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- W3177645360 abstract "We study the non-radial oscillation modes of strange quark stars with a homogeneous core and a crust made of strangelets. Using a 2-component equation of state (core+crust) for strange quark stars that can produce stars as heavy as 2 solar masses, we identify the high-frequency l=2 spheroidal (f, p) in Newtonian gravity, using the Cowling approximation. The results are compared to the case of homogeneous compact stars such as polytropic neutron stars, as well as bare strange stars. We find that the strangelet crust only increases very slightly the frequency of the spheroidal modes, and that Newtonian gravity overestimates the mode frequencies of the strange star, as is the case for neutron stars." @default.
- W3177645360 created "2021-07-19" @default.
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- W3177645360 date "2017-06-01" @default.
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- W3177645360 title "Oscillation modes of strange quark stars with a strangelet crust" @default.
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- W3177645360 doi "https://doi.org/10.1088/1742-6596/861/1/012029" @default.
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