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dc.contributor.authorHegde, K.
dc.contributor.authorKumara A., N.
dc.contributor.authorRizwan C.L., A.
dc.contributor.authorK.M., A.
dc.date.accessioned2021-06-07T06:28:34Z
dc.date.available2021-06-07T06:28:34Z
dc.date.issued2021-06-07
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1755
dc.description.abstractModified gravity theories are of great interest in both observational and theoretical studies. In this article we study the correlation between the null geodesics in the background of a fourdimensional Einstein-Maxwell-Gauss-Bonnet AdS black hole, a modification of Einstein gravity, and it’s thermodynamic phase transition. We study the phase structure of the black hole, using the coexistence and spinodal curves, to understand the phase transition in a extended phase space. The imprints of this phase transition features are observed in the behaviour of photon orbit radius and minimum impact parameter with respect to the Hawking temperature and pressure. The change in these two quantities during the phase transition serve as order parameter which characterises the critical behaviour. The correlation shows that thermodynamic phase transition can be studied by observing the effects of strong gravitational field and vice versa.en_US
dc.language.isoen_USen_US
dc.subject4D Gauss-Bonnet gravityen_US
dc.subjectNull geodesicsen_US
dc.subjectBlack hole thermodynamicsen_US
dc.subjectPhase transitionen_US
dc.titleNull geodesics and thermodynamic phase transition of Four-Dimensional Gauss-Bonnet adS black holeen_US
dc.typeArticleen_US
Appears in Collections:Year-2021

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