Consider the diagram above which indicates all masses and charges. The green chargeless point mass is connected to two charged particles (shown in red) by massless rigid rods of length L . The green mass is given an initial velocity ( v ) along the positive Y-direction at time t = 0 . At time t = 0 , the green mass is located at the origin and the coordinates of each of the red particles are ( L , 0 ) and ( − L , 0 ) . Both the red particles are initially at rest. The goal of this problem is to compute the time period of motion of the whole system.
Enter your answer rounded to the nearest integer.
Note:
m o = L = 2
Q = m = 4 π ϵ o = 1
v = 0 . 5
The force between the charged particles is governed by Coulomb's law.
The green particle's speed does not necessarily remain constant with time. Note that only the initial speed and direction of projection is provided.
Gravity is absent throughout space.
You may need to use Wolfram-Alpha towards the end.
Bonus: Plot the trajectory of each of the masses in a single graph. Comment on the periodicity of the separation between the charges. Do you observe something counter-intuitive?
This follow-up problem is based on a suggestion by Steven Chase
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@Karan Chatrath I have added some additional notes on the relative periods
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Thanks for the addition. When I initially solved it myself, I based the period of motion on the periodicity of the x coordinate. So my initial answer was half of the actual period.
θ varies periodically but not sinusoidally since θ ¨ is not proportional to θ , and here we need help of numerical technique, which is why I couldn't post a solution.
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There is a semi-analytical approach to this problem. You can use the conservation of generalised momentum and energy equations to construct an integral for the time period. The integral, however, does not have a closed-form solution, which is why I suggested using Wolfram-Alpha.
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What I got is
d θ d z = C cos 2 θ − D A sec θ tan θ − B z sin θ ,
where z = θ ˙ 2 , A , B , C , D are constants. This can't be solved analytically any further.
A slightly different solution from that of @Steven Chase
Let the y coordinate of the vertical ball be s . Let θ be the angle between any rigid rod and the Y-axis.
Coordinates of the ball on the right:
x 1 = L sin θ y 1 = s − L cos θ
Coordinates of the ball on the left:
x 2 = − L sin θ y 2 = s − L cos θ
Kinetic energy of the system:
T = 2 m o s ˙ 2 + 2 m ( x ˙ 1 2 + y ˙ 1 2 ) + 2 m ( x ˙ 2 2 + y ˙ 2 2 )
T = 2 s ˙ 2 + 4 s ˙ θ ˙ sin θ + 4 θ ˙ 2
Potential Energy of the system:
V = 4 sin θ 1
Lagrange's equation with respect to s is:
d t d ( ∂ s ˙ ∂ T ) = 0 ⟹ s ˙ + θ ˙ sin θ = C
Where C is an arbitrary constant. The above equation is the generalised momentum conservation law.
The initial conditions of the system are:
θ ( 0 ) = 2 π θ ˙ ( 0 ) = − L v s ( 0 ) = 0 s ˙ ( 0 ) = v
Applying initial conditions gives: C = 4 1 ⟹ s ˙ + θ ˙ sin θ = 4 1 … ( 2 )
Since total energy is conserved:
T + V = C 2
Applying initial conditions gives C 2 = 0 . 5 T + V = 2 1
Eliminating s ˙ from the energy equation using (2) and simplifying:
( 4 − 2 sin 2 θ ) θ ˙ 2 + 8 1 + 4 sin θ 1 = 2 1
θ ˙ 2 = 8 sin θ ( 4 − 2 sin 2 θ ) 3 sin θ − 2
Recall that the minimum separation is:
d = 3 8
That corresponds to: θ o = arcsin ( 2 / 3 )
So when the motion of the system starts, θ reduced. This means:
θ ˙ = − 8 sin θ ( 4 − 2 sin 2 θ ) 3 sin θ − 2
Rearranging:
∫ θ o π / 2 3 sin θ − 2 8 sin θ ( 4 − 2 sin 2 θ ) d θ = ∫ 0 T / 4 d t
We know that θ = π / 2 is the mean position while θ = θ o is the extreme position. The motion from the mean to extreme position in an oscillation takes a quarter of the total time period. Hence:
T = 4 ∫ θ o π / 2 3 sin θ − 2 8 sin θ ( 4 − 2 sin 2 θ ) d θ
@Alak Bhattacharya I hope you find this useful.
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Let θ be the angle of the rod below the horizontal. Let y 0 be the vertical position of the middle ball. The position and velocity of the ball on the right are:
x = L cos θ y = y 0 − L sin θ x ˙ = − L sin θ θ ˙ y ˙ = y ˙ 0 − L cos θ θ ˙
Since x ˙ and y ˙ are zero in the beginning, and θ = 0 as well, we know that θ ˙ = L v in the beginning. The kinetic energy, potential energy, and Lagrangian are:
T = m L 2 θ ˙ 2 + m y 0 ˙ 2 − 2 m L cos θ θ ˙ y 0 ˙ + 2 1 m 0 y 0 ˙ 2 V = 2 L cos θ k q 2 L = T − V = m L 2 θ ˙ 2 + m y 0 ˙ 2 − 2 m L cos θ θ ˙ y 0 ˙ + 2 1 m 0 y 0 ˙ 2 − 2 L cos θ k q 2
Equations of motion:
d t d ∂ y 0 ˙ ∂ L = ∂ y 0 ∂ L d t d ∂ θ ˙ ∂ L = ∂ θ ∂ L
Crunching out the math results in the following coupled linear system:
\[\begin{pmatrix} 2m + m_0 & -2 m L \cos \theta \\ -2 m L \cos \theta & 2 m L^2 \\
\end{pmatrix}
\begin{pmatrix} \ddot{y}_0 \\ \ddot{\theta} \\
\end{pmatrix} = \begin{pmatrix} -2 m L \sin \theta \, \dot{\theta}^2 \\ -\frac{k q^2}{2L} \sec \theta \tan \theta \\
\end{pmatrix} \]
Initialize variables appropriately and solve the linear system for the double-dot terms on every time step. Numerical integration yields a period of motion of θ T θ ≈ 2 2 . 0 3 .
The plot below shows y 0 and θ (in degrees) over time from t = 0 to t = 1 0 0 . You can see that θ oscillates sinusoidally, while y 0 increases steadily with some small oscillation on top.
Interestingly, the period of motion of the x coordinate of the balls seems to be half that of θ and y . Recall that θ is a time sinusoid (or at least a quasi-sinusoid). Since x is the cosine of θ , its period is half that of θ . Since y is the sine of θ , its period is equal to that of θ . You can go to Wolfram Alpha and ask it to expand the cosine of a sine and the sine of a sine to see this.