{"arxiv_id":"1002.4914","incoming":{"papers":16,"sentences":28,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1110.5107","title":"Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae","url":"/paper/1110.5107","section":"On core-collapse supernova simulations","sentence":"These models tend to start exploding at around 300 m after bounce, and the explosion energy for the longest running model of the 25 M$_⊙$ progenitor is reaching to 1 B at 1.2 s after bounce [ref] .","intent_p":0.82,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1112.1913","title":"Core-Collapse Supernovae: Explosion Dynamics, Neutrinos and Gravitational Waves","url":"/paper/1112.1913","section":"General Relativistic Effects in Multi-Dimensional Supernova Models","sentence":"It is noteworthy that the neutrino emission and the shock evolution are similarly sensitive to the neutrino interaction rates (in agreement with the findings of [ref] ).","intent_p":0.86,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1110.4848","title":"Probing Lorentz Violation in Neutrino Propagation from a Core-Collapse Supernova","url":"/paper/1110.4848","section":"Two-Dimensional Simulation of a Core-Collapse Supernova","sentence":"First steps in this direction were reported in Refs. [ref] , but the models are either not evolved for interestingly long post-bounce times or the employed numerical resolution is poor and the neutrino data are not conclusive with respect to the effects discussed here.","intent_p":0.81,"contests_p":null},{"arxiv_id":"2312.16212","title":"Time Scales in Many-Body Fast Neutrino Flavor Conversion","url":"/paper/2312.16212","section":"Introduction","sentence":"Neutrinos play a fundamental role in extreme astrophysical environments, such as core collapse supernovae and neutron star binary mergers, where they, in part, determine the dynamical evolution of the explosion and set the ambient conditions for the ensuing nucleosynthesis, e.g., Refs. [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":24},"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/1002.4914"}}