Abstract
Following the 3+1 formalism of General Relativity we write the Einstein equations for a stationary rotating neutron star specially suited to be solved numerically with spectral methods. We also provide the equations of motion to study the normal modes once the star is perturbed from the stationary axisymmetric equilibrium configuration.
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J.M. Bardeen, T. Piran: Phys. Rep. 96 205 (1965)
S. Bonazzola, J. Schneider: Astrophys. J. 191 273 (1974)
S. Bonazzola, J.A. Marck: Proceedings of the Frontiers in Numerical Relativity Conference (1988)
S. Bonazzola, J.A. Marck: Journ.Comp.Phys. 87 201 (1990)
S. Bonazzola, E. Gourgoulhon, M.Salgado: to be published
B. Carter: J. Math. Phys. 10 70 (1969)
E. Gourgoulhon: PhD thesis, Université Paris 7 (1992)
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© 1993 Springer-Verlag
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Bonazzola, S., Gourgoulhon, E., Salgado, M. (1993). General relativistic stationary axisymmetric rotating systems. In: Chinea, F.J., González-Romero, L.M. (eds) Rotating Objects and Relativistic Physics. Lecture Notes in Physics, vol 423. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-57364-X_204
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DOI: https://doi.org/10.1007/3-540-57364-X_204
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Online ISBN: 978-3-540-48087-7
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