Lecture 4 - 2003 Pure Twist pure twist around center of rotation D => neither axial (σ) nor bending forces (Mx, My) act on section; as previously, D is fixed, but (for now) arbitrary point. as before: a) equilibrium of wall element: b) compatibility (shear strain) d d q + σ ⋅t = 0 ds dx d d u+ v=γ=0 ds dx small deflections c) tangential displacement (δv) in terms of η, ζ and φ (geometry) δv δx = δη δx ⋅cos( α ) + δζ δx ⋅sin( α ) + hp⋅ δφ δx N.B. hp =>hD from definition of problem further assumptions: 1) preservation of cross section shape => ζ = ζ(x); η = η(x) φ = φ(x) d d 2) shear though finite is small ~ 0 => u = − v ds dx δu axial stress 3) Hooke's law holds => σ = E⋅ δx ----------------------------- from equilibrium -------------------------------⌠ σ dA = Nx ⌡ ⌠ τ⋅h dA = p ⌡ ⌠ σ⋅y dA = -M.z ⌡ ⌠ σ⋅z dA = M y ⌡ ⌠ q⋅ h ds = T p p ⌡ pure twist ⌠ σ dA = Nx = 0 ⌡ ⌠ ⌠ τ⋅cos( α ) dA = q⋅cos( α ) ds = Vy ⌡ ⌡ ⌠ σ⋅y dA = −M z = 0 ⌡ ⌠ ⌠ τ⋅sin( α ) dA = q⋅sin( α ) ds = Vz ⌡ ⌡ ⌠ σ⋅z dA = M y = 0 ⌡ pure twist also => only φ is finite i.e. other displacements (and derivatives) ζ = η = 0 => δv δx = δη δx ⋅cos( α ) + δζ δx ⋅sin( α ) + hp⋅ using negligible shear assumption δφ δx becomes δv δx = hD⋅ δφ δx δφ d d d and integration along s => u = − v => u = −hD⋅ δx ds dx ds 1 notes_13_pure_twist.mcd u=− δφ ⌠ ⋅ hD ds + u0( x) δx ⌡ previously u = −η'⋅Y − ζ' ⋅ Z + u0( x) which showed u linear with y and z => plane sections plane. ⌠ here - only if h is constant so it can come outside hD 1 ds ⌡ D is u (longitudinal displacement) linear. u is defined as warping displacement (function). stress analysis can be made analogous for torsion and bending IF the integrand hD⋅ds thought to be a coordinate. calculation of stresses will involve statical moments, moments of inertia and products of inertia which will be designated "sectorial" new coordinate = Ω Ω wrt arbitrary origin and ω wrt normalized sectorial coordinate (as before like wrt center of area) dΩ = hD⋅ds = dω the warping function then becomes: u=− δφ δx ⋅Ω + u0( x) = −φ'⋅ Ω + u0( x) b) warping stresses as before: axial strain = du/dx => u' = −φ''⋅ Ω + u'0( x) and σ = E⋅ u' = −E⋅ φ''⋅Ω + E⋅ u'0( x) ⌠ σ dA = 0 ⌡ E⋅ u'0( x) = E⋅φ'' determines u'0( x) ⌠ Ω dA ⌡ ⌠ ⌡ (−E⋅ φ''⋅Ω + E⋅ u'0(x)) dA = 0 and stress becomes: A ⌠ Ω dA ⌡ that is: σ = −E⋅ φ''⋅ Ω − = −E⋅ φ''⋅ω A σ = −E⋅ φ''⋅Ω + E⋅φ''⋅ where => ⌠ Ω dA ⌡ A = −E⋅ φ''⋅ω ⌠ Ω dA ⌡ ω=Ω− A this defines the normalized coordinate in the same sense as y and Y etc. .............................................................. as an aside: u' = −φ''⋅ ω => u = −φ'⋅ ω + constant dω = hD⋅ds in this sense, ω is defined as the unit warping function displacement per unit change in rotation dependent only on s within a constant ................................................................ 2 notes_13_pure_twist.mcd shear flow follows from integration of d d q = − σ ⋅t ds dx d d q + σ ⋅t = 0 along s as above and leads to : ds dx ⌠ d q( s, x) = − σ⋅t ds + q1( x) dx ⌡ => using the expression for axial stress σ = E⋅ u' = −E⋅ φ''⋅ω ⌠ q( s, x) = q1( x) − ⌡ s 0 s ⌠ s d σ ⋅t ds = q ( x) − ⌠ E⋅ ( ) + E⋅φ''' − φ'''⋅ω⋅t ds = q x ω⋅t ds 1 1 ⌡0 ⌡ dx 0 where q1( x) is f(z) and represents the shear flow at the start of the region. it is 0 at a stress free boundary which is convenient for an open section: q1( x) = 0 as before if we designate the integrals which are the static moments of the cross section area: e.g. Qy and Qz: ⌠ Qω = ω dA = ⌡ s ⌠ ω⋅t ds ⌡ = "sectorial statical moment of the cut-off portion of the cross section" 0 therefore: q( s, x) = E⋅φ'''⋅Qω designate torsional moment wrt D by Tω ⌠ ⌠ now, since dΩ = hD⋅ds = dω => q⋅ hD ds = q dω ⌡ ⌡ parts: ⌠ ⌠ u dv = (u⋅v) ( b) − ( u v) ( 0) − v du ⌡ ⌡ ⌠ τ⋅h dA = D ⌡ ⌠ q⋅ h ds = T D ω ⌡ and using integration by parts u=q v=ω du = dq dv = dω integration along s and as dq = δq/δs*ds ⌠ ⌠ ⌠ δq q dω = q⋅ω(s = b) − q⋅ω(s = 0) − ω dq = q⋅ω(s = b) − q⋅ω(s = 0) − ω⋅ ds δs ⌡ ⌡ ⌡ q⋅ω(s = b) = 0 and q⋅ω(s = 0) = 0 now using equilibrium: as q(s=b) and q(s=0) = 0 (stress free ends) d d q + σ ⋅t = 0 ds dx 3 notes_13_pure_twist.mcd ⌠ ⌠ ⌠ δq d q dω = 0 − ω⋅ ds = ω⋅ σ⋅t ds dx δs ⌡ ⌡ ⌡ d σ = −E⋅ φ'''⋅ω => dx substituting σ = −E⋅ φ''⋅ω from above ⌠ ⌠ ⌠ d q dω = ω⋅ σ⋅t ds = −E⋅ φ'''⋅ ω⋅ ω⋅t ds = −E⋅ φ'''⋅Iωω dx ⌡ ⌡ ⌡ ⌠ ⌠ Iωω = ω⋅ ω dA = ω⋅ ω⋅t ds ⌡ ⌡ where similar to Iz ⌠ ⌠ Iz = y ⋅ y dA = y ⋅ y⋅t ds ⌡ ⌡ N.B. sometimes this is represented by Iyy ⌠ going back to the relationship for torsional moment, where we have derived relationships for q⋅ hD ds ⌡ => ⌠ ⌠ Tω = q⋅ hD ds = q dω = −E⋅ φ'''⋅Iωω ⌡ ⌡ −Tω therefore: φ''' = E⋅ Iωω Tω if we think of a distributed torsional load (moment/unit length) mD; mD equilibrium over element dz => −Tω + mD⋅dx + Tω + d T ⋅dx = 0 ω dx Tω + dTω/dx*dx => T'ω = −mD and just as M'y = Vz the warping moment M'ω may be defined as M'ω = Tω thus: φ'' = −M ω E⋅ Iωω σ = −E⋅ φ''⋅ω = Mω Iωω and the stresses are as follows: ⋅ω and ... from q( s, x) = E⋅φ'''⋅Qω 4 q( s, x) = τ ⋅t = −Tω Iωω ⋅Qω notes_13_pure_twist.mcd c) Center of twist calculation of the sectorial quantities assumes center of twist yD and zD are known. the second and third equilibrium conditions above require: ⌠ σ⋅y dA = 0 ⌡ ⌠ σ⋅z dA = 0 ⌡ for pure twist ⌠ ⌠ using σ = −E⋅ φ''⋅ω this requires ω⋅y dA = 0 and ω⋅z dA = 0 as E ≠ 0 and φ'' ≠ 0 ⌡ ⌡ now for some geometry: determine distance from tangent to wall from hD in terms of the coordinates of the center, the angle (α) that the y axis would have to rotate to line up with the positive direction of the tangent and the perpendicular distance from the origin of the centroidal coordinates hC ds a = y D⋅cos( β ) hC hD D β hD = hC − a − b y tangent a β=α− π 2 β yD β b cos( β ) = cos α − sin( β ) = sin α − α π 2 = sin( α ) π 2 = −cos( α ) C zD z b = zD⋅sin( β ) parallel to tangent hD = hC − a − b = hC − y D⋅cos( β ) − zD⋅sin( β ) = hC − y D⋅sin( α ) + zD⋅cos( α ) α multiply by ds and apply geometry: hD⋅ds = hC⋅ds − y D⋅sin( α ) ⋅ds + zD⋅cos( α ) ⋅ds ds dy β dz ds⋅cos( β ) = dz = ds⋅sin( α ) ds⋅sin( β ) = −dy = ds⋅ ( −cos( α )) y,η dy = ds⋅cos( α ) z,ζ hD⋅ds = hC⋅ds − y D⋅sin( α ) ⋅ds + zD⋅cos( α ) ⋅ds = hC⋅ds − y D⋅dz + zD⋅dy sectorial coordinate ω = hds => hD⋅ds = dωD = hC⋅ds − y D⋅dz + zD⋅dy = dωC − y D⋅dz + zD⋅dy 5 notes_13_pure_twist.mcd which is now integrated: ωD = ωC − y D⋅z + zD⋅y and introduced into the equilibrium equations above where ω is ωD : ⌠ ⌠ ω⋅y dA = 0 and ω⋅z dA = 0 => ⌡ ⌡ ⌠ ω ⋅y dA = 0 = D ⌡ ⌠ ⌡ (ωC − yD⋅z + zD⋅y)⋅y dA ⌠ ω ⋅z dA = 0 = D ⌡ and .... ⌠ ⌡ (ωC − yD⋅z + zD⋅y)⋅z dA now using second moment nomenclature (including treating ω as a coordinate) => ⌠ ⌠ ⌠ ω ⋅y dA − y y ⋅ z dA + z ⋅ y ⋅ y dA = 0 D D C ⌡ ⌡ ⌡ becomes recall that Iyωc is referred to C for ω Izωc − y D⋅Iyz − zD⋅Iz = 0 and ....... ⌠ ⌠ ⌠ ω ⋅z dA − y z⋅ z dA + z ⋅ y ⋅ z dA = 0 D D C ⌡ ⌡ ⌡ becomes Iyωc − y D⋅Iy + zD⋅Iyz = 0 which provides two equations in two unknowns y D and zD Given Iyωc − y D⋅Iy + zD⋅Iyz = 0 yD → Iyωc⋅Iz − Iyz⋅ Izωc 2 Iy ⋅Iz − Iyz and for principal axes Iyz = 0 yD → and ... Iyz := 0 zD → y D := Iyωc Iy yD := Find( y D , zD) zD Izωc − y D⋅Iyz + zD⋅Iz = 0 6 2 Iy ⋅Iz − Iyz (Iyωc⋅Iz − Iyz⋅Izωc) zD → and ... −Izωc⋅Iy + Iyz⋅Iyωc I ⋅I − I 2 y z yz zD := (−Izωc⋅Iy + Iyz⋅Iyωc) I ⋅II − I 2 y z yz −Izωc Iz notes_13_pure_twist.mcd