On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra

Abstract

We model the compact object Cen X-3, which is considered to be a good strange quark star candidate of known mass and radius, incorporating a negative anisotropic factor, and we compute the frequencies of the ten lowest radial oscillation modes. We introduce the anisotropy in three different manners and investigate its impact on the spectra.

arXiv comment17 pages, 1 table, 5 figures, published in Symmetry

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