The Einstein-Schrodinger theory is extended to include spin-0 and spin-1/2
sources, and the theory is derived from a Lagrangian density which allows other
fields to be easily added. The original theory is also modified by including a
cosmological constant caused by zero-point fluctuations. This cosmological
constant which multiplies the symmetric metric is assumed to be nearly
cancelled by Schrodinger’s bare'' cosmological constant which multiplies the nonsymmetric fundamental tensor, such that the total physical’’ cosmological
matches measurement. We show that the resulting Lambda-renormalized
Einstein-Schrodinger theory closely approximates ordinary Einstein-Maxwell
theory and one-particle quantum mechanics. In particular, the field equations
match the ordinary Einstein and Maxwell equations except for additional terms
which are of the usual terms for worst-case field strengths and
rates-of-change accessible to measurement. We also show that the theory
predicts the exact Lorentz force equation and the exact Klein-Gordon and Dirac
equations. And the theory becomes exactly Einstein-Maxwell theory and
one-particle quantum mechanics in the limit as the cosmological constant from
zero-point fluctuations goes to infinity. Lastly, we discuss the merits of our
Lagrangian density compared to the Einstein-Maxwell Lagrangian density.

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