Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

Whose Page Curve? Operator Classes, Charge Reference Frames, and Information Recovery in Charge-Locked Evaporation

Mustafa Boudjerada

Published Aug 25, 2026• 0 citations
Publisher

Abstract

The Page curve is the standard signature of unitary information recovery in an evaporating quantum system. This work asks a question usually left implicit: whose Page curve? In a solvable charge-locked evaporation model, the radiation observables separate into two classes: the charge-coherent algebra, available to an observer with the appropriate charge reference frame, and the charge-invariant algebra of an observer without such a reference frame. These two observers do not recover the same information curve. For the full charge-coherent algebra, the Page curve follows the standard unitary pattern: the radiation entropy rises and then returns exactly to zero, with all interior microstates becoming mutually orthogonal and perfectly decodable radiation records. For the charge-invariant algebra, the turnover is incomplete. The accessible entropy terminates at the charge-distribution entropy, representing the information deficit caused by the missing reference frame. Microstates related by a global charge-phase transformation remain indistinguishable to this observer, not because information is destroyed, but because it is inaccessible within that observable algebra. The work establishes an operator-class Page theorem: complete purification and full information recovery are properties of the charge-coherent algebra, while charge-invariant observers experience a Page curve truncated by the entropy associated with the missing charge reference frame. The model also reveals a mode-structure law. Multi-channel charged radiation can carry relative-charge information internally and locks only the global charge-phase bit, while a single effective channel can lock the full information content. An external reference frame restores accessibility only when its charge quantum matches the charge quantum of the hidden coherence, demonstrating a precise reference-frame selection rule. This work is a circuit-level quantum information model with no gravity and no dynamical backreaction. It does not claim a black-hole evaporation solution. Instead, it provides an exactly solvable framework showing how information recovery can depend on observable algebra and reference frame in systems with conserved charges. All results are accompanied by reproducibility scripts and verification procedures.

DOI
10.5281/zenodo.22088495

Related papers

The Split Page Curve: How Conserved Charges Escape Scrambling

Mustafa Boudjerada

This note studies how conservation laws modify the Page curve of information recovery. A fully scrambled quantum system normally hides information until the Page-time transition. However, realistic scramblers preserve conserved quantities, raising the question of whether all information components follow the same recovery behavior. Using an exactly charge-conserving block-Haar scrambling model, this work separates a record into two classes: 1. Charge records: information stored in different conserved-charge sectors. These records remain readable from the earliest emitted fragments because conservation prevents them from being scrambled into the hidden class. 2. Phase records: information stored within a fixed charge sector. These records follow the conventional Page-curve behavior, exhibiting an initial blackout, a knee at half emission, and late recovery. The study verifies that the Page curve splits into two distinct information channels. The charge component grows monotonically from the first emitted qubits, while the phase component retains the full scrambling structure. Additional diagnostics show that charge records are redundantly accessible across radiation fragments, while phase records remain exclusive until sufficient information is emitted. The work provides an information-theoretic model showing how conservation laws constrain scrambling and create protected record classes. It is a finite-dimensional toy model and does not constitute a calculation of dynamical black-hole physics.

•Aug 26, 2026•0 citations

Information Flow from Zero-Energy Boundary Modes: Exact Quantum-Nondemolition Dynamics of Soft Hair in a Solvable Gauge Model

Mustafa Boudjerada

The black-hole soft-hair proposal raises a central dynamical question: can zero-energy boundary degrees of freedom become correlated with radiation in a way that preserves and reveals information, or are such modes permanently decoupled from observable physics? This work studies that question in an exactly solvable minimal charge-locked emission model derived from the soft-hair structure of the Schwinger model. The model provides a controlled setting to analyze information transfer between boundary hair degrees of freedom and emitted radiation without uncontrolled approximations. The analysis shows that the hair variable acts as a quantum-nondemolition degree of freedom: the hair charge is conserved during emission, while the radiation acquires a coherent record of the initial sector. The emitted radiation remains phase-locked to the vacuum-sector label, and the decay of hair coherences follows an exact closed-form decoherence law. The information flow is characterized using mutual information and explicit state reconstruction. The radiation record approaches a perfect distinguishable record of the hair sector, and pretty-good-measurement decoding achieves exponentially improving recovery accuracy, reaching errors below 10⁻¹² in the verified regime. A central result is an operator-class separation theorem within the model: neutral radiation observables remain completely insensitive to the hair information at all times, while charged observables can access the encoded phase information. Thus, the question of whether soft hair carries information is resolved in this solvable setting by distinguishing the operator algebra available to the observer. The result provides an exactly computable benchmark for discussions of soft hair, information transfer, superselection sectors, and quantum reference frames. The work does not claim a black-hole evaporation solution: the model has no gravitational backreaction, no Page-curve dynamics, and is formulated in a 1+1-dimensional gauge-theory setting. All analytic results, numerical checks, and verification procedures are accompanied by reproducibility materials.

•Aug 25, 2026•0 citations

Horizon-Indistinguishable Quantum Information Unitary Evaporation, Code Subspaces, and the Black-Hole Information-Loss Contradiction

Darren Jeffers

This paper presents a structural resolution of the black-hole information-loss contradiction using standard quantum-information and operator-algebraic ideas. The central argument is that local horizon regularity, unitary evolution, locally thermal-looking radiation, no cloning, and complete final information recovery are not mutually inconsistent unless one additionally assumes that the interior partner and the radiation reconstruction must remain permanently independent physical subsystems. The paper develops an alternative framework in which globally encoded quantum information can remain invisible to the local horizon observable algebra while being preserved exactly in the total quantum state and progressively transferred into correlations within the emitted radiation. An explicit finite-dimensional code model demonstrates that each individual emitted subsystem can appear locally universal while arbitrary quantum information, including entanglement with an external reference system, remains exactly preserved and fully recoverable from the final radiation. The analysis also distinguishes the local horizon-partner role from the global microstate information and from the physical carrier that realizes either role at a given stage of evaporation. This separation removes the apparent monogamy conflict without violating linearity, no cloning, or unitary quantum mechanics. A complementary entropy analysis shows how a Page-like transition can arise when the responsibility for purification becomes progressively reconstructible from the radiation. The paper does not claim a complete dynamical theory of astrophysical black-hole evaporation. Instead, it establishes a mathematically explicit consistency framework showing that the standard information-loss contradiction is not forced by local thermality and unitarity alone, and it identifies the remaining physical problem as the derivation of the appropriate horizon observable algebra and evaporation dynamics from a complete theory of gravity.

•Sep 15, 2026•0 citations

Refined symmetry-resolved Page curve and charged black holes

Pan Li, Yi Ling

The Page curve plotted by the typical random state approximation is not applicable to a system with conserved quantities, such as the evaporation process of a charged black hole during which the electric charge does not radiate out with a uniform rate macroscopically. In this context the symmetry-resolved entanglement entropy may play a significant role in describing the entanglement structure of such a system. We attempt to impose constraints on microscopic quantum states to match with the macroscopic phenomenon of the charge radiation during black hole evaporation. Specifically, we consider a simple qubit system with conserved spin/charge serving as a toy model for the evaporation of charged black holes. We propose refined rules for selecting a random state with conserved quantities to simulate the distribution of charges during the different stages of evaporation, and obtain refined Page curves that exhibit distinct features in contrast to the original Page curve. We find the refined Page curve may have a different Page time and exhibit asymmetric behavior on both sides of the Page time. Such refined Page curves may provide more realistic description for the entanglement between the charged black hole and radiation during the process of evaporation.

arXiv:2311.04436•Nov 8, 2023•0 citations

A dynamical mechanism for the Page curve from quantum chaos

Hong Liu, Shreya Vardhan

A bstract If the evaporation of a black hole formed from a pure state is unitary, the entanglement entropy of the Hawking radiation should follow the Page curve, increasing from zero until near the halfway point of the evaporation, and then decreasing back to zero. The general argument for the Page curve is based on the assumption that the quantum state of the black hole plus radiation during the evaporation process is typical. In this paper, we show that the Page curve can result from a simple dynamical input in the evolution of the black hole, based on a recently proposed signature of quantum chaos, without resorting to typicality. Our argument is based on what we refer to as the “operator gas” approach, which allows one to understand the evolution of the microstate of the black hole from generic features of the Heisenberg evolution of operators. One key feature which leads to the Page curve is the possibility of dynamical processes where operators in the “gas” can “jump” outside the black hole, which we refer to as void formation processes. Such processes are initially exponentially suppressed, but dominate after a certain time scale, which can be used as a dynamical definition of the Page time. In the Hayden-Preskill protocol for young and old black holes, we show that void formation is also responsible for the transfer of information from the black hole to the radiation. We conjecture that void formation may provide a microscopic explanation for the recent semi-classical prescription of including islands in the calculation of the entanglement entropy of the radiation.

arXiv:2002.05734•Journal of High Energy Physics•Mar 1, 2021•39 citations

Refined symmetry-resolved Page curve and charged black holes*

Pan Li, Yi 意 Ling 凌

Abstract The Page curve plotted using the typical random state approximation is not applicable to a system with conserved quantities, such as the evaporation process of a charged black hole, during which the electric charge does not macroscopically radiate out with a uniform rate. In this context, the symmetry-resolved entanglement entropy may play a significant role in describing the entanglement structure of such a system. We attempt to impose constraints on microscopic quantum states to match the macroscopic phenomenon of charge radiation during black hole evaporation. Specifically, we consider a simple qubit system with conserved spin/charge serving as a toy model for the evaporation of charged black holes. We propose refined rules for selecting a random state with conserved quantities to simulate the distribution of charges during the different stages of evaporation and obtain refined Page curves that exhibit distinct features in contrast to the original Page curve. We find that the refined Page curve may have a different Page time and exhibit asymmetric behavior on both sides of the Page time. Such refined Page curves may provide a more realistic description for the entanglement between the charged black hole and radiation during the evaporation process.

Chinese Physics C•Feb 29, 2024•5 citations
The Page curve is the standard signature of unitary information recovery in an evaporating quantum system. This work asks a question usually left implicit: whose Page curve? In a solvable charge-locked evaporation model, the radiation observables separate into two classes: the charge-coherent algebra, available to an observer with the appropriate charge reference frame, and the charge-invariant algebra of an observer without such a reference frame. These two observers do not recover the same information curve. For the full charge-coherent algebra, the Page curve follows the standard unitary pattern: the radiation entropy rises and then returns exactly to zero, with all interior microstates becoming mutually orthogonal and perfectly decodable radiation records. For the charge-invariant algebra, the turnover is incomplete. The accessible entropy terminates at the charge-distribution entropy, representing the information deficit caused by the missing reference frame. Microstates related by a global charge-phase transformation remain indistinguishable to this observer, not because information is destroyed, but because it is inaccessible within that observable algebra. The work establishes an operator-class Page theorem: complete purification and full information recovery are properties of the charge-coherent algebra, while charge-invariant observers experience a Page curve truncated by the entropy associated with the missing charge reference frame. The model also reveals a mode-structure law. Multi-channel charged radiation can carry relative-charge information internally and locks only the global charge-phase bit, while a single effective channel can lock the full information content. An external reference frame restores accessibility only when its charge quantum matches the charge quantum of the hidden coherence, demonstrating a precise reference-frame selection rule. This work is a circuit-level quantum information model with no gravity and no dynamical backreaction. It does not claim a black-hole evaporation solution. Instead, it provides an exactly solvable framework showing how information recovery can depend on observable algebra and reference frame in systems with conserved charges. All results are accompanied by reproducibility scripts and verification procedures.
This note studies how conservation laws modify the Page curve of information recovery. A fully scrambled quantum system normally hides information until the Page-time transition. However, realistic scramblers preserve conserved quantities, raising the question of whether all information components follow the same recovery behavior. Using an exactly charge-conserving block-Haar scrambling model, this work separates a record into two classes: 1. Charge records: information stored in different conserved-charge sectors. These records remain readable from the earliest emitted fragments because conservation prevents them from being scrambled into the hidden class. 2. Phase records: information stored within a fixed charge sector. These records follow the conventional Page-curve behavior, exhibiting an initial blackout, a knee at half emission, and late recovery. The study verifies that the Page curve splits into two distinct information channels. The charge component grows monotonically from the first emitted qubits, while the phase component retains the full scrambling structure. Additional diagnostics show that charge records are redundantly accessible across radiation fragments, while phase records remain exclusive until sufficient information is emitted. The work provides an information-theoretic model showing how conservation laws constrain scrambling and create protected record classes. It is a finite-dimensional toy model and does not constitute a calculation of dynamical black-hole physics.
The black-hole soft-hair proposal raises a central dynamical question: can zero-energy boundary degrees of freedom become correlated with radiation in a way that preserves and reveals information, or are such modes permanently decoupled from observable physics? This work studies that question in an exactly solvable minimal charge-locked emission model derived from the soft-hair structure of the Schwinger model. The model provides a controlled setting to analyze information transfer between boundary hair degrees of freedom and emitted radiation without uncontrolled approximations. The analysis shows that the hair variable acts as a quantum-nondemolition degree of freedom: the hair charge is conserved during emission, while the radiation acquires a coherent record of the initial sector. The emitted radiation remains phase-locked to the vacuum-sector label, and the decay of hair coherences follows an exact closed-form decoherence law. The information flow is characterized using mutual information and explicit state reconstruction. The radiation record approaches a perfect distinguishable record of the hair sector, and pretty-good-measurement decoding achieves exponentially improving recovery accuracy, reaching errors below 10⁻¹² in the verified regime. A central result is an operator-class separation theorem within the model: neutral radiation observables remain completely insensitive to the hair information at all times, while charged observables can access the encoded phase information. Thus, the question of whether soft hair carries information is resolved in this solvable setting by distinguishing the operator algebra available to the observer. The result provides an exactly computable benchmark for discussions of soft hair, information transfer, superselection sectors, and quantum reference frames. The work does not claim a black-hole evaporation solution: the model has no gravitational backreaction, no Page-curve dynamics, and is formulated in a 1+1-dimensional gauge-theory setting. All analytic results, numerical checks, and verification procedures are accompanied by reproducibility materials.
This paper presents a structural resolution of the black-hole information-loss contradiction using standard quantum-information and operator-algebraic ideas. The central argument is that local horizon regularity, unitary evolution, locally thermal-looking radiation, no cloning, and complete final information recovery are not mutually inconsistent unless one additionally assumes that the interior partner and the radiation reconstruction must remain permanently independent physical subsystems. The paper develops an alternative framework in which globally encoded quantum information can remain invisible to the local horizon observable algebra while being preserved exactly in the total quantum state and progressively transferred into correlations within the emitted radiation. An explicit finite-dimensional code model demonstrates that each individual emitted subsystem can appear locally universal while arbitrary quantum information, including entanglement with an external reference system, remains exactly preserved and fully recoverable from the final radiation. The analysis also distinguishes the local horizon-partner role from the global microstate information and from the physical carrier that realizes either role at a given stage of evaporation. This separation removes the apparent monogamy conflict without violating linearity, no cloning, or unitary quantum mechanics. A complementary entropy analysis shows how a Page-like transition can arise when the responsibility for purification becomes progressively reconstructible from the radiation. The paper does not claim a complete dynamical theory of astrophysical black-hole evaporation. Instead, it establishes a mathematically explicit consistency framework showing that the standard information-loss contradiction is not forced by local thermality and unitarity alone, and it identifies the remaining physical problem as the derivation of the appropriate horizon observable algebra and evaporation dynamics from a complete theory of gravity.
The Page curve plotted by the typical random state approximation is not applicable to a system with conserved quantities, such as the evaporation process of a charged black hole during which the electric charge does not radiate out with a uniform rate macroscopically. In this context the symmetry-resolved entanglement entropy may play a significant role in describing the entanglement structure of such a system. We attempt to impose constraints on microscopic quantum states to match with the macroscopic phenomenon of the charge radiation during black hole evaporation. Specifically, we consider a simple qubit system with conserved spin/charge serving as a toy model for the evaporation of charged black holes. We propose refined rules for selecting a random state with conserved quantities to simulate the distribution of charges during the different stages of evaporation, and obtain refined Page curves that exhibit distinct features in contrast to the original Page curve. We find the refined Page curve may have a different Page time and exhibit asymmetric behavior on both sides of the Page time. Such refined Page curves may provide more realistic description for the entanglement between the charged black hole and radiation during the process of evaporation.
A bstract If the evaporation of a black hole formed from a pure state is unitary, the entanglement entropy of the Hawking radiation should follow the Page curve, increasing from zero until near the halfway point of the evaporation, and then decreasing back to zero. The general argument for the Page curve is based on the assumption that the quantum state of the black hole plus radiation during the evaporation process is typical. In this paper, we show that the Page curve can result from a simple dynamical input in the evolution of the black hole, based on a recently proposed signature of quantum chaos, without resorting to typicality. Our argument is based on what we refer to as the “operator gas” approach, which allows one to understand the evolution of the microstate of the black hole from generic features of the Heisenberg evolution of operators. One key feature which leads to the Page curve is the possibility of dynamical processes where operators in the “gas” can “jump” outside the black hole, which we refer to as void formation processes. Such processes are initially exponentially suppressed, but dominate after a certain time scale, which can be used as a dynamical definition of the Page time. In the Hayden-Preskill protocol for young and old black holes, we show that void formation is also responsible for the transfer of information from the black hole to the radiation. We conjecture that void formation may provide a microscopic explanation for the recent semi-classical prescription of including islands in the calculation of the entanglement entropy of the radiation.
Abstract The Page curve plotted using the typical random state approximation is not applicable to a system with conserved quantities, such as the evaporation process of a charged black hole, during which the electric charge does not macroscopically radiate out with a uniform rate. In this context, the symmetry-resolved entanglement entropy may play a significant role in describing the entanglement structure of such a system. We attempt to impose constraints on microscopic quantum states to match the macroscopic phenomenon of charge radiation during black hole evaporation. Specifically, we consider a simple qubit system with conserved spin/charge serving as a toy model for the evaporation of charged black holes. We propose refined rules for selecting a random state with conserved quantities to simulate the distribution of charges during the different stages of evaporation and obtain refined Page curves that exhibit distinct features in contrast to the original Page curve. We find that the refined Page curve may have a different Page time and exhibit asymmetric behavior on both sides of the Page time. Such refined Page curves may provide a more realistic description for the entanglement between the charged black hole and radiation during the evaporation process.