Constraint quantisation of a worldline system invariant under reciprocal relativity. II
P. D. Jarvis, S. O. Morgan (University of Tasmania)

TL;DR
This paper explores the quantisation of a world-line system under reciprocal relativity, revealing a rich spectrum of states including continuous energy-momentum, tachyons, and diverse spin representations, with a novel treatment of spin degrees of freedom.
Contribution
It introduces a new approach to spin degrees of freedom in reciprocal relativity, expanding the physical state space and analyzing the spectrum with standard oscillators.
Findings
Spectrum includes tachyonic and null states.
Enlarged physical state space with towers of integer spin states.
Continuous energy-momentum spectrum with unconventional massless representations.
Abstract
We consider the world-line quantisation of a system invariant under the symmetries of reciprocal relativity. Imposition of the first class constraint, the generator of local time reparametrisations, on physical states enforces identification of the world-line cosmological constant with a fixed value of the quadratic Casimir of the quaplectic symmetry group Q(3,1) ~ U(3,1) x H(4), the semi-direct product of the pseudo-unitary group with the Weyl-Heisenberg group. In our previous paper, J Phys A 40 (2007) 12095--12111, the `spin' degrees of freedom were handled as covariant oscillators, leading to a unique choice of cosmological constant, required for projecting out negative-norm states from the physical gauge-invariant states. In the present paper the spin degrees of freedom are treated as standard oscillators with positive norm states (wherein Lorentz boosts are not number-conserving in…
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