On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra
arXiv:2608.02761 · doi:10.3390/sym18081295
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.
17 pages, 1 table, 5 figures, published in Symmetry
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