Motion of a parametrically driven damped coplanar double pendulum
Rebeka Sarkar, Krishna Kumar, Sugata Pratik Khastgir
Abstract
We present the results of linear stability of a damped coplanar double pendulum and its non-linear motion, when the point of suspension is vibrated sinusoidally in the vertical direction with amplitude $a$ and frequency $ω$. A double pendulum has two pairs of Floquet multipliers, which have been calculated for various driving parameters. We have considered the stability of a double pendulum when it is in any of its possible stationary states: (i) both pendulums are either vertically downward or upward and (ii) one pendulum is downward, and the other is upward. The damping is considered to be velocity-dependent, and the driving frequency is taken in a wide range. A double pendulum excited from its stable state shows both periodic and chaotic motion. The periodic motion about its pivot may be either oscillatory or rotational. The periodic swings of a driven double pendulum may be either harmonic or subharmonic for lower values of $a$. The limit cycles corresponding to the normal mode oscillations of a double pendulum of two equal masses are squeezed into a line in its configuration space. For unequal masses, the pendulum shows multi-period swings for smaller values of $a$ and damping, while chaotic swings or rotational motion at relatively higher values of $a$. The parametric driving may lead to stabilization of a partially or fully inverted double pendulum.
Simulation skipped or failed
no parseable d.../dt equation found
Extracted equations
- (1 + µ sin²(θ₁ - θ₂)) θ̈₁ + (1 - A sin Ωτ) [(1 + µ) sin θ₁ - µ cos(θ₁ - θ₂) sin θ₂] + (µ/λ)[θ̇₂² + λ θ̇₁² cos(θ₁ - θ₂)] sin(θ₁ - θ₂) + 2β(1 + sin²(θ₁ - θ₂)) θ̇₁ + 2βΩA [2 sin θ₁ - cos(θ₁ - θ₂) sin θ₂] cos Ωτ = 0
- (1 + µ sin²(θ₁ - θ₂)) θ̈₂ + λ(1 + µ)(1 - A sin Ωτ) [sin θ₂ - cos(θ₁ - θ₂) sin θ₁] - [λ(1 + µ) θ̇₁² + µ θ̇₂² cos(θ₁ - θ₂)] sin(θ₁ - θ₂) + 2β(µ/λ)[1 + µ sin²(θ₁ - θ₂)] θ̇₂ + 2β(1 - µ) θ̇₁ cos(θ₁ - θ₂) + 2βΩA/λ [µ(1 + µ) sin θ₂ - 2µ² cos(θ₁ - θ₂) sin θ₁] cos Ωτ = 0
Paper claims vs. our run
- For equal masses, limit cycles corresponding to normal mode oscillations are squeezed into a line in configuration spacenot-testableno fidelity score recorded
- For unequal masses, two marginal stability curves merge to form a double-well-shaped instability zonenot-testableno fidelity score recorded
- Parametric driving can stabilize partially or fully inverted double pendulum configurationsnot-testableno fidelity score recorded
- Periodic motion can be harmonic or subharmonic for lower driving amplitudesnot-testableno fidelity score recorded
- Chaotic swings or rotational motion occur at higher driving amplitudesnot-testableno fidelity score recorded
- Multi-period swings appear for unequal masses at smaller driving amplitudes and dampingnot-testableno fidelity score recorded
Parameters
| µ | m₂/m₁ (mass ratio, varied; representative value 1.0 for equal masses) |
| λ | l₁/l₂ (length ratio, representative value 1.0) |
| β | Γ/(2m₁ω₀) (damping coefficient, varied; representative value 0.1) |
| A | aω²/g (dimensionless driving amplitude, varied; representative value 0.5) |
| Ω | ω/ω₀ (dimensionless driving frequency, varied; representative value 2.0) |
| ω₀ | √(g/l₁) (natural frequency scale) |
Run notes
equations tried: ['(1 + µ sin²(θ₁ - θ₂)) θ̈₁ + (1 - A sin Ωτ) [(1 + µ) sin θ₁ - µ cos(θ₁ - θ₂) sin θ₂] + (µ/λ)[θ̇₂² + λ θ̇₁² cos(θ₁ - θ₂)] sin(θ₁ - θ₂) + 2β(1 + sin²(θ₁ - θ₂)) θ̇₁ + 2βΩA [2 sin θ₁ - cos(θ₁ - θ₂) sin θ₂] cos Ωτ = 0', '(1 + µ sin²(θ₁ - θ₂)) θ̈₂ + λ(1 + µ)(1 - A sin Ωτ) [sin θ₂ - cos(θ₁ - θ₂) sin θ₁] - [λ(1 + µ) θ̇₁² + µ θ̇₂² cos(θ₁ - θ₂)] sin(θ₁ - θ₂) + 2β(µ/λ)[1 + µ sin²(θ₁ - θ₂)] θ̇₂ + 2β(1 - µ) θ̇₁ cos(θ₁ - θ₂) + 2βΩA/λ [µ(1 + µ) sin θ₂ - 2µ² cos(θ₁ - θ₂) sin θ₁] cos Ωτ = 0']