{"paper":{"title":"An Holographic Cosmology","arxiv_id":"hep-th/0111142","primary_cat":"hep-th","submitted_at":"2001-11-15T16:59:33+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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$p=\\rho$.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.51,"main_claim_p":0.08,"quantitative":false,"quantitative_p":0.2,"role_probabilities":{"gap":0.0,"method":0.26,"result":0.11,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.63,"interpretation":0.0}},{"i":2,"p":0.56,"id":"s2","own":true,"role":"result","text":"Fluctuations lead to an instability to a phase with a dilute gas of black holes, which later decays via Hawking radiation to a radiation dominated universe.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.66,"main_claim_p":0.12,"quantitative":false,"quantitative_p":0.08,"role_probabilities":{"gap":0.0,"method":0.15,"result":0.56,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.28,"interpretation":0.01}},{"i":3,"p":1.0,"id":"s3","own":true,"role":"result","text":"The quantum fluctuations of the initial state give rise to a scale invariant spectrum of density perturbations, for a range of scales.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.82,"main_claim_p":0.19,"quantitative":false,"quantitative_p":0.11,"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":1.0,"id":"s4","own":true,"role":"limitation","text":"We point out a problem, that appears to prevent the range of scales predicted by the model from coinciding with the range where such a spectrum has been observed.","hedge":{"p":0.7,"label":"asserted"},"own_p":0.84,"main_claim_p":0.11,"quantitative":false,"quantitative_p":0.08,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.0,"background":0.0,"limitation":1.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":5,"p":0.73,"id":"s5","own":false,"role":"interpretation","text":"We speculate that this may be related to our field theoretic treatment of fluctuations in the highly holographic $p=\\rho$ 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