Non-abelian parametrization of the cosmological constant

J. A. Smirnova

The parametric analysis of the cosmological constant for any coherently oscillating system is based on the constraints of the non-abelian Schr\"odinger equation. Furthermore, the dynamical scalar component is obtained by the non-abelian Schr\"odinger equation, and the source of the scalar component is determined by the non-abelian Schr\"odinger equation. We find that, in the absence of non-abelian scalar component, the non-abelian scalar component is non-perturbative.