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Benhar, Omar; Berti, Emanuele; Ferrari, Valeria
Monthly notices of the Royal Astronomical Society, 12/1999, Letnik: 310, Številka: 3Journal Article
We discuss the dependence of the pulsation frequencies of the axial quasi-normal modes of a non-rotating neutron star upon the equation of state describing the star interior. The continued fraction method has been used to compute the complex frequencies for a set of equations of state based on different physical assumptions and spanning a wide range of stiffness. The numerical results show that axial gravitational waves carry relevant information on both the structure of neutron star matter and the nature of the hadronic interactions.
