A particle
of mass
slides on the surface of a rough quarter-pipe of mass
. The cross-sectional profile of the quarter-pipe is a quadrant of a circle of radius
, and the coefficient of (kinetic) friction between the particle and the quarter-pipe is
. The quarter-pipe is standing on a large horizontal layer of ice, which may be treated as a smooth surface. The particle starts at rest at the point
at the top of the quarter-pipe, which is also stationary, and begins to slide down its surface. The quarter-pipe will also begin to slide on the ice.
In the case that kg and kg, there is a value such that the particle will reach the bottom of the quarter-pipe at the point (and then continue sliding on the ice) if , but such that the particle will be brought to rest at some point on the quarter-pipe (and never reach the ice) if . Give the value of .
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− m X ¨ ( 1 0 ) + m a θ ¨ ( sin θ − cos θ ) + m a θ ˙ 2 ( cos θ sin θ ) = m R ( cos θ sin θ ) + μ m R ( − sin θ cos θ ) + m g ( 0 − 1 ) and hence − X ¨ cos θ + a θ ˙ 2 − X ¨ sin θ + a θ ¨ = R − g sin θ = − μ R + g cos θ The only external forces acting on the quarter-pipe and the particle are gravity and the normal reaction from the ice, all of which are vertical. Thus the horizontal component of the center of mass of the particle/quarter-pipe system stays constant throughout the motion. Hence − M X + m ( − X + a − a cos θ ) is constant, and so ( M + m ) X ˙ = m a θ ˙ sin θ Eliminating both R and X from these equations, we obtain the formidable differential equation ( 2 M + m + m cos 2 θ − μ m sin 2 θ ) θ ¨ + ( μ ( 2 M + m ) − m sin 2 θ − μ m cos 2 θ ) θ ˙ 2 = a 2 ( M + m ) g ( cos θ − μ sin θ ) Remarkably, we can find the first integral of this differential equation. To find the required integrating factor, we need to perform the integral ∫ 2 M + m + m cos 2 θ − μ m sin 2 θ 2 ( μ ( 2 M + m ) − m sin 2 θ − μ m cos 2 θ ) d θ = ln ( 2 M + m + m cos 2 θ − μ m sin 2 θ ) + ∫ 2 M + m + m cos 2 θ − μ m sin 2 θ 2 μ ( 2 M + m ) d θ This can be handled using a t = tan θ substitution. Omitting the details, if we define the function F ( θ ) = e x p [ 4 M 2 + 4 M m − μ 2 m 2 2 μ ( 2 M + m ) tan − 1 ( 4 M 2 + 4 M m − μ 2 m 2 2 M tan θ − μ m ) ] then d θ d [ [ 2 M + m + m cos 2 θ − μ m sin 2 θ ] F ( θ ) ] = 2 [ μ ( 2 M + m ) − m sin 2 θ − μ m cos 2 θ ] F ( θ ) so the differential equation becomes d θ d [ 2 1 ( 2 M + m + m cos 2 θ − μ m sin 2 θ ) F ( θ ) θ ˙ 2 ] ( 2 M + m + m cos 2 θ − μ m sin 2 θ ) F ( θ ) θ ˙ 2 = a 2 ( M + m ) g ( cos θ − g sin θ ) F ( θ ) = a 4 ( M + m ) g G ( θ ) where G ( θ ) = ∫ 0 θ ( cos φ − μ sin φ ) F ( φ ) d φ Now ∣ ∣ m cos 2 θ − μ m sin 2 θ ∣ ∣ ≤ m 1 + μ 2 < m 2 < 2 M + m and hence 2 M + m + m cos 2 θ − μ m sin 2 θ > 0 for all 0 < θ < 2 1 π . We can also show that R = 2 M + m + m cos 2 θ − μ m sin 2 θ 2 M ( a θ ˙ 2 + g sin θ ) > 0