A particle is confined to the surface of a cone, and has the following coordinates:
At time , the position and velocity are:
At time , what is the coordinate of the particle?
Details and Assumptions:
1)
Gravitational acceleration is
in the negative
direction
2)
Angles are in radians
Bonus: Plot the trajectory in the plane out to and
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The equations of motion can be easily derived using the Lagrangian approach. Let:
m = 1
The kinetic energy of the particle reads:
T = 2 1 ( 2 r ˙ 2 + r 2 θ ˙ 2 ) V = 1 0 r
Lagrange's equations read:
d t d ( ∂ r ˙ ∂ T ) − ∂ r ∂ T + ∂ r ∂ V = 0 ⟹ r ¨ = 2 r θ ˙ 2 − 5 … ( 1 )
d t d ( ∂ θ ˙ ∂ T ) − ∂ θ ∂ T + ∂ θ ∂ V = 0 d t d ( ∂ θ ˙ ∂ T ) = 0 r 2 θ ˙ = K
Applying initial conditions to the above equation gives:
r 2 θ ˙ = 1 0 … ( 2 )
Replacing (2) in (1) gives:
r ¨ = r 3 5 0 − 5 r 2 θ ˙ = 1 0
Solving the above numerically gives the required result. As for the trajectory, the particle seems to be confined to a 'bucket' as seen in the following figures:
Upto t = 2 0 0
Upto t = 1 0 0
The solution was also attempted analytically and I made some headway but could not proceed beyond a point.
Derivation using Newton's laws:
Consider the particle to be on any point on the given conical surface.
x = r cos θ y = r sin θ z = r
Now, as the particle slides on the conical surface. It experiences the following forces:
The equation of the cone can easily be derived by seeing that:
x 2 + y 2 = z 2 Φ = x 2 + y 2 − z 2 = 0
A vector normal to this surface can be computed as such:
∇ Φ = n = ⎣ ⎡ 2 x 2 y − 2 z ⎦ ⎤
The corresponding unit vector is:
n ^ = x 2 + y 2 + z 2 1 ⎣ ⎡ x y − z ⎦ ⎤
Substituting x , y and z gives:
n ^ = 2 1 ⎣ ⎡ cos θ sin θ − 1 ⎦ ⎤
Now, let the reaction force be N . Applying Newton's second law:
m ⎣ ⎡ x ¨ y ¨ z ¨ ⎦ ⎤ = ⎣ ⎡ 0 0 − m g ⎦ ⎤ + 2 N ⎣ ⎡ cos θ sin θ − 1 ⎦ ⎤
Let:
2 N = P
The equations of motion are:
m ⎣ ⎡ x ¨ y ¨ z ¨ ⎦ ⎤ = ⎣ ⎡ 0 0 − m g ⎦ ⎤ + P ⎣ ⎡ cos θ sin θ − 1 ⎦ ⎤
Now:
m z ¨ = r ¨
r ¨ = − g − P ⟹ P = − g − r ¨
Replacing P in the equations for x ¨ and y ¨ and and also writing x ¨ and y ¨ in terms of r , θ , r ˙ , θ ˙ , r ¨ , θ ¨ gives us two massive equations. Solving those equations for r ¨ , θ ¨ finally gives:
r ¨ = 2 r θ ˙ 2 − 2 g θ ¨ = − r 2 r ˙ θ ˙