1 Ocak 2015 Dergi makalesi Açık Erişim

Abdujabbarov, Ahmadjon; Atamurotov, Farruh; Dadhich, Naresh; Ahmedov, Bobomurat; Stuchlik, Zdenek

Dublin Core

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  <dc:creator>Abdujabbarov, Ahmadjon</dc:creator>
  <dc:creator>Atamurotov, Farruh</dc:creator>
  <dc:creator>Dadhich, Naresh</dc:creator>
  <dc:creator>Ahmedov, Bobomurat</dc:creator>
  <dc:creator>Stuchlik, Zdenek</dc:creator>
  <dc:date>2015-01-01</dc:date>
  <dc:description>We study physical processes around a rotating black hole in pure Gauss-Bonnet (GB) gravity. In pure GB gravity, the gravitational potential has a slower fall-off as compared to the corresponding Einstein potential in the same dimension. It is therefore expected that the energetics of a pure GB black hole would be weaker, and our analysis bears out that the efficiency of energy extraction by the Penrose-process is increased to 25.8% and the particle acceleration is increased to 55.28 %; the optical shadow of the black hole is decreased. These are in principle distinguishing observable features of a pure GB black hole.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/80635</dc:identifier>
  <dc:identifier>oai:zenodo.org:80635</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:source>EUROPEAN PHYSICAL JOURNAL C 75(8)</dc:source>
  <dc:title>Energetics and optical properties of 6-dimensional rotating black hole in pure Gauss-Bonnet gravity</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
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