Neutral Massive Spin 1/2 Particles Emission in a Rindler Spacetime
Pietro Longhi, Roberto Soldati
TL;DR
This paper investigates the Unruh effect for neutral massive Majorana spinor particles in Rindler spacetime, explicitly calculating Bogolyubov coefficients and confirming consistency with Fermi-Dirac statistics and the Pauli principle.
Contribution
It provides a detailed calculation of the Unruh effect for Majorana spinors, including explicit Bogolyubov coefficients and verification of statistical consistency.
Findings
Confirmed the Unruh effect for Majorana spinors in Rindler spacetime.
Explicitly calculated Bogolyubov coefficients for neutral massive spinor particles.
Verified compatibility with Fermi-Dirac statistics and Pauli principle.
Abstract
The Unruh effect for the rate of emission and absorption of neutral massive Majorana spinor particles -- the most plausible consituents of Dark Matter -- in a Rindler spacetime is thoroughly investigated. The corresponding Bogolyubov coefficients are explicitly calculated and the consistency with Fermi-Dirac statistics and the Pauli principle is actually verified.
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