{"arxiv_id":"2009.01539","incoming":{"papers":6,"sentences":6,"groups":[{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2208.11186","title":"The amplification of cosmological magnetic fields in Extended $f(T,B)$ Teleparallel Gravity","url":"/paper/2208.11186","section":"Discussion and Conclusions","sentence":"Indeed, a direct link between PMFs (as constrained by the CMB anisotropy power spectra) and the nowadays cosmic magnetism was also confirmed by simulations [ref] .","intent_p":0.99,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":3,"sentences":3,"quotes":[{"arxiv_id":"2010.09729","title":"Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation","url":"/paper/2010.09729","section":"Introduction","sentence":"A similar – although smaller – investigation was carried out in [ref] and [ref] , where the impact of the primordial seed strength on the properties of galaxies has been studied in the context of a uniform seeding at $z ≳100$, and in [ref] , where the effects of the seed field power spectrum were investigated.","intent_p":0.81,"contests_p":null},{"arxiv_id":"2111.02704","title":"Distribution function of nuclei from $e^\\pm$ scattering in the presence of a strong primordial magnetic field","url":"/paper/2111.02704","section":"Introduction","sentence":"This PMF evolution depends upon the helicity and homogeneity of the magnetic fields [ref] , and its behavior in the late non-linear structure formation phase has been investigated in a number of recent three-dimensional simulations [ref] .","intent_p":0.83,"contests_p":null},{"arxiv_id":"2010.01805","title":"Synchrotron emission and neutral hydrogen in the simulated cosmic web","url":"/paper/2010.01805","section":"Other results and future perspectives","sentence":"The amplitude and topology of magnetic fields simulated for six different variations of input primoridal seed fields was also studied in detail in [ref] .","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":2},"outgoing":{"papers":2,"sentences":6,"groups":[{"kind":"method_or_tool","label":"Uses the method or tool of","papers":1,"sentences":3,"quotes":[{"arxiv_id":"2006.10063","title":null,"url":"/paper/2006.10063","section":"Global properties","sentence":"For the identification of up-stream magnetic field values and of the local shock propagation direction, we rely on our velocity-based shock finder [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":3},"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/2009.01539"}}