{"arxiv_id":"1007.1421","incoming":{"papers":16,"sentences":18,"groups":[{"kind":"background","label":"Cites it as background","papers":7,"sentences":7,"quotes":[{"arxiv_id":"1504.03292","title":"Inhomogeneous seeding of quark bubbles in Neutron Stars","url":"/paper/1504.03292","section":"Introduction","sentence":"Although quantum bubble nucleation has already been discussed theoretically in the literature [ref] in the context of quantum fluctuations of temperature or seeding [ref] , it remains to be tested on earth from the experimental point of view.","intent_p":0.92,"contests_p":null},{"arxiv_id":"1904.13060","title":"On the change of old neutron star masses with galactocentric distance","url":"/paper/1904.13060","section":"Introduction","sentence":"Self-annihilating DM can also produce characteristic effects on NS [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"1702.05871","title":"Equation of state for hybrid stars with strangeness","url":"/paper/1702.05871","section":"Introduction","sentence":"The possibility of the other exotic degrees of freedom are also expected in the core of a neutron star, such as hyperons [ref] , quark matter [ref] , meson condensations [ref] , and/or dark matter [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"1403.1072","title":"Blocking the Hawking Radiation","url":"/paper/1403.1072","section":"Introduction","sentence":"Observations of old compact stars have been used in order to impose constraints on specific types of (a)symmetric dark matter [ref] or to predict new effects [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"1802.08427","title":"Implications of Neutron Star Properties for the Existence of Light Dark Matter","url":"/paper/1802.08427","section":"Concluding remarks","sentence":"Many authors have investigated the consequences for neutron stars if they capture dark matter of various kinds [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":11},"outgoing":{"papers":3,"sentences":3,"groups":[{"kind":"background","label":"Cites as background","papers":2,"sentences":2,"quotes":[{"arxiv_id":"hep-ph/0008223","title":"Self-Interacting Dark Matter from the Hidden Heterotic-String Sector","url":"/paper/hep-ph/0008223","section":"Introduction","sentence":"Other, more exotic, DM candidates include super-heavy WIMPzillas [ref] with masses in the range $10^10-10^15$ $GeV/c^2$ and SIMPzillas - heavy and strongly interacting [ref] (see recent experimental constraints from ICECUBE [ref] ).","intent_p":0.93,"contests_p":null},{"arxiv_id":"hep-ph/0009017","title":"High Energy Neutrinos From Superheavy Dark Matter Annihilation","url":"/paper/hep-ph/0009017","section":"Introduction","sentence":"Other, more exotic, DM candidates include super-heavy WIMPzillas [ref] with masses in the range $10^10-10^15$ $GeV/c^2$ and SIMPzillas - heavy and strongly interacting [ref] (see recent experimental constraints from ICECUBE [ref] ).","intent_p":0.93,"contests_p":null}]}],"unlabelled_sentences":1},"claims":[{"relation":"same_result","label":"States the same result","papers":[{"arxiv_id":"1108.5206","url":"/paper/1108.5206","title":"Dark Matter Seeding in Neutron Stars","main_claim":"We present a mechanism that may seed compact stellar objects with stable lumps of quark matter, or {\\it strangelets}, through the self-annihilation of gravitationally accreted WIMPs.","p":1.0}]}],"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/1007.1421"}}