{"arxiv_id":"hep-th/0006035","incoming":{"papers":11,"sentences":11,"groups":[{"kind":"background","label":"Cites it as background","papers":5,"sentences":5,"quotes":[{"arxiv_id":"2005.01893","title":"JT Supergravity, Minimal Strings, and Matrix Models","url":"/paper/2005.01893","section":"Introduction","sentence":"Recently, there has been renewed interest in Jackiw–Teitelboim (JT) gravity [ref] , a two dimensional theory of gravity that emerges in various physical contexts, such as the study of the near–horizon dynamics of nearly extreme black holes [ref] , or as a partial gravitational dual of certain one–dimensional quantum mechanical systems pertinent to studies of condensed matter and quantum chaos.","intent_p":1.0,"contests_p":null},{"arxiv_id":"2102.02227","title":"A JT supergravity as a double-cut matrix model","url":"/paper/2102.02227","section":"Introduction","sentence":"Describing the low-energy dynamics of a wide class of near-extremal black holes and branes [ref] , JT gravity also features in a precise realization of holographic AdS$_2$/CFT$_1$, arising as the low-energy gravitational dual to the Sachdev-Ye-Kitaev (SYK) 1D quantum mechanical system [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2203.00700","title":"Quasi-local energy and microcanonical entropy in two-dimensional nearly de Sitter gravity","url":"/paper/2203.00700","section":"Two roads to de Sitter JT gravity","sentence":"A popular such model is classical JT gravity in $AdS_2$ [ref] , following from a spherical reduction of the Einstein–Hilbert action describing near-extremal black holes with near-horizon geometry $AdS_2×X$ [ref] , where $X$ is the transverse space whose size is controlled by the dilaton.","intent_p":0.99,"contests_p":null},{"arxiv_id":"2509.05052","title":"Semi-classical spacetime thermodynamics","url":"/paper/2509.05052","section":"Semi-classical 2D gravity","sentence":"The classical JT action is given by [equation] where $ϕ$ is a classical dilaton field, $ϕ_0$ a constant[The classical $2D$ JT gravity can be interpreted as a low-energy model for the classical dynamics of a class of higher-dimensional charged near-extremal black holes and branes [ref] .","intent_p":0.8,"contests_p":null},{"arxiv_id":"2011.06026","title":"Solving Puzzles in Deformed JT Gravity: Phase Transitions and Non-Perturbative Effects","url":"/paper/2011.06026","section":"Introduction","sentence":"This simple theory captures the low energy sector of both near-extremal black holes and branes [ref] and the SYK model [ref] (see ref.","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":6},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[{"relation":"same_result","label":"States the same result","papers":[{"arxiv_id":"hep-th/0012019","url":"/paper/hep-th/0012019","title":"Evaporation of charged black holes near extremality","main_claim":"We find that an infinite amount of time is required for the black hole to decay to extremality.","p":1.0},{"arxiv_id":"hep-th/0004027","url":"/paper/hep-th/0004027","title":"Evaporation of near-extremal Reissner-Nordstrom black holes","main_claim":"The corresponding one-loop quantum theory remains solvable and allows to follow analytically the evaporation process which is shown to require an infinite amount of time.","p":0.96}]}],"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. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/hep-th/0006035"}}