Canonical quantization of the dark positive-energy Dirac field and time asymmetry
Andrei Galiautdinov

TL;DR
This paper develops a canonical quantization framework for a positive-energy Dirac field model, exploring its implications for dark matter, time asymmetry, and potential exotic statistics, with separate treatments for massive and massless cases.
Contribution
It introduces a simplified positive-energy Dirac field quantization approach, extending Dirac's theory to include Bose-Fermi doublets and spontaneous symmetry breaking, with implications for dark matter and cosmology.
Findings
Quantization involves only annihilation operators for positive-energy modes.
Hamiltonian is unambiguous, no normal ordering needed.
Hints at a dark spacetime condensate causing cosmological time asymmetry.
Abstract
We perform canonical quantization of the single-component, spin-zero field that was introduced by Dirac in 1971 and recently suggested as a candidate for dark matter by Bogomolny. The massive and massless cases are treated separately. Since in the massive case only positive-frequency modes are normalizable and regarded as physical, the mode expansion for the field involves annihilation operators only, making the quantization procedure particularly simple. The corresponding Hamiltonian turns out to be unambiguous, with no need for normal ordering. The positive-energy requirement imposed on the second-quantized system leads to equally acceptable Bose and Fermi choices for particle statistics. This suggests a simple extension of original Dirac's theory in which Bose and Fermi single-component positive-energy Dirac fields are combined into a doublet whose members can transform into each…
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Taxonomy
TopicsAlgebraic and Geometric Analysis · Quantum Mechanics and Non-Hermitian Physics · Quantum Mechanics and Applications
