A pendulum consists of a rigid massless rod of length L with one end hinged at the origin of the x y plane. The other end is connected to a ball of mass m . The pendulum rotates in the x y plane, and the ambient gravitational acceleration g is in the negative y direction.
There is also a damping force on the ball, which has the following form:
F D = − D v
In the above equation, D is a damping coefficient, and v is the velocity of the ball. At time t = 0 , the pendulum has zero speed and makes an angle θ with the positive x axis, as shown in the diagram.
At time t = 3 0 , what is the sum of the x and y coordinates of the ball?
Details and Assumptions:
1)
m
=
L
=
1
2)
g
=
1
0
3)
D
=
0
.
1
4)
θ
=
π
/
3
5)
The ball can be treated as a point particle
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@Karan Chatrath nice question.
I think it is interesting how @Karan Chatrath incorporated the rod tension into his solution. My approach was a bit more conventional.
Moment of Inertia:
I = m L 2
Position and velocity:
x = L cos θ y = L sin θ x ˙ = − L sin θ θ ˙ y ˙ = L cos θ θ ˙
Gravity, damping, and total force:
F g = ( 0 , − m g ) F D = ( − D x ˙ , − D y ˙ ) F = F g + F D
Torque from vector cross product:
r = ( x , y ) τ = r × F
The torque is one-dimensional, so it can be thought of as a scalar τ . The sign of τ changes appropriately to yield oscillation. Angular acceleration:
θ ¨ = I τ
Numerical integration takes care of the rest
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At a general time t , let the coordinates of the ball be ( x , y ) = ( cos θ , sin θ ) . The velocity and acceleration components are:
[ x y ] = [ cos θ sin θ ] ⟹ [ x ˙ y ˙ ] = [ − θ ˙ sin θ θ ˙ cos θ ] ⟹ [ x ¨ y ¨ ] = [ − θ ¨ sin θ − θ ˙ 2 cos θ θ ¨ cos θ − θ ˙ 2 sin θ ]
Let the magnitude of tension be T and it is directed towards the origin along the length of the rod. Now, applying Newton's second law gives:
m [ x ¨ y ¨ ] = [ 0 − m g ] − T [ cos θ sin θ ] − D [ x ˙ y ˙ ]
This gives us a system of two equations in θ ¨ and T . Eliminating T from these set of equations leads to the final equation of motion which is the following. Simplifications left out.
θ ¨ = − 1 0 θ ˙ − 1 0 cos θ ; θ ( 0 ) = 3 π ; θ ˙ ( 0 ) = 0
We asked to compute the sum cos θ + sin θ at time t = 3 0 . This has been done numerically as follows: