Gravitational Waves from Relativistic Stars
Yasufumi Kojima (Dept. of Phys., Hiroshima University)
TL;DR
This paper reviews stellar pulsations in rotating relativistic stars, focusing on how slow rotation affects non-axisymmetric oscillations through solutions of Einstein's equations.
Contribution
It provides a detailed analysis of rotational effects on stellar oscillations using the slow rotation approximation in relativistic stars.
Findings
Rotational effects significantly influence non-axisymmetric modes.
Explicit solutions for polar and axial oscillations are presented.
The slow rotation approximation effectively models stellar pulsations.
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.
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