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Abdujabbarov, Ahmadjon; Atamurotov, Farruh; Dadhich, Naresh; Ahmedov, Bobomurat; Stuchlik, Zdenek
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<identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/80635</identifier>
<creators>
<creator>
<creatorName>Abdujabbarov, Ahmadjon</creatorName>
<givenName>Ahmadjon</givenName>
<familyName>Abdujabbarov</familyName>
</creator>
<creator>
<creatorName>Atamurotov, Farruh</creatorName>
<givenName>Farruh</givenName>
<familyName>Atamurotov</familyName>
</creator>
<creator>
<creatorName>Dadhich, Naresh</creatorName>
<givenName>Naresh</givenName>
<familyName>Dadhich</familyName>
</creator>
<creator>
<creatorName>Ahmedov, Bobomurat</creatorName>
<givenName>Bobomurat</givenName>
<familyName>Ahmedov</familyName>
</creator>
<creator>
<creatorName>Stuchlik, Zdenek</creatorName>
<givenName>Zdenek</givenName>
<familyName>Stuchlik</familyName>
<affiliation>Silesian Univ Opava, Inst Phys, Fac Philosophy & Sci, Opava, Czech Republic</affiliation>
</creator>
</creators>
<titles>
<title>Energetics And Optical Properties Of 6-Dimensional Rotating Black Hole In Pure Gauss-Bonnet Gravity</title>
</titles>
<publisher>Aperta</publisher>
<publicationYear>2015</publicationYear>
<dates>
<date dateType="Issued">2015-01-01</date>
</dates>
<resourceType resourceTypeGeneral="Text">Journal article</resourceType>
<alternateIdentifiers>
<alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/80635</alternateIdentifier>
</alternateIdentifiers>
<relatedIdentifiers>
<relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1140/epjc/s10052-015-3604-5</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">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.</description>
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