{"arxiv_id":"0708.1333","incoming":{"papers":1,"sentences":12,"groups":[{"kind":"contests","label":"Contests it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2107.00939","title":"Asymptotic quasinormal frequencies of different spin fields in $d$-dimensional spherically-symmetric black holes","url":"/paper/2107.00939","section":"Introduction","sentence":"Though Hod’s conjecture gained traction for several years, a possible link to a quantum theory of gravity was quickly proven tenuous when the $ln3$ result did not emerge for the 4D Reissner-Nordström BH in Refs. [ref] nor within other multi-horizon BHs inclusive or exclusive of a cosmological constant [ref] .","intent_p":0.57,"contests_p":0.78}]},{"kind":"comparison","label":"Compares with it","papers":1,"sentences":3,"quotes":[{"arxiv_id":"2107.00939","title":"Asymptotic quasinormal frequencies of different spin fields in $d$-dimensional spherically-symmetric black holes","url":"/paper/2107.00939","section":"Reissner-Nordström and extremal Reissner-Nordström BHs","sentence":"Although $ϑ→μ$ and $n →∞$ are also a set of non-commuting limits (just like $ϑ→0$ and $n →∞$), the extremal limit of the aQNF of the non-extremal Reissner-Nordström BH from Ref. [ref] agrees with the extremal limit of the aQNF for the extremal Reissner-Nordström BH calculated in Ref. [ref] .","intent_p":0.9,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2107.00939","title":"Asymptotic quasinormal frequencies of different spin fields in $d$-dimensional spherically-symmetric black holes","url":"/paper/2107.00939","section":"Introduction","sentence":"Within the highly-damped regime, the classical oscillations of a perturbed black hole (BH) known as quasinormal frequencies (QNFs) exhibit a linear, unbounded growth in the imaginary component $( 𝕀m {ω} )$ accompanied by a finite value for the real component $( ℝ e { ω} )$ [ref] .","intent_p":0.95,"contests_p":null}]}],"unlabelled_sentences":7},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[{"relation":"same_result","label":"States the same result","papers":[{"arxiv_id":"2403.13074","url":"/paper/2403.13074","title":"Calculating quasinormal modes of extremal and non-extremal Reissner-Nordstr\\\"om black holes with the continued fraction method","main_claim":"Our investigation further supports the idea that the extremal limit of the non-extremal case, where the charge approaches the mass of the black hole in natural units, leads to the same vibrational spectrum as in the extremal case despite the qualitative differences in their topology.","p":0.88}]}],"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/0708.1333"}}