{"title":"How empty are the voids?","authors":"Anton N. Baushev","doi":"arxiv-2409.02780","DOIUrl":null,"url":null,"abstract":"We find an analytical solution for the minimal matter density of a void, its\ncentral density. It turns out that the voids are not so empty: most of the\nvoids have the central underdensity $\\Delta_c \\sim -50\\%$ (which means that the\nmatter density in their centers is only two times lower than in the Universe on\naverage). For small voids (of radius $R_0\\simeq 5-10$~{Mpc}), the underdensity\ncan be significantly greater, but the number of voids decreases rapidly with\nincreasing of $|\\Delta_c|$ over $50\\%$, and voids with $\\Delta_c < -80\\%$ are\npractically absent. The large voids ($R_0\\ge 40$~{Mpc}) always have $|\\Delta_c|\n< 50\\%$.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"139 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.02780","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We find an analytical solution for the minimal matter density of a void, its
central density. It turns out that the voids are not so empty: most of the
voids have the central underdensity $\Delta_c \sim -50\%$ (which means that the
matter density in their centers is only two times lower than in the Universe on
average). For small voids (of radius $R_0\simeq 5-10$~{Mpc}), the underdensity
can be significantly greater, but the number of voids decreases rapidly with
increasing of $|\Delta_c|$ over $50\%$, and voids with $\Delta_c < -80\%$ are
practically absent. The large voids ($R_0\ge 40$~{Mpc}) always have $|\Delta_c|
< 50\%$.