[Physics] Questions about the Jeans length

cosmologygravitational-collapsegravityuniverse

I have a couple of questions about the Jeans length. Suppose the universe has a homogeneous energy density, except there's a spherical region that is overdense.

  • I understand that if the region is smaller than the Jeans length, then pressure, which travels at the speed of sound (compared to the speed of gravity $c$), can build up fast enough to counteract the gravitational collapse. But if the region is bigger than the Jeans length, it collapses. What exactly does it mean? Does the region get smaller and smaller until it vanishes? Wouldn't this create a black hole, since you're stuffing all the energy of the overdense region into a smaller and smaller place?

  • Or, if the region is collapsing, wouldn't it eventually be smaller than the Jeans length, at which point it stops collapsing?

  • And what happens if the region is underdense, rather than overdense?

Best Answer

Not really my field, but I'll take a crack at it.

I understand that if the region is smaller than the Jeans length, then pressure, which travels at the speed of sound (compared to the speed of gravity c), can build up fast enough to counteract the gravitational collapse. But if the region is bigger than the Jeans length, it collapses. What exactly does it mean? Does the region get smaller and smaller until it vanishes? Wouldn't this create a black hole, since you're stuffing all the energy of the overdense region into a smaller and smaller place?

Notice that the expression for the Jean's length $$ \lambda = \sqrt{\frac{k_B T r^3}{G M \mu}}$$ depends on both the size of the region in containing the mass and temperature of the cloud.

It should be obvious that the if a region of the cloud is contracting then $r$ gets smaller while $M$ remains the same. You need one more fact: gravitational potential energy is being converted into thermal energ (i.e. largely the kinetic energy of the particles, see also the Virial Theorem).

The wikipedia article takes it up from there "It is only when thermal energy is not equal to gravitational work that the cloud either expands and cools or contracts and warms, a process that continues until equilibrium is reached."

Notice *"until equilibrium is reached"**.

Or, if the region is collapsing, wouldn't it eventually be smaller than the Jeans length, at which point it stops collapsing?

You've asked about the case from the wikipedia quote above where it contracts and warms. That said, if it gets warm enough it will lose energy relative it's surroundings by radiation, which means $T$ will drop and the cloud will again contract and warm. This continues until either the cloud stops behaving like a gas or the onset of fusion provides some new energy to keep the temperature up.

And what happens if the region is underdense, rather than overdense?

This is the case addressed above where it expands and cools.

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