What is the component (radial inertia) of the generalized inertia tensor?

The component MrrM_{rr} represents the effective generalized mass or radial inertia associated with the generalized velocity r˙\dot{r} (the radial speed of mass m1m_1 and the vertical speed of mass m2m_2). The formula for the component is: Mrr=2Tr˙2=m1+m2M_{rr} = \frac{\partial^2 T}{\partial \dot{r}^2} = m_1 + m_2

Here is the explanation for why this result is simply the sum of the two masses:

The total kinetic energy of the system is the sum of the kinetic energies of the two masses, grouped by their associated generalized velocities (r˙\dot{r} and φ˙\dot{\varphi}):

T=12(m1+m2)r˙2+12(m1r2)φ˙2 T = \frac{1}{2} (m_1 + m_2) \dot{r}^2 + \frac{1}{2} (m_1 r^2) \dot{\varphi}^2

To find MrrM_{rr}, we first take the partial derivative of TT with respect to r˙\dot{r}:

Tr˙=r˙[12(m1+m2)r˙2+12(m1r2)φ˙2] \frac{\partial T}{\partial \dot{r}} = \frac{\partial}{\partial \dot{r}} \left[ \frac{1}{2} (m_1 + m_2) \dot{r}^2 + \frac{1}{2} (m_1 r^2) \dot{\varphi}^2 \right]

  • The first term, 12(m1+m2)r˙2\frac{1}{2} (m_1 + m_2) \dot{r}^2, differentiates to (m1+m2)r˙(m_1 + m_2)\dot{r}.

  • The second term, 12(m1r2)φ˙2\frac{1}{2} (m_1 r^2) \dot{\varphi}^2, is treated as a constant with respect to r˙\dot{r}, so its derivative is 0.

    Tr˙=(m1+m2)r˙ \frac{\partial T}{\partial \dot{r}} = (m_1 + m_2) \dot{r}

Next, we take the partial derivative of the result with respect to r˙\dot{r} again:

Mrr=2Tr˙2=r˙[(m1+m2)r˙] M_{rr} = \frac{\partial^2 T}{\partial \dot{r}^2} = \frac{\partial}{\partial \dot{r}} \left[ (m_1 + m_2) \dot{r} \right]

  • Since (m1+m2m_1 + m_2) is a constant, the derivative is simply:

    Mrr=m1+m2 M_{rr} = m_1 + m_2

Physical Interpretation: Total Radial Mass

The result Mrr=m1+m2M_{rr} = m_1 + m_2 has a direct physical meaning:

  • Mass m1m_1 is moving horizontally.2 Its radial component of velocity is r˙\dot{r}.

  • Mass m2m_2 is moving vertically, but its speed is also r˙\dot{r} (since the string length LL is fixed, z˙2=r˙\dot{z}_2 = \dot{r}).

Since the velocity of both masses is directly dependent on the r˙\dot{r} generalized velocity, and the velocity is linearly proportional to r˙\dot{r}, their inertias are fully additive in the radial direction. The generalized inertia for motion in the $r$ direction is simply the total mass of the system.

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