Combining gravity with the forces of the standard model on a cosmological scale

Details Combining gravity with the forces of the standard model on a cosmological scale Combining gravity with the forces of the standard model on a cosmological scale

2010-03-22

arxiv.org/abs/1003.4246v6

Class.Quant.Grav.27:155008,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

53 pages, v6: some typos corrected

Scientific paper

10.1088/0264-9381/27/15/155008

We prove the existence of a spectral resolution of the Wheeler-DeWitt equation when the underlying spacetime is a Friedman universe with flat spatial slices and where the matter fields are comprised of the strong interaction, with $\SU(3)$ replaced by a general $\SU(n)$, $n\ge 2$, and the electro-weak interaction. The wave functions are maps from $\R[4n+10]$ to a subspace of the antisymmetric Fock space, and one noteworthy result is that, whenever the electro-weak interaction is involved, the image of an eigenfunction is in general not one dimensional, i.e., in general it makes no sense specifying a fermion and looking for an eigenfunction the range of which is contained in the one dimensional vector space spanned by the fermion.

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