Special and General Relativity Special and General Relativity Physics Help Forum 
Aug 18th 2017, 02:56 AM

#1  Senior Member
Join Date: Nov 2013 Location: New Zealand
Posts: 534
 Am I doomed to never understand the relativistic rotating disk?
Ok, I am really out of my depth here so I am wondering whether I can get any mileage with this with just flat minkowski space with uniformly rotating polar coordinates and some vector calculus and linear algebra? (I'm really not good with tensors).
Is it worth me trying to understand some basic concepts about this now or do I really need "to climb the tensor mountain" to get there? Or can I do some "good enough" analysis with just some vector calculus and linear algebra?
I am basically trying to understand why, in rotating polar coordinates, that the circumference undergoes fitzgerald contraction but the radius does not and whether it annihilates the minkowski flat spacetime assumption.

 
Aug 18th 2017, 07:22 AM

#2  Physics Team
Join Date: Apr 2009 Location: Boston's North Shore
Posts: 1,491

Originally Posted by kiwiheretic Ok, I am really out of my depth here so I am wondering whether I can get any mileage with this with just flat minkowski space with uniformly rotating polar coordinates and some vector calculus and linear algebra? (I'm really not good with tensors).
Is it worth me trying to understand some basic concepts about this now or do I really need "to climb the tensor mountain" to get there? Or can I do some "good enough" analysis with just some vector calculus and linear algebra?
I am basically trying to understand why, in rotating polar coordinates, that the circumference undergoes fitzgerald contraction but the radius does not and whether it annihilates the minkowski flat spacetime assumption. 
I understand your dilemma since I too had a problem with it for a very long time until I realized the nature of the geometry.
First of all, the spacetime is flat regardless of the geometry. It's not possible to introduce spacetime curvature simply by changing from an inertial frame to a noninertial frame.
This problem is known as the Ehrenfest Paradox. It's described here with a possible resolution to the paradox given by Gron. https://en.wikipedia.org/wiki/Ehrenf...of_the_paradox
I have a solution that I'm considering at the moment myself. Its possible that the geometry changes from a surface of a flat disk to the surface of a cone. A cone, while having a different spatial geometry than the disk still has zero intrinsic curvature so its still flat in that sense.
Last edited by Pmb; Aug 18th 2017 at 07:31 AM.

 
Aug 18th 2017, 02:52 PM

#3  Senior Member
Join Date: Nov 2013 Location: New Zealand
Posts: 534

I notice they use a different metric tensor for rotating polar/spherical coordinates as opposed to straight Euclidean coordinates. Is this just "cosmetic" or does changing to a different metric tensor signify a warping of the manifold (if that's the correct term)?

 
Aug 19th 2017, 07:01 AM

#4  Member
Join Date: Dec 2012 Location: Boulder, Colorado
Posts: 64

You're making it a lot harder than it needs to be. When viewed from the inertial frame with spatial origin at the center of the disk (but not rotating with it), basic SR says that there will be length contraction along the direction of the motion, but no length contraction in the direction perpendicular to the motion. So in the direction parallel to the circumference of the circle, there will be length contraction, but along the radius, there will be no length contraction. The length contraction along the circumference means that it takes more yardsticks laid out (and stationary wrt the disk) along the complete circumference that there would be if the disk weren't rotating. But the number of yardsticks laid out (and stationary wrt the disk) along a radius will be the same with or without rotation of the disk. If the disk weren't rotating, the ratio of the number of circumference yardsticks to the number of radius yardsticks would be 2pi, but when rotating, the ratio is greater than 2pi. That's when Einstein realized that, according to the creatures at rest on the disk (and who believe that the disk is stationary in a very weird gravitational field), their geometry isn't Euclidean. And Einstein realized then that his general relativity theory would have to utilize nonEuclidean geometry.
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Aug 19th 2017, 01:36 PM

#5  Senior Member
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That's kind of a mind bender though. What would an observer see while looking at that given that we can only see 3 dimensions?

 
Aug 19th 2017, 03:56 PM

#6  Member
Join Date: Dec 2012 Location: Boulder, Colorado
Posts: 64

You're still misunderstanding what it is that makes the rotating disk thoughtexperiment important. Einstein thought up the rotating disk scenario right after he finished his special relativity. At that point, he knew no general relativity at all. The significance of the rotating disk scenario is twofold:
First, it allowed him, using only SR, to determine that the ratio of the number of yardsticks required to fill up the circumference, to the number of yardsticks required to fill up a radius, does not equal 2pi. That conclusion only requires knowledge of the length contraction result of SR.
Second, Einstein used the equivalence principle to tell him what creatures who occupied fixed positions on the disk (and who were entitled to insist that they were motionless) would conclude about their situation. Einstein knew that they would insist that they were NOT accelerating (because they are motionless), but instead are experiencing a gravitational force directed radially outward, which increases in strength in direct proportion to their distance from the center of the disk. (The equivalence principle (in its simplest form) says that someone in an enclosed box can't tell if he's being accelerated at 1g upward in no gravitational field, or else being motionless in a constant, uniform 1g gravitational field.) And those creatures would then conclude that something about that strange radial gravitational force that they could feel was associated with the fact that the geometry of their world was nonEuclidean. (The creatures knew that their world was nonEuclidean, because they could see that there were more yardsticks required to fill up the circumference than there would be if their geometry were Euclidean).
The important thing is that Einstein knew at that moment that his general theory of relativity (which he didn't know anything else about at that moment) would have to involve nonEuclidean geometry. So his first job in arriving at his general theory of relativity was to learn nonEuclidean geometry. Fortunately, a very good friend of Einstein's (Marcel Grossman), from his undergraduate days at the Zurick Polytechnical school, was now a professor of mathematics at that same school, and Marcel had written his PhD thesis on nonEuclidean geometry! Marcel was instrumental in helping Einstein learn the nonEuclidean geometry that was required to arrive at his GR theory (and Marcel continued to help with the math right up until the final field equations were determined).
Where you're going wrong is in thinking that you need to apply GR to the rotating disk scenario. You don't. You only need SR and the equivalence principle ... that's all that Einstein had at that point, and his solution was critical in pointing him in the right direction to ultimately get to his GR theory.
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Mike Fontenot

 
Aug 19th 2017, 04:45 PM

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So, if I understand you correctly, we can just add in minkowski space and set it to a rotating polar coordinate system so all we need is the standard polar coordinate vector calculus expression $\displaystyle \mathbf{\ddot{r}}= (\ddot{r}  r \dot{\phi}^2)\mathbf{\hat{r}} + (r \ddot{\phi}+2 \dot{r}\dot{\phi})\hat{\mathbf{\phi}}$ to make the disk appear to be stationary with respect to an observer ??

 
Aug 20th 2017, 07:09 AM

#8  Member
Join Date: Dec 2012 Location: Boulder, Colorado
Posts: 64

Originally Posted by kiwiheretic So, if I understand you correctly, we can just add in minkowski space and set it to a rotating polar coordinate system so all we need is the standard polar coordinate vector calculus expression $\displaystyle \mathbf{\ddot{r}}= (\ddot{r}  r \dot{\phi}^2)\mathbf{\hat{r}} + (r \ddot{\phi}+2 \dot{r}\dot{\phi})\hat{\mathbf{\phi}}$ to make the disk appear to be stationary with respect to an observer ?? 
You don't need to do ANYTHING beyond what I've already specified. The stationary observer at the center of the rotating disk (who is not rotating wrt the disk) just computes the centripetal acceleration v*v/r acting on a creature fixed at a point on the disk. The creature perceives a force of that same magnitude that is pulling him radially outward (called the centrifugal force). Since v = omega*r, v*v/r = omega*omega*r, so the perceived centrifugal force increases linearly with the distance from the center of the disk. The creatures conclude that they are under the influence of a strange gravitational field that causes that force.
The creatures on the disk don't NEED any mathematical equations of motion, because they aren't (in their opinion) moving. They are entitled to insist that they are stationary. If they DO decide to move on the surface of the disk, it is a very slow and irregular movement that requires no equations or formalism. For example, they can cooperate among themselves to slowly lay out the yardsticks along the circumference of the disk and along some radius extending out to that circumference. Or they can slowly lay out yardsticks along any circle of any radius on the disk ... they need no equations or mathematical formalism to do those things. And once they have done those things, they can conclude (without any further help) that in their world, the ratio of a circumference to the corresponding radius ISN'T 2pi (it's greater than 2pi), and therefore that the geometry of their world ISN'T Euclidean. THAT is the critically important result that this example gave to Einstein. It established a constraint that the (at that time) unknown general theory of relativity HAD to satisfy, and it pointed Einstein in the right direction to (eventually) formulate that theory.
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Mike Fontenot

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