Newtonian- yeah I doubt Wikepedia to be the best source for this stuff, a bit outdated/subjective. They often use different notation. The Omega that you quote is indeed the density parameter, and is called Omga_M that which I was talking about before. <br /><br />Due to our present limitations, observations have only revealed Omega_M to be close to 1 with no great certainty. And in actuality it seems that, in looking at recent data, Omega_M might actually be slightly greater than 1. The problem with the argument that: Omega_M is 'close' to 1, and therefore is 1, and hence the universe is not accelerating, is: <br /><br />-If this were true, then Omega_k = 0 <br />-However, because we can only say that Omega_M is slightly larger than 1, or close to one, then we cannot say k is identically zero <br />-k tells us the geometry of the universe, open, closed and flat, the FLRW metric that all these equations come from, has this parameter in it<br />-k MUST be either 0, +ve or -ve, but we don't know how +ve or -ve it might/could be, chances are, that we could not conclude with any observables nowadays with enough certainty <br /><br />Also, to add to this, there are several models for which Omega_M ~ 1 throughout their evolution even though they are not spatially flat. The solution with Omega_M ~1, and closed universe, is not unique.<br /><br />Do you follow me? Sorry this stuff is really hard to explain without math...