Time taken to slide down a circular path (with friction)

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SUMMARY

The discussion focuses on solving the time taken to slide down a circular path with friction, specifically avoiding the conservation of energy principle. Participants suggest using differential equations, with the correct formulation being $$R\ddot \theta = g\cos \theta - \mu \frac{N}{m}$$, where $$N = mg\sin \theta + mR\dot \theta^2$$. The conversation emphasizes transforming the second-order differential equation into a first-order linear form through substitutions, ultimately aiming to express angular velocity as a function of angle, $$\omega(\theta)$$.

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  • Understanding of differential equations, particularly second-order and first-order linear ODEs.
  • Familiarity with kinematic equations and angular motion concepts.
  • Knowledge of frictional forces and their impact on motion.
  • Proficiency in calculus, specifically the chain rule and variable substitution techniques.
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eddiezhang
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Homework Statement
A point mass (m) is acted on by gravity, the normal force, and friction (μN). It starts at the point A(0,1). It then slides down a circular 'ramp', stopping when it touches the x-axis at B(1,0). It does not leave the surface of the ramp.

Find the general time of descent.
Relevant Equations
Centripetal force, friction etc.
This is for a math report that I'm supposed to write, which means I'm not supposed to use conservation of energy. This makes life much harder... so please bear with me. I am interested to see how you'd solve this purely kinematically though (if it can be solved that way).

Please tell me if this is posted to the wrong place. I asked a similar question in a math forum to no luck (they told me to post on a physics forum, so here I am).

Attached is a pdf with some diagrams and my working.

Thanks so much for your help,
Ed
 

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My first thought is that I'd be surprised if this has a closed form solution. Especially with friction involved.

Conservation of energy would give you the final speed, but not the time.
 
Your differential equation is almost correct. The mass must cancel completely from the equations. And, by taking a dimensionless unit as radius, your equation has become dimensionally suspect. Better to take the radius as ##R##.
 
PS if you take ##\mu =0## you'll see that you may have got sines and cosines mixed up as well.
 
After you fix it up. You can make it first order-linear if you do a few variable substitutions.

First ## \dot \theta \to \omega ##, Then ## \ddot \theta \to \dot \omega ##

The you use anther sub like ## u = \omega^2 ## and its implications for the derivative ## \frac{du}{d \theta}## via the Chain Rule.

It doesn't get you time, but I think it gets something analytical... which is a step in the right direction? It's at least a worthy exploration in its own right.

EDIT: it might even get you time via ## \omega ( \theta) = \frac{d \theta}{dt}##. Its surely going to be a fight(which is what you are looking for).
 
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PS with ##\mu =0## the problem reduces to a pendulum. Without the small angle approximation, the solution involves elliptic integrals.
 
PeroK said:
PS with ##\mu =0## the problem reduces to a pendulum. Without the small angle approximation, the solution involves elliptic integrals.

So bad news for ##t##? But still plenty of material for exploration in the report.
 
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PeroK said:
PS if you take ##\mu =0## you'll see that you may have got sines and cosines mixed up as well.
oops :oops: that's pretty embarrassing. I take it the correct DE is gcos(φ) - φ'' = μ(φ')^2 +μgsin(φ)?
 
eddiezhang said:
oops :oops: that's pretty embarrassing. I take it the correct DE is gcos(φ) - φ'' = μ(φ')^2 +μgsin(φ)?
The differential equation must be (I'll use the more standard ##\theta## for the angle.
$$R\ddot \theta = g\cos \theta - \frac{F_f}{m} = g\cos \theta - \mu \frac N m$$Where ##F_f## is the frictional resistance and ##N## the magnitude of the normal force. And, we must have:
$$N = mg\sin \theta + mR\dot \theta^2$$That gives you:
$$\ddot \theta = \frac g R(\cos \theta - \mu \sin \theta) - \mu\dot \theta^2$$Which is what you have, given the missing ##R##.
 
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  • #10
erobz said:
After you fix it up. You can make it first order-linear if you do a few variable substitutions.

First ## \dot \theta \to \omega ##, Then ## \ddot \theta \to \dot \omega ##

The you use anther sub like ## u = \omega^2 ## and its implications for the derivative ## \frac{du}{d \theta}## via the Chain Rule.

It doesn't get you time, but I think it gets something analytical... which is a step in the right direction? It's at least a worthy exploration in its own right.

EDIT: it might even get you time via ## \omega ( \theta) = \frac{d \theta}{dt}##. Its surely going to be a fight(which is what you are looking for).
I think I follow the chain rule part - would I be correct in saying ## \frac{du}{d \theta} =2\ddot{\theta}##?

You may need to walk me through the rest of that approach... how exactly do you get it first-order linear? Similarly, if you start me off on the ## \omega ( \theta) = \frac{d \theta}{dt}## thing I'd be more than happy to try and bash out the rest of the algebra myself.

Thanks so much
 
  • #11
eddiezhang said:
I think I follow the chain rule part - would I be correct in saying ## \frac{du}{d \theta} =2\ddot{\theta}##?

You may need to walk me through the rest of that approach... how exactly do you get it first-order linear? Similarly, if you start me off on the ## \omega ( \theta) = \frac{d \theta}{dt}## thing I'd be more than happy to try and bash out the rest of the algebra myself.

Thanks so much
Use chain rule on ##\frac{d \omega}{dt}## to switch to ##\theta## as the independent variable (keep in terms of ##\omega## for the dependent)Once you see the trick you won’t forget it.
 
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  • #12
erobz said:
Use chain rule on ##\frac{d \omega}{dt}## to switch to ##\theta## as the independent variable. Once you see the trick you won’t forget it.
Attempt:

##\frac{d \omega}{dt} = \frac{d \omega}{d\theta} \times \frac{d \theta}{dt} = \omega \frac{d \omega}{d\theta}##

Am I barking up the wrong tree?

I'll probably kick myself hard, but I'm just not seeing it yet...
 
  • #13
eddiezhang said:
Attempt:

##\frac{d \omega}{dt} = \frac{d \omega}{d\theta} \times \frac{d \theta}{dt} = \omega \frac{d \omega}{d\theta}##
That’s it.
 
  • #14
haruspex said:
That’s it.
Oh yay!

OK so looking at the DE again:

##\ddot{\theta} = \frac{g}{R} \left( \cos\theta - \mu \sin\theta \right) - \mu \dot{\theta}^2##

##\dot{\theta}## substitutes out directly, but how do I deal with ##\ddot{\theta}##? Plus don't the trig terms still make it non-linear?

Edit: I don't have much experience with ODEs - you can probably tell.
 
  • #15
eddiezhang said:
, but how do I deal with ##\ddot{\theta}##?
Using your formula in post #12.
 
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  • #16
eddiezhang said:
Oh yay!

OK so looking at the DE again:

##\ddot{\theta} = \frac{g}{R} \left( \cos\theta - \mu \sin\theta \right) - \mu \dot{\theta}^2##

##\dot{\theta}## substitutes out directly, but how do I deal with ##\ddot{\theta}##? Plus don't the trig terms still make it non-linear?

Edit: I don't have much experience with ODEs - you can probably tell.
It linear ODE by my understanding of classification. The ODE will no longer have nonlinear terms in the dependent variable.

$$ y’ + p(x)y = f(x) $$

Trig functions in ##x## as don’t change the classification to non-linear. They can make the integration harder.
 
  • #17
haruspex said:
Using your formula in post #12.

True.
OK... I'm not sure how exactly:

##\ddot{\theta} = \frac{d}{dt} (\omega \frac{d \omega}{d\theta})##

Bear with me because I haven't done much calculus... multiplying infinitesimals still gives me the heebie-jeebies. Is this right?

##\ddot{\theta} = \frac{d\omega}{dt} \times \frac{d \omega}{d\theta} = \omega (\frac{d \omega}{d\theta})^2##
 
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  • #18
eddiezhang said:
OK... I'm not sure how exactly:

##\ddot{\theta} = \frac{d}{dt} (\omega \frac{d \omega}{d\theta})##

Bear with me because I haven't done much calculus... multiplying infinitesimals still gives me the heebie-jeebies. Is this right?

##\ddot{\theta} = \frac{d\omega}{dt} \times \frac{d \omega}{d\theta} = \omega (\frac{d \omega}{d\theta})^2##
if thats how you want to think about it - not saying it’s mathematically sound- does that eliminate time?
 
  • #19
erobz said:
if thats how you want to think about it - not saying it’s mathematically sound- does that eliminate time?
It does... I see. OK I'll see if I can solve the ODE with the subs. and (maybe?) get the time of descent (too optimistic?)
 
  • #20
You have
eddiezhang said:
##\ddot{\theta} = \frac{g}{R} \left( \cos\theta - \mu \sin\theta \right) - \mu \dot{\theta}^2##
and of course
##\dot\theta=\omega, \ddot{\theta} =\dot\omega##,
and
eddiezhang said:
##\frac{d \omega}{dt} = \frac{d \omega}{d\theta} \times \frac{d \theta}{dt} = \omega \frac{d \omega}{d\theta}##
Substitute as necessary to get an equation relating ##\theta, \omega, \frac{d\omega}{d\theta}##.
 
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  • #21
eddiezhang said:
It does... I see. OK I'll see if I can solve the ODE with the subs. and (maybe?) get the time of descent (too optimistic?)
Just to be clear, I’ll just give you this to be sure.

$$\ddot \theta = \frac{d\omega}{dt} = \frac{d\omega}{d \theta} \frac{d\theta}{dt} = \frac{d\omega}{d \theta}\omega $$
 
  • #22
If you can get time, not saying that’s the case it would go through ##\omega## as a function of ##\theta##. So finding that is your immediate goal.
 
  • #23
Well, let’s just make sure you get the right ODE first.
 
  • #24
erobz said:
Just to be clear, I’ll just give you this to be sure.

$$\ddot \theta = \frac{d\omega}{dt} = \frac{d\omega}{d \theta} \frac{d\theta}{dt} = \frac{d\omega}{d \theta}\omega $$
Oh wait 🤦‍♂️I don't know why I worded it that way but it's literally just the chain rule. Oops.

Thanks for the help so far... I might come back here if the algebra gets too rough.
 
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  • #25
erobz said:
Well, let’s just make sure you get the right ODE first.
So ##\dot{\theta} = \omega## and ##\ddot{\theta} = \omega \frac{d\omega}{d\theta}## (I was clearly having a brain fart before with this part)

Substituting into ##\ddot{\theta} = \frac{g}{R} \left( \cos\theta - \mu \sin\theta \right) - \mu \dot{\theta}^2##

Produces ##\omega \frac{d\omega}{d\theta} = \frac{g}{R} \left(\cos\theta - \mu \sin\theta \right) - \mu \omega^2##

Which I should try solve to find ##\omega(\theta)##
 
  • #26
eddiezhang said:
So ##\dot{\theta} = \omega## and ##\ddot{\theta} = \omega \frac{d\omega}{d\theta}## (I was clearly having a brain fart before with this part)

Substituting into ##\ddot{\theta} = \frac{g}{R} \left( \cos\theta - \mu \sin\theta \right) - \mu \dot{\theta}^2##

Produces ##\omega \frac{d\omega}{d\theta} = \frac{g}{R} \left(\cos\theta - \mu \sin\theta \right) - \mu \omega^2##

Which I should try solve to find ##\omega(\theta)##
You still have another couple subs to make. What you have is still currently nonlinear.

Let ##u = \omega^2##

The take the derivative of ##u## wrt ##\theta##.

This is the step that converts it to linear ODE.
 
  • #27
erobz said:
You still have another couple subs to make. What you have is still currently nonlinear.

Let ##u = \omega^2##

The take the derivative of ##u## wrt ##\theta##.

This is the step that converts it to linear ODE.
Ah right...

##\frac{du}{d\theta} = \frac{d}{d\theta}\omega^2 = 2\omega \frac{d\omega}{d\theta} = 2\ddot{\theta}##

So the ODE turns into:
##\frac{1}{2} \times \frac{du}{d\theta} = \frac{g}{R} \left(\cos\theta - \mu \sin\theta \right) - \mu u^2##

And if I'm not mistaken, the strategy is to find u(θ) ##\rightarrow## find ω(θ) ##\rightarrow## see what happens from there wrt ##\frac{d\theta}{dt}##?
 
  • #28
eddiezhang said:
Ah right...

##\frac{du}{d\theta} = \frac{d}{d\theta}\omega^2 = 2\omega \frac{d\omega}{d\theta} = 2\ddot{\theta}##

So the ODE turns into:
##\frac{1}{2} \times \frac{du}{d\theta} = \frac{g}{R} \left(\cos\theta - \mu \sin\theta \right) - \mu u^2##

You made a sub for ##u## incorrectly in there.

And if I'm not mistaken, the strategy is to find u(θ) ##\rightarrow## find ω(θ) ##\rightarrow## see what happens from there wrt ##\frac{d\theta}{dt}##?

yea, first comes ##u(\theta)##
 
  • #29
eddiezhang said:
##\frac{1}{2} \times \frac{du}{d\theta} =##
Having eliminated t, I would simplify the notation by writing ##u'##.
eddiezhang said:
the strategy is to find u(θ) ##\rightarrow## find ω(θ) ##\rightarrow## see what happens from there wrt ##\frac{d\theta}{dt}##?
Yes, but generally the equation of velocity as a function of displacement is effectively the energy equation. Don’t be too hopeful about finding displacement as a function of time, or v.v., from there.
 
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  • #30
erobz said:
You made a sub for ##u## incorrectly in there.
Ooops. Just ##\mu u ## at the end, right?
 
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