{"paper":{"title":"Structure Formation with Mirror Dark Matter: CMB and LSS","arxiv_id":"astro-ph/0312605","primary_cat":"astro-ph","submitted_at":"2003-12-23T17:49:24+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-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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matter?","hedge":{"p":0.93,"label":"unclear"},"own_p":0.04,"main_claim_p":0.02,"quantitative":false,"quantitative_p":0.16,"role_probabilities":{"gap":0.72,"method":0.0,"result":0.0,"background":0.28,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":2,"p":0.98,"id":"s2","own":true,"role":"contribution","text":"In this paper we answer quantitatively to this question.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.77,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.02,"method":0.0,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.98,"interpretation":0.0}},{"i":3,"p":0.81,"id":"s3","own":true,"role":"method","text":"First we discuss the dependence of the relevant scales for the structure formation (Jeans and Silk scales) on the two macroscopic parameters necessary to define the model: the temperature of the mirror plasma (limited by the Big Bang Nucleosynthesis) and the amount of mirror baryonic matter.","hedge":{"p":0.86,"label":"asserted"},"own_p":0.69,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.07,"role_probabilities":{"gap":0.0,"method":0.81,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.19,"interpretation":0.0}},{"i":4,"p":0.72,"id":"s4","own":true,"role":"method","text":"Then we perform a complete quantitative calculation of the implications of mirror dark matter on the cosmic microwave background and large scale structure power spectrum.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.96,"main_claim_p":0.07,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.72,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.28,"interpretation":0.0}},{"i":5,"p":0.94,"id":"s5","own":true,"role":"result","text":"Finally, confronting with the present observational data, we obtain some bounds on the mirror parameter 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