{"paper":{"title":"Fluxbrane Inflation","arxiv_id":"1104.5016","primary_cat":"hep-th","submitted_at":"2011-04-26T20:00:03+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-1.13-20260917 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 v3","sentences":[{"i":0,"p":0.99,"id":"s0","own":true,"role":"contribution","text":"As a first step towards inflation in genuinely F-theoretic setups, we propose a scenario where the inflaton is the relative position of two 7-branes on holomorphic 4-cycles.","hedge":{"p":0.36,"label":"asserted"},"own_p":0.83,"main_claim_p":0.12,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.0,"method":0.01,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.99,"interpretation":0.0}},{"i":1,"p":0.5,"id":"s1","own":false,"role":"result","text":"Non-supersymmetric gauge flux induces an attractive inter-brane potential.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.42,"main_claim_p":0.06,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.13,"result":0.5,"background":0.04,"limitation":0.0,"future_work":0.0,"contribution":0.33,"interpretation":0.0}},{"i":2,"p":0.95,"id":"s2","own":true,"role":"result","text":"The latter is sufficiently flat in the supergravity regime of large volume moduli.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.64,"main_claim_p":0.06,"quantitative":false,"quantitative_p":0.19,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.95,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.04}},{"i":3,"p":0.71,"id":"s3","own":true,"role":"interpretation","text":"Thus, in contrast to brane-antibrane inflation, fluxbrane inflation does not require warping.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.55,"main_claim_p":0.18,"quantitative":false,"quantitative_p":0.42,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.28,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.71}},{"i":4,"p":0.9,"id":"s4","own":true,"role":"method","text":"We calculate the inflaton potential both in the supergravity approximation and via an open-string one-loop computation on toroidal backgrounds.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.96,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.0,"method":0.9,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.1,"interpretation":0.0}},{"i":5,"p":0.88,"id":"s5","own":true,"role":"future_work","text":"This leads us to propose a generalisation to genuine Calabi-Yau manifolds.","hedge":{"p":0.48,"label":"hedged_possibility"},"own_p":0.67,"main_claim_p":0.1,"quantitative":false,"quantitative_p":0.02,"role_probabilities":{"gap":0.0,"method":0.01,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.88,"contribution":0.06,"interpretation":0.04}},{"i":6,"p":0.65,"id":"s6","own":true,"role":"contribution","text":"We also comment on competing F-term effects.","hedge":{"p":0.8,"label":"unclear"},"own_p":0.6,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.03,"result":0.01,"background":0.01,"limitation":0.24,"future_work":0.03,"contribution":0.65,"interpretation":0.03}},{"i":7,"p":0.71,"id":"s7","own":true,"role":"result","text":"The end of inflation is marked by the condensation of tachyonic recombination fields between the 7-branes, triggering the formation of a bound state described as a stable extension along the 7-brane divisor.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.72,"main_claim_p":0.18,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.71,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.12,"interpretation":0.15}},{"i":8,"p":0.99,"id":"s8","own":true,"role":"interpretation","text":"Hence our model fits in the framework of hybrid D-term inflation.","hedge":{"p":0.87,"label":"asserted"},"own_p":0.57,"main_claim_p":0.25,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.99}},{"i":9,"p":0.98,"id":"s9","own":true,"role":"contribution","text":"We work out the main phenomenological properties of our D-term inflaton potential.","hedge":{"p":0.95,"label":"asserted"},"own_p":0.94,"main_claim_p":0.09,"quantitative":false,"quantitative_p":0.02,"role_probabilities":{"gap":0.0,"method":0.01,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.98,"interpretation":0.0}},{"i":10,"p":0.79,"id":"s10","own":true,"role":"result","text":"In particular, our scenario of D7/D7 inflation avoids the familiar observational constraints associated with cosmic strings.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.77,"main_claim_p":0.23,"quantitative":false,"quantitative_p":0.1,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.79,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.2}}]},"compiled":{"main_claim":{"p":0.36,"text":"In particular, our scenario of D7/D7 inflation avoids the familiar observational constraints associated with cosmic strings.","location":"abstract 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