Coordination Transformations for Strain & Stress Rates To keep the presentation as simple as possible, we will look at purely two-dimensional stress-strain rates. Given an original coordinate system ( x, y ) and a rotated system ( x̂, yˆ ) as shown below: y x' y' θ x Recall that the strain rates in the x-y coordinate system are: 1 ∂u ∂v ∂v ∂u ε xx = ε xy = + ε yy = 2 ∂y ∂x ∂y ∂x Or, in index notation: 1 ∂u ∂u j ε ij = i + 2 ∂x j ∂xi Also, we note that the unit vectors for the rotated axes are: K K K iˆ = cos θ i + sin θ j K K K ĵ = − sin θ i + cos θ j Thus, the location of a point in ( x̂, yˆ ) is: x̂ cos θ ŷ = − sin θ sin θ cos θ x y Similarly, the velocity components are related by: û cos θ v̂ = − sin θ sin θ u cos θ v For differential changes, we also have dx̂ cos θ dŷ = − sin θ sin θ dx cos θ dy Coordination Transformations for Strain & Stress Rates Thus, defining T as the rotation matrix, we note that: ∂xˆ ∂xˆ ∂x ∂y cos θ sin θ = T = ∂yˆ − sin θ cos θ ∂yˆ ∂x ∂y Inverting this: ∂x ∂x ∂xˆ ∂yˆ cos θ = T −1 = ∂y − sin θ ∂y ∂xˆ ∂yˆ Thus to find −1 sin θ cos θ = cos θ sin θ − sin θ cos θ ∂uˆ in terms of u, v and their derivatives: ∂xˆ ∂uˆ ∂uˆ ∂x ∂uˆ ∂y ∂uˆ ∂uˆ = + = cos θ + sin θ ∂xˆ ∂x ∂xˆ ∂y ∂xˆ ∂x ∂y Then, substituting uˆ = u cos θ + v sin θ : ∂uˆ ∂ ∂ = cos θ + sin θ (u cos θ + v sin θ ) ∂xˆ ∂x ∂y ∂u ∂v ∂u ∂v = cos2 θ + cos θ sin θ + cos θ sin θ + sin 2 θ ∂x ∂x ∂y ∂y ⇒ ε xxˆ ˆ = cos2 θε xx + 2 cos θ sin θε xy + sin 2 θε yy ∂vˆ ∂ ∂ = − sin θ + cos θ ( −u sin θ + v cos θ ) ∂yˆ ∂x ∂y ∂u ∂v ∂u ∂v = sin 2 θ − sin θ cos θ − sin θ cos θ + cos2 θ ∂x ∂x ∂y ∂y ⇒ ε yyˆ ˆ = sin 2 θε xx + 2sin θ cos θε xy + cos2 θε yy 1 ∂uˆ ∂vˆ 1 ∂ ∂ ∂ ∂ + = − sin θ + cos θ (u cos θ + v sin θ ) + cos θ + sin θ ( − sin θ + v cos θ ) ∂x ∂y ∂x ∂y 2 ∂yˆ ∂xˆ 2 ⇒ ε xyˆˆ = sin θ cos θ (ε yy − ε xx ) + (cos2 θ − sin 2 θ )ε xy 16.100 2002 2 Coordination Transformations for Strain & Stress Rates If x − y are the principal strain directions, then ε xy = 0 and ε xˆxˆ , ε xˆyˆ & ε yˆyˆ are ε xˆxˆ = cos 2 θε xx + sin 2 θε yy ε yˆyˆ = sin 2 θε xx + cos 2 θε yy if ε xy = 0 ε xˆyˆ = sin θ cos θ (ε yy − ε xx ) The next step is to relate the stresses in (x, y ) to (xˆ , yˆ ) . Consider a differential surface with ŷ normal: τ τyy y τyx dy τxx x' dx y' τyy θ θ x τxy τyx dx K The resultant stress is given as the vector τ and the force on the surface is Decomposing the stress vector into the coordinate axes gives: K K K τ ds. K τ d xˆ = (τ yˆ xˆ i + τ yˆ yˆ j ) d xˆ K K = ( − τ xx d y + τ yx d x ) i + (τ y y d x − τ xy d y ) j Note that: dx = cos θ dxˆ dy = sin θ dxˆ K K K i = cos θ iˆ − sin θ ˆj K K K ˆ j = sin θ i + cos θ ˆj 16.100 2002 3 Coordination Transformations for Strain & Stress Rates Thus, the second line becomes: K K ( −τ xx sin θ + τ yx cos θ )(cos θ iˆ − sin θ ˆj )dxˆ K K K K +(τ yy cos θ − τ xy sin θ )(sin θ iˆ + cos θ ˆj )dxˆ = (τ yxˆ ˆ iˆ + τ yyˆ ˆ ˆj )dxˆ So collecting all the iˆ & ˆj terms (and enforcing τ xy = τ yx ) gives: τ yxˆ ˆ = (τ yy − τ xx )sin θ cos θ + τ yx (cos2 θ − sin 2 θ ) τ yyˆ ˆ = τ xx sin 2 θ + τ yy cos2 θ − 2τ yx sin θ cos θ For the principal strain axes, τ xx = 2µε xx + λ (ε xx + ε yy ) τ yy = 2 µε yy + λ (ε xx + ε yy ) τ xy = 0 Plugging this into τ yˆxˆ andτ yˆyˆ gives τ yxˆ ˆ = 2 µ (ε yy − ε xx ) sin θ cos θ ε xy ˆˆ τ yy = 2 µ (ε xx sin 2 θ + ε yy cos2 θ ) + λ (ε xx + ε yy ) ε yy ˆˆ ε xx ˆ ˆ +ε yy ˆˆ Thus, we arrive at the known result: τ yxˆ ˆ = 2 µ ε xyˆˆ τ yyˆ ˆ = 2 µ ε yyˆ ˆ + λ (ε xxˆ ˆ + ε yyˆ ˆ ) A similar derivation would give: τ xxˆ ˆ = 2 µε xxˆ ˆ + λ (ε xxˆ ˆ + ε yyˆ ˆ ) 16.100 2002 4