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Impact of the equation of state on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi></mml:mrow></mml:math> - and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi></mml:math> - mode oscillations of neutron stars
We investigate the impact of the neutron-star matter equation of state on the $f$- and ${p}_{1}$-mode oscillations of neutron stars obtained within the Cowling approximation and linearized general relativity. The $f$- and ${p}_{1}$-mode oscillation frequencies, and their damping times are calculated using representative sets of Skyrme Hartree-Fock and relativistic mean-field …