{"arxiv_id":"astro-ph/9912180","incoming":{"papers":16,"sentences":21,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1505.06028","title":"Spectral distortions of the CMB dipole","url":"/paper/1505.06028","section":"Introduction","sentence":"The amplitude of these signals is more uncertain, but even within our standard cosmological paradigm, one expects an average $y$-parameter of $y≃10^-7-10^-6$ due to the large-scale structure and the reionization epoch [ref] , with the most recent computations giving $y≃2-6$ [ref] .","intent_p":0.91,"contests_p":null},{"arxiv_id":"2502.05188","title":"The Cosmic Microwave Background: Spectral Distortions","url":"/paper/2502.05188","section":"Reionization and structure formation","sentence":"Several estimates for this contribution were obtained, yielding values for the total $y$-parameter at the level $y≃few-6$ [ref] .","intent_p":0.88,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":5,"sentences":6,"quotes":[{"arxiv_id":"2105.15043","title":"Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation","url":"/paper/2105.15043","section":"The density-weighted mean electron temperature Te","sentence":"The mean electron pressure $⟨P_e⟩$ is related to the density-weighted mean temperature of electrons in the universe, defined as $T̅_e ≡⟨n_eT_e⟩/⟨n_e⟩$ [ref] .","intent_p":0.96,"contests_p":null},{"arxiv_id":"1505.00781","title":"Limits on the fluctuating part of $y$-type distortion monopole from Planck and SPT results","url":"/paper/1505.00781","section":"Introduction","sentence":"The contribution from the peaks in the large scale structure and the effect of baryonic physics to the $y$-type distortion fluctuations has been studied by many groups using numerical simulations as well as analytically [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"1712.04583","title":"CMB Spectral $\\mu$-Distortion of Multiple Inflation Scenario","url":"/paper/1712.04583","section":"Introduction","sentence":"However, we have many astrophyscial/cosmological sources inducing spectral distortions: decaying or annihilating particles [ref] , reionization and structure formation [ref] , primordial black holes [ref] , cosmic strings [ref] , small-scale magnetic fields [ref] , the adiabatic cooling of matter [ref] , cosmological recombination [ref] , gravitino decay [ref] , and the dissipation of primordial density perturbations [ref] which is the main concern of this paper.","intent_p":0.94,"contests_p":null},{"arxiv_id":"1705.02741","title":"CMB Spectral Distortion Constraints on Thermal Inflation","url":"/paper/1705.02741","section":"Introduction","sentence":"However, there are many possible sources of energy release that could affect the CMB energy spectrum and lead to spectral distortions, including the dissipation of primordial density perturbations [ref] , reionization and structure formation [ref] , decaying or annihilating particles [ref] , cosmic strings [ref] , primordial black holes [ref] , small-scale magnetic fields [ref] , the adiabatic cooling of matter [ref] , cosmological recombination [ref] and gravitino decay [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"1512.04816","title":"Another look to distortions of the CMB spectrum","url":"/paper/1512.04816","section":"Introduction","sentence":"The evolution of distorted spectra and constraints on processes that can produce them have been investigated, both analytically and numerically, by numerous subsequent studies [ref] .","intent_p":0.98,"contests_p":null}]}],"unlabelled_sentences":13},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"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/astro-ph/9912180"}}