Acceleration radiation for massive vector fields near black hole horizons has a universal thermal detailed-balance factor from the Rindler transformation, with mass thresholds and polarization-dependent spectra, yielding an entropy flux relation identical in form to the scalar HBAR case.
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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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Horizon brightened acceleration radiation from massive vector fields
Acceleration radiation for massive vector fields near black hole horizons has a universal thermal detailed-balance factor from the Rindler transformation, with mass thresholds and polarization-dependent spectra, yielding an entropy flux relation identical in form to the scalar HBAR case.
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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.