{"arxiv_id":"1003.0905","incoming":{"papers":27,"sentences":46,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1308.5693","title":"Angular Power Spectrum of B-mode Polarization from Cosmic String Wakes","url":"/paper/1308.5693","section":"Polarization Signal of a Cosmic String Wake","sentence":"This accretion process can be studied [ref] by means of the Zel'dovich approximation [ref] with the result that the comoving distance $q_nl(t, t_i)$ from the central plane of the wake which is beginning to fall in at time $t > t_i$ is given by [ref]","intent_p":0.92,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":2,"quotes":[{"arxiv_id":"1401.4619","title":"Probing Particle Physics from Top Down with Cosmic Strings","url":"/paper/1401.4619","section":"CMB Polarization Patterns from a Cosmic String Wake","sentence":"Inserting numbers, the result is [ref]","intent_p":0.89,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites it as support","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1603.05834","title":"Bouncing Cosmologies: Progress and Problems","url":"/paper/1603.05834","section":"Tilt of the Tensor Spectrum","sentence":"For example, cosmic strings can produce direct $B$-mode polarization [ref] .","intent_p":0.96,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":5,"sentences":6,"quotes":[{"arxiv_id":"2205.02725","title":"Signal of Cosmic Strings in Cross-Correlation of 21-cm Redshift and CMB Polarization Maps","url":"/paper/2205.02725","section":"Cosmic String Wake signature in CMB polarization","sentence":"In this section, we present a brief description of the polarisation signal from cosmic string wakes, the full derivation of which can be found in [ref] .","intent_p":0.83,"contests_p":null},{"arxiv_id":"2107.07289","title":"Extracting the Signal of Cosmic String Wakes from 21-cm Observations","url":"/paper/2107.07289","section":"Introduction","sentence":"The extra Thomson scattering in wakes thus leads to a characteristic CMB polarization signal [ref] , a rectangle in the sky with extra polarization (including a B-mode component).","intent_p":0.83,"contests_p":null},{"arxiv_id":"1608.05079","title":"Differentiating G-inflation from String Gas Cosmology using the Effective Field Theory Approach","url":"/paper/1608.05079","section":"Introduction","sentence":"B-mode polarization can originate from gravitational waves generated in the primordial epoch, or from vector and tensor perturbations at late times, such as in topological defect models [ref] .","intent_p":0.84,"contests_p":null},{"arxiv_id":"1403.4927","title":"Closed String Thermodynamics and a Blue Tensor Spectrum","url":"/paper/1403.4927","section":"Introduction","sentence":"Hence in the context of the simplest models, primordial B-mode polarization must be due to gravitational waves [Note, 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work, the conversion of E-mode to B-mode polarization via the gravitational lensing induced by cosmic strings was studied in [ref] [While this paper was being finalized for submission, a preprint appeared [ref] computing the local B-mode polarization power spectrum from cosmic strings.].","intent_p":0.86,"contests_p":null},{"arxiv_id":"astro-ph/9907103","title":"Reionization Revisited: Secondary CMB Anisotropies and Polarization","url":"/paper/astro-ph/9907103","section":"Analysis","sentence":"If unpolarized cosmic microwave background radiation with a quadrupolar anisotropy scatters off free electrons, then the scattered radiation is polarized (see e.g. [ref] for reviews of the theory of CMB polarization).","intent_p":1.0,"contests_p":null},{"arxiv_id":"astro-ph/9505031","title":"ACCRETION OF HOT DARK MATTER ONTO SLOWLY MOVING COSMIC STRINGS","url":"/paper/astro-ph/9505031","section":"Cosmic String Wakes","sentence":"The gravitational accretion onto string filaments was studied in 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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/1003.0905"}}