REVIEW 3 major objections 3 minor 1 cited by
Islands for black holes in a hybrid quantum state
T0 review · 3 major / 3 minor · reviewed 2026-08-12 · deepseek-v4-flash
Pith's one-line read For a hybrid Unruh/Boulware state with negative total central charge, radiation entanglement entropy follows a Page curve even before islands are included, and the island entropy is always larger, so minimality selects the no-island curve.
desk verdict A technically careful island calculation whose central claim rests on using the standard CFT entropy formula for negative central charge, producing negative entropies that diverge to minus infinity. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing object is the conformal-factor entanglement entropy formula $S_{\rm ent}=4\kappa(\rho_O+\ln L/\epsilon)$, where $\rho$ is the conformal factor in asymptotically flat coordinates and $\kappa=N/24$; in the hybrid state $\kappa=\kappa_1+\kappa_2<0$ because the ghost fields contribute negatively to the central charge. Since $\Delta S_{\rm ent}=4\kappa\rho$, the negativity of $\kappa$ flips the sign of the entropy relative to $\rho$: at past infinity $\rho\to 0^-$, while near $x^-=0$ one has $\rho\sim(\kappa_1/2\kappa)\ln(-\lambda x^-)\to +\infty$, so a maximum appears in between. The island machinery is the generalized entropy functional (5.5), extremized over the location of the quantum extremal surface; with $\kappa<0$ the extremal surface lies on the reflected apparent-horizon curve, but its on-shell value $S_{\rm gen}=2m/\lambda-\kappa\lambda\tilde\sigma^-_O$ is always above the no-island entropy, so the minimum in the island prescription discards the island.
What would settle it
Construct the reduced density matrix of the radiation subsystem in the hybrid state and compute its von Neumann entropy directly; if the result is not $4\kappa(\rho+\ln L/\epsilon)$ or is negative where $\Delta S_{\rm ent}$ is decreasing, the claimed Page curve is not the true entanglement entropy. A simpler check is to test a lattice or exact two-dimensional model in which only the ghost sector is present and see whether its entanglement entropy is non-negative and follows the same sign-flipped curve.
Extended reading notes
Core claim
The paper's central claim is that, for the hybrid Unruh/Boulware solution with negative total central charge, the entanglement entropy of black hole radiation follows a Page curve without any island. Along a null line $x^+=\mathrm{const}$, the change in entanglement entropy $\Delta S_{\rm ent}=4\kappa\rho$ starts at zero at past infinity, grows to a maximum on the curve (4.8), then decreases and crosses zero on the curve (4.9), tending to $-\infty$ as $x^-\to 0$. At future infinity the limit is $\Delta S^\infty_{\rm ent}=-2\kappa\ln(1-x^-_h/x^-)$, a monotonically decreasing function because $\kappa<0$. The island computation gives, at leading order, $S_{\rm gen}=2m/\lambda-\kappa\lambda\tilde\sigma^-_O$, which is always larger than the no-island branch $2\kappa\lambda\tilde\sigma^-_O$ when $\kappa<0$, so the equilibrium entropy $S_{\rm isl}=\min(\ldots)$ chooses the no-island curve. The authors conclude that the Page curve is already present in the entanglement entropy alone, and that islands do not contribute to the generalized black hole entropy here.
Load-bearing premise
The load-bearing assumption is that the formula $S_{\rm ent}=4\kappa(\rho+\ln L/\epsilon)$ remains a legitimate, non-negative entanglement entropy when the total central charge $\kappa=\kappa_1+\kappa_2$ is negative, even though the ghost fields' density matrix is not manifestly positive; the Page curve is produced entirely by that negative sign.
Editorial extensions
If this is right
- In this hybrid model the fine-grained entropy of the radiation already has the rising-then-falling shape of a Page curve, so unitary information recovery does not require an island.
- When the island prescription is applied, the generalized entropy of the island is always larger than the no-island entropy, so the minimum selects the no-island branch and the island has no effect.
- The entanglement-entropy computation reproduces, by an independent route, the earlier thermodynamic-entropy result that the radiation entropy follows a Page curve; this is a consistency check internal to the model.
- The negative outgoing energy flux of the non-physical fields is the mechanism behind the decrease: for the purely physical Boulware case with $\kappa>0$ the same method gives a monotonically increasing entropy and islands are necessary for a Page curve.
- For an observer at finite future null infinity the maximum of the entropy occurs at a finite retarded time; only in the exact limit $x^+\to\infty$ does the maximum recede to past infinity.
Reading between the lines
- If the ghost sector is interpreted as the re-emerging partner modes of the thermal radiation, this model gives a concrete two-dimensional setting in which information recovery is carried by negative-energy flux rather than by islands; a testable signature is non-zero mutual information between early and late radiation.
- The paper does not reconstruct the radiation reduced density matrix; a direct computation of its von Neumann entropy would either confirm $S_{\rm ent}=4\kappa(\rho+\ln L/\epsilon)$ or show that the negative-central-charge entropy is not a physical entropy, which is the most direct check of the central claim.
- In other two-dimensional or higher-dimensional semiclassical models, the same cancellation could be engineered by adding a negative-central-charge sector; the prediction would be that islands remain subdominant whenever the total central charge is negative.
- The late-time branch of the selected entropy decreases without bound in the regulated variables (to $-\infty$ as $x^-\to 0$), which means the model's Page curve is only a qualitative signal of information recovery; interpreting that branch as a true entropy will require accounting for the negative values.
Signed reviews
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper analyzes the entanglement entropy of radiation in a hybrid Unruh/Boulware state of the two-dimensional RST model, in which physical fields have positive central charge κ1 and non-physical 'ghost' fields have negative central charge κ2, with total κ = κ1 + κ2 < 0. Using the standard CFT entanglement formula Sent = 4κ(ρ + ln L/ε), the authors find that along a fixed x+ null line the entropy change ΔSent rises from zero to a maximum and then decreases, which they identify as a Page curve. They then apply the island prescription and find that, because κ < 0, the no-island branch is always selected over the island branch, so islands play no role. The main technical problem is that the decreasing branch is negative and diverges to −∞, and the island comparison inherits this issue.
Significance. The paper is careful and explicit in its algebra. It reproduces the known Boulware-state results of Hartman et al. in Section 3, including the matching of Eqs. (3.13)–(3.15) with [16], and it carries out the island extremization in detail. If the negative-central-charge entanglement entropy were a genuine entanglement entropy, the model would provide a clean example where the island prescription is unnecessary and a Page-curve-like behavior arises without islands. However, the central object is precisely the contested one: the quantity whose sign produces the decrease is the same negative-entropy branch that is later selected by the min prescription. The significance therefore depends entirely on whether Eq. (2.3) is valid for a ghost sector with κ < 0, which the manuscript neither proves nor discusses.
major comments (3)
- [Sec. 4, Eqs. (4.7) and (4.10)] The claimed Page curve is not a Page curve. Along a fixed x+ line, Eq. (4.7) gives ΔSent → −∞ as x− → 0−, and at future infinity Eq. (4.10) is monotonically decreasing from 0 to −∞ for κ < 0. A von Neumann entropy is non-negative and a Page curve for unitary evaporation must return to zero. The decrease is produced solely by multiplying the standard positive-central-charge formula (2.3) by κ < 0. The manuscript does not supply a reduced density matrix for the ghost sector nor a derivation of (2.3) for negative central charge. Since this negative branch is what is later identified as the Page curve and selected by the min prescription, this is not an interpretive subtlety but the central technical assumption of the paper.
- [Sec. 5.2, Eqs. (5.38) and (5.39)] The island conclusion inherits the same problem. For κ < 0, the no-island branch 2κλσ̃O is negative and decreasing, while the island branch 2m/λ − κλσ̃O is positive and increasing, so the min in Eq. (5.39) always selects the negative branch. Thus the statement that islands do not contribute is equivalent to the validity of the negative no-island entropy. If Eq. (2.3) is not applicable to the hybrid state, the min-prescription result is unsupported. If it is applicable, the quantity is not a physical entanglement entropy, and the comparison in Eq. (5.39) does not establish a unitary Page curve.
- [Sec. 5.2, Eq. (5.37)] The perturbative island solution cannot be carried over from the Boulware case by simply replacing κ with a negative value. Eq. (5.37) states that e^{λσ+_Q} = λx+_Q = (3κ/2)e^{λσ̃O}(1 + O(...)); for κ < 0 the right-hand side is negative, while the left-hand side is positive by construction. Hence the claimed quantum extremal surface does not exist in the perturbative regime considered, and Eq. (5.38) for Sgen is not justified. The extremization must be rederived with the sign of κ taken into account, and all subsequent conclusions about the island branch need to be re-examined.
minor comments (3)
- [Sec. 3, first paragraph] There are missing spaces in the opening sentence: 'Wewillstartbycomputingtheentanglemententropyforthesolutiondescribingphysicalfieldsin theBoulwarestate.' Similar spacing issues appear in the surrounding text.
- [Sec. 5.1, Eqs. (5.15) and following paragraph] The condition for the island curve to be partially outside the singularity is written as m/λ > κ, and a few lines later the small-mass case is described as 'm < λκ'. The manuscript should use a single dimensionless form, such as m/λ > κ and m/λ < κ, to avoid confusing κ and λκ.
- [Fig. 6 and Sec. 4, Eq. (4.10)] Figure 6 labels the curve a 'typical behavior for the Page Curve', but the asymptotic result in Eq. (4.10) shows that for an observer at future infinity the maximum is pushed to past infinity and the entropy is monotonically decreasing. The caption and the text should reconcile the finite-x+ behavior with the asymptotic behavior, since the latter does not exhibit the rising part of a Page curve.
Circularity Check
No significant circularity: the Page-curve shape is solved from the adopted master equation and the standard entanglement formula, not fitted or imported as a conclusion.
full rationale
The derivation chain is not circular. The background hybrid solution and its master equation (4.1) are taken from the authors' prior work [13], but the new quantities are then computed, not assumed: the entanglement entropy is obtained by applying the standard formula Sent = 4κ(ρ + ln L/ε) (Eq. (2.3)) to the solution, and the sign of ΔSent is derived from the sign of ρ and of the total central charge κ. The apparent-maximum-then-decrease behavior along null lines follows from the asymptotic limits (4.4) and (4.6)-(4.7) and from the extremum condition (4.8); it is not obtained by fitting a Page-curve ansatz, nor is the curve defined in terms of the desired conclusion. The island analysis likewise solves the extremization conditions (5.30)-(5.31) and evaluates Sgen at the resulting saddle, giving Eq. (5.38); the min prescription (5.39) then selects the no-island branch because of the sign of κ. No parameter is fitted to a subset of data and renamed a prediction, and no uniqueness theorem or ansatz is imported from the authors' own papers to force the result. The cited prior work [1,13] provides the hybrid solution and a previous thermodynamic-entropy result, but the entanglement and island computations here are self-contained algebraic consequences of the stated equations. The physical concern that κ < 0 leads to negative and unbounded-below entanglement entropy values (e.g., Eq. (4.7)) is a question about the validity or interpretation of the input formula for ghost fields, not a circularity in the derivation.
Assumptions & free parameters
free parameters (2)
- Total central charge κ = κ1 + κ2 =
negative (κ < 0)
- Shock mass m =
large mass limit m/λ >> 1
assumptions (4)
- domain assumption Entanglement entropy of a collection of N massless scalar fields on a causal diamond in 2D conformal gauge is Sent = (N/6)(ρ_O + ln L/ε), hence 4κ(ρ+ln L/ε).
- domain assumption The island prescription: S_isl(P_O) = min ext_{P_Q} S_gen(I ∪ R), with S_gen given by Eqs 5.3-5.5.
- domain assumption The hybrid state master equation (4.1) describes physical Unruh fields (central charge κ1>0) and ghost Boulware fields (κ2<0), with κ=κ1+κ2<0.
- ad hoc to paper The same entropy and quantum extremal surface formulas apply when κ < 0 (non-unitary ghost sector).
invented entities (1)
-
Non-physical (ghost) fields with negative central charge, in the Boulware state
Cite this review
Pith. "Pith review of Islands for black holes in a hybrid quantum state." pith.science (2026). https://pith.science/paper/22FGRWQB
@misc{pith2026241109574,
author = {Pith},
title = {Pith review of: Islands for black holes in a hybrid quantum state},
year = {2026},
howpublished = {\url{https://pith.science/paper/22FGRWQB}},
note = {Machine review of arXiv:2411.09574}
}
read the original abstract
Following our previous work on hybrid quantum states in the RST model, we study its most interesting solution representing a completely regular spacetime with the structure of causal diamond, containing an apparent horizon and radiation at infinity. Adapting recent computations of radiation entropy in terms of the entropy of entanglement, we find that this entropy follows a Page curve. This confirms our previous result [1], which was obtained by directly calculating the thermodynamic entropy of radiation at infinity. We also investigate the presence of a possible island in these systems, and find that it does not seem to play a role in contributing to the generalized black hole entropy.
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Forward citations
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Reference graph
Works this paper leans on
-
[16]
T. Hartman, E. Shaghoulian, and A. Strominger. Islands in Asymptotically Flat 2D Grav- ity. JHEP, 07:022, 2020
work page 2020
- [1]
-
[2]
D. Harlow. Jerusalem lectures on black holes and quantum information.Rev. Mod. Phys., 88:015002, 2016
work page 2016
-
[3]
J. M. Maldacena. The Large N limit of superconformal field theories and supergravity. Adv. Theor. Math. Phys., 2:231–252, 1998
work page 1998
- [4]
-
[5]
Susskind
L. Susskind. The World as a hologram.J. Math. Phys., 36:6377–6396, 1995
1995
-
[6]
S. D. Mathur. The Information paradox: A Pedagogical introduction.Class. Quant. Grav., 26:224001, 2009
work page 2009
-
[7]
D. N. Page. Information in black hole radiation.Phys. Rev. Lett., 71:3743–3746, 1993
work page 1993
Show all 24 references
-
[8]
D. N. Page. Time Dependence of Hawking Radiation Entropy.JCAP, 09:028, 2013
2013
-
[9]
N Engelhardt and A. C. Wall. Quantum Extremal Surfaces: Holographic Entanglement Entropy beyond the Classical Regime.JHEP, 01:073, 2015
2015
-
[10]
Almheiri, T
A. Almheiri, T. Hartman, J. Maldacena, E. Shaghoulian, and A. Tajdini. The entropy of hawking radiation. Rev. Mod. Phys., 93:035002, 2021
2021
-
[11]
Almheiri, N
A. Almheiri, N. Engelhardt, D. Marolf, and H. Maxfield. The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole.JHEP, 12:063, 2019
2019
-
[12]
Potaux, D
Y. Potaux, D. Sarkar, and S. N. Solodukhin. Quantum states and their back-reacted geometries in 2d dilaton gravity.Phys. Rev. D, 105:025015, 2022
2022
-
[13]
Potaux, D
Y. Potaux, D. Sarkar, and S. N. Solodukhin. Hybrid quantum states in 2d dilaton gravity. Phys. Rev. D, 108:125012, 2023
2023
-
[14]
J. G. Russo, L. Susskind, and L. Thorlacius. Black hole evaporation in 1+1 dimensions. Physics Letters B, 292(1):13–18, 1992
1992
-
[15]
C. G. Callan, S. B. Giddings, J. A. Harvey, and A. Strominger. Evanescent black holes. Phys. Rev. D, 45:R1005–R1009, 1992. 22
1992
-
[17]
F. F. Gautason, L. Schneiderbauer, W. Sybesma, and L. Thorlacius. Page Curve for an Evaporating Black Hole.JHEP, 05:091, 2020
2020
-
[18]
T. M. Fiola, John P., A. Strominger, and S. P. Trivedi. Black hole thermodynamics and information loss in two dimensions.Phys. Rev. D, 50:3987–4014, 1994
1994
-
[19]
J. G. Russo and A. A. Tseytlin. Scalar tensor quantum gravity in two-dimensions.Nucl. Phys. B, 382:259–275, 1992
1992
-
[20]
S. P. de Alwis. Quantum black holes in two-dimensions.Phys. Rev. D, 46:5429–5438, 1992
1992
-
[21]
Bilal and C
A. Bilal and C. G. Callan, Jr. Liouville models of black hole evaporation.Nucl. Phys. B, 394:73–100, 1993
1993
-
[22]
Penington
G. Penington. Entanglement Wedge Reconstruction and the Information Paradox.JHEP, 09:002, 2020
2020
-
[23]
Germani and D
C. Germani and D. Sarkar. Firewalls as artefacts of inconsistent truncations of quantum geometries. Fortsch. Phys., 64:131–143, 2016
2016
-
[24]
Berthiere, D
C. Berthiere, D. Sarkar, and S. N. Solodukhin. The fate of black hole horizons in semiclas- sical gravity.Phys. Lett. B, 786:21–27, 2018. 23
2018
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