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Design and Stress Analysis of Extraterrestrial ... - The Black Vault

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dr dr r<br />

d• _._._.• .d~t 1 •t--%)"(3.61)<br />

Thus, in order to determine the radial <strong>and</strong> circular stresses<br />

in a disk we derived a system <strong>of</strong> two differential equations (3.55)<br />

<strong>and</strong> (3.61)<br />

System <strong>of</strong> equations (3.55) <strong>and</strong> (3.61) can be replaced by one<br />

differential equation <strong>of</strong> the second order relative to displacement u.<br />

For this we solve a system <strong>of</strong> equations (3.60) relative to or <strong>and</strong><br />

a with equalities (3.56) <strong>and</strong> (3.57) taken into account:<br />

E (du u u dE u<br />

"-+1 ; ' -- 'iht'rJ"_ + 1 (3.62)<br />

12 dr r I'~ dr<br />

If we substitute equalities (3.62) into (3.55) we obtain a<br />

differential equation <strong>of</strong> the second order relative to u:<br />

d1 2 t --- I dhh ldu .drdh I \ u Isu2<br />

'<br />

dr dr r ]dr h dr .r -- r = --F<br />

Cr, (3.63)<br />

where<br />

C--•w2. (3.64)<br />

If we can obtain a solution to equation (3.63) relative to the<br />

radial displacement <strong>of</strong> u for a disk <strong>of</strong> any shape (defined by function<br />

h = h(r)), then stresses or <strong>and</strong> 1f are determined from expressions<br />

(3.62).<br />

Thus, stresses in a rotating disk can be obtained either<br />

directly from equations (3.55) <strong>and</strong> (3.61) or from expressions (3.62)<br />

after determining u from equation (3.63).<br />

294

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