- #1
Weran
- 8
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I was discussing a problem related to Einstein's universe model. As we all know its an unstable equilibrium. So a small fluctuation in the density would result in an either expanding or contracting universe. However, I read that
"There are static and stable solutions in Newtonian gravity theory: stars, planets, etc... Even large nebulae. The Newtonian universe could be a large spherical ball in a state of stable equilibrium. The instability occurs mainly when you assume an infinite distribution of homogeneous matter, and even there, the potential is ill-defined. The theory breaks down at this point, and we can't use the math to show anything."
How can the Newtonian spherical ball be in stable equilibrium? What's the difference between this and Einstein's Universe model?
"There are static and stable solutions in Newtonian gravity theory: stars, planets, etc... Even large nebulae. The Newtonian universe could be a large spherical ball in a state of stable equilibrium. The instability occurs mainly when you assume an infinite distribution of homogeneous matter, and even there, the potential is ill-defined. The theory breaks down at this point, and we can't use the math to show anything."
How can the Newtonian spherical ball be in stable equilibrium? What's the difference between this and Einstein's Universe model?