Relativistic velocity - potential hydrodynamics and stellar stability

Relativistic velocity - potential hydrodynamics and stellar stability

<p>The equations of relativistic, perfect-fluid hydrodynamics are cast in Eulerian form using six scalar "velocity-potential" fields, each of which has an equation of evolution. These equations determine the motion of the fluid through the equation </p> <p>U<sub>...

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Bibliographic Details
Main Author: Schutz, Bernard Frederick
Format: Others
Published: 1972
Online Access:https://thesis.library.caltech.edu/9630/1/Schutz_bf_1972.pdf
Schutz, Bernard Frederick (1972) Relativistic velocity - potential hydrodynamics and stellar stability. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/05NX-9C06. https://resolver.caltech.edu/CaltechTHESIS:03212016-112353716 <https://resolver.caltech.edu/CaltechTHESIS:03212016-112353716>

Internet

https://thesis.library.caltech.edu/9630/1/Schutz_bf_1972.pdf
Schutz, Bernard Frederick (1972) Relativistic velocity - potential hydrodynamics and stellar stability. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/05NX-9C06. https://resolver.caltech.edu/CaltechTHESIS:03212016-112353716 <https://resolver.caltech.edu/CaltechTHESIS:03212016-112353716>

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