{"paper":{"title":"Towards Axion Monodromy Inflation with Warped KK-Modes","arxiv_id":"1512.04463","primary_cat":"hep-th","submitted_at":"2015-12-14T19:05:26+00:00","version_compiled":"v3"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13.0 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 v3","sentences":[{"i":0,"p":0.98,"id":"s0","own":true,"role":"contribution","text":"We present a particularly simple model of axion monodromy: Our axion is the lowest-lying KK-mode of the RR-2-form-potential $C_2$ in the standard Klebanov-Strassler throat.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.84,"main_claim_p":0.11,"quantitative":false,"quantitative_p":0.15,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.98,"interpretation":0.0}},{"i":1,"p":0.63,"id":"s1","own":false,"role":"contribution","text":"One can think of this inflaton candidate as being defined by the integral of $C_2$ over the $S^2$ cycle of the throat.","hedge":{"p":0.75,"label":"hedged_possibility"},"own_p":0.34,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.27,"result":0.0,"background":0.01,"limitation":0.0,"future_work":0.0,"contribution":0.63,"interpretation":0.09}},{"i":2,"p":0.83,"id":"s2","own":true,"role":"result","text":"It obtains an exponentially small mass from the IR-region in which the $S^2$ shrinks to zero size both with respect to the Planck scale and the mass scale of local modes of the throat.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.6,"main_claim_p":0.07,"quantitative":true,"quantitative_p":0.77,"role_probabilities":{"gap":0.0,"method":0.03,"result":0.83,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.13,"interpretation":0.01}},{"i":3,"p":0.51,"id":"s3","own":false,"role":"contribution","text":"Crucially, the $S^2$ cycle has to be shared between two throats, such that the second locus where the $S^2$ shrinks is also in a warped region.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.49,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.14,"role_probabilities":{"gap":0.0,"method":0.43,"result":0.02,"background":0.0,"limitation":0.04,"future_work":0.0,"contribution":0.51,"interpretation":0.0}},{"i":4,"p":0.76,"id":"s4","own":true,"role":"result","text":"Well-known problems like the potentially dangerous back-reaction of brane/antibrane pairs and explicit supersymmetry breaking are not present in our scenario.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.52,"main_claim_p":0.09,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.76,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.11,"interpretation":0.13}},{"i":5,"p":0.83,"id":"s5","own":true,"role":"limitation","text":"However, the inflaton back-reaction starts to deform the geometry strongly once the field excursion approaches the Planck scale.","hedge":{"p":0.91,"label":"asserted"},"own_p":0.71,"main_claim_p":0.12,"quantitative":true,"quantitative_p":0.76,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.17,"background":0.0,"limitation":0.83,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":6,"p":0.74,"id":"s6","own":true,"role":"method","text":"We derive the system of differential equations required to treat this effect quantitatively.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.94,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.74,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.26,"interpretation":0.0}},{"i":7,"p":0.62,"id":"s7","own":false,"role":"future_work","text":"Numerical work is required to decide whether back-reaction makes the model suitable for realistic inflation.","hedge":{"p":0.85,"label":"asserted"},"own_p":0.3,"main_claim_p":0.09,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.0,"background":0.0,"limitation":0.36,"future_work":0.62,"contribution":0.0,"interpretation":0.0}},{"i":8,"p":0.68,"id":"s8","own":true,"role":"interpretation","text":"While we have to leave this crucial issue to future studies, we find it interesting that such a simple and explicit stringy monodromy model allows an originally sub-Planckian axion to go through many periods with full quantitative control before back-reaction becomes strong.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.91,"main_claim_p":0.46,"quantitative":true,"quantitative_p":0.79,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.12,"background":0.0,"limitation":0.1,"future_work":0.09,"contribution":0.01,"interpretation":0.68}},{"i":9,"p":0.56,"id":"s9","own":true,"role":"interpretation","text":"Also, the mere existence of our 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