{"arxiv_id":"1403.2608","incoming":{"papers":6,"sentences":6,"groups":[{"kind":"background","label":"Cites it as background","papers":4,"sentences":4,"quotes":[{"arxiv_id":"1705.10054","title":"Thermal Sunyaev-Zel'dovich effect in the intergalactic medium with primordial magnetic fields","url":"/paper/1705.10054","section":"Introduction","sentence":"Many authors have discussed the observational constraints on PMFs from the Thomson optical depth [ref] , 21 cm anisotropies [ref] , cosmic shear [ref] , and galaxy surveys [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"2411.00089","title":"Does it matter? A more careful treatment of density fluctuations in 21-cm simulations","url":"/paper/2411.00089","section":"Introduction","sentence":"This exciting signal has the potential to expand our knowledge on the formation mechanism of the first galaxies [ref] , the thermal history of the intergalactic medium (IGM) [ref] , the epoch of reionization [ref] , physics beyond the standard model [ref] , and possibly shed some light on the nature of dark matter [ref] .","intent_p":0.88,"contests_p":null},{"arxiv_id":"1408.2571","title":"The Effects of Dark Matter-Baryon Scattering on Redshifted 21 cm Signals","url":"/paper/1408.2571","section":"Introduction","sentence":"There have been related paper s investigating the 21 cm signal due to energy injection during the dark ages including the dissipation of magnetic fields [ref] , energy injection from primordial black holes [ref] , and the decay or annihilation of dark matter [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"2403.16763","title":"LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields","url":"/paper/2403.16763","section":"Introduction","sentence":"Connected to the impact on large-scale structure, but observed at an earlier stage when structures are not yet fully nonlinear, the 21-cm signal [ref] offers interesting perspectives for forthcoming radio observatories.","intent_p":0.95,"contests_p":null}]}],"unlabelled_sentences":2},"outgoing":{"papers":13,"sentences":23,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":2,"sentences":2,"quotes":[{"arxiv_id":"astro-ph/9909275","title":"A New Calculation of the Recombination Epoch","url":"/paper/astro-ph/9909275","section":"Temperature and ionization evolution of IGM gas","sentence":"For these coefficients and $C$, we refer to Refs. [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"astro-ph/9912182","title":"How exactly did the Universe become neutral?","url":"/paper/astro-ph/9912182","section":"Temperature and ionization evolution of IGM gas","sentence":"For these coefficients and $C$, we refer to Refs. [ref] .","intent_p":0.87,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":10,"sentences":12,"quotes":[{"arxiv_id":"astro-ph/0405413","title":"Primordial Magnetic Fields in the Post-recombination Era and Early Reionization","url":"/paper/astro-ph/0405413","section":"Theory of ambipolar diffusion in the dark age","sentence":"This process is the so-called ambipolar diffusion [ref] and can happen at the late-time Universe in the dark age under the presence of electrically neutral particles [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"astro-ph/0607169","title":"Probing Primordial Magnetic Fields with the 21cm Fluctuations","url":"/paper/astro-ph/0607169","section":"Introduction","sentence":"In particular, Refs. [ref] have investigated these global effect on the 21cm signals.","intent_p":0.87,"contests_p":null},{"arxiv_id":"astro-ph/0512626","title":"The early reionization with the primordial magnetic fields","url":"/paper/astro-ph/0512626","section":"Introduction","sentence":"The global effects of the heating from primordial magnetic fields have already been studied in Refs. [ref] .","intent_p":0.95,"contests_p":null},{"arxiv_id":"astro-ph/0603631","title":"Cosmological Magnetic Field: a fossil of density perturbations in the early universe","url":"/paper/astro-ph/0603631","section":"Introduction","sentence":"A variety of mechanisms to generate the primordial magnetic fields have been proposed, which include inflation with a break of conformal invariance [ref] , effects at phase transitions in the early Universe [ref] , and cosmological vector modes in first and/or second order cosmological perturbations [ref] .","intent_p":1.0,"contests_p":null},{"arxiv_id":"astro-ph/0701329","title":"Magnetic Field Spectrum at Cosmological Recombination","url":"/paper/astro-ph/0701329","section":"Introduction","sentence":"A variety of mechanisms to generate the primordial magnetic fields have been proposed, which include inflation with a break of conformal invariance [ref] , effects at phase transitions in the early Universe [ref] , and cosmological vector modes in first and/or second order cosmological perturbations [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":9},"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/1403.2608"}}