{"paper":{"title":"Neutrinos from Fallback onto Newly Formed Neutron Stars","arxiv_id":"0711.0551","primary_cat":"astro-ph","submitted_at":"2007-11-04T22:47:53+00:00","version_compiled":"v1"},"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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than 1e52erg of additional potential energy.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.71,"main_claim_p":0.26,"quantitative":true,"quantitative_p":0.98,"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":0.45,"id":"s4","own":false,"role":"interpretation","text":"Most of this energy is emitted in the form of neutrinos and we must understand this fallback neutrino emission if we are to use neutrino observations to study the behavior of matter at high densities.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.16,"main_claim_p":0.19,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.39,"method":0.0,"result":0.02,"background":0.13,"limitation":0.0,"future_work":0.01,"contribution":0.0,"interpretation":0.45}},{"i":5,"p":0.94,"id":"s5","own":true,"role":"contribution","text":"Here we present both a 1-dimensional study of fallback using energy-injected, 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