## Relativity, Thermodynamics, and Cos

- N. Stergioulas, J. L. Friedman
- Stoeckly, R. 1965,
- 1995

@inproceedings{Kim2009PseudoNewtonianMF, title={Pseudo-Newtonian Models for the Equilibrium Structures of Rotating Relativistic Stars}, author={Jinho Kim and Hee Il Kim and Hyung Mok Lee}, year={2009} }

- Published 2009

We obtain equilibrium solutions for rotating compact stars including the special relativistic effects. The gravity is assumed to be Newtonian, but we used the active mass density, which takes into account all the energies such as motions of the fluids, internal energy, pressure energy in addition to the rest mass energy, in computing the gravitational… CONTINUE READING

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