Molecular Cloud Collapse - Help!

1. The problem statement, all variables and given/known data
To show how conservation of angular momentum applied to to a collapsing MC core implies flattening during cloud collapse consider the equation of motion of a parcel mass m in a rotating initially spherical cloud of total mass M, initial angular speed w0 and radius r0. Consider the acceleration experienced by a particle of mass (m) on the equator of a spherical cloud spinning about a vertical axis relative to that at the poles. You should be able to show that the inward acceleration is less at the equator than at the poles and hence the cloud will inevitably flatten in the equatorial plane during Jeans collapse.

2. Relevant equations
Show that the collapse of the cloud will stop in the plane perpendicular to its axis of rotation when the radius reaches rf = (w20r40)/GMr where M is the mass and w0 and r0 are the original angular velocity and radius of the surface of the cloud. Do this by balancing gravitational and centripetal forces so that a parcel of mass at the equator becomes weightless.

{Hints: (1) the equation of motion in this case is m(d2r/dt2) = -((GMrm)/r2) + mrcos(theta)w2 ; (2) angular momentum is conserved during collapse so that I0w0 = Iw, where I is the moment of inertia for a uniform sphere of mass M and radius r and theta is the colatitude = 90˚-latitude}

3. The attempt at a solution
So first of all, I'm not particularly sure what this is asking me to do. I'm trying to use the equations for gravitation and centripetal force to achieve the equation for the radius of when collapse stops:

Since the mass is at the equator, theta = 0, so cos(theta) = 1, therefore I get:

GMrm/r2 = mrw2

But I have no idea what to do from here... any thoughts? Thanks! Sorry for the long problem.
 

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