{"paper":{"title":"Continuous Gravitational Waves and Magnetic Monopole Signatures from Single Neutron Stars","arxiv_id":"1909.12855","primary_cat":"hep-ph","submitted_at":"2019-09-27T18:00:35+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-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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fields of neutron stars, such as magnetars.","hedge":{"p":0.99,"label":"hedged_possibility"},"own_p":0.05,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.18,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.0,"background":0.97,"limitation":0.0,"future_work":0.0,"contribution":0.03,"interpretation":0.0}},{"i":4,"p":0.68,"id":"s4","own":false,"role":"background","text":"This non-perturbative production furnishes a new, direct dissipative mechanism for the neutron star magnetic fields.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.09,"main_claim_p":0.06,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.01,"method":0.01,"result":0.03,"background":0.68,"limitation":0.0,"future_work":0.0,"contribution":0.08,"interpretation":0.19}},{"i":5,"p":0.59,"id":"s5","own":false,"role":"interpretation","text":"Through their consequent effect on the magnetic-field-induced quadrupole ellipticity, they may then potentially leave imprints in the early stage 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