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- W2939668941 abstract "The mechanics of star interiors has remained a subject of much research concern. Many theories have been proposed to account for the behavior of stars. However, these theories have one shortcoming or the other. A star model based on general relativity theory and current astrophysical observations was recently proposed. High gravitational forces, mass concentration in cores, rapid rates of spin and high centripetal forces gives stars their spheroidal shapes. In this article, the gravitational metric tensor of a spherically symmetric sphere containing a non compressible liquid is extended to formulate an oblate spheroidal plasma star model. Using removable space singularities at the Hilbert radius and in outer space, the plasma stars are classified into three major groups (regular, neutron stars and pulsars, black holes). The metric tensor for an oblate spheroidal liquid star obtained has six non zero components as opposed to four for spherical plasma star model." @default.
- W2939668941 created "2019-04-25" @default.
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- W2939668941 date "2019-01-01" @default.
- W2939668941 modified "2023-09-23" @default.
- W2939668941 title "General Relativity Model for Oblate Spheroidal Plasma Stars" @default.
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