{"arxiv_id":"astro-ph/9912301","incoming":{"papers":5,"sentences":8,"groups":[{"kind":"background","label":"Cites it as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2604.22680","title":"Dense Matter and Compact Stars in Strong Magnetic Fields","url":"/paper/2604.22680","section":"Numerical results - for nucleon ($n,p,e^-$) matter","sentence":"Nucleon matter in strong magnetic field has been studied in many literature [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"1112.0193","title":"Pion Configurations in the Presence of Baryons","url":"/paper/1112.0193","section":"Back to $M_π≠0$","sentence":"Although the structure of the interior of neutron stars[For a short discussion on neutron stars and an estimation of their densities see appendix [ref].] is not yet known in all details, there are models that include the phenomenon of pion condensation inside these superdense star remnants (see e.g. [ref] ).","intent_p":0.93,"contests_p":null}]}],"unlabelled_sentences":6},"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/9912301"}}