{"arxiv_id":"1403.6327","incoming":{"papers":14,"sentences":15,"groups":[{"kind":"background","label":"Cites it as background","papers":6,"sentences":6,"quotes":[{"arxiv_id":"1312.5637","title":"Model-dependent estimate on the connection between fast radio bursts and ultra-high energy cosmic rays","url":"/paper/1312.5637","section":"Introduction","sentence":"Currently quite a few models have been proposed to interpret FRBs, including the mergers of binary neutron stars [ref] , energetic magnetar radio flares [ref] , delayed collapses of supramassive neutron stars (SMNS) to black holes (i.e., the so-called blitzar model [ref] , a highly relevant hypothesis is the possible connection between Gamma-ray Bursts and FRBs [ref] ), mergers of binary white dwarfs [ref] , and flaring stars if FRBs are instead in the Galaxy [ref] .","intent_p":0.98,"contests_p":null},{"arxiv_id":"2106.10235","title":"The Gravitational-Wave Physics II: Progress","url":"/paper/2106.10235","section":"Constraints on the neutron star maximum mass from GW170817","sentence":"Depending on the size relationship between the merger remnant (gravitational) mass and the maximum mass of a single NS, a BNS merger can give a variety of post-merger products [ref] : (1) a black hole (BH) by immediate collapse after the merger; (2) a differential rotation supported hypermassive NS (HMNS), which would survive $10∼100$ ms before collapsing; (3) a rigid rotation supported supermassive NS (SMNS), which would collapse after the NS spins down; and (4) a stable NS (SNS).","intent_p":0.85,"contests_p":null},{"arxiv_id":"2408.02534","title":"Quantifying the coincidence between gravitational waves and fast radio bursts from neutron star - black hole mergers","url":"/paper/2408.02534","section":"Introduction","sentence":"A long-lived neutron star can dissipate energy in different ways, either through magnetic flaring activities or via the blitzar mechanism upon collapse [ref] .","intent_p":0.81,"contests_p":null},{"arxiv_id":"2310.12463","title":"Piecewise frequency model for searches for long-transient gravitational waves from young neutron stars","url":"/paper/2310.12463","section":"Introduction","sentence":"The remnant object after coalescence may: i) immediately collapse into a black hole; ii) form a hypermassive neutron star before collapsing into a black hole; iii) form a supramassive neutron star before collapsing into a black hole; or iv) form a stable long-lived neutron star [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"2101.01091","title":"The failure of the Fisher Matrix when including tidal terms: Considering construction of template banks of tidally deformed binary neutron stars","url":"/paper/2101.01091","section":"Neutron stars are not black holes","sentence":"Will a short-lived hypermassive neutron star be formed, emitting gravitational radiation before collapsing to a black hole [ref] ?","intent_p":0.9,"contests_p":null}]}],"unlabelled_sentences":9},"outgoing":{"papers":6,"sentences":9,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1309.6635","title":"The Neutron Star Mass Distribution","url":"/paper/1309.6635","section":"Predicting supramassive neutron star collapse times","sentence":"From [ref] , $M_BNS∼N(μ_BNS=1.32 M_⊙,σ_BNS=0.11)$, where $N(μ_BNS,σ_BNS)$ specifies a normal distribution with mean $μ_BNS$ and standard deviation $σ_BNS$.","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"1307.1409","title":"Fast radio bursts: the last sign of supramassive neutron stars","url":"/paper/1307.1409","section":"Introduction","sentence":"Numerous physical mechanisms have been suggested to produce FRBs at cosmological distances, including magnetar hyperflares [ref] , binary white dwarf [ref] or neutron star [ref] mergers, and the collapse of supramassive NSs to form black holes [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"1307.4924","title":"Millisecond extragalactic radio bursts as magnetar flares","url":"/paper/1307.4924","section":"Introduction","sentence":"Numerous physical mechanisms have been suggested to produce FRBs at cosmological distances, including magnetar hyperflares [ref] , binary white dwarf [ref] or neutron star [ref] mergers, and the collapse of supramassive NSs to form black holes [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"1307.4985","title":"Cosmological Fast Radio Bursts from Binary Neutron Star Mergers","url":"/paper/1307.4985","section":"Introduction","sentence":"Numerous physical mechanisms have been suggested to produce FRBs at cosmological distances, including magnetar hyperflares [ref] , binary white dwarf [ref] or neutron star [ref] mergers, and the collapse of supramassive NSs to form black holes [ref] .","intent_p":0.95,"contests_p":null}]}],"unlabelled_sentences":5},"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/1403.6327"}}