
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/">
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:creator id="https://orcid.org/0000-0003-3092-2295">Dimitrijević, Ivan</dc:creator>
  <dc:creator id="https://orcid.org/0000-0002-5818-0150">Dragovich, Branko</dc:creator>
  <dc:creator>Rakić, Zoran</dc:creator>
  <dc:creator id="https://orcid.org/0000-0003-2596-7827">Stanković, Jelena</dc:creator>
  <dc:source>Russian Journal of Mathematical Physics</dc:source>
  <dc:source>volume: 32</dc:source>
  <dc:source>number: 1</dc:source>
  <dc:source>startpage: 1</dc:source>
  <dc:source>endpage: 17</dc:source>
  <dc:format>application/pdf</dc:format>
  <dc:format>562769 bytes</dc:format>
  <dc:language>eng</dc:language>
  <dc:title xml:lang="eng">Nonlocal de Sitter √dS Gravity Model and Its Applications</dc:title>
  <dc:description xml:lang="srp">Abstract— A simple nonlocal de Sitter gravity model (√dS) shows good properties on cosmological
and galactic scales. Its cosmological solution agrees very well with the experimental data. The rotation
curves of spiral galaxies (Milky Way and M33) are also well described by the √dS model. This article
contains a brief overview of earlier results, including a new result on finding an appropriate local
description with a scalar field for cosmological solutions.</dc:description>
  <dc:rights>All rights reserved</dc:rights>
  <dc:date>2025</dc:date>
  <dc:identifier>https://phaidrabg.bg.ac.rs/o:37728</dc:identifier>
  <dc:identifier>doi:10.1134/S1061920824601824</dc:identifier>
  <dc:identifier>ISSN: 061-9208</dc:identifier>
</oai_dc:dc>