Gravitational Waves from Relativistic Stars
arXiv:gr-qc/0002079 · doi:10.1143/PTPS.136.135
Abstract
Stellar pulsations in rotating relativistic stars are reviewed. Slow rotation approximation is applied to solving the Einstein equations. The rotational effects on the non-axisymmetric oscillations are explicitly shown in the polar and axial modes.
11 pages, Latex file without figures. Proceedings of Yukawa International Seminar 99