A Numerical Study of Normal Modes of Rotating Neutron Star Models by the Cowling Approximation

S. Yoshida, Yoshiharu Eriguchi

Type: Article

Publication Date: 1999-04-10

Citations: 48

DOI: https://doi.org/10.1086/307012

Abstract

A numerical method of mode analysis of rapidly rotating relativistic stellar models by the Cowling approximation is applied to rotating neutron stars with realistic equations of state. For selected equations of state, eigenvalues and eigenfunctions of f-modes are numerically solved for stellar models from nonrotating to maximally rotating states.

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The Astrophysical Journal - View - PDF
arXiv (Cornell University) - PDF
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