This manuscript addresses the black hole information paradox using the quantum extremal surface (QES)/island formula prescription within Jackiw-Teitelboim (JT) gravity coupled to a non-gravitational bath. The abstract and introduction promise an explicit derivation of the QES location and the resulting unitary Page curve for both an eternal two-sided black hole and an evaporating black hole. However, upon reviewing the body of the paper, none of these explicit computations are actually carried out or presented. The 'Page Curve Calculation' section merely restates the well-known qualitative results from the foundational island-formula papers (Penington 2019; Almheiri-Engelhardt-Marolf-Maxfield 2019; Almheiri-Hartman-Maldacena-Shaghoulian-Tajdini 2019): that the no-island entropy grows linearly with time (the standard Hawking result, S ~ (πc/3β) t), that a stationary island at the bifurcation surface gives a constant entropy 2S_BH, and that comparing the two saddles reproduces the Page curve. For the evaporating case, the paper only qualitatively states that the dilaton decreases, the QES moves inward, and the island appears near the Page time, with the entropy eventually vanishing — again without any explicit equations, dilaton profiles, or boundary-particle trajectories that would substantiate the claim of an explicit calculation.
This is a serious shortcoming for a paper whose stated contribution is precisely the explicit computation of the QES location in JT gravity. JT-gravity island calculations already exist in the literature (most notably Almheiri, Mahajan, and Maldacena, arXiv:1910.11077), which derive the extremization conditions, the dilaton profile in the presence of a bath, and the resulting Page curve in detail, including both eternal and evaporating cases. The present paper does not engage with or build upon this prior work in any technical way, nor does its reference list include it, despite its clear relevance. The reference list is minimal (only four entries), omitting many essential works in this area (e.g., Almheiri-Mahajan-Maldacena 2019, Penington-Shenker-Stanford-Yang 2019, Hartman-Maldacena replica wormhole papers, and follow-up JT-specific island analyses).
In terms of rigour, the paper falls short of standard research-paper expectations: there are no equations beyond the JT action and the generic island formula (both textbook expressions), no derivation of the generalized entropy extremization, no specification of the CFT matter content or the number of fields used, and no explicit boundary conditions at the JT-bath interface. The 'Discussion' section is likewise generic, offering no new physical insight, subtlety, or technical result that would differentiate this work from an introductory review of the island-formula literature.
On the positive side, the paper's exposition of the conceptual picture (why the Page curve emerges, the role of the island, the competition between island and no-island saddles) is accurate and clearly written, and could serve as a decent pedagogical introduction for readers unfamiliar with the topic. The choice of JT gravity as a tractable toy model is well-motivated and consistent with the field's standard approach.
However, as a research contribution, the paper does not meet the bar for publication. It lacks explicit new calculations, fails to differentiate itself from existing literature that already performs the claimed computations in greater detail, and does not offer any novel physical insight, extension, or quantitative result. I recommend rejection in the current form. If the authors wish to resubmit, they should include the actual explicit derivations promised in the abstract (dilaton profiles, extremization equations, explicit QES trajectories, and quantitative Page curves with plots), position their results relative to the closely related prior JT-gravity island literature (especially Almheiri-Mahajan-Maldacena), and expand the reference list and discussion of open issues (e.g., replica wormhole justification, backreaction, boundary particle dynamics) to establish the novelty and technical rigor of the work.