Exploring the fluid landscape: three new regimes of relativistic hydrodynamics

dc.contributor.authorHernandez, Juan
dc.contributor.supervisorKovtun, Pavel
dc.date.accessioned2017-08-22T18:37:37Z
dc.date.available2017-08-22T18:37:37Z
dc.date.copyright2017en_US
dc.date.issued2017-08-22
dc.degree.departmentDepartment of Physics and Astronomyen_US
dc.degree.levelMaster of Science M.Sc.en_US
dc.description.abstractIn this work, we use the recently developed equilibrium generating functional and systematic derivative expansion approach to hydrodynamics to explore three new regimes of relativistic hydrodynamics. First, we derive the equations of motion and write the constitutive relations to first order in derivatives for relativistic fluids coupled to an external vector field. Next, for relativistic fluids in strong magnetic fields B ~ O(1), we derive the equations of motion and present the constitutive relations to first order in derivatives. From the resulting system of equations, we find the hydrodynamic modes for these systems. We also find the constraints on the transport coefficients due to the entropy production argument and derive the corresponding Kubo formulas. Finally, we repeat the same analysis for relativistic fluids coupled to dynamical electromagnetic fields with <B> ~ O(1).en_US
dc.description.scholarlevelGraduateen_US
dc.identifier.urihttp://hdl.handle.net/1828/8449
dc.languageEnglisheng
dc.language.isoenen_US
dc.rightsAvailable to the World Wide Weben_US
dc.subjectrelativityen_US
dc.subjecthydrodynamicsen_US
dc.subjectmagnetohydrodynamicsen_US
dc.subjectthermodynamicsen_US
dc.subjecttransporten_US
dc.subjecteffective field theoryen_US
dc.titleExploring the fluid landscape: three new regimes of relativistic hydrodynamicsen_US
dc.typeThesisen_US

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