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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/14260
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dc.contributor.authorMishra, Madhukar-
dc.date.accessioned2024-02-13T09:42:49Z-
dc.date.available2024-02-13T09:42:49Z-
dc.date.issued2020-12-
dc.identifier.urihttps://academic.oup.com/ptep/article/2021/1/013B09/6054816?login=true-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14260-
dc.description.abstractThermal systems have traditionally been modeled via Euclideanized space by analytical continuation of time to an imaginary time. We extend the concept to static thermal gradients by recasting the temperature variation as a variation in the Euclidean metric. We apply this prescription to determine the quark–antiquark potential in a system with a thermal gradient. A naturally occurring QCD medium with thermal gradients is a quark–gluon plasma (QGP). However, the QGP evolves in time. Hence, we use a quasi-stationary approximation, which is applicable only if the rate of time evolution is slow. The application of our proposal to a quark–antiquark potential in QGP can be seen as a step towards a more exact theory that would incorporate time-varying thermal gradients. The effect of a static temperature gradient on the quark–antiquark potential is analyzed using a gravity dual model. A non-uniform black string metric is developed by perturbing the Schwarzschild metric, which allows us to incorporate the temperature gradient in the dual anti-de Sitter space. Finally, an expression for the quark–antiquark potential in the presence of a static temperature gradient is derived.en_US
dc.language.isoenen_US
dc.publisherOUPen_US
dc.subjectPhysicsen_US
dc.subjectB21 AdS/CFT correspondenceen_US
dc.subjectB68 Holographic approach to QCDen_US
dc.subjectThermal systemsen_US
dc.titleEffect of temperature gradient on heavy quark anti-quark potential using gravity dual modelen_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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