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Wick Rotation as a Cooling Process: A Novel Perspective on the Origin of Quantum Mechanics and the Arrow of Time
Yong Tao
Posted: 13 April 2026
Experimental Proof that Bell’s Inequality Cannot Falsify Local Realism, Together with Corresponding Cause Analysis and Conjectures
Ting Zhou
Posted: 10 April 2026
Proposed Test for Complex versus Quaternion Quantum Theory via Quantum Superdense Coding
Songsong Dai
Posted: 08 April 2026
Giant Mpemba Effect via Weak Interactions in Open Quantum Systems
Stefano Longhi
Posted: 08 April 2026
Black Holes as Landauer-Saturating Erasure Channels: Horizon Diagnostics, Area Quantization, and the Measurement Counterpart
Moses Rahnama
We develop a quantitative framework in which black holes function as erasure channels for exterior classical records at the horizon-side Landauer bound. At asymptotic infinity, greybody scattering turns the full radiation channel into a thermodynamically dissipative filter (in the sense of excess entropy production, not energy loss) whose entropy efficiency \( \eta_\infty \equiv |dS_{BH}|/dS_{\mathrm{rad}} \) is field-content dependent; for the spin-2 (graviton) channel in Schwarzschild evaporation, \( \eta_\infty \approx 0.74 \) (quoted here as the closest-to-saturation channel, not the dominant total-flux channel; Page [1]). Starting from the Cortês-Liddle result that Hawking evaporation saturates the Landauer principle, we make three contributions. First, we define a Landauer saturation ratio \( \mathcal{R}_L \) as a bookkeeping diagnostic for horizon thermodynamics, using exact-first-law black holes as the saturating benchmark and non-unity cases as the main diagnostic payoff: Schwarzschild black holes yield \( \mathcal{R}_L = 1 \) exactly, while the cosmological apparent horizon yields \( \mathcal{R}_L = 1/2 \) in Trivedi’s quasi-local energy accounting. Second, we show that within the standard Bekenstein-Hawking area law and the discrete transition model of Bagchi, Ghosh, and Sen, one-step Landauer-saturating area transitions select the Bekenstein-Mukhanov spacing \( \Delta A = 4\ln 2\, l_P^2 \); this discrete compatibility result complements, rather than derives, the continuous holographic scaling \( S \propto M^2 \). Third, we argue that the black hole scrambling time \( t_* \sim (\hbar/2\pi k_B T_H)\ln (S_{BH}/k_B) \) provides a partial gravitational analogue of the reversibility time \( \tau_c \) in quantum measurement: for an old black hole it sets the delay after which newly injected information can begin to reappear in Hawking radiation. We formalize the horizon as an effective coarse-grained erasure channel within fixed-charge sectors via a semiclassical proposition that combines a strict exterior coarse-graining definition with GSL-compatible entropy bookkeeping and horizon-side first-law accounting. Within a fixed-charge sector, the Bekenstein-Hawking entropy increase supplies the erased-record capacity \( \Delta S_{BH}/(k_B \ln 2) \), with exact Landauer saturation when that capacity is filled. We check the supporting identities numerically across the Schwarzschild, Kerr, and Reissner-Nordström parameter spaces, and analyze robustness to the memory burden effect. The framework positions black holes as the thermodynamic counterpart to quantum measurement: measurement creates classical records by paying Landauer costs; horizons erase exterior access to those records at the quasi-static Landauer limit, while the asymptotic Hawking channel is greybody-dissipative. The manuscript is intentionally synthetic and classificatory: rather than proposing a new gravitational field equation or a single isolated theorem, it organizes several horizon regimes within one Landauer-based bookkeeping framework.
We develop a quantitative framework in which black holes function as erasure channels for exterior classical records at the horizon-side Landauer bound. At asymptotic infinity, greybody scattering turns the full radiation channel into a thermodynamically dissipative filter (in the sense of excess entropy production, not energy loss) whose entropy efficiency \( \eta_\infty \equiv |dS_{BH}|/dS_{\mathrm{rad}} \) is field-content dependent; for the spin-2 (graviton) channel in Schwarzschild evaporation, \( \eta_\infty \approx 0.74 \) (quoted here as the closest-to-saturation channel, not the dominant total-flux channel; Page [1]). Starting from the Cortês-Liddle result that Hawking evaporation saturates the Landauer principle, we make three contributions. First, we define a Landauer saturation ratio \( \mathcal{R}_L \) as a bookkeeping diagnostic for horizon thermodynamics, using exact-first-law black holes as the saturating benchmark and non-unity cases as the main diagnostic payoff: Schwarzschild black holes yield \( \mathcal{R}_L = 1 \) exactly, while the cosmological apparent horizon yields \( \mathcal{R}_L = 1/2 \) in Trivedi’s quasi-local energy accounting. Second, we show that within the standard Bekenstein-Hawking area law and the discrete transition model of Bagchi, Ghosh, and Sen, one-step Landauer-saturating area transitions select the Bekenstein-Mukhanov spacing \( \Delta A = 4\ln 2\, l_P^2 \); this discrete compatibility result complements, rather than derives, the continuous holographic scaling \( S \propto M^2 \). Third, we argue that the black hole scrambling time \( t_* \sim (\hbar/2\pi k_B T_H)\ln (S_{BH}/k_B) \) provides a partial gravitational analogue of the reversibility time \( \tau_c \) in quantum measurement: for an old black hole it sets the delay after which newly injected information can begin to reappear in Hawking radiation. We formalize the horizon as an effective coarse-grained erasure channel within fixed-charge sectors via a semiclassical proposition that combines a strict exterior coarse-graining definition with GSL-compatible entropy bookkeeping and horizon-side first-law accounting. Within a fixed-charge sector, the Bekenstein-Hawking entropy increase supplies the erased-record capacity \( \Delta S_{BH}/(k_B \ln 2) \), with exact Landauer saturation when that capacity is filled. We check the supporting identities numerically across the Schwarzschild, Kerr, and Reissner-Nordström parameter spaces, and analyze robustness to the memory burden effect. The framework positions black holes as the thermodynamic counterpart to quantum measurement: measurement creates classical records by paying Landauer costs; horizons erase exterior access to those records at the quasi-static Landauer limit, while the asymptotic Hawking channel is greybody-dissipative. The manuscript is intentionally synthetic and classificatory: rather than proposing a new gravitational field equation or a single isolated theorem, it organizes several horizon regimes within one Landauer-based bookkeeping framework.
Posted: 08 April 2026
Quantum Correlations in Classical Systems
Ghenadie N. Mardari
Posted: 08 April 2026
Windowed Quantum Field Theory: Domain-Restricted Actions, Standard Model Recovery, and the Vanishing of Delocalized Stress-Energy
Shawn Hackett
Posted: 06 April 2026
Qudit Propagation Through Multimode Optical Fiber and the Geometry of the Quantum State
Daniel A Nolan
Posted: 02 April 2026
Born's Rule from Record-Formation Constraints: A Conditional Uniqueness Theorem
Moses Rahnama
Posted: 01 April 2026
Calorimetric Signature of Quantum Measurement: A Record-Formation Heat Bound and Differential Microcalorimetry Test
Moses Rahnama
Posted: 01 April 2026
Quantum Control of Metrological Quantities in Two-Component Bose–Einstein Condensates
Henan Wang
,Qimeng Zhang
,Hengyan Wang
,Hai-Jun Xing
,Yixiao Huang
Posted: 31 March 2026
The Lorentz Force and the Nature of Charge from a Photonic Toroidal Vortex Model
Barry R. Clarke
Posted: 27 March 2026
Degrees, Levels, and Profiles of Contextuality
Ehtibar N. Dzhafarov
,Víctor H. Cervantes
Posted: 26 March 2026
The Natural Philosophical Nature of Light: A Hypothesis of Energetic Mass Points in Uniform Spiral Linear Motion in Space
Cheng Jinjun
,Cheng Dian
Posted: 25 March 2026
Hubble Tension Resolved by Standard Model Dark Matter
Frank J. Tipler
Posted: 18 March 2026
New Quantum Spin Perspective, Matter Waves and Uncertainty Principle
Rakshit P. Vyas
Posted: 18 March 2026
On Feasibility of Quantum Computation and Quantum Communication
Guang-Liang Li
Posted: 16 March 2026
Operational Test of No-Signaling and a Near-Identity Binary Channel Criterion
Lorenzo Albanese
Posted: 12 March 2026
From Quantum Geometry to Emergent Gravity
Salim Yasmineh
Posted: 09 March 2026
Intrinsic Quantum Geometry and the Emergence of General Relativity Gravitation
Salim Yasmineh
Posted: 07 March 2026
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