On Non-Linear Quantum Mechanics, Space-Time Wavefunctions, and Compatibility with General Relativity
W. David Wick

TL;DR
This paper demonstrates that non-linear quantum mechanics can be integrated with general relativity using space-time wavefunctions and additional algebraic structures, potentially affecting black hole singularity formation.
Contribution
It introduces a framework for compatible non-linear quantum mechanics and general relativity using space-time wavefunctions and bitensors, expanding the theoretical landscape.
Findings
NLQM can be compatible with Einstein's gravity
Space-time wavefunctions are essential for curved space-times
Possible implications for black hole singularities
Abstract
In previous papers I expounded non-linear Schrodingerist quantum mechanics as a solution of the Measurement Problem. Here I show that NLQM is compatible with Einstein's theory of General Relativity. The extension to curved space-times presumes adoption of "space-time wavefunctions" (sometimes called "multi-time wavefunctions") and some additional algebraic structure: a "bitensor" supplementing Einstein's metric tensor. This kind of matter may violate the Strong Energy Condition even without a mass term, possibly with implications for the formation of singularities within Black Holes.
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Taxonomy
TopicsQuantum Mechanics and Applications · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
