Double pendulum: energy function

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SUMMARY

The discussion focuses on deriving the energy function for a double pendulum under two conditions: motion restricted to a vertical plane and motion in three-dimensional space. The energy function is defined as the sum of potential energy (PE) and kinetic energy (KE). The potential energy is expressed as $PE=m_1gy_1+m_2gy_2$, while the kinetic energy varies based on the motion constraints, leading to different formulations for each case. For motion in a vertical plane, the kinetic energy is $KE=\frac{1}{2}m_1(\dot x_1^2 + \dot y_1^2)+\frac{1}{2}m_2(\dot x_2^2 + \dot y_2^2)$, and for motion in space, it includes a third coordinate, resulting in $KE=\frac{1}{2}m_1(\dot x_1^2 + \dot y_1^2 + \dot z_1^2)+\frac{1}{2}m_2(\dot x_2^2 + \dot y_2^2 + \dot z_2^2)$.

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  • Understanding of classical mechanics, specifically energy conservation principles.
  • Familiarity with potential and kinetic energy equations.
  • Knowledge of coordinate systems, including Cartesian and polar coordinates.
  • Basic calculus for understanding derivatives and motion equations.
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mathmari
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Hey! :o

I am looking at the following:

Find the energy function for the double pendulum, with vertical constant and uniform gravity field
  • for motion restricted at vertical plane
  • for motion in space
We have that the energy function is the sum of the potential and the kinetic energy, right?

The potential energy of the system is given by $PE=m_1gy_1+m_2gy_2$.

The kinetic energy is given by $KE=\frac{1}{2}m_1v_1^2+\frac{1}{2}m_2v_2^2$.

Therefore, the energy function is equal to $$E=PE+KE=m_1gy_1+m_2gy_2+\frac{1}{2}m_1v_1^2+\frac{1}{2}m_2v_2^2$$ Is this correct?

How can we distinct between motion restricted at vertical plane and motion in space? And what does a uniform gravitational field imply?

(Wondering)
 
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mathmari said:
How can we distinct between motion restricted at vertical plane and motion in space?

Hey mathmari! (Smile)

In a vertical plane we only have $x$ and $y$.
So $v_1^2 = \dot x_1^2 + \dot y_1^2$.

For motion in space we also have a 3rd coordinate (perhaps we should pick the vertical coordinate to be $z$ instead of $y$ to avoid confusion.) (Thinking)

mathmari said:
And what does a uniform gravitational field imply?

That we have constant vertical acceleration by gravity $g$, which is what you already have.
That is as opposed to how gravity actually works, which is $\frac{GM}{r^2}$, where $M$ is the mass of the earth, and $r$ is the distance to the center of the earth. At the surface we can treat it as a uniform field though. (Thinking)
 
I like Serena said:
Hey mathmari! (Smile)

In a vertical plane we only have $x$ and $y$.
So $v_1^2 = \dot x_1^2 + \dot y_1^2$.

For motion in space we also have a 3rd coordinate (perhaps we should pick the vertical coordinate to be $z$ instead of $y$ to avoid confusion.) (Thinking)

So, to difference between the two motions is at the kinetic energy?

Do we get for the first case:

The potential energy of the system is given by $PE=m_1gy_1+m_2gy_2$.
The kinetic energy is given by $KE=\frac{1}{2}m_1v_1^2+\frac{1}{2}m_2v_2^2=\frac{1}{2}m_1\left (\dot x_1^2 + \dot y_1^2\right )+\frac{1}{2}m_2\left (\dot x_2^2 + \dot y_2^2\right )$.

and for the second case:

The potential energy of the system is given by $PE=m_1gy_1+m_2gy_2$.
Here do we have to use also $z_1,z_2$ ? But how?
The kinetic energy is given by $KE=\frac{1}{2}m_1v_1^2+\frac{1}{2}m_2v_2^2=\frac{1}{2}m_1\left (\dot x_1^2 + \dot y_1^2+\dot z_1^2\right )+\frac{1}{2}m_2\left (\dot x_2^2 + \dot y_2^2+\dot z_2^2\right )$.

? Or do we have to use for example polar coordinates? (Wondering)
 
Last edited by a moderator:
Yep. (Nod)

We can write the same thing in polar coordinates, but there is no need.
The only reason to do so, is if it helps us to solve a follow up question, and we can do it then.
 
I like Serena said:
Yep. (Nod)

So, we do we get the following energy function?

  1. for motion restricted at vertical plane

    The potential energy of the system is given by $PE=m_1gy_1+m_2gy_2$.
    The kinetic energy is given by $KE=\frac{1}{2}m_1v_1^2+\frac{1}{2}m_2v_2^2=\frac{1}{2}m_1\left (\dot x_1^2 + \dot y_1^2\right )+\frac{1}{2}m_2\left (\dot x_2^2 + \dot y_2^2\right )$.

    So, the total energy is given by $$E=PE+KE=m_1gy_1+m_2gy_2+\frac{1}{2}m_1\left (\dot x_1^2 + \dot y_1^2\right )+\frac{1}{2}m_2\left (\dot x_2^2 + \dot y_2^2\right )$$
  2. for motion in space

    The potential energy of the system is given by $PE=m_1gy_1+m_2gy_2$.
    The kinetic energy is given by $KE=\frac{1}{2}m_1v_1^2+\frac{1}{2}m_2v_2^2=\frac{1}{2}m_1\left (\dot x_1^2 + \dot y_1^2+\dot z_1^2\right )+\frac{1}{2}m_2\left (\dot x_2^2 + \dot y_2^2+\dot z_2^2\right )$.

    So, the total energy is given by $$E=PE+KE=m_1gy_1+m_2gy_2+\frac{1}{2}m_1\left (\dot x_1^2 + \dot y_1^2+\dot z_1^2\right )+\frac{1}{2}m_2\left (\dot x_2^2 + \dot y_2^2+\dot z_2^2\right )$$
Is the potential energy in both cases the same? (Wondering)
 
Yes and yes. (Mmm)
 
I like Serena said:
Yes and yes. (Mmm)

Ok! Thank you very much! (Smile)
 

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