{"arxiv_id":"0912.4025","incoming":{"papers":27,"sentences":31,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1008.1796","title":"Light Higgs Boson, Light Dark Matter and Gamma Rays","url":"/paper/1008.1796","section":"Introduction","sentence":"The DAMA/LIBRA signal corresponds a DM cross-section/nucleon of order $10^-39$ cm$^2$, at a WIMP mass of 5 GeV [ref] with a signal band that extends roughly linearly down to 5-42 cm$^2$ at a mass of 50 GeV [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"1011.4743","title":"Discussing direct search of dark matter particles in the Minimal Supersymmetric extension of the Standard Model with light neutralinos","url":"/paper/1011.4743","section":"Confronting results from experiments of direct detection of DM particles","sentence":"The yellow hatched regions are related to the two CDMS candidate events [ref] , as derived in [ref] under the hypothesis that these events might be due to DM .","intent_p":0.88,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":9,"sentences":10,"quotes":[{"arxiv_id":"1003.0437","title":"Low Mass Neutralino Dark Matter in the MSSM with Constraints from $B_s\\to \\mu^+\\mu^-$ and Higgs Search Limits","url":"/paper/1003.0437","section":"Introduction","sentence":"Indeed light neutralinos with masses $O(10) GeV$ have been entertained by several authors within the MSSM framework [ref] and light dark matter using different frameworks has also been investigated [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"1006.0972","title":"XENON10/100 dark matter constraints in comparison with CoGeNT and DAMA: examining the Leff dependence","url":"/paper/1006.0972","section":"Introduction","sentence":"Our focus is on elastic scattering of spin-independent WIMPs from a standard Maxwellian halo; recent examinations comparing experimental studies in this case include [ref] .","intent_p":0.9,"contests_p":null},{"arxiv_id":"0912.4507","title":"Non-Universal Gaugino Masses, CDMS, and the LHC","url":"/paper/0912.4507","section":"Introduction","sentence":"The implications of these events has already been studied in a number of interesting model contexts [ref] .","intent_p":0.89,"contests_p":null},{"arxiv_id":"1005.0924","title":"Dark energy and light WIMP dark matter from the cosmological viewpoint","url":"/paper/1005.0924","section":"Introduction","sentence":"The low mass dark matter problem can be analyzed, e.g., within the context of the standard model with scalar dark matter, ADM models, or the minimal supersymmetric standard model with neutralino dark matter (see, for instance, bibliographies in Refs [ref] and Refs [ref] ).","intent_p":0.99,"contests_p":null},{"arxiv_id":"1007.0595","title":"Particle Dark Matter in DAMA/LIBRA","url":"/paper/1007.0595","section":"Conclusions","sentence":"[ref] and in literature (as e.g. [ref] , etc.); other possibilities are open.","intent_p":0.84,"contests_p":null}]}],"unlabelled_sentences":19},"outgoing":{"papers":5,"sentences":8,"groups":[{"kind":"contests","label":"Contests","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0909.1063","title":"Scintillation efficiency and ionization yield of liquid xenon for mono-energetic nuclear recoils down to 4 keV","url":"/paper/0909.1063","section":"Introduction","sentence":"In particular, the XENON upper bound [ref] suffers from large uncertaities due to conflicting determinations of the scintillation efficiency at low nuclear recoils (as shown in Fig. 12 of [ref] ). �Calculations performed in Ref. [ref] (though with a threshold energy somewhat smaller than the one of XENON10) indicate that at a WIMP mass of order 10 GeV the bound of Ref. [ref] should be relaxed by more than an order of magnitude.","intent_p":0.65,"contests_p":0.77}]},{"kind":"comparison","label":"Compares with","papers":1,"sentences":1,"quotes":[{"arxiv_id":"0912.4264","title":"Global interpretation of direct Dark Matter searches after CDMS-II results","url":"/paper/0912.4264","section":"Introduction","sentence":"In the case of Fig. [ref], the contours refer to 68% and 85% C.L., and they evolve into an open region (i.e. into an upper bound) at the 90% C.L., a result compatible to the one obtained in Ref. [ref] , where a slightly different statistical analysis is adopted.","intent_p":0.99,"contests_p":null}]}],"unlabelled_sentences":6},"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/0912.4025"}}