FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3126044598> ?p ?o ?g. }

• W3126044598 endingPage "300" @default.
• W3126044598 startingPage "289" @default.
• W3126044598 abstract "Lyman-limit absorption systems can play many important roles during and after cosmological reionization. Unfortunately, due to the prohibitively large dynamic range required, it is impossible to self-consistently include these systems in cosmological simulations. Using fast and versatile seminumeric simulations, we systematically explore the spatial distribution of absorption systems during and following reionization. We self-calibrate the resulting number of absorbers to the mean free path (mfp) of the ionizing ultraviolet background (UVB), and present results at a given mfp and neutral hydrogen fraction. We use a simple optical depth criterion to identify the locations of absorbers. Our approach is fairly robust to uncertainties such as missing subgrid structure. Unlike at lower redshifts where the UVB is relatively uniform, at higher redshifts the fluctuations in the UVB and the H ii morphology of reionization can drive the large-scale distribution of absorption systems. Specifically, we find that absorbers are highly correlated with the density field on small scales, and then become anti-correlated with the UVB on large scales. After reionization, the large-scale power spectrum of the absorbers traces the UVB power spectrum, which can be predicted with a simple analytic extension of the halo model. During reionization, absorbers tend to preferentially lie inside overdensities (i.e. filaments) of the recently ionized intergalactic medium. Absorbers may also dominate the small-scale (k≳ 1 Mpc−1) 21-cm power during and after reionization. Conversely, they smooth the contrast on moderate scales. Once the H ii regions grow to surpass the mfp, the absorbers add to the large-scale 21-cm power. Our results should prove useful in interpreting future observations of the reionization epoch." @default.
• W3126044598 created "2021-02-01" @default.
• W3126044598 creator A5026171348 @default.
• W3126044598 creator A5047666459 @default.
• W3126044598 creator A5070588335 @default.
• W3126044598 creator A5071294469 @default.
• W3126044598 date "2010-10-25" @default.
• W3126044598 modified "2023-10-02" @default.
• W3126044598 title "The distribution of Lyman-limit absorption systems during and after reionization" @default.
• W3126044598 cites W1496755246 @default.
• W3126044598 cites W1690489517 @default.
• W3126044598 cites W1731370316 @default.
• W3126044598 cites W1792022697 @default.
• W3126044598 cites W1936459059 @default.
• W3126044598 cites W1966022526 @default.
• W3126044598 cites W1968869120 @default.
• W3126044598 cites W1970323694 @default.
• W3126044598 cites W1971162484 @default.
• W3126044598 cites W1975679485 @default.
• W3126044598 cites W1976791843 @default.
• W3126044598 cites W1980993402 @default.
• W3126044598 cites W1984479246 @default.
• W3126044598 cites W1985869482 @default.
• W3126044598 cites W1990996854 @default.
• W3126044598 cites W1998577648 @default.
• W3126044598 cites W2001085255 @default.
• W3126044598 cites W2003182532 @default.
• W3126044598 cites W2008380968 @default.
• W3126044598 cites W2009327527 @default.
• W3126044598 cites W2018719255 @default.
• W3126044598 cites W2024914408 @default.
• W3126044598 cites W2025549670 @default.
• W3126044598 cites W2026801727 @default.
• W3126044598 cites W2027643543 @default.
• W3126044598 cites W2027815038 @default.
• W3126044598 cites W2029085756 @default.
• W3126044598 cites W2034830951 @default.
• W3126044598 cites W2036818875 @default.
• W3126044598 cites W2038251620 @default.
• W3126044598 cites W2041013883 @default.
• W3126044598 cites W2049728682 @default.
• W3126044598 cites W2051357441 @default.
• W3126044598 cites W2051885722 @default.
• W3126044598 cites W2056653735 @default.
• W3126044598 cites W2056976797 @default.
• W3126044598 cites W2062492997 @default.
• W3126044598 cites W2066071309 @default.
• W3126044598 cites W2068368465 @default.
• W3126044598 cites W2071952242 @default.
• W3126044598 cites W2078734230 @default.
• W3126044598 cites W2079374409 @default.
• W3126044598 cites W2090655001 @default.
• W3126044598 cites W2099603107 @default.
• W3126044598 cites W2101025274 @default.
• W3126044598 cites W2115967849 @default.
• W3126044598 cites W2117105462 @default.
• W3126044598 cites W2127036548 @default.
• W3126044598 cites W2134203113 @default.
• W3126044598 cites W2140098883 @default.
• W3126044598 cites W2141806264 @default.
• W3126044598 cites W2147029159 @default.
• W3126044598 cites W2147638840 @default.
• W3126044598 cites W2148573472 @default.
• W3126044598 cites W2154152284 @default.
• W3126044598 cites W2154219156 @default.
• W3126044598 cites W2160253850 @default.
• W3126044598 cites W2161377637 @default.
• W3126044598 cites W2599720466 @default.
• W3126044598 cites W2617336294 @default.
• W3126044598 cites W3099863073 @default.
• W3126044598 cites W3101667439 @default.
• W3126044598 cites W3102672361 @default.
• W3126044598 cites W3104738275 @default.
• W3126044598 cites W3125389789 @default.
• W3126044598 cites W3125688855 @default.
• W3126044598 doi "https://doi.org/10.1111/j.1365-2966.2010.17680.x" @default.
• W3126044598 hasPublicationYear "2010" @default.
• W3126044598 type Work @default.
• W3126044598 sameAs 3126044598 @default.
• W3126044598 citedByCount "33" @default.
• W3126044598 countsByYear W31260445982012 @default.
• W3126044598 countsByYear W31260445982013 @default.
• W3126044598 countsByYear W31260445982014 @default.
• W3126044598 countsByYear W31260445982015 @default.
• W3126044598 countsByYear W31260445982016 @default.
• W3126044598 countsByYear W31260445982018 @default.
• W3126044598 countsByYear W31260445982019 @default.
• W3126044598 countsByYear W31260445982020 @default.
• W3126044598 countsByYear W31260445982021 @default.
• W3126044598 countsByYear W31260445982022 @default.
• W3126044598 crossrefType "journal-article" @default.
• W3126044598 hasAuthorship W3126044598A5026171348 @default.
• W3126044598 hasAuthorship W3126044598A5047666459 @default.
• W3126044598 hasAuthorship W3126044598A5070588335 @default.
• W3126044598 hasAuthorship W3126044598A5071294469 @default.
• W3126044598 hasBestOaLocation W31260445982 @default.
• W3126044598 hasConcept C105795698 @default.
• W3126044598 hasConcept C120665830 @default.

• next