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5.120: a) There are many ways to do these sorts of problems; the method presented is<br />

fairly straightforward in terms of application of Newton’s laws, but involves a good deal<br />

of algebra. For both parts, take the x-direction to be horizontal and positive to the right,<br />

and the y-direction to be vertical and positive upward. The normal force between the<br />

block and the wedge is n; the normal force between the wedge and the horizontal surface<br />

will not enter, as the wedge is presumed to have zero vertical acceleration. The horizontal<br />

acceleration of the wedge is A, and the components of acceleration of the block are a<br />

x<br />

and a<br />

y<br />

. The equations of motion are then<br />

MA = −n<br />

sin α<br />

ma<br />

ma<br />

x<br />

y<br />

= n sin α<br />

= n cosα − mg.<br />

Note that the normal force gives the wedge a negative acceleration; the wedge is expected<br />

to move to the left. These are three equations in four unknowns, A, a , a and n. Solution<br />

is possible with the imposition of the relation between A, a<br />

x<br />

and a<br />

y<br />

.<br />

An observer on the wedge is not in an inertial frame, and should not apply Newton’s<br />

laws, but the kinematic relation between the components of acceleration are not so<br />

restricted. To such an observer, the vertical acceleration of the block is a<br />

y,<br />

but the<br />

horizontal acceleration of the block is a x<br />

− A.<br />

To this observer, the block descends at an<br />

angle α , so the relation needed is<br />

ay<br />

= − tan α.<br />

ax<br />

− A<br />

At this point, algebra is unavoidable. Symbolic-manipulation programs may save some<br />

M<br />

solution time. A possible approach is to eliminate a<br />

x<br />

by noting that ax<br />

= − A (a result<br />

m<br />

that anticipates conservation of momentum), using this in the kinematic constraint to<br />

eliminate a<br />

y<br />

and then eliminating n. The results are:<br />

− gm<br />

A =<br />

( M + m)<br />

tan α + ( M<br />

a<br />

x<br />

gM<br />

=<br />

( M + m)<br />

tan α + ( M<br />

tan α)<br />

tan α)<br />

− g(<br />

M + m) tan α<br />

ay<br />

=<br />

( M + m)<br />

tan α + ( M tan α)<br />

(b) When M >> m, A → 0,<br />

as expected (the large block won’t move). Also,<br />

g<br />

tanα<br />

ax →<br />

tanα<br />

+ (1 tanα<br />

)<br />

= g 2 = g sin α cosα,<br />

which is the acceleration of the block<br />

tan α + 1<br />

( g sin α in this case), with the factor of cos α giving the horizontal component. Similarly,<br />

a y<br />

→ −g sin 2 α.<br />

(c) The trajectory is a spiral.<br />

x<br />

y

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