{"arxiv_id":"astro-ph/0408047","incoming":{"papers":20,"sentences":36,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1708.02959","title":"Time-integrated directional detection of dark matter","url":"/paper/1708.02959","section":"Rejecting isotropy","sentence":"Reference [ref] found that the most powerful test for doing this uses the average of the cosine of the recoil directions [ref] : [equation] The angles $θ^i_rec$ are each measured between the recoil vector $i$ and some chosen preferred direction $_exp$.","intent_p":0.92,"contests_p":null},{"arxiv_id":"1505.07406","title":"New directional signatures from the non-relativistic effective field theory of dark matter","url":"/paper/1505.07406","section":"Rejecting isotropy","sentence":"We follow Morgan et al. [ref] and use the modified Rayleigh-Watson statistic $𝒲^⋆$, defined in Ref. 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[ref] , which found that 5 to 9 events are required for exclusion of isotropy at 90% CL in 90% of the cases, which is a stricter statistical requirement than ours.","intent_p":1.0,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":3,"sentences":4,"quotes":[{"arxiv_id":"2102.04596","title":"Directional recoil detection","url":"/paper/2102.04596","section":"INTRODUCTION","sentence":"Directional detectors are uniquely capable of discriminating against the otherwise irreducible background of astrophysical neutrinos [ref] —and a directional detector should generally enable the identification of a DM signal with far fewer events under any kind of background [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"1708.02959","title":"Time-integrated directional detection of dark matter","url":"/paper/1708.02959","section":"Conclusions","sentence":"In agreement with previous work, e.g. Ref. [ref] , we reiterate that head-tail sensitivity is of crucial importance for detecting dark matter.","intent_p":0.99,"contests_p":null},{"arxiv_id":"2203.05914","title":"Recoil imaging for directional detection of dark matter, neutrinos, and physics beyond the Standard Model","url":"/paper/2203.05914","section":"Directionality for dark matter discovery","sentence":"Under the conditions that DM nuclear recoil-based searches currently operate (i.e. roughly isotropic backgrounds) a set of well-measured recoil directions would be enough to make a non-parametric discovery of DM with as few as tens of events [ref] .","intent_p":0.99,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":4,"sentences":4,"quotes":[{"arxiv_id":"1202.5035","title":"Probing the Local Velocity Distribution of WIMP Dark Matter with Directional Detectors","url":"/paper/1202.5035","section":"Introduction","sentence":"Nevertheless, some theoretical studies on directional dark-matter detection have likewise been conducted [ref] , and a small number of directional detectors are currently under development [ref] .","intent_p":0.92,"contests_p":null},{"arxiv_id":"1505.07406","title":"New directional signatures from the non-relativistic effective field theory of dark matter","url":"/paper/1505.07406","section":"Discussion","sentence":"In Ref. [ref] , the impact of different halo models on the number of events required to reject isotropy was studied.","intent_p":0.85,"contests_p":null},{"arxiv_id":"1609.08630","title":"Reconstructing the three-dimensional local dark matter velocity distribution","url":"/paper/1609.08630","section":"Velocity parameters","sentence":"Attempts have previously been made to use non-parametric statistics in directional experiments to search for substructure or anisotropies in the velocity distribution [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"1106.3778","title":"Detection of WIMP-like dark matter in some extensions of the Standard Model","url":"/paper/1106.3778","section":"Direct Detection","sentence":"Finally, it should be mentioned that since a few years there has been increasing interest in yet another mode of direct dark matter detection, called directional detection [ref] , in which the full variation of the event rate is reconstructed in an effort to obtain a full map of dark matter in the earth's vicinity.","intent_p":0.97,"contests_p":null}]}],"unlabelled_sentences":24},"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/0408047"}}