{"paper":{"title":"Cardy-Verlinde formula in FRW Universe with inhomogeneous generalized fluid and dynamical entropy bounds near the future singularity","arxiv_id":"1002.1942","primary_cat":"hep-th","submitted_at":"2010-02-09T19:00:33+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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state.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.42,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.55,"result":0.0,"background":0.08,"limitation":0.0,"future_work":0.0,"contribution":0.37,"interpretation":0.0}},{"i":2,"p":0.57,"id":"s2","own":true,"role":"contribution","text":"A viscous dark fluid is included, and we include also modified gravity using its fluid representation.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.88,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.43,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.57,"interpretation":0.0}},{"i":3,"p":0.77,"id":"s3","own":true,"role":"result","text":"It is demonstrated how such an expression reduces to the standard Cardy-Verlinde formula corresponding to the 2d CFT entropy only in some special cases.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.91,"main_claim_p":0.12,"quantitative":false,"quantitative_p":0.34,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.77,"background":0.0,"limitation":0.09,"future_work":0.0,"contribution":0.01,"interpretation":0.13}},{"i":4,"p":0.68,"id":"s4","own":true,"role":"result","text":"The dynamical entropy bound for a closed FRW universe with dark components is obtained.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.94,"main_claim_p":0.1,"quantitative":true,"quantitative_p":0.85,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.68,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.32,"interpretation":0.0}},{"i":5,"p":0.98,"id":"s5","own":true,"role":"contribution","text":"The universality of the dynamical entropy bound near a future singularity (of all four types), as well as near the Big Bang singularity, is investigated.","hedge":{"p":0.59,"label":"unclear"},"own_p":0.88,"main_claim_p":0.11,"quantitative":false,"quantitative_p":0.36,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.02,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.98,"interpretation":0.0}},{"i":6,"p":1.0,"id":"s6","own":true,"role":"result","text":"It is demonstrated that except from some special cases of Type II and Type IV singularities the dynamical entropy bound is violated near the singularity even if quantum effects are taken into account.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.91,"main_claim_p":0.41,"quantitative":true,"quantitative_p":0.63,"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":7,"p":0.95,"id":"s7","own":true,"role":"result","text":"The dynamical entropy bound seems to be universal for the case of a regular universe, including the asymptotic de Sitter 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