ Theory and1 Problems3 σ 2 + τ2 − (σ + σ )σ + σ σ − A 2 = ( ) ⎪ 2 3 2 3 (σ − σ )n2 0 II ⎪ 2 3 ⎪ (4.57) ⎩⎪ σ 2 + τ2 − (σ + σ )σ + σ σ − A 2 = ( ) Continuum1 2 Mechanics1 2 forn3 Engineers0 III © X. Oliver and(σ1 C.− σ Agelet2) de Saracibar
with A =(σ1 − σ2)(σ2 − σ3)(σ1 − σ3) .
Given, for example, equation (III) of the system in (4.57), it is easily verifiable that it can be written as
2 2 2 1 (σ − a) + τ = R with a = (σ1 + σ2) 2 (4.58) 1 and R = (σ − σ )2 +(σ − σ )(σ − σ )n2 , 4 1 2 2 3 1 3 3
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Mohr’s Circle in 3 Dimensions 155 which corresponds to the equation of a semicircle in the half-space σ − τ of center C3 and a radius R3, given by 1 C3 = (σ1 + σ2), 0 and 2 (4.59) 1 R = (σ − σ )2 +(σ − σ )(σ − σ )n2 . 3 4 1 2 2 3 1 3 3 2 ∈ [ , ] The different values of n3 0 1 determine a set of concentric semicircles of center C3 and radii R3 (n3) belonging to the half-space σ − τ and whose points occupy a certain region of this half-space. This region is delimited by the maximum and minimum values of R3 (n3). Observing that the radical in the 2 = expression of R3 in (4.59) is positive, these values are obtained for n3 0 (the 2 = minimum radius) and n3 1 (the maximum radius).
2 = =⇒ min = 1 (σ − σ ) n3 0 R3 1 2 2 (4.60) 1 n2 = 1 =⇒ R max = (σ + σ ) − σ 3 3 2 1 2 3 The domain delimited by both semicircles defines an initial limitation of the feasible domain, shown in Figure 4.24. This process is repeated for the other two equations, (I) and (II),in(4.57), resulting in: ⎧ ⎨ min 1 1 R = (σ2 − σ3) − ( ) = (σ + σ ), =⇒ 1 2 Equation I : C1 2 3 0 ⎩ 2 max = |σ − | R1 1 a1 a Theory1 and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.24: Initial limitation of the feasible domain.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 156 CHAPTER 4. STRESS
Figure 4.25: Feasible region.
⎧ ⎨ min 1 1 R = (σ1 − σ3) − ( ) = (σ + σ ), =⇒ 2 2 Equation II : C2 1 3 0 ⎩ 2 max = |σ − | R2 2 a2 a2 ⎧ ⎨ min 1 1 R = (σ1 − σ2) − ( ) = (σ + σ ), =⇒ 3 2 Equation III : C3 1 2 0 ⎩ 2 max = |σ − | R3 3 a3 a3 For each case, a feasible region that consists in a semi-annulus defined by the minimum and maximum radii is obtained. Obviously, the final feasible region must be in the intersection of these semi-annuli, as depicted in Figure 4.25. Figure 4.26 shows the final construction that results of the three Mohr’s semi- circles that contain pointsTheoryσ1, σ2 and andσ3. It can Problems also be shown that every point within the domain enclosed by the Mohr’s circles is feasible (in the sense that σ τ the correspondingContinuum values of Mechanicsand correspond for to stress Engineers states on a certain plane that contains point P). © X. Oliver and C. Agelet de Saracibar The construction of Mohr’s circle is trivial (once the three principal stresses are known) and is useful for discriminating possible stress states on planes, de- termining maximum values of shear stresses, etc.
Figure 4.26: Mohr’s circle in three dimensions.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Mohr’s Circle in 2 Dimensions 157
Example 4.3 – The principal stresses at a certain point in a continuous medium are σ1 = 10 , σ2 = 5 and σ3 = 2 . The normal and tangential stresses on a plane that contains this point are σ and τ, respectively. Justify if the following values of σ and τ are possible or not. a) σ = 10 and τ = 1. b) σ = 5 and τ = 4. c) σ = 3 and τ = 1. Solution The Mohr’s circle for the defined stress state is drawn and the given points are marked in the half-space σ − τ.
Only the points belonging to the gray zone represent stress states (feasible points). It is verified that none of the given points are feasible. Theory and Problems 4.7 Mohr’s Circle in 2 Dimensions Continuum Mechanics for Engineers Many real-life problems© in X. engineering Oliver and are assimilated C. Agelet to de an idealSaracibar bi-dimensional stress state9 in which one of the principal stress directions is known (or assumed) a priori. In these cases, the Cartesian axis x3 (or z-axis) is made to coincide with said principal direction (see Figure 4.25) and, thus, the components of the stress tensor can be written as ⎡ ⎤ ⎡ ⎤ σ σ 0 σ τ 0 ⎢ 11 12 ⎥ ⎢ x xy ⎥ σ not≡ = . ⎣ σ12 σ22 0 ⎦ ⎣ τxy σy 0 ⎦ (4.61)
00σ33 00σz
9 This type of problems will be analyzed in depth in Chapter 7, dedicated to bi-dimensional elasticity.
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Consider now only the family of planes parallel to the x3-axis (therefore, the component n3 of its unit normal vector is null). The corresponding traction vec- tor is ⎡ ⎤ ⎡ ⎤⎡ ⎤ t σ σ 0 n ⎢ 1 ⎥ ⎢ 11 12 ⎥⎢ 1 ⎥ ( , )=σ · =⇒ = t P n n ⎣t2 ⎦ ⎣ σ12 σ22 0 ⎦⎣ n2 ⎦ (4.62)
0 00σ33 0 and its component t3 vanishes. In (4.61) and (4.62) the components of the stress tensor, σ , of the unit normal vector defining the plane, n, and of the traction vector, t, associated with direction x3 are either well known (this is the case for σ13, σ23, n3 or t3), or do not intervene in the problem (as is the case for σ33). This circumstance suggests ignoring the third dimension and reducing the analysis to the two dimensions associated with the x1- and x2-axes (or x- and y-axes), as indicated in Figure 4.27. Then, the problem can be defined in the plane through the components of the stress tensor σ σ σ τ σ not≡ 11 12 = x xy (4.63) σ12 σ22 τxy σy and the components of the traction vector t σ σ n t(P,n)=σ · n not≡ 1 = 11 12 1 . (4.64) t2 σ12 σ22 n2
Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.27: Reduction of the problem from three to two dimensions.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Mohr’s Circle in 2 Dimensions 159
4.7.1 Stress State on a Given Plane Consider a plane (always parallel to the z-axis) whose unit normal vector n forms an angle θ with the x-axis. A unit vector m is defined in the tangential direction to the trace of the plane as indicated in Figure 4.28.
Remark 4.17. The unit normal vector n, the unit tangent vector m, and the angle θ in Figure 4.28 have the following positive directions associated with them. • Unit normal vector n: towards the exterior of the plane (with re- spect to the position of point P). • Unit tangent vector m: generates a clockwise rotation with re- spect to point P. • Angle θ: defined as counterclockwise.
Consider σ , the stress tensor at a given point, whose components are defined in a Cartesian base, σ τ σ not≡ x xy . (4.65) τxy σy Using (4.64), the traction vector on the given point, which belongs to the plane considered, is σ τ cosθ σ cosθ + τ sinθ t = σ · n not≡ x xy = x xy . (4.66) τ σ θ τ θ + σ θ xy Theoryy sin andxy Problemscos y sin
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.28: Stress state on a given plane.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 160 CHAPTER 4. STRESS
Taking into consideration the expression t = σθ n + τθ m, the normal stress σθ and the tangent stress τθ on the plane with inclination θ (see Figure 4.28) are defined, respectively, as not cosθ σθ = t · n ≡ [σx cosθ + τxy sinθ, τxy cosθ + σy sinθ] = sinθ (4.67) 2 2 = σx cos θ + τxy2sinθ cosθ + σy sin θ and not sinθ τθ = t · m ≡ [σ cosθ + τ sinθ, τ cosθ + σ sinθ] = x xy xy y −cosθ (4.68) 2 2 = σx sinθ cosθ − σy sinθ cosθ + τxy sin θ − cos θ , which can be rewritten as10
σx + σy σx − σy σθ = + cos(2θ)+τxy sin(2θ) 2 2 (4.69) σx − σy τθ = sin(2θ) − τ cos(2θ) 2 xy
Direct problem
Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Inverse problem
Figure 4.29: Direct and inverse problems.
10 The following trigonometric relations are used here: sin(2θ)=2sinθ cosθ, cos2 θ =(1 + cos(2θ))/2 and sin2 θ =(1 − cos(2θ))/2.
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4.7.2 Direct Problem: Diagonalization of the Stress Tensor The direct problem consists in obtaining the principal stresses and the principal stress directions given the components of the stress tensor (4.65) in a certain system of axes x − y (see Figure 4.29). The principal stress directions associated with the x- and y-axes defined by the angles α and π/2 + α (see Figure 4.29) determine the inclinations of the two planes on which the stresses only have a normal component σα , being the tangent component τα null. Imposing this condition on (4.69) yields
σ − σ τ τ = x y ( α) − τ ( α)= =⇒ ( α)= xy , α sin 2 xy cos 2 0 tan 2 σ − σ 2 x y 2 τ ( α)=± 1 = ± xy , sin 2 1 σ − σ 2 1 + x y tan2 (2α) + τ2 2 xy (4.70)
σx − σy ( α)=± 1 = ± 2 . cos 2 1 + tan2 (2α) σ − σ 2 x y + τ2 2 xy
Equation (4.70) provides two solutions (associated with the + and − signs) α1 and α2 = α1 +π/2, which define the two principal stress directions (orthogonal) to the plane being analyzed11. The corresponding principal stress directions are θ = α obtained replacing the angleTheoryin and (4.70)in( Problems4.69), resulting in σx + σy σx − σy σα = + cos(2α)+τ sin(2α) . (4.71) 2 2 xy Continuum Mechanics for Engineers ⎧ © X. Oliver and C. Agelet de Saracibar ⎪ ⎪ σ + σ σ − σ 2 ⎨⎪ σ = x y + x y + τ2 1 2 2 xy σα → (4.72) ⎪ ⎪ σ + σ σ − σ 2 ⎩⎪ σ = x y − x y + τ2 2 2 2 xy
11 The third principal stress direction is the direction perpendicular to the plane being ana- lyzed (z-orx3-axis), see (4.61) and Figure 4.27.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 162 CHAPTER 4. STRESS
Figure 4.30: Inverse problem.
4.7.3 Inverse Problem The problem consists in obtaining the stress state on any plane given the prin- cipal stresses and the principal stress directions σ1 and σ2 in the plane being analyzed. The stress state on any plane is characterized by the angle β that forms the unit normal vector of the plane with the principal stress direction cor- responding to σ1. As a particular case, the components of the stress tensor on an elemental rectangle associated with the system of axes x − y can be obtained (see Figure 4.29). Consider now the Cartesian system x −y, associated with the principal stress σ = σ σ = σ τ = directions (see Figure 4.30). Applying (4.69) with x 1, y 2, x y 0 and θ ≡ β results in
σ1 + σ2 σ1 − σ2 σβ = + cos(2β) 2 2 (4.73) σ1 − σ2 τβTheory= sin and(2β) Problems 2 Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar 4.7.4 Mohr’s Circle for Plane States (in 2 Dimensions) Consider all the possible planes that contain point P and the values of the normal and tangent stresses, σθ and τθ , defined in (4.69) for all the possible values of θ ∈ [0,2π]. The stress state in the point for an inclined plane θ can now be characterized by means of the pair
(σ = σθ , τ = τθ ) where σ ∈ R and τ ∈ R , (4.74) which, in turn, determines a point (x ≡ σ, y ≡ τ) ∈ R × R of the plane σ − τ in Figure 4.31. To determine the locus of points of said plane that characterizes
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 Mohr’s Circle in 2 Dimensions 163 all the possible stress states for planes that contain the point being analyzed, the ensuing procedure is followed. Considering a reference system that coincides with the principal stress di- rections (as in Figure 4.30) and characterizing the inclination of the planes by means of the angle β with the principal stress direction σ1, one obtains from (4.73) ⎧ ⎪ σ + σ σ − σ ⎨ σ − 1 2 = 1 2 cos(2β) 2 2 ⎪ (4.75) ⎩⎪ σ1 − σ2 τ = sin(2β) 2 and, squaring both equations and adding them up results in σ + σ 2 σ − σ 2 σ − 1 2 + τ2 = 1 2 . (4.76) 2 2
Note that this equation, which will be valid for any value of the angle β,or, in other words, for any arbitrarily oriented plane that contains the point, corre- sponds to a circle with center C and radius R in the plane σ − τ given by (see Figure 4.31) σ + σ σ − σ C = 1 2 , 0 and R = 1 2 . (4.77) 2 2 Consequently, the locus of points representative of a stress state on the planes that contain P is a circle (named Mohr’s circle), whose construction is defined in Figure 4.31. The inverse proposition is also true: given a point of Mohr’s circle with co- ordinates (σ, τ), there exists a plane that contains P whose normal and tangent stresses are σ and τ, respectively. In effect, using (4.75) the following trigono- metric expressions are obtained.Theory and Problems
Continuum Mechanics for Engineers © X. Oliver and C. Agelet de Saracibar
Figure 4.31: Mohr’s circle for plane stress states.
X. Oliver and C. Agelet de Saracibar Continuum Mechanics for Engineers.Theory and Problems doi:10.13140/RG.2.2.25821.20961 164 CHAPTER 4. STRESS
Figure 4.32: Interpretation of the angle β.