The Scaler Curvature in the Cosmic Condensate

If you put these equations on a sphere, they wouldn't be satisfied if the t term had a zero expectation value. So it's fundamentally the scaler curvature that would coax the eve on the augmented torsion out of the vacuum to have a non zero level. If you pumped up that sphere and it smeared out the curvature, which you can't get rid of because of topological consider rations, let's say, from churn ay theory, you would have a very diffuse, very small term. And that term would be the term that was playing the role of the cosmological constant.