Please use this identifier to cite or link to this item: https://doi.org/10.1088/0264-9381/31/2/025009
DC FieldValue
dc.titleShearing black holes and scans of the quark matter phase diagram
dc.contributor.authorMcInnes, B.
dc.date.accessioned2014-10-28T02:45:22Z
dc.date.available2014-10-28T02:45:22Z
dc.date.issued2014-01-21
dc.identifier.citationMcInnes, B. (2014-01-21). Shearing black holes and scans of the quark matter phase diagram. Classical and Quantum Gravity 31 (2) : -. ScholarBank@NUS Repository. https://doi.org/10.1088/0264-9381/31/2/025009
dc.identifier.issn13616382
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/104109
dc.description.abstractFuture facilities such as FAIR and NICA are expected to produce collisions of heavy ions generating quark-gluon plasmas (QGPs) with large values of the quark chemical potential; peripheral collisions in such experiments will also lead to large values of the angular momentum density, associated with the internal shearing motion of the plasma. It is well known that shearing motions in fluids can lead to instabilities which cause a transition from laminar to turbulent flow, and such instabilities in the QGP have recently attracted some attention. We set up a holographic model of this situation by constructing a gravitational dual system exhibiting an instability which is indeed triggered by shearing angular momentum in the bulk. We show that holography indicates that the transition to an unstable fluid happens more quickly as one scans across the quark matter phase diagram towards large values of the chemical potential. This may have negative consequences for the observability of quark polarization effects. © 2014 IOP Publishing Ltd.
dc.sourceScopus
dc.subjectblack branes
dc.subjectgauge/gravity duality
dc.subjectholography
dc.typeArticle
dc.contributor.departmentMATHEMATICS
dc.description.doi10.1088/0264-9381/31/2/025009
dc.description.sourcetitleClassical and Quantum Gravity
dc.description.volume31
dc.description.issue2
dc.description.page-
dc.identifier.isiut000329984900010
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