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fisica1-youn-e-freedman-exercicios-resolvidos

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2<br />

10.67: For the disk, K = (3 4) Mv ( see Example10.6)<br />

K = MgL sin , from which<br />

1<br />

β<br />

. From the work-energy theorem,<br />

L =<br />

2<br />

3v<br />

=<br />

4g<br />

sin β<br />

2<br />

3(2.50 m s)<br />

= 0.957 m.<br />

2<br />

4(9.80 m s ) sin 30.0°<br />

This same result may be obtained by an extension of the result of Exercise 10.26; for the<br />

disk, the acceleration is ( 2 3) g sin β,<br />

leading to the same result.<br />

b) Both the translational and rotational kinetic energy depend on the mass which<br />

cancels the mass dependence of the gravitational potential energy. Also, the moment of<br />

inertia is proportional to the square of the radius, which cancels the inverse dependence<br />

of the angular speed on the radius.<br />

10.68: The tension is related to the acceleration of the yo-yo by ( 2m ) g − T = (2m)<br />

a,<br />

and<br />

a<br />

to the angular acceleration by Tb = Iα = I<br />

b<br />

. Dividing the second equation by b and<br />

adding to the first to eliminate T yields<br />

2m<br />

a = g<br />

(2m<br />

+ I<br />

2<br />

= g<br />

2<br />

b ) 2 + ( R<br />

b)<br />

2<br />

,<br />

2<br />

α = g<br />

2b<br />

+ R<br />

2<br />

,<br />

b<br />

1 2 2<br />

where I = 2 mR = mR<br />

2<br />

has been used for the moment of inertia of the yo-yo. The<br />

tension is found by substitution into either of the two equations; e.g.,<br />

T =<br />

⎛ 2<br />

2m)(<br />

g − a)<br />

= (2mg)<br />

⎜1−<br />

⎝ 2 + ( R<br />

b)<br />

2<br />

⎞ ( R b)<br />

⎟ = 2mg<br />

⎠ 2 + ( R b)<br />

2mg<br />

=<br />

.<br />

(2( b R)<br />

+ 1)<br />

(<br />

2<br />

2<br />

2

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