
<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:identifier>https://phaidrabg.bg.ac.rs/o:32435</dc:identifier>
  <dc:identifier>doi:doi.org/10.2298/FIL2325641D</dc:identifier>
  <dc:identifier>ISSN: 0354-5180 </dc:identifier>
  <dc:date>2023</dc:date>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:rights>All rights reserved</dc:rights>
  <dc:language>eng</dc:language>
  <dc:source>Filomat</dc:source>
  <dc:source>startpage: 8641</dc:source>
  <dc:source>endpage: 8650</dc:source>
  <dc:publisher>Niš : University of Niš, Faculty of Philosophy, Department of Mathematics</dc:publisher>
  <dc:title xml:lang="eng">On the Schwarzschild-de Sitter metric of nonlocal de Sitter gravity</dc:title>
  <dc:description xml:lang="eng">Abstract. Earlier constructed a simple nonlocal de Sitter gravity model has a cosmological solution in a
very good agreement with astronomical observations. In this paper, we continue the investigation of the
nonlocal de Sitter model of gravity, focusing on finding an appropriate solution for the Schwarzschild-de
Sitter metric. We succeeded to solve the equations of motion in a certain approximation. The obtained
approximate solution is of particular interest for examining the possible role of non-local de Sitter gravity
in describing the effects in galactic dynamics that are usually attributed to dark matter.</dc:description>
  <dc:creator>Димитријевић, Иван</dc:creator>
  <dc:creator>Драговић, Бранко</dc:creator>
  <dc:creator>Ракић, Зоран</dc:creator>
  <dc:creator id="https://orcid.org/0000-0003-2596-7827">Станковић, Јелена</dc:creator>
  <dc:format>application/pdf</dc:format>
  <dc:format>146616 bytes</dc:format>
</oai_dc:dc>
