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We have recently shown that the space of initial data (covariant phase space) of the relativistic oscillator in Minkowski space R3,1 R 3 , 1 is a homogeneous Kähler–Einstein manifold Z₆=AdS₇/U(1) =U(3,1)/U(3)× U(1) Z 6 = AdS 7 / U ( 1 ) = U ( 3 , 1 ) / U ( 3 ) × U ( 1 ) . It was also shown that the energy eigenstates of the quantum relativistic oscillator form a direct sum of two weighted Bergman spaces of holomorphic (particles) and antiholomorphic (antiparticles) square-integrable functions on the covariant phase space Z₆ Z 6 of the classical oscillator. Here we show that the covariant phase space of the supersymmetric version of the relativistic oscillator (oscillating spinning particle) is the odd tangent bundle of the space Z₆ Z 6 . Quantizing this model yields a Dirac oscillator equation on the phase space whose solution space is a direct sum of two spinor spaces parametrized by holomorphic and antiholomorphic functions on the odd tangent bundle of Z₆ Z 6 . After expanding the general solution in Grassmann variables, we obtain components of the spinor field that are holomorphic and antiholomorphic functions from Bergman spaces on Z₆ Z 6 with different weight functions. Thus, the supersymmetric model under consideration is exactly solvable, Lorentz covariant and unitary.
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Alexander D. Popov (2025) studied this question.
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