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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11 Pith papers cite this work. Polarity classification is still indexing.
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The Boulware vacuum RVP and RSET for spherical thin shells are computed analytically near the surface and center, and numerically throughout, showing finite interior effects and rapid exterior convergence to Schwarzschild values in the black-hole limit.
A corner in the Euclidean black hole geometry enables direct derivation of the Wald entropy formula in F(R_abcd) gravity and the ADM Hamiltonian conjugate to the horizon Killing vector as the conjugate variable to inverse temperature.
Modular channels induce universal thermal filtering that explains Unruh and Page phenomena, reinterprets entanglement first law as Clausius relation to derive Einstein equations, and proposes MCFC linking causal screen area to filtered information storage.
Magnetic dipole transitions dominate electric ones for circular Unruh detection in atoms, with a multilevel scheme to suppress emission and enable measurement in free space or cavities.
Combining regular black hole metrics with memory burden suppresses evaporation and opens a 10^6-10^8 g PBH mass window that can comprise all dark matter.
Computes density of states for inverted harmonic oscillator on circle via stationary phase approximation to demonstrate semi-classical thermalization from Lyapunov instability.
An RG-improved Schwarzschild metric with de Sitter core is studied for shadow radius, scalar/EM/Dirac quasinormal modes via WKB and time-domain methods, SCC compliance at the inner horizon, and a Davies-type thermodynamic phase transition.
In Michel accretion, Eulerian perturbations generate an acoustic black hole metric where outward acoustic waves tunnel through the sonic horizon, producing Hawking phonons with temperature and frequency enhanced by the background spacetime geometry.
Dark matter halos suppress Hawking temperature and emission rates in regular black holes while enabling a range of horizon radii with positive specific heat capacity and a Davies-type phase transition.
Euler-Heisenberg coupling and surrounding matter fields modify the temperature profile, stability structure, and critical point location of AdS black holes, while changing Hawking radiation sparsity, photon sphere, and shadow size.
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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Vacuum polarization and renormalized stress-energy tensor of spherical thin shells
The Boulware vacuum RVP and RSET for spherical thin shells are computed analytically near the surface and center, and numerically throughout, showing finite interior effects and rapid exterior convergence to Schwarzschild values in the black-hole limit.
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Black hole thermodynamics is around the corner
A corner in the Euclidean black hole geometry enables direct derivation of the Wald entropy formula in F(R_abcd) gravity and the ADM Hamiltonian conjugate to the horizon Killing vector as the conjugate variable to inverse temperature.
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Modular Channels, Thermal Filtering and the Spectral Emergence of Spacetime
Modular channels induce universal thermal filtering that explains Unruh and Page phenomena, reinterprets entanglement first law as Clausius relation to derive Einstein equations, and proposes MCFC linking causal screen area to filtered information storage.
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Signatures of the circular Unruh effect in electric and magnetic dipole transitions of multilevel atoms
Magnetic dipole transitions dominate electric ones for circular Unruh detection in atoms, with a multilevel scheme to suppress emission and enable measurement in free space or cavities.
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Memory burden effect of regular primordial black holes
Combining regular black hole metrics with memory burden suppresses evaporation and opens a 10^6-10^8 g PBH mass window that can comprise all dark matter.
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Semi-classical Imprint of Horizon Induced Instability
Computes density of states for inverted harmonic oscillator on circle via stationary phase approximation to demonstrate semi-classical thermalization from Lyapunov instability.
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Renormalization-group improved Schwarzschild black hole: shadow, ringdown, and strong cosmic censorship
An RG-improved Schwarzschild metric with de Sitter core is studied for shadow radius, scalar/EM/Dirac quasinormal modes via WKB and time-domain methods, SCC compliance at the inner horizon, and a Davies-type thermodynamic phase transition.
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Acoustic Hawking radiation as a tunnelling effect in Michel accretion
In Michel accretion, Eulerian perturbations generate an acoustic black hole metric where outward acoustic waves tunnel through the sonic horizon, producing Hawking phonons with temperature and frequency enhanced by the background spacetime geometry.
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Hawking Temperature, Sparsity and Energy Emission Rate of Dark Matter Halo Regular Black Holes
Dark matter halos suppress Hawking temperature and emission rates in regular black holes while enabling a range of horizon radii with positive specific heat capacity and a Davies-type phase transition.
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Thermodynamic and Radiative Properties of Euler-Heisenberg AdS Black Holes Surrounded by Quintessence and Dark Matter with a Cloud of Strings
Euler-Heisenberg coupling and surrounding matter fields modify the temperature profile, stability structure, and critical point location of AdS black holes, while changing Hawking radiation sparsity, photon sphere, and shadow size.