Using two null-displaced Rindler wedges, the work shows that positive-momentum scalar modes can be thermalized while negative modes stay in vacuum, and that left-handed fermions can be selectively excited while right-handed ones remain near vacuum.
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The authors analyze formation and evolution of trapped surfaces during matter collapse in de Sitter spacetime and conclude that black hole and cosmological horizons develop as time evolution of marginally trapped surfaces.
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Selective Thermalization, Chiral Excitations, and a Case of Quantum Hair in the Presence of Event Horizons
Using two null-displaced Rindler wedges, the work shows that positive-momentum scalar modes can be thermalized while negative modes stay in vacuum, and that left-handed fermions can be selectively excited while right-handed ones remain near vacuum.
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Gravitational collapse of matter fields in de Sitter spacetimes
The authors analyze formation and evolution of trapped surfaces during matter collapse in de Sitter spacetime and conclude that black hole and cosmological horizons develop as time evolution of marginally trapped surfaces.