{"arxiv_id":"astro-ph/0003163","incoming":{"papers":2,"sentences":4,"groups":[{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2606.09987","title":"Mode Instability and a Massive, Isolated Outburst in the Pulsating White Dwarf GD 1212","url":"/paper/2606.09987","section":"Rotational Multiplets Suggest 17-hr Rotation","sentence":"These close frequency overlaps may work to strongly enhance resonance and nonlinear mode coupling in the star, since limit cycles happen most frequently when the frequency mismatch is minimized, which happens more often as the mode density increases [ref] .","intent_p":0.98,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2107.13339","title":"Nonlinear mode-tide coupling in coalescing binary neutron stars with relativistic corrections","url":"/paper/2107.13339","section":"Introduction","sentence":"Another possibility that has generated great excitement is one where the three-mode couplings can be strong even away from resonance, when the two daughter modes have similar wave numbers [ref] .","intent_p":0.8,"contests_p":null}]}],"unlabelled_sentences":2},"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/astro-ph/0003163"}}