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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
-
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.
-
Lightcone fluctuations in a nonlinear medium due to thermal fluctuations
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.