The quadrupole oscillations of neutron stars
Sep, 1983Citations per year
Abstract: (ADS)
The influence of the equation of state of matter (in the nuclear density regime) on the dynamical behavior of neutron stars is investigated. The properties of the quadrupole (f-mode) oscillations of neutron stars constructed from 13 equations of state are presented. An efficient algorithm for computing the complex eigenfrequencies of the nonradial (p and f-mode) oscillations of neutron stars is presented. The results of the present computations are compared to relevant astrophysical observations.References(44)
Figures(0)