Two rigid hemispheres and with uniform volume density have radii and respectively. Hemisphere has its flat face glued to a plane. Hemisphere is then balanced on top of hemisphere such that their curved surfaces are in contact.
Naturally, is in equilibrium when its flat face lies parallel to the flat face of . However, if given a small nudge, rolls without slipping on the curved surface of and will either oscillate about the equilibrium position or fall.
The constraint on such that can oscillate is given to be where is some positive real number.
Find the value of .
For this problem, assume gravity points down, perpendicular to the plane of 's flat face.
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Let θ be the angle formed with the axis of hemisphere B and the center of the flat surface of hemisphere A . Since all forces which do work in this scenario (gravity) are conservative, we will analyze this problem using conservation of energy, and determine for which a give a gravitational potential energy well about θ = 0 .
Let the U ( θ ) = 0 line be the plane of hemisphere B 's flat surface, and let the center of mass position of each hemisphere with respect to its flat face be a ′ and b ′ respectively. For example, hemisphere B is flat on the ground with its curved surface up, the center of mass position would be at b ′ above the plane.
For hemisphere A , we need some more variables - Let ϕ be the angle formed by the axis of hemisphere A , and the line connecting the centers of both hemisphere's flat surfaces. Then ϕ + θ gives the angle formed by the axis of hemisphere A and the vertical. Here, it is important to note that due to the no-slip condition, the arcs traced out by θ and ϕ are the same, and so a ϕ = b θ ⇒ ϕ = a b θ . Then θ + ϕ = ( 1 + a b ) θ . Let k = 1 + a b → θ + ϕ = k θ .
We can then find the gravitational potential energy of the system to be
U ( θ ) = ρ V b g b ′ + ρ V a g [ ( a + b ) cos ( θ ) − a ′ cos ( θ + ϕ ) ] = ρ V b g b ′ + ρ V a g [ ( a + b ) cos ( θ ) − a ′ cos ( k θ ) ]
Let ρ V a g = c ˉ . Then
U ′ ( θ ) = c ˉ [ a ′ k sin ( k θ ) − ( a + b ) sin ( θ ) ] ⇒ U ′ ′ ( θ ) = c ˉ [ a ′ k 2 cos ( k θ ) − ( a + b ) cos ( θ ) ]
For stable equilibrium to hold, U ′ ′ > 0 . We then plug in our equilibrium theta and find our constraint on a
U ′ ′ ( 0 ) = c ˉ [ a k 2 − ( a + b ) ] > 0 ⇒ a + b < a ′ k 2
We then use the fact that the center of mass position of a hemisphere lies on the axis a distance 8 3 r from the flat face.
a + b < 8 3 a ( 1 + a b ) 2 ⇒ a 2 ( a + b ) < 8 3 a ( a + b ) 2 ⇒ a < 8 3 a + 8 3 b ⇒ a < 5 3 b
And so our answer is 5 3 = . 6 0 0