{"arxiv_id":"2502.14981","incoming":{"papers":1,"sentences":1,"groups":[{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2608.21120","title":"New Limits on $n \\rightarrow n'$ Transformation from HFIR Cold Neutron Beam","url":"/paper/2608.21120","section":"Introduction","sentence":"The Mirror Matter model of dark matter [ref] posits that neutron can be a state of a mixture of an ordinary neutron and a mirror neutron $(n,n')^T$ [ref] .","intent_p":0.92,"contests_p":null}]}],"unlabelled_sentences":0},"outgoing":{"papers":15,"sentences":26,"groups":[{"kind":"data_used","label":"Uses data or values from","papers":2,"sentences":3,"quotes":[{"arxiv_id":"1807.06209","title":"Planck 2018 results. VI. Cosmological parameters","url":"/paper/1807.06209","section":"7.3 Dark radiation and $ΔN_eff$","sentence":"The current bound on $ΔN_eff < 0.284$ at 95% C.L. from Planck data [ref] then implies $Br < 0.041$.","intent_p":1.0,"contests_p":null},{"arxiv_id":"astro-ph/0309303","title":"Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56","url":"/paper/astro-ph/0309303","section":"8. Self-interacting Dark Matter (SIDM) and massive mirror photon","sentence":"The bullet cluster bound [ref] on SIDM is $σ_DM-DM/m_DM≤1 cm^2/ g≃1.8×10^-24 cm^2$/GeV.","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":10,"sentences":13,"quotes":[{"arxiv_id":"2008.04339","title":"A Minimal Approach to Baryogenesis via Affleck-Dine and Inflaton Mass Terms","url":"/paper/2008.04339","section":"5. Baryon-Dark matter coincidence","sentence":"The various subsequent stages in the evolution of $Φ$ in the universe leading to leptogenesis are as follows [ref] :","intent_p":0.93,"contests_p":null},{"arxiv_id":"2107.01514","title":"Affleck-Dine Baryogenesis with Observable Neutron-Anti-Neutron Oscillation","url":"/paper/2107.01514","section":"5. Baryon-Dark matter coincidence","sentence":"The various subsequent stages in the evolution of $Φ$ in the universe leading to leptogenesis are as follows [ref] :","intent_p":0.93,"contests_p":null},{"arxiv_id":"1809.08108","title":"Affleck-Dine baryogenesis via mass splitting","url":"/paper/1809.08108","section":"5. Baryon-Dark matter coincidence","sentence":"To discuss this, we first briefly review the evolution of inflaton and the AD-field $Φ$ [ref] in the early universe.","intent_p":0.95,"contests_p":null},{"arxiv_id":"1909.12300","title":"Affleck-Dine inflation","url":"/paper/1909.12300","section":"5. Baryon-Dark matter coincidence","sentence":"To discuss this, we first briefly review the evolution of inflaton and the AD-field $Φ$ [ref] in the early universe.","intent_p":0.95,"contests_p":null},{"arxiv_id":"1309.0007","title":"Baryogenesis from the Inflaton Field","url":"/paper/1309.0007","section":"5. Baryon-Dark matter coincidence","sentence":"To discuss this, we first briefly review the evolution of inflaton and the AD-field $Φ$ [ref] in the early universe.","intent_p":0.95,"contests_p":null}]}],"unlabelled_sentences":10},"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/2502.14981"}}