{"arxiv_id":"1106.2339","incoming":{"papers":49,"sentences":78,"groups":[{"kind":"contests","label":"Contests it","papers":1,"sentences":6,"quotes":[{"arxiv_id":"1108.4539","title":"A comment on AdS collapse of a scalar field in higher dimensions","url":"/paper/1108.4539","section":"Introduction","sentence":"Thus, we found it surprising that Garfinkle and Pando Zayas, who later looked at the same problem in $4+1$ dimensions (apparently unaware of Ref. [ref] as they did not cite it), wrote in [ref] : \"We [...] establish that for small values of the initial amplitude of the scalar field there is no [sic!] black hole formation, rather, the scalar field performs an oscillatory motion typical of geodesics in AdS.\" The purpose of this comment is to show that, contrary to the above quoted claim, $AdS_d+1$ is unstable against gravitational collapse for all $d≥3$.","intent_p":0.94,"contests_p":0.92}]},{"kind":"extends","label":"Builds on it","papers":1,"sentences":2,"quotes":[{"arxiv_id":"1110.5823","title":"On Field Theory Thermalization from Gravitational Collapse","url":"/paper/1110.5823","section":"Introduction","sentence":"In this publication we largely expand, clarify and sharpen the results presented in our short letter [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses its method or tool","papers":4,"sentences":5,"quotes":[{"arxiv_id":"1110.5823","title":"On Field Theory Thermalization from Gravitational Collapse","url":"/paper/1110.5823","section":"Understanding the numerical accuracy","sentence":"The precise version used here produced the results presented in [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"1208.1393","title":"On holographic thermalization and gravitational collapse of massless scalar fields","url":"/paper/1208.1393","section":"Introduction","sentence":"We will deal with more general cases using a numerical method similar to that used in the global patch of $AdS_d+1$ [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1305.2237","title":"Quantum corrections to dynamical holographic thermalization: entanglement entropy and other non-local observables","url":"/paper/1305.2237","section":"Introduction and motivation","sentence":"We consider a model of dynamical holographic thermalization [ref] which has been recently used to study thermalization time scale of strongly coupled plasmas.","intent_p":0.8,"contests_p":null},{"arxiv_id":"1402.3592","title":"Gravitational Collapse, Chaos in CFT Correlators and the Information Paradox","url":"/paper/1402.3592","section":"Introduction","sentence":"The constancy of this quantity is customarily used in simulations [ref] to test the precision of the numerics; we use it here as well.","intent_p":0.91,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1108.4539","title":"A comment on AdS collapse of a scalar field in higher dimensions","url":"/paper/1108.4539","section":"Introduction","sentence":"For easy comparison of results, we take the same approximately ingoing Gaussian initial data as Ref. [ref] : $Φ(0,x)=∂_x ϕ(0,x)=Π(0,x)$, where [equation] with $r_0=4$, $σ=1.5$.","intent_p":0.8,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1310.7179","title":"The physical mechanism of AdS instability and Holographic Thermalization","url":"/paper/1310.7179","section":"Mechanism of energy cascade to UV in wave collapse.","sentence":"We believe that this is what is happening in recent numerical works [ref] with initial spherical shell.","intent_p":0.99,"contests_p":null},{"arxiv_id":"1401.5106","title":"Dynamical Meson Melting in Holography","url":"/paper/1401.5106","section":"Setup","sentence":"The thermalization time scale is typically fast for the Vaidya-AdS metric [ref] , and hence it would be suitable to focus on the effect of rapid thermalization.","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":24,"sentences":24,"quotes":[{"arxiv_id":"1508.02709","title":"Classes of Stable Initial Data for Massless and Massive Scalars in Anti-de Sitter Spacetime","url":"/paper/1508.02709","section":"Introduction","sentence":"In 2011, [ref] pioneered numerical work on these questions (see also [ref] ).","intent_p":1.0,"contests_p":null},{"arxiv_id":"1412.6002","title":"Collapse and Revival in Holographic Quenches","url":"/paper/1412.6002","section":"Revival time","sentence":"Different aspects of scalar collapse in AdS$_d+1$ have been studied in [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1205.1548","title":"Thermalization with a chemical potential from AdS spaces","url":"/paper/1205.1548","section":"Introduction","sentence":"In fact, in a series of papers the issue has been studied considering the collapse of a thin shell of matter, by using an AdS-Vaidya type metric [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"1212.5234","title":"Dynamics of holographic thermalization","url":"/paper/1212.5234","section":"Introduction and motivation","sentence":"In these papers the dual process is modeled as the collapse of a thin shell moving at the speed of light, using an AdS-Vaidya type metric, which represents a thermal quench [ref] .","intent_p":0.8,"contests_p":null},{"arxiv_id":"1711.00454","title":"Phase Diagram of Stability for Massive Scalars in Anti-de Sitter Spacetime","url":"/paper/1711.00454","section":"Introduction","sentence":"Starting with the pioneering work of [ref] , numerical studies have suggested that these dynamics may in fact be generically unstable toward formation of (asymptotically) AdS$_d+1$ black holes even for arbitrarily small amplitudes.","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":38},"outgoing":{"papers":4,"sentences":7,"groups":[{"kind":"supports_this_paper","label":"Cites as support","papers":3,"sentences":3,"quotes":[{"arxiv_id":"1010.5443","title":"Instantaneous Thermalization in Holographic Plasmas","url":"/paper/1010.5443","section":"Introduction","sentence":"Other studies supporting rapid thermalization in the context of the gauge/gravity correspondence include [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1103.2683","title":"Holographic Thermalization","url":"/paper/1103.2683","section":"Introduction","sentence":"Other studies supporting rapid thermalization in the context of the gauge/gravity correspondence include [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1104.5469","title":"Evidence for fast thermalization in the plane-wave matrix model","url":"/paper/1104.5469","section":"Introduction","sentence":"Other studies supporting rapid thermalization in the context of the gauge/gravity correspondence include [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":4},"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/1106.2339"}}