Massive fields in null-shifted Rindler wedges produce non-thermal spectra for accelerated observers, as mass eliminates the exponential Bogoliubov mixing that creates thermality.
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Null-shifted Rindler wedges yield selective non-Gibbsian thermality in one chiral sector via Bogoliubov transformations, with the global Minkowski state remaining pure.
Semiclassical RN-dS evaporation via 2D dilaton gravity and anomaly flux yields monotonic neutral mass loss and rapid discharge, making classical equilibrium loci non-attractors and leading to empty de Sitter space.
citing papers explorer
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Thermality Breakdown in Null-Shifted Rindler Wedges
Massive fields in null-shifted Rindler wedges produce non-thermal spectra for accelerated observers, as mass eliminates the exponential Bogoliubov mixing that creates thermality.
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Four inequivalent paths to Thermality in Minkowski spacetime
Null-shifted Rindler wedges yield selective non-Gibbsian thermality in one chiral sector via Bogoliubov transformations, with the global Minkowski state remaining pure.
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The fate of Reissner--Nordstr\"om--de Sitter black holes: nonequilibrium discharge and evaporation
Semiclassical RN-dS evaporation via 2D dilaton gravity and anomaly flux yields monotonic neutral mass loss and rapid discharge, making classical equilibrium loci non-attractors and leading to empty de Sitter space.