{"paper":{"title":"Mechanical laws of the Rindler horizon","arxiv_id":"1305.4986","primary_cat":"gr-qc","submitted_at":"2013-05-21T23:35:25+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. No sentence in this record was written by a language model.","schema":"pith.compiled-record/v0","status":"compiled","abstract":{"source":"arXiv listing abstract v1","sentences":[{"i":0,"p":0.85,"id":"s0","own":true,"role":"result","text":"Gravitational perturbations of flat Minkowski space make the Rindler horizon dynamical: the horizon satisfies mechanical laws analogous to the ones followed by black holes.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.55,"main_claim_p":0.9,"quantitative":false,"quantitative_p":0.25,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.85,"background":0.06,"limitation":0.0,"future_work":0.0,"contribution":0.07,"interpretation":0.02}},{"i":1,"p":0.99,"id":"s1","own":true,"role":"method","text":"We describe the gravitational perturbation of Minkowski space using perturbative field-theoretical methods.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.92,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.02,"role_probabilities":{"gap":0.0,"method":0.99,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.0}},{"i":2,"p":0.44,"id":"s2","own":true,"role":"method","text":"The change in the area of the Rindler horizon is described in terms of the deflection of light rays by the gravitational field.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.77,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.44,"result":0.38,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.17,"interpretation":0.01}},{"i":3,"p":0.99,"id":"s3","own":true,"role":"result","text":"The difference between the area of the perturbed and the unperturbed horizon is related to the energy of matter crossing the horizon.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.8,"main_claim_p":0.15,"quantitative":false,"quantitative_p":0.13,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.99,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.0}},{"i":4,"p":0.42,"id":"s4","own":true,"role":"contribution","text":"We derive consistency conditions for the validity of our approximations, and compare our results to similar ones present in the literature.","hedge":{"p":0.95,"label":"asserted"},"own_p":0.94,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.13,"role_probabilities":{"gap":0.0,"method":0.36,"result":0.0,"background":0.0,"limitation":0.22,"future_work":0.0,"contribution":0.42,"interpretation":0.0}},{"i":5,"p":0.55,"id":"s5","own":true,"role":"interpretation","text":"Finally, we discuss how this setting can be used in perturbative quantum gravity to extend the classical mechanical laws to thermodynamic laws, with the entanglement of field 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