References
- Bardeen, J. M. Wagoner, R. V. Uniformly Rotating Disks in General Relativity apjl, 1969, 158, L65.
- Brill, D. R. and Cohen, J. M. (1966). Rotating masses and their effect on inertial frames. Phys. Rev., 143:1011–1015.
- Dimmelmeier, H., Font, J. A., and Mller, E. (2001). Gravitational waves from relativistic rotational core collapse. The Astrophysical Journal, 560(2):L163–L166.
- Durney, B. and Roxburgh, I. (1967). Rotating massive stars in general relativity. Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 296(1445):189–200.
- Dyks, J., Harding, A. K., and Rudak, B. (2004). Relativistic effects and polarization in three high-energy pulsar models. The Astrophysical Journal, 606(2):1125.
- Hartle, J. B. (1967). Slowly Rotating Relativistic Stars. I. Equations of Structure., 150:1005.
- Hartle, J. B. and Thorne, K. S. (1968). Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars., 153:807.
- Kraniotis, G. V. (2004). Precise relativistic orbits in kerr and kerr–(anti) de sitter spacetimes. Classical and Quantum Gravity, 21(19):4743–4769.
- Miralles, J. A., van Riper, K. A., and Lattimer, J. M. (1993). The Boltzmann equation in general relativistic rotating systems - Cooling of rotating neutron stars. Astrophys. J., 407:687.
- Nakamura, T. (1981). General Relativistic Collapse of Axially Symmetric Stars Leading to the Formation of Rotating Black Holes. Progress of Theoretical Physics, 65(6):1876–1890.
- Ostriker, J. P. and Gunn, J. E. (1969). On the Nature of Pulsars. I. Theory., 157:1395.
- Wang, A. (2013). Stationary axisymmetric and slowly rotating space-times in horava-lifshitz gravity. Phys. Rev. Lett., 110:091101.
- Weber, F. and Glendenning, N. (1991). Applicability of hartle’s method for the construction of general relativistic rotating neutron star models. Technical report.