Eigenfrequencies of Radial Pulsations of Strange Quark Stars
arXiv:astro-ph/9304024 · doi:10.1016/0370-2693(92)90025-Y
Abstract
We calculate the range of eigenfrequencies of radial pulsations of stable strange quark stars, using the general relativistic pulsation equation and adopting realistic equation of state for degenerate strange quark matter.
11pages + 1 figure available upon request,Tex
Cited by in corpus (11)
- Small, Dense Quark Stars from Perturbative QCD
- Physics and Astrophysics of Strange Quark Matter
- Constraint on energy-momentum squared gravity from neutron stars and its cosmological implications
- Quark Hadron Phase Transition and Hybrid Stars
- A reliable description of the radial oscillations of compact stars
- Quark Models and Radial Oscillations: Decoding the HESS J1731-347 Compact Object's Equation of State
- Effect of magnetic field on the strange star
- Radial oscillations and gravitational wave echoes of strange stars for various equations of state
- Radial Modes of Neutron Stars with a Quark Core
- Radial oscillations and gravitational wave echoes of strange stars with nonvanishing lambda
- Mixed Phase in Compact Starts : M-R relations and radial oscillations