{"paper":{"title":"Implications of the DAMA and CRESST experiments for mirror matter-type dark matter","arxiv_id":"hep-ph/0308254","primary_cat":"hep-ph","submitted_at":"2003-08-26T02:45:53+00:00","version_compiled":"v3"},"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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e$.","hedge":{"p":0.69,"label":"asserted"},"own_p":0.05,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.16,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.0,"background":1.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":2,"p":0.94,"id":"s2","own":false,"role":"background","text":"This means that the nuclei of mirror atoms can elastically scatter off the nuclei of ordinary atoms, leading to nuclear recoils, which can be detected in existing dark matter experiments.","hedge":{"p":0.92,"label":"asserted"},"own_p":0.06,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.0,"background":0.94,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.03}},{"i":3,"p":0.61,"id":"s3","own":true,"role":"result","text":"We show that the dark matter experiments most sensitive to this type of dark matter candidate (via the nuclear recoil signature) are the DAMA/NaI and CRESST/Sapphire experiments.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.89,"main_claim_p":0.2,"quantitative":false,"quantitative_p":0.14,"role_probabilities":{"gap":0.0,"method":0.01,"result":0.61,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.38,"interpretation":0.0}},{"i":4,"p":0.98,"id":"s4","own":true,"role":"result","text":"Furthermore, we show that the impressive annual modulation signal obtained by the DAMA/NaI experiment can be explained by mirror matter-type dark matter for $|\\epsilon | \\sim 4 \\times 10^{-9}$ and is supported by DAMA's absolute rate measurement as well as the CRESST/Sapphire data.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.89,"main_claim_p":0.76,"quantitative":true,"quantitative_p":0.99,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.98,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.01}},{"i":5,"p":0.56,"id":"s5","own":false,"role":"interpretation","text":"This value of $|\\epsilon |$ is consistent with the value obtained from various solar system anomalies including the Pioneer spacecraft anomaly, anomalous meteorite events and lack of small craters on the asteroid Eros.","hedge":{"p":0.72,"label":"hedged_possibility"},"own_p":0.19,"main_claim_p":0.06,"quantitative":false,"quantitative_p":0.28,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.43,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.56}},{"i":6,"p":0.52,"id":"s6","own":false,"role":"interpretation","text":"It is also consistent with standard BBN.","hedge":{"p":0.57,"label":"asserted"},"own_p":0.2,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.47,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.52}}]},"compiled":{"main_claim":{"p":1.0,"text":"Furthermore, we show that the impressive annual modulation signal obtained by the 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