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The imprint of the equation of state on the axial w-modes of oscillating neutron stars

Monthly Notices of the Royal Astronomical Society, no. 3 (1999): 797-803

Cited: 89|Views27

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equation of stategravitationwavesstars: neutronstars: oscillations

Abstract

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...More

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Omar Benhar

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Emanuele Berti

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Valeria Ferrari

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