{"arxiv_id":"astro-ph/0406531","incoming":{"papers":33,"sentences":47,"groups":[{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2303.03416","title":"Dark Matter Annihilation inside Large Volume Neutrino Detectors","url":"/paper/2303.03416","section":"Introduction","sentence":"This is simply because a strongly interacting DM component would be slowed significantly by scattering with matter in the atmosphere or the Earth before reaching the target, leading to energy depositions in the detector that are too small to be observed with standard methods [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":8,"sentences":9,"quotes":[{"arxiv_id":"1611.05453","title":"Signatures of Earth-scattering in the direct detection of Dark Matter","url":"/paper/1611.05453","section":"Introduction","sentence":"The effect of Earth-scattering on DM particles for contact, long range or dipole interactions has been studied before in Refs. [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"2405.05312","title":"Optimal Celestial Bodies for Dark Matter Detection","url":"/paper/2405.05312","section":"Maximum Capture Rates","sentence":"This was first pointed out in Ref. [ref] and formulated for the Earth for very light dark matter in Ref. [ref] , and simulations to determine the reflection factor across a wider dark matter mass range and in multiple celestial bodies have been presented in Ref. [ref] .","intent_p":0.84,"contests_p":null},{"arxiv_id":"2309.11003","title":"Cosmic-ray dark matter confronted by constraints on new light mediators","url":"/paper/2309.11003","section":"Attenuation","sentence":"For a detailed study of attenuation of non-relativistic DM, see [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"0705.4298","title":"Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth's Heat Flow","url":"/paper/0705.4298","section":"Introduction","sentence":"In some cases [ref] , DM annihilation was invoked to explain the anomalously large heat flow values of Jupiter and Saturn, while in other cases [ref] , the low heat flow value of Uranus was used to constrain DM annihilation.","intent_p":0.9,"contests_p":null},{"arxiv_id":"1905.06348","title":"Direct Detection of Strongly Interacting Sub-GeV Dark Matter via Electron Recoils","url":"/paper/1905.06348","section":"Introduction","sentence":"In the latter case, MC simulations were used to predict diurnal signal modulations [ref] , and to describe the stopping effect of a detector's overburden, first in [ref] and then later in [ref] .","intent_p":0.83,"contests_p":null}]}],"unlabelled_sentences":37},"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/0406531"}}