{"arxiv_id":"hep-ph/0401099","incoming":{"papers":33,"sentences":43,"groups":[{"kind":"comparison","label":"Compares with it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1608.02358","title":"Dynamics of neutrino lumps in growing neutrino quintessence","url":"/paper/1608.02358","section":"Introduction","sentence":"This differs from other mass varying neutrino cosmologies (usually known as MaVaN's) [ref] .","intent_p":0.81,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":17,"sentences":17,"quotes":[{"arxiv_id":"1108.3339","title":"Testing Nonstandard Neutrino Properties with a M\\\"ossbauer Oscillation Experiment","url":"/paper/1108.3339","section":"Introduction","sentence":"We will consider four scenarios: the possible presence of a light sterile neutrino, mixing with a Kaluza-Klein tower of sterile neutrinos in a model with large extra dimensions (LED) [ref] , nonstandard quantum decoherence (NQD) [ref] , and a model with the so called mass varying neutrinos (MaVaN) [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"2606.12915","title":"Mass Varying Neutrino Oscillation in Teleparallel Gravity","url":"/paper/2606.12915","section":"Introduction","sentence":"Additionally, it is essential to explore whether other types of interactions, particularly those mediated by scalar fields, could produce analogous or competing effects in the calculations of neutrino oscillations [ref] .","intent_p":0.86,"contests_p":null},{"arxiv_id":"2412.20766","title":"Probing Long-Range Forces Between Neutrinos with Cosmic Structures","url":"/paper/2412.20766","section":"Introduction","sentence":"Indeed, the cosmological influence of long-range forces between neutrinos has been considered in the past [ref] .","intent_p":0.83,"contests_p":null},{"arxiv_id":"0709.1128","title":"Adiabatic instability in coupled dark energy-dark matter models","url":"/paper/0709.1128","section":"Mass Varying Neutrino (“MaVaN”) models","sentence":"The impact of adiabatic instabilities has been discussed extensively in the context of MaVaN models, in which the light mass of the neutrino and the recent accelerative era are twinned together through a scalar field coupling [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2601.19550","title":"Testing Modified Teleparallel Gravity by Neutrino Oscillations","url":"/paper/2601.19550","section":"Introduction","sentence":"In these models [ref] , neutrinos and a scalar field are linked by the neutrino mass, which has roots in the dark energy model.","intent_p":0.85,"contests_p":null}]}],"unlabelled_sentences":25},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"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/hep-ph/0401099"}}