{"arxiv_id":"hep-th/9111056","incoming":{"papers":191,"sentences":322,"groups":[{"kind":"extends","label":"Builds on it","papers":4,"sentences":4,"quotes":[{"arxiv_id":"2504.16162","title":"Postcarrollian gravity","url":"/paper/2504.16162","section":"Postcarrollian CGHS model","sentence":"Starting from the postcarrollian JT model introduced in the previous subsection, we perform the limit $Λ→0$ to obtain a postcarrollian version of the CGHS model [ref] in the formulation of Cangemi and Jackiw [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2012.12277","title":"The Stringy Origins of Galileons and their Novel Limit","url":"/paper/2012.12277","section":"Galileons from Strings","sentence":"For example, when we impose $α=-1/32$, $β=-1/8$, we have an $α'$-corrected Callan-Giddings-Harvey-Strominger (CGHS)-like model[Notably we have not included the $e^-2ϕ4λ^2$ contribution or the minimally coupled matter action.] [ref] : I_CGHSα' =-1/2∫d^2x√(-g)[e^-2ϕ(R+4(∇ϕ)^2) -α'/4e^-31/16ϕ(ℒ_GB+105/16ϕ(∇ϕ)^2-1635/256(∇ϕ)^4)] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2206.07111","title":"Ghost-free infinite-derivative dilaton gravity in two dimensions","url":"/paper/2206.07111","section":"Conclusions","sentence":"Another example would be to study ghost-free infinite-derivative modifications of the CGHS theory containing additional scalar matter fields such as the model considered in [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"1404.5330","title":"Global and local properties of AdS(2) higher spin gravity","url":"/paper/1404.5330","section":"Conclusions and outlooks","sentence":"The resulting theory should be a higher spin extension of the two-dimensional Poincare gravity suggested in [ref] and further discussed in [ref] .","intent_p":0.8,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses its method or tool","papers":6,"sentences":7,"quotes":[{"arxiv_id":"2008.07994","title":"Pure de Sitter space and the island moving back in time","url":"/paper/2008.07994","section":"Introduction","sentence":"To comply with this requirement, we study pure de Sitter space in three dimensions by doing a dimensional reduction to two dimensions such that we are able to take into account semi-classical corrections using the conformal anomaly along the lines of Refs. [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"1806.07796","title":"Quantum fluctuating CGHS geometries and the information paradox","url":"/paper/1806.07796","section":"Energy density","sentence":"Using this conformal anomaly [ref] the energy that reaches $ℐ^+_R$ at time $σ_out^-$ is [equation] Here we follow an alternative procedure.","intent_p":0.85,"contests_p":null},{"arxiv_id":"0709.3738","title":"Thermodynamics of Large AdS Black Holes","url":"/paper/0709.3738","section":"One-loop action","sentence":"For $N≫1$ the one-loop effective action describing the semiclassical back-reaction due to this matter sector is given by adding the following conformal anomaly term to the action [ref] , S_q = - N/12 ∫d^2x √(-g) ( 1/2 R ^-1 R - 6 (∇r)^2/r^2 ^-1 R - 6 R lnr ) .","intent_p":0.83,"contests_p":null},{"arxiv_id":"2104.00183","title":"Evaporation of black holes in flat space entangled with an auxiliary universe","url":"/paper/2104.00183","section":"Two disjoint asymptotically flat universes","sentence":"As the gravitational part $I_grav$ of the above effective action, we choose the $CGHS$ action [ref] , I_grav= 14π∫dx^2 -g (ΦR -Λ),","intent_p":0.92,"contests_p":null},{"arxiv_id":"1010.5443","title":"Instantaneous Thermalization in Holographic Plasmas","url":"/paper/1010.5443","section":"Linear Dilaton Black Hole Formation","sentence":"The method used in [ref] is based on trace anomaly argument[We will explain this method in more details in the appendix [ref].] which gives a novel way of calculating a time-dependent Hawking radiation for the process of black hole formation.","intent_p":0.98,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1911.06800","title":"Holographic Complexity: Stretching the Horizon of an Evaporating Black Hole","url":"/paper/1911.06800","section":"Complexity of a two-sided black hole","sentence":"We note that the Hawking temperature of a CGHS black hole is $T_H=1/2π$, independent of the black hole mass [ref] , and the Bekenstein-Hawking entropy is given by $S_BH=2 M$.","intent_p":0.98,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":9,"sentences":11,"quotes":[{"arxiv_id":"0712.3775","title":"Liouville gravity from Einstein gravity","url":"/paper/0712.3775","section":"Constructing the limiting action","sentence":"It is straightforward to take the limit $→0$ of [ref]. Ĩ_C := lim_→0Ĩ^_2dg = -1/κ̃ ∫_ ^2 x √(|g|) (ϕ̃ R - 2a ) eq:2de9 The action $Ĩ_C$ coincides with the geometric part of the CGHS action [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"1304.7836","title":"A local true Hamiltonian for the CGHS model in new variables","url":"/paper/1304.7836","section":"Gauge fixing the vacuum theory","sentence":"Now if we use these transformations in ([ref]), the form of $E^x$ will becomes exactly the same as the form it gets in the vacuum case in the conformal gauge in [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"1010.5443","title":"Instantaneous Thermalization in Holographic Plasmas","url":"/paper/1010.5443","section":"Linear Dilaton Black Hole Formation","sentence":"This is exactly the result obtained in [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"2008.07994","title":"Pure de Sitter space and the island moving back in time","url":"/paper/2008.07994","section":"Semi-classical corrections","sentence":"This value in the $x^±$ coordinates is analogous to what happens in the semi-classical eternal black hole, see e.g. [ref] , which is also in thermal equilibrium.","intent_p":0.95,"contests_p":null},{"arxiv_id":"2502.04924","title":"Hilbert Bundles and Holographic Space-time: the Hydrodynamic Approach to Gravity","url":"/paper/2502.04924","section":"Low Dimensional Models","sentence":"Let us compare these statements to the predictions of linear dilaton gravity for linear dilaton black holes [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":3,"sentences":3,"quotes":[{"arxiv_id":"0901.3156","title":"Conservative solutions to the black hole information problem","url":"/paper/0901.3156","section":"Introduction","sentence":"This result has been derived in a study of the CGHS [ref] model by Ashtekar et al in [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"2205.07382","title":"JT Gravity Coupled to Fermions","url":"/paper/2205.07382","section":"Introduction","sentence":"The interpretation of entropy as a scalar function can be motivated by dimensional reduction, and has also been validated in linear dilaton models [ref] [ref] [ref] , where the variation in area comes from variation of the Planck scale at fixed string scale.","intent_p":0.98,"contests_p":null},{"arxiv_id":"2504.15076","title":"Note on Type $III_1$ Algebras in $ c= 1$ String Theory and Bulk Causal Diamonds","url":"/paper/2504.15076","section":"Introduction","sentence":"The analysis of [ref] shows that it's not surprising that classical physics fails for the Type 0B EFT, because validity of the classical field equations near the black hole horizon requires a large number of Ramond-Ramond fields.","intent_p":0.98,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":97,"sentences":127,"quotes":[{"arxiv_id":"2403.19136","title":"Quantum focusing conjecture in two-dimensional evaporating black holes","url":"/paper/2403.19136","section":"2D black holes and Islands","sentence":"In this section, we briefly review two-dimensional black holes in the RST model [ref] and the island rule to calculate the generalized entropy of Hawking radiation in the RST model.","intent_p":0.97,"contests_p":null},{"arxiv_id":"2004.13745","title":"Dilaton gravity with a boundary: from unitarity to black hole evaporation","url":"/paper/2004.13745","section":"Weyl transformation","sentence":"The action of the model [equation] includes the classical part representing CGHS dilaton gravity [ref] and a quantum counter-term [ref] — the last term in the integrand — providing exact solvability at one-loop level.","intent_p":0.89,"contests_p":null},{"arxiv_id":"2004.00598","title":"Page Curve for an Evaporating Black Hole","url":"/paper/2004.00598","section":"Coupling to matter","sentence":"In the original CGHS model [ref] , the dilaton gravity sector is coupled to matter in the form of $N$ minimally coupled free scalars, with $N≫24$ so that semi-classical corrections are dominated by one-loop effects due to the matter fields.","intent_p":0.85,"contests_p":null},{"arxiv_id":"2310.03416","title":"Island Formula from Wald-like Entropy with Backreaction","url":"/paper/2310.03416","section":"Two-dimensional dilaton-gravity theories","sentence":"As an illustration of the above proposal, we study the black holes in two solvable models of two-dimensional dilaton-gravity theories: the Jackiw-Teitelboim (JT) gravity [ref] and the Russo-Susskind-Thorlacius (RST) model [ref] , built on the Callan-Giddings-Harvey-Strominger (CGHS) model [ref] , in which Hawking radiation is represented by conformal scalars.","intent_p":0.81,"contests_p":null},{"arxiv_id":"2608.07182","title":"Anomaly quenching and dynamical cooling of Hawking evaporation in Horndeski gravity","url":"/paper/2608.07182","section":"Introduction","sentence":"Among these, the Callan-Giddings-Harvey-Strominger (CGHS) model [ref] stands as the paradigmatic workhorse: it admits exact classical BH solutions, yields a thermal flux, and has served as the primary laboratory for studying quantum backreaction for over three decades [ref] .","intent_p":0.87,"contests_p":null}]}],"unlabelled_sentences":169},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. 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A later paper is listed under a label only when the classifier gives one of its sentences that label at intent probability 0.8 or more (0.95 for support), Pith's reading of the sentence finds that the citing paper itself did it, and a second check of the paraphrase against the sentence passes. The section lists uses only: building on the paper, using its method, tool, data or values, comparing with it and citing it as support. It does not list criticism or disagreement, so their absence says nothing about how the paper has been received. Code counted the papers, wrote the summary from the listed entries, set the evidence level and linked each entry to its citing paper. Quotes are copied from the citing sentence and shown only when the citing paper's licence is CC BY, CC BY-SA or CC0; otherwise the paraphrase is shown. Papers that share an author with this one are listed apart. A paper with fewer citing papers gets a line counted by code, which names uses only: a later paper whose only label is a contest is counted as not described.","line":null,"summary":"2 later papers by other authors are listed below: 2 used its method or tool."},"_links":{"html":"https://pith.science/paper/hep-th/9111056"}}