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The Unruh effect for the rate of emission and absorption of neutral massiveMajorana spinor particles -- the most plausible consituents of Dark Matter --in a Rindler spacetime is thoroughly investigated. The corresponding Bogolyubovcoefficients are explicitly calculated and the consistency with Fermi-Diracstatistics and the Pauli principle is actually verified.

Neutral Massive Spin 1/2 Particles Emission in a Rindler Spacetime