{"paper":{"title":"Radion Dynamics and Electroweak Physics","arxiv_id":"hep-th/0008151","primary_cat":"hep-th","submitted_at":"2000-08-18T21:24:08+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. No sentence in this record was written by a language model.","schema":"pith.compiled-record/v0","status":"compiled","abstract":{"source":"arXiv listing abstract v2","sentences":[{"i":0,"p":0.99,"id":"s0","own":true,"role":"contribution","text":"The dynamics of a stabilized radion in the Randall-Sundrum model (RS) with two branes is investigated, and the effects of the radion on electroweak precision observables are evaluated.","hedge":{"p":0.95,"label":"asserted"},"own_p":0.91,"main_claim_p":0.14,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.0,"background":0.01,"limitation":0.0,"future_work":0.0,"contribution":0.99,"interpretation":0.0}},{"i":1,"p":0.92,"id":"s1","own":false,"role":"method","text":"The radius is assumed to be stabilized using a bulk scalar field as suggested by Goldberger and Wise.","hedge":{"p":0.83,"label":"asserted"},"own_p":0.18,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.92,"result":0.0,"background":0.07,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.0}},{"i":2,"p":0.82,"id":"s2","own":true,"role":"result","text":"First the mass and the wavefunction of the radion is determined including the backreaction of the bulk stabilization field on the metric, giving a typical radion mass of order the weak scale.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.91,"main_claim_p":0.13,"quantitative":true,"quantitative_p":0.79,"role_probabilities":{"gap":0.0,"method":0.04,"result":0.82,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.14,"interpretation":0.0}},{"i":3,"p":0.99,"id":"s3","own":true,"role":"method","text":"This is demonstrated by a perturbative computation of the radion wavefunction.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.88,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.04,"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":4,"p":0.97,"id":"s4","own":true,"role":"result","text":"A consequence of the background configuration for the scalar field is that after including the backreaction the Kaluza-Klein (KK) states of the bulk scalars couple directly to the Standard Model fields on the TeV brane.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.74,"main_claim_p":0.09,"quantitative":false,"quantitative_p":0.07,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.97,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.02}},{"i":5,"p":0.93,"id":"s5","own":true,"role":"result","text":"Some cosmological implications are discussed, and in particular it is found that the shift in the radion at late times is in agreement with the four-dimensional effective theory result.","hedge":{"p":0.96,"label":"asserted"},"own_p":0.91,"main_claim_p":0.08,"quantitative":false,"quantitative_p":0.31,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.93,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.04,"interpretation":0.03}},{"i":6,"p":0.83,"id":"s6","own":true,"role":"method","text":"The effect of the radion on the oblique parameters is evaluated using an effective theory approach.","hedge":{"p":0.94,"label":"asserted"},"own_p":0.92,"main_claim_p":0.08,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.83,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.17,"interpretation":0.0}},{"i":7,"p":1.0,"id":"s7","own":true,"role":"result","text":"In the absence of a curvature-scalar Higgs mixing operator, these corrections are small and give a negative contribution to S.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.84,"main_claim_p":0.17,"quantitative":false,"quantitative_p":0.44,"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":8,"p":0.98,"id":"s8","own":true,"role":"result","text":"In the presence of such a mixing operator, however, the corrections can be sizable due to the modified Higgs and radion couplings.","hedge":{"p":0.74,"label":"hedged_possibility"},"own_p":0.78,"main_claim_p":0.17,"quantitative":false,"quantitative_p":0.28,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.98,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.02}}]},"compiled":{"main_claim":{"p":0.62,"text":"In the presence of such a mixing operator, however, the corrections can be sizable due to the modified Higgs and radion couplings.","location":"abstract s8","hedge_strength":{"p":0.74,"label":"hedged 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