1 Ocak 2004 Dergi makalesi Açık Erişim

Ozdemir, F; Odemir, N; Kaynak, BT

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/93685</identifier>
  <creators>
    <creator>
      <creatorName>Ozdemir, F</creatorName>
      <givenName>F</givenName>
      <familyName>Ozdemir</familyName>
    </creator>
    <creator>
      <creatorName>Odemir, N</creatorName>
      <givenName>N</givenName>
      <familyName>Odemir</familyName>
    </creator>
    <creator>
      <creatorName>Kaynak, BT</creatorName>
      <givenName>BT</givenName>
      <familyName>Kaynak</familyName>
    </creator>
  </creators>
  <titles>
    <title>Multi-Black Holes Solution With Cosmic Strings</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2004</publicationYear>
  <dates>
    <date dateType="Issued">2004-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/93685</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.81043/aperta.93684</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.81043/aperta.93685</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
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  <descriptions>
    <description descriptionType="Abstract">Some black hole-cosmic string models such as Reissner-Nordstrom, RN-de Sitter, Kerr-Newman and multi-black holes with cosmic string are given. Energy and angular momentum of a timelike particle in circular orbits in multi-black hole space-time are calculated. The geodesic equations for the timelike particles for the far region of the multi-black hole sources are calculated and small oscillations around the circular orbit obtained. It is seen that the particle's orbit precesses like the Lens-Thirring effect.</description>
  </descriptions>
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