Einstein-Schrodinger theory in the presence of zero-point fluctuations
J. A. Shifflett

TL;DR
This paper extends Einstein-Schrodinger theory to include zero-point fluctuation effects, deriving modified field equations that closely resemble Einstein-Maxwell theory with negligible deviations, and demonstrating the theory's consistency and ghost-free nature.
Contribution
It introduces a modified Einstein-Schrodinger theory incorporating zero-point fluctuations, deriving its field equations, and showing its near equivalence to Einstein-Maxwell theory with negligible deviations.
Findings
Field equations match Einstein-Maxwell with minimal deviations
Exact electric monopole solution similar to Reissner-Nordstrom
Theory remains ghost-free and consistent with known physics
Abstract
The Einstein-Schrodinger theory is modified by adding a cosmological constant contribution 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 constant matches measurement. We first derive the field equations of the theory from a Lagrangian density. We show that the divergence of the Einstein equations vanishes using the Christoffel connection formed from the symmetric metric, allowing additional fields to be included in the same manner as with ordinary general relativity. We show that the field equations match the ordinary electro-vac Einstein and Maxwell equations except for additional terms which are of the usual terms for worst-case field…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Quantum Electrodynamics and Casimir Effect
