Axial w-mode frequencies of neutron stars are computed for a dark-matter-admixed quarkyonic EOS, but the claimed axial modes are actually computed with a polar formalism.
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$w$-mode oscillation of neutron star in a new relativistic hybrid model
Axial w-mode frequencies of neutron stars are computed for a dark-matter-admixed quarkyonic EOS, but the claimed axial modes are actually computed with a polar formalism.