The gravitational production of dark matter from stochastic gravitational waves requires the produced fermion to acquire a mass by unspecified late-time physics. We show that this mass is supplied by spacetime torsion alone – no Higgs sector and no free mass parameter. In the Quadratic Spinor Lagrangian formulation of general relativity, extended to Einstein–Cartan, a cosmological spinor condensate generates a vectorial trace torsion ; an explicit Clifford reduction confers on the produced spin-1/2 fermion a pure Dirac mass , with no pseudoscalar or cross terms, locked to the Hubble rate at production, . The relic abundance is then a one-parameter prediction, , and the spin is fixed: the same framework admits no propagating spin-3/2 mode, so the composite spin-1/2 Dirac fermion is its unique dark-matter candidate.

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