{"arxiv_id":"2308.07166","incoming":{"papers":7,"sentences":8,"groups":[{"kind":"background","label":"Cites it as background","papers":5,"sentences":6,"quotes":[{"arxiv_id":"2406.08728","title":"Exploring Faraday rotation signatures and population bounds for primordial magnetic black holes","url":"/paper/2406.08728","section":"Introduction","sentence":"In recent times, the last of these proposed candidates—PBHs—have been of significant interest [ref] .","intent_p":0.93,"contests_p":null},{"arxiv_id":"2606.17617","title":"Synergy between CSST and future gravitational-wave detectors: Probing primordial black holes by cross-correlating dark sirens with galaxies","url":"/paper/2606.17617","section":"Introduction","sentence":"The black holes in these mergers may have two distinct origins: astrophysical black holes (ABHs) formed through stellar evolution [ref] , and primordial black holes (PBHs) formed in the early universe when enhanced curvature perturbations re-entered the horizon and collapsed [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2605.21281","title":"Self-Consistent Parker Bound on Magnetic Monopoles","url":"/paper/2605.21281","section":"Introduction","sentence":"Cosmological phase transitions [ref] can produce them through the Kibble or Kibble-Zurek mechanism [ref] , with their surviving abundance determined by phase transition dynamics and defect evolution [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"2401.00555","title":"The primordial black holes solution to the cosmological monopole problem","url":"/paper/2401.00555","section":"Summary and discussion","sentence":"Note added — As this work was nearing completion, we found new papers discussing similar topics on Arxiv [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"2404.04926","title":"On the cosmological abundance of magnetic monopoles","url":"/paper/2404.04926","section":"Conclusion","sentence":"The subsequent evolution of their abundance depends on a number of issues such as monopole annihilation, capture by primordial black holes [ref] , and interaction with other topological defects [ref] .","intent_p":0.94,"contests_p":null}]}],"unlabelled_sentences":2},"outgoing":{"papers":69,"sentences":91,"groups":[{"kind":"contests","label":"Contests","papers":1,"sentences":2,"quotes":[{"arxiv_id":"hep-ph/0403248","title":"A black hole solution to the cosmological monopole problem","url":"/paper/hep-ph/0403248","section":"Modelling of diffusive monopole capture by PBHs","sentence":"Ref. 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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/2308.07166"}}