{"arxiv_id":"1211.4573","incoming":{"papers":13,"sentences":18,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":2,"sentences":3,"quotes":[{"arxiv_id":"1411.2985","title":"Z-portal dark matter","url":"/paper/1411.2985","section":"Direct detection cross section","sentence":"The limit on the spin independent cross section settled by LUX experiment [ref] being so stringent (almost 4 to 5 orders of magnitudes compared to the spin dependent one, also set by LUX) that the conservative upper limit on $⟨σv ⟩$ is uniquely determined by the upper limit on $σ^SD_χN$, and more precisely $σ^SD_χn$ given by LUX[LUX, like other xenon-type detectors, is much more sensitive to the scattering cross section on neutrons since the contribution from neutrons to the nuclear spin exceeds by an order of magnitude the one of protons.] which is the strongest spin dependent constraint[An analysis on the spin dependent constraint from $χn$ interaction was already made in 2012 for the XENON experiment in [ref] .] at present [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"1510.05378","title":"Prospects for Higgs- and Z-resonant Neutralino Dark Matter","url":"/paper/1510.05378","section":"Introduction","sentence":"We include the following constraints and prospects. * relic abundance $Ω_χh^2 = 0.120$ [ref] . * DM direct detection. * constraints on the spin-independent (SI) scattering cross section from the LUX [ref] , and on the spin-dependent (SD) scattering cross section from the XENON 100 [ref] . * prospects of the XENON 1T for the SI [ref] and SD [ref] scattering cross sections. * Higgs invisible decay. * current constraint from global fit [ref] . * expected sensitivity of the HL-LHC [ref] , and of the ILC [ref] . * chargino/neutralino search at the LHC. * expected sensitivity at 14 TeV for 300 fb$^-1$ and 3000 fb$^-1$ [ref] .","intent_p":0.88,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1703.10379","title":"Study of dark matter physics in non-universal gaugino mass scenario","url":"/paper/1703.10379","section":"Indirect detection","sentence":"This limit is comparable to the expected limit at the XENON1T [ref] .","intent_p":0.83,"contests_p":null},{"arxiv_id":"1212.2730","title":"Top Quark Mediated Dark Matter","url":"/paper/1212.2730","section":"Introduction","sentence":"For the choice of parameter $Λ$ that can account for the monochromatic photon cross section within the Fermi LAT sensitivity, the corresponding spin-dependent cross section is found to be less than $10^-20$pb, far below the recent direct detection [ref] and neutrino telescope [ref] bounds.","intent_p":0.93,"contests_p":null}]}],"unlabelled_sentences":13},"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/1211.4573"}}