On 5/14/15 7:53 AM, brad wrote:
In the early Universe there was essentially
an unlimited amount of matter available to carry away angular momentum
allowing much more massive objects to result before the developing
object could clear a volume around itself.

[[Mod. note -- As well as low angular momentum, collapse also needs
low internal pressure.

In these formation studies,
does vacuum viscosity come into play?

Ref1: http://arxiv.org/abs/0806.3165
Hydrodynamics of spacetime and vacuum viscosity

viscosity*entropy density = hbar/4pi

Richard D Saam