{"arxiv_id":"hep-th/9612146","incoming":{"papers":161,"sentences":243,"groups":[{"kind":"contests","label":"Contests it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1504.00882","title":"Entropy and quantum gravity","url":"/paper/1504.00882","section":"Introduction","sentence":"Really, before one takes the logarithm, one would need to multiply $σ_ls(ϵ)$ by a constant with the dimensions of energy but, in [ref] no such constant is provided by the theory.","intent_p":0.95,"contests_p":0.79}]},{"kind":"extends","label":"Builds on it","papers":6,"sentences":8,"quotes":[{"arxiv_id":"2307.03573","title":"The correspondence between rotating black holes and fundamental strings","url":"/paper/2307.03573","section":"Introduction","sentence":"Nevertheless, it provides a convenient starting point to understand how the correspondence between black holes and fundamental strings, as proposed in [ref] , acquires new richness and intricacy when rotation is present.","intent_p":0.84,"contests_p":null},{"arxiv_id":"1104.5556","title":"Closed string transport coefficients and the membrane paradigm","url":"/paper/1104.5556","section":"Introduction","sentence":"This correspondence has been generalized in the case of charged black holes [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"2406.17851","title":"On the Origin of Species Thermodynamics and the Black Hole - Tower Correspondence","url":"/paper/2406.17851","section":"The Black Hole - Tower Correspondence: black hole entropy from non-gravitational thermodynamics","sentence":"The following discussion can be understood as a generalization of the celebrated Black Hole - String correspondence[In this work we refer to the correspondence, as opposed to the transition, to emphasize the fact that we are not studying the details of the transition as a dynamical process, but focusing instead on the correspondence of the entropies of the black hole system and the tower system to obtain a microscopic interpretation of the entropy of the former in terms of the microstate counting of the latter.] [ref] (see also [ref] for recent discussions on the topic), which accounted for the entropy of general Schwarzschild black holes (up numerical prefactors, but crucially matching the area dependence) by the microscopic counting of the microstates associated to a free string in the limit of vanishing string coupling.","intent_p":0.85,"contests_p":null},{"arxiv_id":"0909.5264","title":"Fundamental Strings and Higher Derivative Corrections to d-Dimensional Black Holes","url":"/paper/0909.5264","section":"$d$-dimensional black holes with $(p_L,p_R)$ charges – leading order in $α'$","sentence":"The gravitational thermodynamics of this solution was also inspected in [ref] , and we generalize it here to $d>4$ dimensions.","intent_p":0.99,"contests_p":null},{"arxiv_id":"2403.14544","title":"Conformal Perturbation Theory and Tachyon-Dilaton Eschatology via String Fields","url":"/paper/2403.14544","section":"Introduction","sentence":"A simple application of our approach is the construction of the Horowitz-Polchinski “string star” solution [ref] , that describes a self-gravitating thermal ensemble of strings, in the SFT framework for slow-varying fields.","intent_p":0.91,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses its method or tool","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2604.03720","title":"How to Expose a Black Hole","url":"/paper/2604.03720","section":"Introduction","sentence":"The main idea will be to use the correspondence principle formulated in [ref] , following earlier suggestions in [ref] .","intent_p":0.9,"contests_p":null},{"arxiv_id":"1104.5556","title":"Closed string transport coefficients and the membrane paradigm","url":"/paper/1104.5556","section":"Black hole solutions","sentence":"One can construct an electric NS-NS charged black hole from the Schwarzshild solution by using the solution generating method [ref] .","intent_p":0.87,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":4,"sentences":4,"quotes":[{"arxiv_id":"1504.00882","title":"Entropy and quantum gravity","url":"/paper/1504.00882","section":"Introduction","sentence":"Our first set of results concerns the impressive quantitative agreement between the results of Strominger and Vafa [ref] and subsequent authors for the entropy of extremal and near-extremal black holes and the original Hawking entropy formulae and also between the semi-qualitative results of Susskind [ref] and of Horowitz and Polchinski [ref] for the entropy of, say, Schwarzschild black holes and the original Hawking entropy formula for those.","intent_p":0.85,"contests_p":null},{"arxiv_id":"0706.3996","title":"Phase transitions in higher derivative gravity and gauge theory: R-charged black holes","url":"/paper/0706.3996","section":"Introduction and Summary","sentence":"At this point it may be mentioned that appearance of string states in boundary theory also occurred in [ref] which corresponds to the Gross-Witten transition [ref] and which was identified with a crossover from supergravity black hole solution to string state [ref] .] Beyond the critical potential we encounter different possible situations depending on the position (expectation value of the Polyakov loop) of the extra saddle point.","intent_p":0.8,"contests_p":null},{"arxiv_id":"2301.04069","title":"The chaotic emergence of thermalization in highly excited string decays","url":"/paper/2301.04069","section":"Conclusion and future directions","sentence":"The chaotic nature of the decay process together with the non trivial dependence of final microstates gave rise to a greybody emission spectrum with an effective temperature $T_eff=T_H/√(N)$, which is different from the temperature of the string/BH transition [ref] .","intent_p":0.84,"contests_p":null},{"arxiv_id":"2303.12422","title":"Comments on Single-Trace $T\\bar T$ Holography","url":"/paper/2303.12422","section":"Introduction","sentence":"For $E≪E_c$ the entropy of the deformed theory is given by the CFT entropy, while for $E≫E_c$ it is given by the Hagedorn one.[This is reminiscent of the discussion of the string/black hole transition [ref] , where the roles of the CFT and Hagedorn phases are played by fundamental strings and large black holes, respectively.]","intent_p":0.85,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1810.05338","title":"Symmetries in quantum field theory and quantum gravity","url":"/paper/1810.05338","section":"Introduction","sentence":"This interpretation has been confirmed in many examples in string theory [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"2211.16448","title":"Off-Shell Strings II: Black Hole Entropy","url":"/paper/2211.16448","section":"After Tachyon Condensation","sentence":"Some evidence for this can be seen in the work of Horowitz and Polchinski [ref] , based on earlier work in [ref] , who found a string background, that involves a winding condensate near the Hagedorn inverse temperature $_Hag$ in the form of highly excited self-gravitating oscillating strings.","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":47,"sentences":53,"quotes":[{"arxiv_id":"2604.03720","title":"How to Expose a Black Hole","url":"/paper/2604.03720","section":"Review of the correspondence principle","sentence":"According to the correspondence principle [ref] , at some particular value of $g_s$, the description of the system changes from that of a black hole to that of a fundamental string.","intent_p":0.86,"contests_p":null},{"arxiv_id":"0903.3977","title":"Self-interacting fundamental strings and black holes","url":"/paper/0903.3977","section":"Introduction","sentence":"String theory represents probably the best candidate nowadays for such a theory and it has a general principle (known as the “String-Black holes correspondence principle” [ref] ) individuating those microstates.","intent_p":0.81,"contests_p":null},{"arxiv_id":"2210.12033","title":"On Small Black Holes in String Theory","url":"/paper/2210.12033","section":"Introduction and summary","sentence":"Of particular interest for the discussion of [ref] is the nature of this CFT in the limit where $β$ approaches the inverse Hagedorn temperature of string theory in flat spacetime, $β_H$.","intent_p":0.81,"contests_p":null},{"arxiv_id":"2312.02127","title":"Chaotic and Thermal Aspects in the Highly Excited String S-Matrix","url":"/paper/2312.02127","section":"Context","sentence":"The Susskind-Horowitz-Polchinski correspondence principle [ref] conjectures that the Schwarzchild black hole is adiabatically connected to a single free string state.","intent_p":0.8,"contests_p":null},{"arxiv_id":"1104.5556","title":"Closed string transport coefficients and the membrane paradigm","url":"/paper/1104.5556","section":"The black hole correspondence principle","sentence":"The black hole correspondence principle states that as one decreases the string coupling $g_s$, a black hole will turn into string states when the curvature length scale at the horizon of the black hole in string frame is of the order of the string length scale $l_s$ [ref] .","intent_p":0.96,"contests_p":null}]}],"unlabelled_sentences":173},"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. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/hep-th/9612146"}}