The general relativistic balance of a spherically symmetric core-and-shell of charged perfect fluid

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dc.contributor.authorChurchill, Lorne Winstonen_US
dc.date.accessioned2024-08-13T17:54:19Z
dc.date.available2024-08-13T17:54:19Z
dc.date.copyright1982en_US
dc.date.issued1982
dc.degree.departmentDepartment of Physics
dc.degree.departmentDepartment of Physics and Astronomy
dc.degree.levelMaster of Science M.Sc.en
dc.description.abstractIn this thesis General Relativistic and Newtonian solutions are derived for a spherically symmetric core and shell of charged perfect fluid in balanced equilibrium. The Darmois junction con­ditions are imposed in order to prevent the occurrence of singular boundary surfaces in the solutions. This enables a simple, logical definition of balance for the system. Newtonian solutions are der­ived and these show that this system possesses more freedom than that of two balanced particles. No single balance condition is found. Relativistic solutions are derived and compared to the Newtonian system. It is found that the properties of the Relativ­istic case are similar to, but more restricted than, those of the Newtonian case.
dc.format.extent97 pages
dc.identifier.urihttps://hdl.handle.net/1828/17486
dc.rightsAvailable to the World Wide Weben_US
dc.titleThe general relativistic balance of a spherically symmetric core-and-shell of charged perfect fluiden_US
dc.typeThesisen_US

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