Do We Really Need to Reopen That Can of Ex-Mouse-Eating Maggots?
Denton said:
Suppose you have a very strong, spinning disc with a diameter of say 10 km in length. At the centre the centripetal velocity is approaching the speed of light, how would we observe the outer edge of the disc to be.
This is a FAQ; see for example
this Physics FAQ article and these previous PF threads:
- the locked thread rotational kinematics from April 2004,
- the thread [thread=149176]Spinning disk and the speed of light[/thread] from Dec 2006,
- the locked thread (about a closely related and also "faux-contentious" and long-ago resolved "paradox") [thread=153770] Why is the Wikipedia article about Bell's spaceship "paradox" disputed at all?[/thread] from January 2007,
- the very long and contentious thread [thread=168121] Stress-energy tensor of a wire under stress[/thread] (about stresses in a relativistically spinning hoop) from April 2007.
What dave said is correct and I hope that will satisfy all readers.
If not, to reformulate the question:
"What is the geometry of a relativistic spinning disk? Especially, a rigidly rotating disk? What is the physical experience of observers riding on the disk?"
Please understand that this is exactly the topic of a huge and mostly ill-informed/incorrect discussion* in the research literature since Ehrenfest first raised the subject in 1907. The discussion was resolved c. 1927 but bad physicists have kept the "debate" alive out of failure to read and understand prior work and failure to master now standard mathematical tools. As usual, Einstein's intuition (expressed in private correspondence) was basically correct, but he was smart enough to recognize that he lacked the relevant mathematical tools (in particular, the
kinematic decomposition of a certain non-geodesic
timelike congruence, the world lines of particles in spinning disk, or equivalently spinning cylindrical slug) required to most conveniently analyze the situation, and consequently shared his thoughts only with some close friends.
[*I exempt good review papers and good expositions from my criticism of the recent arXiv literature on this topic, since the issues were all resolved by about 1930, but bad/cranky eprints continue to appear, incorrectly claiming that "it's all perfectly simple" or that the mainstream explanations are incorrect.]
I stress that mathematically speaking, there is no doubt about what str predicts, but to understand the mainstream (mathematically correct!) analysis of what str predicts, one needs to be familiar with not only the kinematic decomposition but also
quotient manifolds versus
submanifolds, the existence of
multiple operationally significant notions of "distance in the large" even in flat spacetime, careful discussion of what we mean by "observe", and dozens of other topics which are probably too advanced for this forum.
As typically happens when someone reopens a can of worms, Denton, you have already committed several all-too familiar "errors of discourse" which would have to be patiently corrected in order to discuss this topic. To mention just one, you failed to specify that you are asking for the answer given by standard relativistic physics in flat spacetime (str), assuming that is what you had in mind. (Gtr is not required unless you believe--- largely incorrectly--- that gravitational phenomena are relevant here, but techniques often first encountered in gtr courses, such as the kinematic decomposition, are essential to avoid endless and pointless confusion over mathematical trivialities.)
See [thread=168121]this long PF thread[/thread] (which also discussed the closely related so-called "Ehrenfest's paradox" and "Bell's paradox", which are of course not paradoxical at all)--- in particular, please see my Post #27 in that thread, which warns
Chris Hillman said:
it's not nearly that simple!
Please see also the excellent book by Poisson,
A Relativist's Toolkit, Cambridge University Press, the quartet of Wikipedia articles in the versions I cited, and the invaluable review paper by Oyvind Gron in the book edited by Rizzi and Ruggiero,
Relativity in Rotating Frames, Kluwer, 1994.
DaleSpam said:
I think this question would require a relativistic version of Hooke's law in order to properly analyze
If you want to carefully compare rigidly spinning disks with different constant angular velocities (say \omega = 0 vice \omega=0.01), you will probably need to model a "spinup phase". This was extensively discussed in the thread just cited, but that discussion will go over the heads of anyone who has not mastered a good deal of relativistic physics at the research level. At the very least, I believe it is reasonable to demand that no-one discuss "relativistic spinup scenarios" who has not previously very carefully analyzed Newtonian spinup scenarios using the theory of elastic materials, and perhaps also "microscopic models" using Hooke's law (as I suggested in the cited thread).
Everyone:
please don't raise this subject again until you have at least carefully studied the sources cited above Plus kinematic decomposition (see the book by Poisson just cited) and the
Langevin congruence and other topics discussed in the cited thread. Pervect, myself, and greg egan all worked hard to clarify numerous conceptual subtleties which invariably cause confusion if they are not recognized and overcome, so naturally I at least have no wish to reslay the slain!
And everyone: please don't resurrect long-dormant threads, and
please don't illustrate the phenomenon discussed in [thread=200063]this thread[/thread]! Thanks to all in advance for their cooperation!