{"arxiv_id":"1201.3942","incoming":{"papers":28,"sentences":29,"groups":[{"kind":"background","label":"Cites it as background","papers":18,"sentences":18,"quotes":[{"arxiv_id":"1511.00570","title":"Primordial $^4\\text{He}$ constraints on inelastic macro dark matter revisited","url":"/paper/1511.00570","section":"Introduction","sentence":"Whether or not they have a Standard Model origin, macros [ref] remain a viable dark matter candidate and an alternative to the comparatively light candidates, such as weakly interacting massive particles or axions (see, e.g., [ref] for a brief review of those candidates).","intent_p":0.97,"contests_p":null},{"arxiv_id":"1510.03868","title":"Concentration, Ellipsoidal Collapse, and the Densest Dark Matter haloes","url":"/paper/1510.03868","section":"Introduction","sentence":"Dark matter haloes have been extensively studied in the literature using both N-body simulations and analytical approaches [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"2209.07690","title":"New Constraints on Macroscopic Dark Matter Using Radar Meteor Detectors","url":"/paper/2209.07690","section":"Introduction","sentence":"The particle nature of dark matter (DM) remains elusive, even after decades of ever-more sensitive astrophysical, cosmological, collider, and direct detection searches [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1705.00632","title":"Warm dark matter constraints from high-$z$ Direct Collapse Black Holes using the JWST","url":"/paper/1705.00632","section":"Introduction","sentence":"Some of the most popular CDM candidates [ref] are: (i) WIMPS: with a mass between $10 GeV$-$TeV$ stable Weakly Interacting Massive Particles may be produced as a thermal relic of the Big Bang, with a relic density consistent with that required for DM, making them the preferred CDM candidate; (ii) Axions: with a mass $∼10^-5 eV$, although axions provide a natural solution to the strong charge-parity problem in particle physics, they require fine-tuning to match to the observed DM number density and (iii) Gravitinos: are a supersymmetric counterpart of the graviton whose mass could lie anywhere between the $eV$ to $TeV$ scales depending on how super-symmetry is broken, with $$ keV gravitinos being a possible CDM candidate.","intent_p":1.0,"contests_p":null},{"arxiv_id":"2011.08917","title":"Gamma-ray and Synchrotron Radiation from Dark Matter annihilations in Ultra-faint Dwarf Galaxies","url":"/paper/2011.08917","section":"Introduction","sentence":"The presence of an abundant non-baryonic dark matter (DM) component in our universe has not only been established through a variety of independent observations [ref] , but is also expected to have played a key role in the evolution of structure at a multitude of scales [ref] .","intent_p":0.99,"contests_p":null}]}],"unlabelled_sentences":11},"outgoing":{"papers":11,"sentences":17,"groups":[{"kind":"supports_this_paper","label":"Cites as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1111.4217","title":"Constraining Sterile Neutrino Warm Dark Matter with Chandra Observations of the Andromeda Galaxy","url":"/paper/1111.4217","section":"The particle zoo","sentence":"The simplest model of sterile neutrino dark matter (Dodelson-Widrow neutrinos) are excluded by a combination of small-scale structure observations and non-detections of X-rays from galaxies [ref] (for an alternative view, see [ref] ).","intent_p":0.96,"contests_p":null}]}],"unlabelled_sentences":16},"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/1201.3942"}}