QUESTION: An object of mass m is mounted in on a horizontal, massive rotating table within a tight-fitting (but frictionless) recessed groove as shown in the figure below. [NOTE: The necessity of the groove is to limit all acceleration to the radial direction. As the mass changes position in the track there will be a tangential forces acting against the mass but since it is constrained and the table is massive the rotation rate will remain unchanged (hence NO work will be done with respect to this action).]
To the mass a massless and inflexible string is tied and then passed through a frictionless hole in the center of the table. The other end of the string is tied to a second mass, M, which is hanging freely. The position the first mass is initially at a point, R, which produces an equilibrium configuration so that the second mass remains stationary. An infinitesimal radial displacement of the first mass (m) towards the center causes the second mass to descend.
What is the velocity of the first mass when it just reaches the hole in rotating table?
![\includegraphics [height=3.1in]{table_top_fig1.eps}](img1.gif)
At the end point the velocity of the first mass must go to zero
since the the tangential velocity in the track is proportion to the radius.
However since the two masses are tied together their final velocities must
be the same. The second mass (M) will have fallen to a height of
h-R.
The final relationship is therefore:
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or
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which is clearly wrong. The upshot of this is that non-inertial reference frames do not universally allow you to use the fact that a system experiencing conservative forces has the sum of the kinetic and the potential energies as a constant of the motion. (This is perhaps obvious if you cut the massless string and watch the first mass (m) fly off the rotating table gaining kinetic energy the entire time it is in the track.)
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with Fc = mv2/r. Notice that,
for the track, v (tangential) is a function of radial position.
This is not good. As a pre-step we need to relate v to the rotation
motion of the table. To do we need to relate the angular displacement of
the table,
,to
the velocity v. This is a ``two'' step argument:
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It is convenient to reference this integral to the center of the circle (were Fc is zero)
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and this sign convention signifies that centripetal ``potential'' energy is lost as an object moves from the center outward (the opposite of a gravitational potential).
For the two tethered masses we can, finally, write down a potential
energy expression with two terms
.
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At the initial equilibrium position (at R) F(r)=-dU(r)/dr=0
but the second derivative
is negative implying an unstable equilibrium. With this U(r)
above we can obtain the velocity of the two masses (radial component in
the case of mass m) at any radius along the track correctly in the
non-inertial reference frame. This expression can also be used in
the inertial frame as long as we are careful to not include tangential
componets of the velocity in the kinetic energy
term.