Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23540
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Massara, Elena | en_US |
dc.contributor.author | Villaescusa-Navarro, Francisco | en_US |
dc.contributor.author | VIEL, MATTEO | en_US |
dc.contributor.author | Sutter, P. M. | en_US |
dc.date.accessioned | 2020-03-25T15:04:55Z | - |
dc.date.available | 2020-03-25T15:04:55Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 1475-7516 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23540 | - |
dc.description.abstract | Cosmic voids are a promising environment to characterize neutrino-induced effects on the large-scale distribution of matter in the universe. We perform a comprehensive numerical study of the statistical properties of voids, identified both in the matter and galaxy distributions, in massive and massless neutrino cosmologies. The matter density field is obtained by running several independent N-body simulations with cold dark matter and neutrino particles, while the galaxy catalogs are modeled by populating the dark matter halos in simulations via a halo occupation distribution (HOD) model to reproduce the clustering properties observed by the Sloan Digital Sky Survey (SDSS) II Data Release 7. We focus on the impact of massive neutrinos on the following void statistical properties: number density, ellipticities, two-point statistics, density and velocity profiles. Considering the matter density field, we find that voids in massive neutrino cosmologies are less evolved than those in the corresponding massless neutrinos case: there is a larger number of small voids and a smaller number of large ones, their profiles are less evacuated, and they present a lower wall at the edge. Moreover, the degeneracy between σ<SUB>8</SUB> and Ω<SUB>ν</SUB> is broken when looking at void properties. In terms of the galaxy density field, we find that differences among cosmologies are difficult to detect because of the small number of galaxy voids in the simulations. Differences are instead present when looking at the matter density and velocity profiles around these voids. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | Voids in massive neutrino cosmologies | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1088/1475-7516/2015/11/018 | en_US |
dc.identifier.scopus | 2-s2.0-84948773427 | en_US |
dc.identifier.isi | 000365821200019 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.1088/1475-7516/2015/11/018 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 2015 | en_US |
dc.relation.issue | 11 | en_US |
dc.relation.firstpage | 018 | en_US |
dc.relation.lastpage | 018 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | USA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015JCAP...11..018M | en_US |
dc.relation.fund | FP7 | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò il file al passo 5-Carica) | en_US |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 1475-7516 | - |
crisitem.journal.ance | E184073 | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.orcid | 0000-0002-2642-5707 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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1506.03088.pdf | 2.57 MB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.