Lagrangian of Pendulum with Oscillating Hinge

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SUMMARY

The discussion focuses on deriving the Lagrangian for a pendulum with an oscillating hinge defined by the function ##y_0=f(t)##. The derived Lagrangian is given as ##\mathcal{L}=\frac{1}{2}m\left( l^2 \dot{\theta}^2 + \dot{y}^2_0(t) + 2 \dot{y}_0(t)l \dot{\theta} \sin\theta \right) - mg y_0(t)+mgl\cos\theta##. The challenge lies in modifying this Lagrangian to account for a time-varying gravitational field by introducing a gauge transformation ##\frac{d F(\theta,t)}{dt}##. The solution involves recognizing that part of the integral of the kinetic term can be expressed as ##-ml \dot{y_0(t)}\cos\theta##, allowing for the cancellation of extra terms through the gauge transformation.

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Xyius
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1.) The Problem Statement:

a.) Find the Lagrangian of a pendulum where the height of the hinge is oscillating in the y direction and is is defined as a function ##y_0=f(t)##

b.) Add a function (a gauge transformation) of the form ##\frac{d F(\theta,t)}{dt}## to the original lagrangian ##\mathcal{L}## to obtain a new lagrangian ##\mathcal{L}'=T'-V'## where ##T'## is the "usual kinetic energy of a pendulum" and ##V'## is the potential of a time varying gravitational field. Compare their Hamiltonians

2.) Relevant Equations

Lagranges equations

3.) Attempt at a Solution
Part a I got. The Lagrangian I got is the following. (I can go into more detail about how I got this if required)

\mathcal{L}=\frac{1}{2}m\left( l^2 \dot{\theta}^2 + \dot{y}^2_0(t) + 2 \dot{y}_0(t)l \dot{\theta} \sin\theta \right) - mg \dot{y}_0(t)+mgl\cos\theta

I know this answer is correct because for when ##y_0(t)=a\cos\omega t## it yields the equation of motion that is the same as the result in the text with a function of this form.

Part b is where I am stuck. When I see "potential of a time varying gravitational field," I think something of the form ##m g(t) y##. The only idea I can come up with is to write the function ##\frac{dF}{dt}## in a form that cancels out most of the terms of the original Lagrangian, but only keeps the kinetic term, ##\frac{1}{2}l^2\dot{\theta}^2## and other terms so that I can write the potential in the form I desire. But I cannot seem to make any headway with this, and I am very iffy on if this approach is correct or not. I think I understand the premise of the problem, instead of viewing the pendulum to have an oscillating hinge, instead cast the problem as a normal pendulum in an oscillating gravitational field. Does anyone have any thoughts or suggestions??
 
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Xyius said:
The only idea I can come up with is to write the function ##\frac{dF}{dt}## in a form that cancels out most of the terms of the original Lagrangian, but only keeps the kinetic term, ##\frac{1}{2}l^2\dot{\theta}^2## and other terms so that I can write the potential in the form I desire.

I think you have the right idea. You just need to play around with constructing the appropriate function F(θ,t). Take it one term at a time. For example, it is easy to construct a term in F such that dF/dt yields a term of the form ##mg\dot{y}_0##.
 
I made a typo in my original post, the one term at the end of the lagrangian should be ##mg y_0## not ##mg \dot{y_0}##.

I figured it out! I was correct in my reasoning as you pointed out, but the trick was to realize that part of the integral of the third term can be written in the form ##-ml \dot{y_0(t)}\cos\theta.## So you can re-write it in terms of it's integral and cancel out the extra terms by the gauge transformation.
 

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