1 Ocak 2018 Dergi makalesi Açık Erişim

Sert, Özcan; Çeliktaş, Fatma; Adak, Muzaffer

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/106341</identifier>
  <creators>
    <creator>
      <creatorName>Sert, Özcan</creatorName>
      <givenName>Özcan</givenName>
      <familyName>Sert</familyName>
      <affiliation>Department of Mathematics, Faculty of Arts and Sciences, Pamukkale University, Denizli, 20070, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Çeliktaş, Fatma</creatorName>
      <givenName>Fatma</givenName>
      <familyName>Çeliktaş</familyName>
      <affiliation>Department of Mathematics, Faculty of Arts and Sciences, Pamukkale University, Denizli, 20070, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Adak, Muzaffer</creatorName>
      <givenName>Muzaffer</givenName>
      <familyName>Adak</familyName>
      <affiliation>Department of Physics, Faculty of Arts and Sciences, Pamukkale University, Denizli, 20070, Turkey</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Anisotropic Stars In The Non-Minimal   $Y\Left(R\Right){F}^{2}$  Gravity</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2018</publicationYear>
  <dates>
    <date dateType="Issued">2018-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/106341</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1140/epjc/s10052-018-6302-2</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>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;We investigate anisotropic compact stars in the non-minimal   $Y\left(R\right){F}^{2}$  model of gravity which couples an arbitrary function of curvature scalar Y(R) to the electromagnetic field invariant   ${F}^{2}$ . After we obtain exact anisotropic solutions to the field equations of the model, we apply the continuity conditions to the solutions at the boundary of the star. Then we find the mass, electric charge, and surface gravitational redshift by the parameters of the model and radius of the star.&lt;/p&gt;</description>
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