From Generalized Dirac Equations to a Candidate for Dark Energy
U. D. Jentschura, B. J. Wundt

TL;DR
This paper extends the Dirac equation to include tachyonic mass terms, deriving solutions and sum rules, and explores the potential of tachyonic neutrinos as a candidate for dark energy in the universe.
Contribution
It introduces new generalized Dirac equations with tachyonic mass terms, derives their solutions, and proposes a novel role for tachyonic neutrinos in explaining dark energy.
Findings
Derived explicit solutions for generalized Dirac equations.
Established sum rules linking field anticommutators and eigenspinors.
Proposed tachyonic neutrinos as a candidate for dark energy.
Abstract
We consider extensions of the Dirac equation with mass terms m1+i*gamma5*m2 and i*m_1+gamma*m2. The corresponding Hamiltonians are Hermitian and pseudo-Hermitian ("gamma5 Hermitian"), respectively. The fundamental spinor solutions for all generalized Dirac equations are found in the helicity basis and brought into concise analytic form. We postulate that the time-ordered product of field operators should yield the Feynman propagator (i*epsilon prescription), and we also postulate that the tardyonic as well as tachyonic Dirac equations should have a smooth massless limit. These postulates lead to sum rules that connect the form of the fundamental field anticommutators with the tensor sums of the fundamental plane-wave eigenspinors and the projectors over positive-energy and negative-energy states. In the massless case, the sum rules are fulfilled by two egregiously simple, distinguished…
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