Simple Harmonic Motion/Period of a Physical Pendulum

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Discussion Overview

The discussion revolves around the period of a physical pendulum, focusing on the derivation of the period formula and the underlying principles of simple harmonic motion. Participants explore mathematical approaches, including differential equations and energy conservation, while also addressing practical applications and error analysis in experiments.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning
  • Experimental/applied
  • Homework-related

Main Points Raised

  • One participant presents a formula for the period of a physical pendulum derived from dimensional analysis, T=\sqrt{\frac{I}{mgb}}, and seeks to understand how to arrive at the full equation T=2\pi\sqrt{\frac{I}{mgb}}.
  • Another participant corrects a notation error regarding the use of \omega, indicating it should not be squared in the context discussed.
  • Several participants discuss methods for deriving the period, including solving second-order differential equations and using conservation of energy, with some noting the need for calculus knowledge.
  • There is confusion regarding the expression for angular frequency \omega and its relationship to the period, with participants questioning the derivation of \theta=A cos(\omega t).
  • One participant expresses a desire to learn how to prove solutions to differential equations related to the motion of the pendulum.
  • Another participant explains the relationship between torque, moment of inertia, and angular acceleration, leading to a second-order differential equation for the pendulum's motion.
  • A participant shares insights on the significance of the factor 2\pi in the period of simple harmonic motion and its connection to sine functions.
  • One participant seeks assistance with error calculations related to their experimental setup, mentioning uncertainties in measurements and how they affect the period formula.
  • Another participant suggests resources for understanding error analysis and propagation in measurements.

Areas of Agreement / Disagreement

Participants express varying levels of understanding regarding the derivation of the period formula and the role of angular frequency. There is no consensus on the best approach to proving the relationships discussed, and multiple methods are proposed. The discussion on error analysis also reflects differing levels of familiarity with the topic.

Contextual Notes

Some participants indicate limitations in their mathematical background, particularly in solving differential equations, which may affect their ability to fully engage with the derivations discussed. Additionally, there are unresolved questions about the application of error analysis to their specific experimental setups.

Kusu
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I'm studying the motion of a physical pendulum, could someone help me make the final step in figuring out how to find the period so I can make predictions before carrying out a practical? Basically I have a meter rule with holes drilled along the length and will be pivoting it at various points.

I've done lots of reading and watched lots of videos, I know simple calculus, I understand moment of inertia and torque, small angle approximations and parallel axis theory. I've done dimensional analysis which resulted in:

T=\sqrt{\frac{I}{mgb}}

where T = Period, I = Moment of inertia, m = Mass and b = distance from center of mass to pivot.

I know dimensional analysis doesn't give any constants, and I've seen in books that the actual equation is

T=2\pi\sqrt{\frac{I}{mgb}}

but I'd like to be able to prove this. I know it has to do with angular acceleration and angular frequency, but not sure how. Can anyone point me in the right direction? Most the videos I watch just make the jump and say "we've previously shown why... \omega^2=\sqrt{\frac{mgb}{I}} but I can't find any previous videos that show! :D
I think it's the \omega^2 that I can't see where it comes from.

Any help much appreciated!

K(p.s. If the Latex is messed up I'm probably working on fixing it, I've not used it much)
 
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You made a typo it should be ##\omega## not ##\omega^2##.
 
The easiest derivations of this result requires you to be able to solve a second order differential equation.
Another method using the conservation of energy requires you to solve a first - order differential equation, or equivalently solving a trigonometric integral like integral dx over square root of (a squared - x squared) with a constant. This is usually attacked about second semester calculus.
 
I've seen it written \omega^2 in several places though, what makes you say that? Here's a screen clipping of a video from (credit to Dan Fullerton on Youtube)

upload_2017-5-14_0-11-36.png
I don't know where \theta=A cos(\omega t) comes from either, but heard there are two uses for \omega in rotional motion?
 
Ah, I'm not at university. I know integration and differentiation, but don't know how to solve equations, I'll turn my attention there, thank you!
 
In general torque = moment of inertia times the angular acceleration = I alpha = I d / dt angular velocity = I second derivative of theta with respect to time.
This torque is also equal to Force ( - mg ) times moment arm (b sin theta). Now for small angles sin theta is approximated by theta, so the torque is -mgb theta.
equating the torques gives a second order differential equation for theta. I times second derivative (d 2 theta / d t squared) = - m g b times theta

Now most text "guess" the solution theta = A cos w t. (w is the frequency)

Then they show the second derivative of this solution using calculus is : d 2 theta / d t squared = - A w squared time theta.
we also have derivative (d 2 theta / d t squared) = - (m g b / I ) times theta
This allows us to make the identification of w squared with mgb / I
 
Thanks for all your input, I think I need to learn how to solve differential equations, or at least how to prove something is the solution of one. Probably the same thing :)

Just to clear up:
\tau=I\alpha
\tau=I\frac{d}{dt}\mbox{angular velocity (sometimes }\omega\mbox{)}
\tau=I\frac{d^2\theta}{dt^2}
Because of small angle approximations we can get rid of 'sin' in the calculation of the torque cased by mg:
\tau=-mgb\theta
Equating the torques gives
-mgb\theta=I\frac{d^2\theta}{dt^2}
rearranged to
\frac{d^2\theta}{dt^2}+\frac{mgb}{I}\theta =0

So what I need to do is learn how to prove that solving the above gives
\theta =A\cos \ \omega \ t\mbox{ (this time }\omega\mbox{ is frequency)}
and then learn how to show the second derivative of that is
\frac{d^2\theta}{dt^2}=-\frac{mgb}{I}\theta
which I can do from reading textbooks/videos?

(again, if the Latex is screwy I'm working on it :D )
 
Kusu said:
I've seen it written \omega^2 in several places though, what makes you say that? Here's a screen clipping of a video from (credit to Dan Fullerton on Youtube)

View attachment 203485I don't know where \theta=A cos(\omega t) comes from either, but heard there are two uses for \omega in rotional motion?

Is ##\omega^2=\sqrt{\dfrac{mgb}{I}}## correct ?

Sorry I don't know much.
 
Buffu said:
Is ##\omega^2=\sqrt{\dfrac{mgb}{I}}## correct ?

Sorry I don't know much.

it is ##\omega=\sqrt{\dfrac{mgb}{I}}##, that's because a general ##\alpha(t)=-\omega^2*x(t)##
 
  • #10
If you are specifically interested in where the factor of 2\pi comes into play, have a look at a simple harmonic motion where the displacement s(t) is described by a sine function.

T is the period of the motion, so we need to have s(T) = s(0). Since the period of the sine is 2\pi, this number needs to be involved somehow. Now check that the following ansatz
s (t) = A \sin\left(\frac{t}{T} 2\pi\right)
has the desired properties: as t goes from 0 to T, the argument for the sine goes from 0 to 2\pi (sketching the function may help).

From this, you see that \omega = \frac{2\pi}{T}.
 
  • #11
Thanks to everyone that commented, it's starting to make much more sense now I've been reading up and done some kitchen practicals! Think I'll have a nice grasp soon. Buffu, I see what you mean with my typo now in post #1, I'd mixed the two equations together, even the screenshot I posted in post #3 showed I was wrong! Kith and mpresic you've been really helpful.

We had a lot of fun doing the practicals and we're now trying to get a practical as close as possible to the prediction. Materials and fabrication have helped a lot :) , but could someone help me with error calculations? I watched a Walter Lewin video where he talks about a simple pendulum, and the uncertainty in the length being 1%, and once the root is taken it becomes 0.5%. My equations is much more complicated, I have simplified T=\sqrt{\frac{I}{mgb}} to cancel the mass, and include the parallel axis theorem, giving T=\sqrt{\frac{L^2+12b^2}{12gb}}

Is there a simple explanation as to what to do with my percentage errors in measurement? I have the uncertainty of L to be 0.1% and b varies so will need to be calculated at each pivot point, but I'm sure will follow 1 rule for any position?
 
  • #12
There's the general formula and many special cases. A superb text about this is "An introduction to error analysis" by Taylor. Or search for things like "gaussian error propagation" or "error analysis introductory lab".
 
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