Pendulum in polar coordinate system problem

AI Thread Summary
The discussion focuses on solving the dynamics of a pendulum in a polar coordinate system, specifically addressing the displacement of the particle and the tension force in the thread. The user, Mikael, initially attempted to apply Newton's second law but struggled with the transition to polar coordinates, particularly the use of vectors and their derivatives. Responses clarified that in polar coordinates, position is described using the radius and angle, and emphasized the importance of decomposing forces into radial and tangential components. The correct approach involves setting up the equations of motion in terms of the angle, leading to a differential equation for the angular displacement. Overall, the conversation provided guidance on how to properly apply polar coordinates to analyze the pendulum's motion.
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Homework Statement


A pendulum consists of a particle of the mass m and a thread of the length l (we don't consider the threads mass). The acceleration caused by gravity is g. Solve the particles displacement and the force caused by the tension in the thread T in a polar coordinate system. The pendulums oscillations are of small amplitude. What is the period of the particle?


Homework Equations


NII: \sumF=ma
sin\theta=\theta
T=2\pi\sqrt{}(l/g)

The Attempt at a Solution



First of all I'd like to introduce myself. My name is Mikael, and I have recently started studying at Helsinki University of Technology. One thing that causes me a fair bit of difficulties is that Swedish is my native language, and all the lessons are in Finnish. I read the most advanced physics and maths courses the University offer, and it's been quite tough. Now here's my attempt at a solution:

I started by drawing a picture with all the forces and the components where needed, in this case I chose to keep T and divided mg into mgsin\theta in the direction of x and mgcos\theta in the direction of y. I applied NII so that

-mgsin\theta=max.
m disappears and I wrote a as seen below, which leads to

d2x/dt2=-gsin\theta.
After integrating twice I had

x3/6=-1/2*gsin\thetat2, but since

sin\theta=\theta

x=\sqrt[]{}3-3g\thetat2

At this point, I had a look at the tips and tricks one of our teachers gave us, and it looked nothing like this. He had used the vectors r and e\varphi, and lots of dots above them, that I don't even know what they mean. I started to think that maybe the polar coordinate system means I must write the answers with these vectors, but I have no idea how to do that, because the tips made no sense to me at all. Therefore, what I first of all want to know, is wath is the correct way to give the answer. Can I do as I have done, or is it completely wrong. If I'm wrong I appreciate all help because I'm not even sure what a polar coordinate system is. So some help to get me started would be great in that case. Thank you for your time!
 
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Hi mkerikss! :smile:

(have a theta: θ and a phi: φ and a pi: π and a square-root: √ and a sigma: ∑ :wink:)
mkerikss said:
… Solve the particles displacement and the force caused by the tension in the thread T in a polar coordinate system.

I started by drawing a picture with all the forces and the components where needed, in this case I chose to keep T and divided mg into mgsin\theta in the direction of x and mgcos\theta in the direction of y.

At this point, I had a look at the tips and tricks one of our teachers gave us, and it looked nothing like this. He had used the vectors r and e\varphi, and lots of dots above them, that I don't even know what they mean.

(dots are the same as dashes … they mean d/dt :wink:)

The question asks you to use a polar coordinate system …

so position is (r,θ), and velocity is measured along the local directions er and eθ

er is the unit vector along the r direction, and eθ is the unit vector perpendicular to er, in the direction of increasing θ.

Also, (er)' = θ'eθ, and (eθ)' = -θ'er

Then, for example, r = rer, and so r' = rθ'eθ, and r'' = … ? :smile:
 
Polar coordinates:

http://en.wikipedia.org/wiki/Polar_coordinate_system"

instead of x and y you use r: distance from origin and \phi angle from a fixed direction.

you use this with problems that deal with rotation. problems will often be easier when converted to polar coordinates

In the case of a pendulum, r always the length of the pendulum, so you only have to deal with a differential equation for phi. phi =0 corresponds to straight down.
you have to split the force of gravity on the particle in a component in the direction of the origin (the r direction) and a component in the direction tangential to the arc that the particle makes. Only this component works in the phi direction. you get

F_{tangential} = m r \frac {d^2\phi} {dt^2}

instead of F=ma
 
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Thanks for all the help, I'll give it another try. At least now I understand what it's all about :smile:
 
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