For the vector MIT bag model tuned to recent NICER and HESS J1731 data, strange quark stars have f-mode gravitational-wave frequencies of about 1.5 to 1.8 kHz and a universal relation with a near-zero intercept.
For instance, near to the maximum mass of the stellar models, the f -mode curves downwards
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Oscillatory properties of strange quark stars described by the vector MIT bag model
For the vector MIT bag model tuned to recent NICER and HESS J1731 data, strange quark stars have f-mode gravitational-wave frequencies of about 1.5 to 1.8 kHz and a universal relation with a near-zero intercept.