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Qubit Transport Model for Unitary Black Hole Evaporation without Firewalls

High Energy Physics - Theory · Submitted 15 Jul 2016

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We give an explicit toy qubit transport model for transferring information from the gravitational field of a black hole to the Hawking radiation by a continuous unitary transformation of the outgoing radiation and the black hole gravitational field.

how it is stated · asserted 1.00 read the record →

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arXiv ID1607.04642 (version 5)
Pith IDSO6KFKKU, Pith's permanent record of this paper and its review
CitationDon N. Page, Kento Osuga. "Qubit Transport Model for Unitary Black Hole Evaporation without Firewalls." arXiv:1607.04642 (2016). https://pith.science/paper/SO6KFKKU
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,347 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.97 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.10 · compares with prior results 0.60 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v5. Results and the main claim are underlined; .

We give an explicit toy qubit transport model for transferring information from the gravitational field of a black hole to the Hawking radiation by a continuous unitary transformation of the outgoing radiation and the black hole gravitational field. The model has no firewalls or other drama at the event horizon, and it avoids a counterargument that has been raised for subsystem transfer models as resolutions of the firewall paradox. Furthermore, it fits the set of six physical constraints that Giddings has proposed for models of black hole evaporation. It does utilize nonlocal qubits for the gravitational field but assumes that the radiation interacts locally with these nonlocal qubits, so in some sense the nonlocality is confined to the gravitational sector. Although the qubit model is too crude to be quantitively correct for the detailed spectrum of Hawking radiation, it fits qualitatively with what is expected.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 We give an explicit toy qubit transport model for transferring information from the gravitational field of a black hole to the Hawking radiation by a continuous unitary transformation of the outgoing radiation and the black hole gravitational field. contribution 0.97 0.93 0.61 asserted 1.00
s1 The model has no firewalls or other drama at the event horizon, and it avoids a counterargument that has been raised for subsystem transfer models as resolutions of the firewall paradox. result 0.65 0.81 0.25 asserted 1.00
s2 Furthermore, it fits the set of six physical constraints that Giddings has proposed for models of black hole evaporation. result 0.85 0.71 0.09 asserted 1.00
s3 It does utilize nonlocal qubits for the gravitational field but assumes that the radiation interacts locally with these nonlocal qubits, so in some sense the nonlocality is confined to the gravitational sector. method 0.53 0.78 0.07 asserted 0.95
s4 Although the qubit model is too crude to be quantitively correct for the detailed spectrum of Hawking radiation, it fits qualitatively with what is expected. limitation 1.00 0.71 0.08 asserted 0.65

What kind of paper the classifier reports this is: theoretical result 0.98 · evidence from argument 0.74.

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sources read
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not examined
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  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

We give an explicit toy qubit transport model for transferring information from the gravitational field of a black hole to the Hawking radiation by a continuous unitary transformation of the outgoing radiation and the black hole gravitational field. The model has no firewalls or other drama at the event horizon, and it avoids a counterargument that has been raised for subsystem transfer models as resolutions of the firewall paradox. Furthermore, it fits the set of six physical constraints that Giddings has proposed for models of black hole evaporation. It does utilize nonlocal qubits for the gravitational field but assumes that the radiation interacts locally with these nonlocal qubits, so in some sense the nonlocality is confined to the gravitational sector. Although the qubit model is too crude to be quantitively correct for the detailed spectrum of Hawking radiation, it fits qualitatively with what is expected.

Human review
References
How the literature uses it

10 arXiv papers cite this in 16 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 7 sentences without a confident label

Cites it as support 1 paper
Cites it as background 6 papers

What it cites · 4 sentences without a confident label

Compares with 3 papers
Cites as support 1 paper
Cites as background 36 papers
  • Giddings [ref] has proposed a list of physical constraints on models of black hole evaporation.

    Black holes, quantum information, and unitary evolution · Giddings' Physical Conditions · 0.90

  • If one believes in local quantum field theory outside a black hole and also that one would not experience extreme harmful conditions (`drama') immediately upon falling into any black hole sufficiently large that the curvature at the surface would not be expected to be dangerous, then recent papers by Almheiri, Marolf, Polchinski, and Sully (AMPS) [ref] , and by them and Stanford (AMPSS) [ref] , give a new challenge to unitarity, as they argued that unitarity, locality, and no drama are mutually inconsistent.

    An Apologia for Firewalls · Introduction · 0.86

  • If one believes in local quantum field theory outside a black hole and also that one would not experience extreme harmful conditions (`drama') immediately upon falling into any black hole sufficiently large that the curvature at the surface would not be expected to be dangerous, then recent papers by Almheiri, Marolf, Polchinski, and Sully (AMPS) [ref] , and by them and Stanford (AMPSS) [ref] , give a new challenge to unitarity, as they argued that unitarity, locality, and no drama are mutually inconsistent.

    Black Holes: Complementarity or Firewalls? · Introduction · 0.86

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