Computation of boundary-induced fermionic Casimir densities and energy-momentum tensor VEVs for an accelerating mirror in the Fulling-Rindler vacuum, decomposed into boundary-free and boundary-induced parts across RL and RR regions in (D+1) dimensions.
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Thermal photon fluctuations in a nonlinear medium produce light flight-time fluctuations that scale as T^4 at low temperature and linearly with T at high temperature, remaining smaller than vacuum contributions even at room temperature.
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Fermionic Casimir densities for a uniformly accelerating mirror in the Fulling-Rindler vacuum
Computation of boundary-induced fermionic Casimir densities and energy-momentum tensor VEVs for an accelerating mirror in the Fulling-Rindler vacuum, decomposed into boundary-free and boundary-induced parts across RL and RR regions in (D+1) dimensions.