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So let's ignore the results for a moment, and instead let's think about the assumptions. Are the assumptions that guided the development of the equations applicable at infinity?farolero said:im not even sure if those equations are valid for a mid point i would have to see the result
Are you talking about an infinitely long tube or about the behavior of the system a long time after the astronauts leave the end of the tube? I had thought that the length of the tube was fixed to a couple of meters and you were discussing the behavior of the system as the astronauts fly off to infinityfarolero said:if there's a slight rotation of the tube angular momentum would be infinite as the arm is infinitely long
Yes, but there are also other constraints that are important to reducing the number of variables.farolero said:I think that going the astronauts in opposites senses limits the degrees of freedom of the system
Dale said:Are you talking about an infinitely long tube or about the behavior of the system a long time after the astronauts leave the end of the tube?
That is not a correct equation. The angular momentum of the system is not equal to ##m \omega R^2##. The angular momentum of the system includes the angular momentum of the tube as well as the angular momentum of the astronauts.farolero said:I understand your point fully that L=6.6=mwR2 where m is the mass of the astronauts w is the rotational speed of the tube and R its the distance to the center of the tube of the astronauts but I do not see where it is wrong.
That is allowed, certainly. But it is a different problem than you had proposed. In this modified setup, you are correct that the rotation rate of the tube must decrease toward zero as the astronauts recede toward infinity if angular momentum is to be conserved.farolero said:Well I imagine a 2 m long tube of 2kg and along it till infinity a massless force field, i hope this is allowed.
jbriggs444 said:My suspicion is that @farolero is under the impression that angular momentum has something to do with an instantaneous center of rotation rather than with an arbitrary fixed reference point or axis. But, I am having a an extremely difficult time making sense of his claims.
You are mistaken. The center of the system (like any other point whatsoever) is perfectly valid to take as the reference point for calculation of angular momentum. Nothing impossible results. @Dale would certainly agree.farolero said:Think that in the beginning of the discussion taking arbitrarily the center of the system as center of reference failed to explain the relation between tangent and normal accelerations and the astronaut G forces that he feels and doing this lead Dale to consider it an imposible motion.
jbriggs444 said:You still have not bothered to write down the formula for the total angular momentum of the system in terms of m, R, I and ##\omega## that I asked for some 50 posts ago.
jbriggs444 said:That is allowed, certainly. But it is a different problem than you had proposed. In this modified setup, you are correct that the rotation rate of the tube must decrease toward zero as the astronauts recede toward infinity if angular momentum is to be conserved.
As I had written previously:farolero said:It is not that I have not bother, it is that I have tried but I have not been able to, I just don't know how to put the moment of inertia of the tube in function of the radius of the astronaut, I took last physics five years ago, I am too rusty.
It is a different problem because you are considering what happens after the astronauts have receded toward infinity. If there is a force field extending to infinity, that ties the rotation of the tube to the motion of the astronauts. If there is no such field, the rotation of the tube is not tied to the motion of the astronauts after they drop out of the ends of the tube.If tubes rotation is zero then angular momentum is zero, either way you take it there's trouble.
And it is not a different problem is solving a centrifugal gravity problem similarly to real gravity problem
In this problem you can NOT take an arbitrary center of reference as the center of the spiral for it would lead to contradictions:
It seems that you have never taken your mathematics education as far as a course on real analysis. Or perhaps your last mathematics course was taken long ago.farolero said:If tubes rotation is zero then angular momentum is zero, either way you take it there's trouble.
You assert that a proportion applies, but you continue to refuse to write down the formula that could confirm or deny that assertion. I will save you some time. The assertion is false. There is no inverse proportion.farolero said:I see thanks for pointing me to the Galilean Invariance and allow me to go back to the orginal question that seems to not have been cleared up yet:
A pilot is on artificial gravity free fall along a tube that decreases its rotational speed in proportion to the pilot radius, that is, when the pilot radius doubles w halfs.
That is meaningless gibberish. Further, the acceleration of the astronauts as they fall through the tube most definitely has a non-zero component normal to the walls of the tube.Analizing this problem from the center of the spiral acounting for galileo invariance the normal acceleration is zero for he is in centrifugal gravity free fall.
I am not sure what you mean. If the tube is 2 m long then how can there be anything "along it till infinity". If the tube is 2 m long then anything that is along the tube can only be 2 m long also, otherwise it is beyond the tube.farolero said:Well I imagine a 2 m long tube of 2kg and along it till infinity a massless force field, i hope this is allowed.
I took this to mean that only the center 2m of the tube has mass. The rest of the tube is rigid but massless.Dale said:I am not sure what you mean. If the tube is 2 m long then how can there be anything "along it till infinity".
Ah, yes, I agree. If that is what he meant then it is no particular problem to analyze. Indeed, it makes it easier than a finite tube.jbriggs444 said:I took this to mean that only the center 2m of the tube has mass. The rest of the tube is rigid but massless.
That is, despite being infinitely long, the tube has a finite moment of inertia. Depite being physically unrealizable, this understanding of the problem poses no particular problem for classical Newtonian physics.
It would greatly help if you would pose just one scenario and stick with that one scenario until you have finished it. In this thread I count at least 3 scenarios that you jump between with no warning and without finishing the previous one. It is very confusing for your respondents.farolero said:allow me to go back to the orginal question that seems to not have been cleared up yet
Let me tweak that a bit to account for the fact that there are two astronauts.farolero said:I think i have the formula you want:
L of the tube=Iw , L of the astronaut=mwR2
So Ltotal=lw+mwR2
Excellent. I look forward to seeing that result.From there i could calculate the w at R=1 and obtained clockwise speed as you kindly pointed to me.
Excellent. So, from this since ##L=I \omega + 2 m \omega R^2## and since L is conserved we can immediately see that if ##R## increases then ##\omega## must decrease. In fact, without even solving for ##R(t)## as a function of time we can still describe the behavior of ##\omega## as ##R## increases without bound.farolero said:So Ltotal=lw+mwR2
I can post that later today when I return home where my notes are. I knew that the conservation of angular momentum was "supposed" to fall out automatically, and it was nice to see that it did.jbriggs444 said:[Note that I'd be interested in seeing how Dale's formula for energy plays out. I have never played with the Lagrangian formulation of classical mechanics.]
See the "link" Problem 1: https://www.physicsforums.com/threads/micromass-big-october-challenge.887447/Charles Link said:To comment on the first post above, to get an object moving in a spiral path, you can apply a normal (perpendicular to direction of travel) force that increases linearly with time. In this case, the object will spiral inward and maintain a constant speed. Alternatively, to spiral outward at constant speed, you simply decrease the normal force at a linear (with time) rate.
So, since there is no potential energy the Lagrangian is equal to the kinetic energy and can be written (trying to be consistent with @farolero's variables as much as possible):$$\mathcal L = \frac{1}{2} I \dot{\theta}{}^2+m(\dot{R}{}^2+R^2 \dot{\theta}{}^2)$$ where ##I## is the moment of inertia of the tube, ##m## is the mass of one astronaut, ##R## is the distance of the astronauts from the center, and ##\omega=\dot{\theta}## is the angular velocity of the system.jbriggs444 said:[Note that I'd be interested in seeing how Dale's formula for energy plays out. I have never played with the Lagrangian formulation of classical mechanics.]
@Dale I think you need a 1/2 factor on your ## m ( \dot{R}^2+R^2 \dot{\theta}^2) ## term to get the kinetic energy for the Lagrangian. The term in parenthesis is ## v^2 ## in polar coordinates.## \\ ## editing: Please ignore. You have it correct=I see there are two astronauts, each of mass ## m ##.Dale said:So, since there is no potential energy the Lagrangian is equal to the kinetic energy and can be written (trying to be consistent with farolero's variables as much as possible):$$\mathcal L = \frac{1}{2} I \dot{\theta}{}^2+m(\dot{R}{}^2+R^2 \dot{\theta}{}^2)$$ where ##I## is the moment of inertia of the tube, ##m## is the mass of one astronaut, ##R## is the distance of the astronauts from the center, and ##\omega=\dot{\theta}## is the angular velocity of the system.
Then the Euler-Lagrange equation for ##\theta## is $$ \frac{d}{dt}\left( \frac{\partial \mathcal L}{\partial \dot{\theta}} \right) = \frac{\partial \mathcal L}{\partial \theta}$$ $$ \frac{d}{dt}\left( I \dot{\theta} + 2 m R^2 \dot{\theta} \right) = 0$$ $$ I \dot{\theta} + 2 m R^2 \dot{\theta} = L$$ which is our expression for the conserved angular momentum, ##L##, but obtained automatically from the Lagrangian.
Then the Euler-Lagrange equation for ##R## is $$ \frac{d}{dt}\left( \frac{\partial \mathcal L}{\partial \dot{R}} \right) = \frac{\partial \mathcal L}{\partial R}$$ $$ 2m\ddot{R} = 2 m R \dot{\theta}{}^2$$ combining that with the expression for angular momentum and simplifying we get the equation of motion $$\ddot{R}=\frac{L^2 R}{(I+2mR^2)^2}$$