Observing the list of compatible second order equations of Absolute Parallelism (AP) found by Einstein and Mayer (they used D=4), we choose the one-parameter class of equations which take on a 3-linear form (when contra-frame density of some weight is in use). Spherically symmetric solutions to these equations are considered, and we try not to add any delta-sources (ie, $\delta(x)$-sources of unknown nature) during integrations allowed due to this high symmetry.
Using two different ways to fix the radius and time, we have found that only non-static solutions (except for trivial one, of course) are possible. If D=5, such solutions, looking like a single wave moving along the radius, could serve as an expanding cosmological model (with a simple Hubble diagram).
With one coordinate choice (gauge), a single second order equation remains and there exist spherically symmetric solutions with arising singularities. On the other hand, a more reasonable (covariant) choice of the radius and time reduces the problem to a system of two first order equations looking like Chaplygin gas dynamics, where solutions are seemingly free of emerging singularities and gradient catastrophe.
I. I.L.Zhogin
Thu, 8 Sep 22
23/77
Comments: v.2: 7 pages, in Latex; a bit expanded version, with more detailed derivations and explanations; typos corrected; v.3: minor corrections, one reference is added [quite a number of mistypes, e.g. in eqs (5),(9),(15)]
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