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

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.

v2: clarifications added to Introduction and Conclusions, added appendices; v3 removed review part, published version

References in corpus (3)

• The Unruh effect and its applications
• The Unruh effect revisited
• On the Unruh effect in de Sitter space

Cited by in corpus (3)

• On the beta-decay of the accelerated proton and neutrino oscillations: a three-flavor description with CP violation
• Nonextensive Tsallis statistics in Unruh effect for Dirac neutrinos
• On the Massless Vector Fields in a Rindler Space