Physics Technology Update (4th Edition)

Published by Pearson
ISBN 10: 0-32190-308-0
ISBN 13: 978-0-32190-308-2

Chapter 11 - Rotational Dynamics and Static Equilibrium - Problems and Conceptual Exercises - Page 374: 113

Answer

$a=\frac{2}{3}g$

Work Step by Step

We can show that the required linear acceleration is $\frac{2}{3}g$ as follow: $\tau=T\times r$ $\implies T=\frac{\tau}{r}$ $\implies T=\frac{I\alpha}{r}$ But $I=\frac{1}{2}mr^2$ and $\alpha=\frac{a}{r}$ $\implies T=\frac{(\frac{1}{2}mr^2)(\frac{a}{r})}{r}$ $T=\frac{1}{2}ma$ Now the net balancing force acting downward is given as $ma=mg-T$ $\implies ma=mg-\frac{1}{2}ma$ $\implies \frac{3}{2}ma=mg$ $a=\frac{2}{3}g$
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