{"arxiv_id":"2603.22246","incoming":{"papers":1,"sentences":1,"groups":[{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2604.25687","title":"Collective neutrino-antineutrino pair oscillations","url":"/paper/2604.25687","section":"Introduction","sentence":"These effects are of significant interest due to their potential impact on astrophysical explosions such as core-collapse supernovae and binary neutron star mergers, and have been under active investigation in recent years; see, e.g., [ref] .","intent_p":0.83,"contests_p":null}]}],"unlabelled_sentences":0},"outgoing":{"papers":13,"sentences":18,"groups":[{"kind":"background","label":"Cites as background","papers":5,"sentences":5,"quotes":[{"arxiv_id":"1001.2799","title":"Collective Neutrino Oscillations","url":"/paper/1001.2799","section":"Introduction","sentence":"This phenomenon is particularly interesting in core-collapse supernovae and neutron star mergers, where the extremely dense neutrino media can experience flavor oscillations collectively (see, e.g., [ref] for some reviews).","intent_p":0.99,"contests_p":null},{"arxiv_id":"1602.02766","title":"Collective neutrino flavor conversion: Recent developments","url":"/paper/1602.02766","section":"Introduction","sentence":"This phenomenon is particularly interesting in core-collapse supernovae and neutron star mergers, where the extremely dense neutrino media can experience flavor oscillations collectively (see, e.g., [ref] for some reviews).","intent_p":0.99,"contests_p":null},{"arxiv_id":"2011.01948","title":"New Developments in Flavor Evolution of a Dense Neutrino Gas","url":"/paper/2011.01948","section":"Introduction","sentence":"This phenomenon is particularly interesting in core-collapse supernovae and neutron star mergers, where the extremely dense neutrino media can experience flavor oscillations collectively (see, e.g., [ref] for some reviews).","intent_p":0.99,"contests_p":null},{"arxiv_id":"2301.11814","title":"Neutrinos from dense environments : Flavor mechanisms, theoretical approaches, observations, and new directions","url":"/paper/2301.11814","section":"Introduction","sentence":"This phenomenon is particularly interesting in core-collapse supernovae and neutron star mergers, where the extremely dense neutrino media can experience flavor oscillations collectively (see, e.g., [ref] for some reviews).","intent_p":0.99,"contests_p":null},{"arxiv_id":"2503.05959","title":"Neutrino Oscillations in Core-Collapse Supernovae and Neutron Star Mergers","url":"/paper/2503.05959","section":"Introduction","sentence":"This phenomenon is particularly interesting in core-collapse supernovae and neutron star mergers, where the extremely dense neutrino media can experience flavor oscillations collectively (see, e.g., [ref] for some reviews).","intent_p":0.99,"contests_p":null}]}],"unlabelled_sentences":13},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/2603.22246"}}