{"paper":{"title":"BPS Black Hole Horizons in N=2 Gauged Supergravity","arxiv_id":"1308.1439","primary_cat":"hep-th","submitted_at":"2013-08-06T22:58:19+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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\\Sigma_g$.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.95,"main_claim_p":0.23,"quantitative":false,"quantitative_p":0.09,"role_probabilities":{"gap":0.0,"method":0.79,"result":0.04,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.17,"interpretation":0.0}},{"i":2,"p":0.53,"id":"s2","own":true,"role":"result","text":"In particular this means we solve for the scalar fields as well as the metric of these black holes as a function of the gauging parameters and background charges.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.95,"main_claim_p":0.2,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.53,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.36,"interpretation":0.09}},{"i":3,"p":0.97,"id":"s3","own":true,"role":"result","text":"When the special Kahler manifold is a symmetric space, our solution is completely explicit and the entropy is related to the familiar quartic invariant.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.91,"main_claim_p":0.16,"quantitative":false,"quantitative_p":0.15,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.97,"background":0.0,"limitation":0.01,"future_work":0.0,"contribution":0.01,"interpretation":0.01}},{"i":4,"p":0.59,"id":"s4","own":true,"role":"result","text":"For more general models our solution is implicit up to a set of holomorphic quadratic equations.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.93,"main_claim_p":0.13,"quantitative":false,"quantitative_p":0.13,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.59,"background":0.0,"limitation":0.38,"future_work":0.0,"contribution":0.03,"interpretation":0.0}},{"i":5,"p":0.53,"id":"s5","own":true,"role":"contribution","text":"For particular models which have known embeddings in M-theory, we derive new horizon geometries with dyonic charges and numerically construct black hole 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