{"paper":{"title":"CMB Imprints of a Pre-Inflationary Climbing Phase","arxiv_id":"1202.6630","primary_cat":"hep-th","submitted_at":"2012-02-29T18:13:04+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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exponential potential of \"brane SUSY breaking\" scenarios, and as a result the ensuing descent gives rise to an inflationary epoch that begins when the system is still well off its eventual attractor.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.12,"main_claim_p":0.09,"quantitative":false,"quantitative_p":0.16,"role_probabilities":{"gap":0.0,"method":0.2,"result":0.01,"background":0.76,"limitation":0.0,"future_work":0.0,"contribution":0.03,"interpretation":0.0}},{"i":2,"p":0.88,"id":"s2","own":false,"role":"result","text":"If a pre-inflationary climbing phase of this type had occurred within 6-7 e-folds of the horizon exit for the largest observable wavelengths, displacement off the attractor and initial-state effects would conspire to suppress power in the primordial scalar spectrum, enhancing it in the tensor spectrum and typically superposing oscillations on both.","hedge":{"p":0.81,"label":"hedged_possibility"},"own_p":0.29,"main_claim_p":0.71,"quantitative":true,"quantitative_p":0.96,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.88,"background":0.02,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.09}},{"i":3,"p":0.87,"id":"s3","own":true,"role":"contribution","text":"We investigate these imprints on CMB observables over a range of parameters, examine their statistical significance, and provide a semi-analytic rationale for our results.","hedge":{"p":0.84,"label":"asserted"},"own_p":0.96,"main_claim_p":0.06,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.13,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.87,"interpretation":0.0}},{"i":4,"p":1.0,"id":"s4","own":false,"role":"interpretation","text":"It is tempting to ascribe at least part of the large-angle anomalies in the CMB to pre-inflationary dynamics of this 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