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dc.contributor.authorDrake, S. P. (Samuel Pictor)en
dc.descriptionBibliography: leaves 126-131.en
dc.description131 leaves : ill. ; 30 cm.en
dc.description.abstractAddresses the problem of obtaining exact solutions to Einstein's field equation describing rotating perfect fluids and also whether or not the known chaotic nature of geodesics in the relativistic fixed two centre problem is due to the non-linear nature of general relativity or the kinematic properties relativistic mechanics. The conclusion drawn from the two studies is that the properties of relativistic stationary axisymmetric spacetime are quite different from what is found in Newtonian physics.en
dc.format.extent60167 bytesen
dc.subject.lcshRelativity (Physics)en
dc.subject.lcshSpace and timeen
dc.titleAxisymmetric spacetimes in relativity / S.P. Drake.en
dc.contributor.schoolDept. of Physics and Mathematical Physicsen
dc.provenanceThis electronic version is made publicly available by the University of Adelaide in accordance with its open access policy for student theses. Copyright in this thesis remains with the author. This thesis may incorporate third party material which has been used by the author pursuant to Fair Dealing exception. If you are the author of this thesis and do not wish it to be made publicly available or If you are the owner of any included third party copyright material you wish to be removed from this electronic version, please complete the take down form located at:
dc.description.dissertationThesis (Ph.D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1999?en
Appears in Collections:Research Theses

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