A small block having a mass
m
= 1.00 kg is released from rest on a circular track with radius
R
= 1.00 m. The block is released from point
A
at a height
R
above the floor and slides down along the surface. Find the exact coefficient of kinetic friction
that would stop the block exactly when it reaches point
B
. Consider
g
= 9.81 m/s
.
(I found
= 0.604016)
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Let the coordinates of the block be:
x = − R cos ϕ y = − R sin ϕ
Computing time derivatives:
x ˙ = R ϕ ˙ sin ϕ y ˙ = − R ϕ ˙ cos ϕ
Therefore, the speed of the block is:
v = x ˙ 2 + y ˙ 2 = R ϕ ˙
x ¨ = R ϕ ¨ sin ϕ + R ϕ ˙ 2 cos ϕ y ¨ = − R ϕ ¨ cos ϕ + R ϕ ˙ 2 sin ϕ
Let the normal force acting on the block due to contact with the circular surface be N at point P . The friction force acting on the block is f = μ N acting tangentially to the circular surface against the block's motion.
The equations of motion along X and Y can be computed as such:
m x ¨ = N cos ϕ − μ N sin ϕ m y ¨ = N sin ϕ + μ N cos ϕ − m g
Replacing the double derivative terms and eliminating N from the above two equations after some simplification gives the equation of motion:
ϕ ¨ + μ ϕ ˙ 2 = R g ( cos ϕ − μ sin ϕ ) = f ( ϕ )
Since the block starts from rest, ϕ ( 0 ) = ϕ ˙ ( 0 ) = 0 .
The differential equation:
ϕ ¨ + μ ϕ ˙ 2 = f ( ϕ ) ϕ ˙ d ϕ d ϕ ˙ + μ ϕ ˙ 2 = f ( ϕ ) 2 ϕ ˙ d ϕ d ϕ ˙ + 2 μ ϕ ˙ 2 = 2 f ( ϕ )
Multiplying both sides by e 2 μ ϕ gives:
e 2 μ ϕ 2 ϕ ˙ d ϕ d ϕ ˙ + 2 μ e 2 μ ϕ ϕ ˙ 2 = 2 f ( ϕ ) e 2 μ ϕ
d ϕ d ( ϕ ˙ 2 e 2 μ ϕ ) = 2 f ( ϕ ) e 2 μ ϕ
Now, separating and integrating (and applying initial conditions) gives:
ϕ ˙ 2 e 2 μ ϕ = ∫ 0 ϕ 2 f ( x ) e 2 μ x d x
Where f ( x ) = R g ( cos x − μ sin x )
Solving this tedious integral and simplifying gives:
ϕ ˙ = ( R 2 g ( − 4 μ 2 + 1 ( 2 μ 2 − 1 ) sin ( ϕ ) − 3 μ cos ( ϕ ) − 4 μ 2 + 1 3 μ e − 2 μ ϕ ) ) 1 / 2
Now, given that R = 1 the speed of the block v = ϕ ˙ . For this to be zero at ϕ = π / 2 , the above expression on the right hand side must be evaluated at ϕ = π / 2 and equated to zero. On simplification, this given the following non-linear equation:
1 − 2 μ 2 3 μ = e π μ
This equation can be solved numerically to obtain the solution of approximately:
μ ≈ 0 . 6 0 3