Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study
G. Panotopoulos, A. Rincon, I. Lopes
gr-qc, astro-ph.HE, astro-ph.SR
Submitted: 2026-06-28
Comments: 26 pages, 1 table, 2 figures, accepted for publication in Fortschritte der Physik
Journal ref: Fortschritte der Physik, Volume 74, Issue 7, July 2026
DOI: 10.1002/prop.70132
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Nuclear Equation of State and Neutron Star Masses
- Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
- The Physics of Neutron Stars
- The Equation of State of Hot, Dense Matter and Neutron Stars
- Equations of state for supernovae and compact stars
- Neutron Stars and the Nuclear Equation of State
- Asteroseismology: radial oscillations of neutron stars with realistic equation of state
- Radial Oscillations of Hybrid Stars and Neutron Stars including Delta baryons: The Effect of a Slow Quark Phase Transition
- Color-superconducting quarkyonic matter
- Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement
- Towards gravitational-wave asteroseismology
- Quasi-Normal Modes of Stars and Black Holes
- Signatures of hadron-quark mixed phase in gravitational waves
- The stability of relativistic stars and the role of the adiabatic index
- A reliable description of the radial oscillations of compact stars
- Radial oscillations and gravitational wave echoes of strange stars for various equations of state
- Radial stability of anisotropic strange quark stars
- Stellar Structure and Stability of Charged Interacting Quark Stars and Their Scaling Behaviour
- Anisotropic strange quark stars with a non-linear equation-of-state
- Exact solutions for compact stars with CFL quark matter
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