{"paper":{"title":"On the spin-dependent sensitivity of XENON100","arxiv_id":"1211.4573","primary_cat":"hep-ph","submitted_at":"2012-11-19T21:00:01+00:00","version_compiled":"v2"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13-20260917 on the question bank abstract-p1-20260923, exactly as returned. 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models.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.19,"main_claim_p":0.32,"quantitative":false,"quantitative_p":0.08,"role_probabilities":{"gap":0.09,"method":0.0,"result":0.0,"background":0.01,"limitation":0.0,"future_work":0.0,"contribution":0.9,"interpretation":0.0}},{"i":2,"p":0.99,"id":"s2","own":true,"role":"result","text":"We show in particular that the constraints set by XENON100 on the spin-dependent neutron cross-section are by far the best at present, whereas the corresponding spin-dependent proton limits lag behind other direct detection results.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.75,"main_claim_p":0.27,"quantitative":true,"quantitative_p":0.92,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.99,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.0}},{"i":3,"p":0.58,"id":"s3","own":true,"role":"limitation","text":"The effect of nuclear uncertainties on the structure functions of xenon isotopes is analysed in detail and found to lessen the robustness of the constraints, especially for spin-dependent proton couplings.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.93,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.08,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.39,"background":0.0,"limitation":0.58,"future_work":0.0,"contribution":0.03,"interpretation":0.0}},{"i":4,"p":0.64,"id":"s4","own":false,"role":"future_work","text":"Notwithstanding, the spin-dependent neutron prospects for XENON1T and DARWIN are very encouraging.","hedge":{"p":0.68,"label":"asserted"},"own_p":0.35,"main_claim_p":0.06,"quantitative":false,"quantitative_p":0.07,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.13,"background":0.0,"limitation":0.0,"future_work":0.64,"contribution":0.0,"interpretation":0.23}},{"i":5,"p":0.79,"id":"s5","own":true,"role":"result","text":"We apply our constraints to well-motivated dark matter models and demonstrate that in both mass-degenerate scenarios and the minimal supersymmetric standard model the spin-dependent neutron limits can actually override the spin-independent limits.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.91,"main_claim_p":0.23,"quantitative":true,"quantitative_p":0.74,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.79,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.08,"interpretation":0.13}},{"i":6,"p":0.91,"id":"s6","own":false,"role":"interpretation","text":"This opens the possibility of probing additional unexplored regions of the dark matter parameter space with the next generation of ton-scale direct detection experiments.","hedge":{"p":0.98,"label":"hedged_possibility"},"own_p":0.37,"main_claim_p":0.16,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.09,"contribution":0.0,"interpretation":0.91}}]},"compiled":{"main_claim":{"p":0.42,"text":"The main goal of this paper is to stress 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