{"paper":{"title":"General-relativistic electromagnetic fields around a slowly rotating neutron star: time-dependent pseudo-spectral simulations","arxiv_id":"1401.1367","primary_cat":"astro-ph.HE","submitted_at":"2014-01-07T13:27:33+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. 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effects.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.06,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.11,"role_probabilities":{"gap":1.0,"method":0.0,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":2,"p":0.95,"id":"s2","own":false,"role":"background","text":"Estimates are usually given according to the flat spacetime magnetodipole formula.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.04,"main_claim_p":0.02,"quantitative":false,"quantitative_p":0.07,"role_probabilities":{"gap":0.05,"method":0.0,"result":0.0,"background":0.95,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":3,"p":0.98,"id":"s3","own":true,"role":"contribution","text":"The present paper pursue our effort to look for accurate solutions of the general-relativistic electromagnetic field around a slowly rotating magnetized neutron star.","hedge":{"p":0.87,"label":"asserted"},"own_p":0.58,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.0,"background":0.02,"limitation":0.0,"future_work":0.0,"contribution":0.98,"interpretation":0.0}},{"i":4,"p":0.88,"id":"s4","own":true,"role":"background","text":"In a previous work, we already found approximate stationary solutions to this problem.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.88,"main_claim_p":0.02,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.01,"method":0.0,"result":0.0,"background":0.88,"limitation":0.01,"future_work":0.0,"contribution":0.1,"interpretation":0.0}},{"i":5,"p":0.79,"id":"s5","own":true,"role":"contribution","text":"Here we address again this problem but using a more general approach.","hedge":{"p":0.95,"label":"asserted"},"own_p":0.55,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.08,"result":0.0,"background":0.13,"limitation":0.0,"future_work":0.0,"contribution":0.79,"interpretation":0.0}},{"i":6,"p":0.82,"id":"s6","own":true,"role":"method","text":"We indeed solve the full set of time-dependent Maxwell equations in a curved vacuum space-time following the 3+1 formalism.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.94,"main_claim_p":0.09,"quantitative":false,"quantitative_p":0.09,"role_probabilities":{"gap":0.0,"method":0.82,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.18,"interpretation":0.0}},{"i":7,"p":1.0,"id":"s7","own":true,"role":"method","text":"The numerical code is based on our pseudo-spectral method exposed in a previous paper for flat space-time.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.67,"main_claim_p":0.02,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":1.0,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.0}},{"i":8,"p":0.96,"id":"s8","own":true,"role":"method","text":"We adapted it to an arbitrary fixed background metric.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.9,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.96,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.04,"interpretation":0.0}},{"i":9,"p":0.5,"id":"s9","own":true,"role":"result","text":"Stationary solutions are readily obtained and compared to semi-analytical 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