Elasticity/Spinning disk

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Thin spinning disk

Problem 1:

A thin disk of radius a is spinning about its axis with a constant angular velocity θ˙. Find the stress field in the disk using an Airy stress function and a body force potential.

File:Elastic spinning disk.png
An elastic disk spinning around its axis of symmetry

Solution:

The acceleration of a point (r,θ) on the disk is

(1)ar=θ˙2r;aθ=0

The body force field is

(2)fr=ρθ˙2r;fθ=0

Since there is no rotational acceleration, the body force can be derived from a potential V. The relations between the stresses, the Airy stress function and the body force potential are

(3)σrr=1rφr+1r22φθ2+V(4)σθθ=2φr2+V(5)σrθ=r(1rφθ)

where

(6)fr=Vr;fθ=1rVθ

From equations (2) and (6) , we have,

(7)ρθ˙2r=Vr(8)0=1rVθ

Integrating equation (7), we have

(9)V=ρθ˙2r22+h(θ)

Substituting equation (9) into equation (8), we get

(10)dh(θ)dθ=0h(θ)=C

This constant can be set to zero without loss of generality. Therefore,

(11)V=ρθ˙2r22

The spinning disk problem is a plane stress problem. Hence the compatibility condition is

(12)4φ+(21α)2V=04φ+(1ν)2V=0

where

(13)2()=2()r2+1r()r+1r22()θ(14)4()=2[2()]

Now, from equations (11) and (13)

(15)2V=ρθ˙2[1+1+0]=2ρθ˙2

Therefore, equation (12) becomes

(16)4φ=2ρθ˙2(1ν)

Since the problem is axisymmetric, there can be no shear stresses, i.e. σrθ=0 and no dependence on θ. From Michell's solution, the appropriate terms of the Airy stress function are

(17)r2;r2ln(r);ln(r)

Axisymmetry also requires that uθ, the displacement in the θ direction must be zero. However, if we look at Mitchell's solution, we see that uθ is non-zero if the term r2ln(r) is used in the Airy stress function. Hence, we reject this term and are left with

(18)φ=C1r2+C2ln(r)

If we plug this stress function into equation (16) we see that 4φ=0. Therefore, equation (18) represents a homogeneous solution of equation (16). The φ that is a general solution of equation (16) is obtained by adding a particular solution of the equation.

One such particular solution is the stress function φ=C0r4 since the biharmonic equation must evaluate to a constant. Plugging this into equation (16) we have

(19)4φ=64C0=2ρθ˙2(1ν)

or,

(20)C0=ρθ˙2(1ν)32

Therefore, the general solution is

(21)φ=ρθ˙2(1ν)32r4+C1r2+C2ln(r)

The corresponding stresses are (from equations (3, 4, 5)),

(22)σrr=(3+ν)θ˙2ρr28+2C1+C2r2(23)σθθ=(1+3ν)θ˙2ρr28+2C1C2r2(24)σrθ=0

At r=0, the stresses must be finite. Hence, C2=0. At r=a, σrr=σrθ=0. Evaluating σrr at r=a we get

(25)C1=(3+ν)ρθ˙2a216

Substituting back into equations (22) and (23), we get

(26)σrr=ρθ˙28(3+ν)(a2r2)
(27)σθθ=ρθ˙28[(3+ν)a2(1+3ν)r2]
(28)σrθ=0

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