{"paper":{"title":"Indirect and direct detection prospect for TeV dark matter in the MSSM-9","arxiv_id":"1503.00599","primary_cat":"hep-ph","submitted_at":"2015-03-02T16:33:19+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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independently.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.24,"main_claim_p":0.02,"quantitative":true,"quantitative_p":0.91,"role_probabilities":{"gap":0.0,"method":0.68,"result":0.0,"background":0.2,"limitation":0.0,"future_work":0.0,"contribution":0.12,"interpretation":0.0}},{"i":2,"p":1.0,"id":"s2","own":true,"role":"method","text":"We perform a Bayesian Monte Carlo scan of the parameter space taking into consideration all available particle physics constraints such as the Higgs mass of 126 GeV, upper limits on the scattering cross-section from direct-detection experiments, and assuming that the MSSM-9 provides all the dark matter abundance through thermal freeze-out mechanism.","hedge":{"p":0.96,"label":"asserted"},"own_p":0.92,"main_claim_p":0.05,"quantitative":true,"quantitative_p":0.95,"role_probabilities":{"gap":0.0,"method":1.0,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":3,"p":1.0,"id":"s3","own":true,"role":"result","text":"Within this framework we find two most probable regions for dark matter: 1-TeV higgsino-like and 3-TeV wino-like neutralinos.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.96,"main_claim_p":0.66,"quantitative":true,"quantitative_p":0.94,"role_probabilities":{"gap":0.0,"method":0.0,"result":1.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":4,"p":0.59,"id":"s4","own":true,"role":"contribution","text":"We discuss prospects for future indirect (in particular the Cherenkov Telescope Array, CTA) and direct detection 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