The exact quantum evolution under nonclassical light is decomposed into a mixture of quasi-classical branches governed by classical-pulse master equations, allowing analytical and scalable solutions for Fock, thermal, and squeezed states up to N~100 photons.
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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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An efficient framework for quantum dynamics driven by nonclassical light
The exact quantum evolution under nonclassical light is decomposed into a mixture of quasi-classical branches governed by classical-pulse master equations, allowing analytical and scalable solutions for Fock, thermal, and squeezed states up to N~100 photons.
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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.