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CONTINUUM MECHANICS for ENGINEERS

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where A 1 and A 2 are constants of integration depending on the boundary<br />

conditions. Eq 6.9-3 written in terms of displacement derivatives has the<br />

<strong>for</strong>m<br />

( )<br />

σ = λδ u + µ u + u<br />

ij ij kk , ij , ji ,<br />

It follows by making use of Eqs 6.9-23 and 6.9-25 that<br />

i j<br />

σij λAδ ij µ A δij<br />

A ⎡⎛<br />

⎞ 3Axx⎤<br />

2<br />

2<br />

= 3 1 + 2 ⎢⎜<br />

1+<br />

⎟ − 3<br />

5<br />

⎣⎝<br />

r ⎠<br />

⎥<br />

r ⎦<br />

(6.9-26)<br />

(6.9-27)<br />

Recall that the traction vector in the radial direction (see Eq 3.7-1) is<br />

σ = σ nn which upon substitution of Eq 6.9-25 becomes<br />

N ij i j<br />

σ = 3λ + 2µ<br />

A<br />

N<br />

( ) +<br />

4µ<br />

A<br />

3<br />

r<br />

(6.9-28)<br />

where the identity x has been used. Similarly, the tangential traction<br />

i = rni<br />

can be calculated using σ where the unit vectors νi are perpendic-<br />

S = σijνν i j<br />

ular to ni. The result is<br />

σ = 3λ + 2µ<br />

A<br />

S<br />

(6.9-29)<br />

since ν . ix i = 0<br />

The constants A1 and A2 are determined from boundary conditions on the<br />

tractions. Clearly,<br />

σ<br />

σ<br />

N<br />

N<br />

Carrying out the indicated algebra, we have the well-known <strong>for</strong>mulas<br />

σ N<br />

σ S<br />

(6.9-30a)<br />

(6.9-30b)<br />

These equations may be easily modified to cover the case where p 1 = 0, or<br />

the case where p 2 = 0.<br />

1<br />

( ) +<br />

1<br />

2µ<br />

A<br />

3<br />

r<br />

=− p at r = r<br />

1 1<br />

=− p at r = r<br />

3<br />

pr 11 − pr<br />

= 3 3<br />

r − r<br />

2<br />

2 2<br />

3<br />

22<br />

1<br />

3<br />

pr 11 − pr<br />

= 3 3<br />

r − r<br />

2<br />

3<br />

22<br />

1<br />

3<br />

rr 1 − 3<br />

r<br />

3<br />

rr 1 +<br />

2r<br />

3<br />

2<br />

3<br />

2<br />

3<br />

2<br />

2<br />

p − p<br />

3<br />

r − r<br />

1 2<br />

3<br />

2 1<br />

p − p<br />

3<br />

r − r<br />

1 2<br />

3<br />

2 1

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