In this work, we make the first step to derive nonradial pulsation equations in extra
dimensions and investigate how the f-and p 1-mode frequencies of strange quark stars …

The influence of the dimensions on the f and p 1 pulsation modes from strange quark stars,
in the Cowling approximation, are investigated. For that purpose, the d-dimensional …

In this work we study, within the framework of Cowling approximation, the effect of the
electric charge on the gravitational wave frequency of fluid oscillation modes of strange …

Matter in compact stars is dense enough that transient events within the star could have
sufficiently high energies to produce detectable gravitational waves (GWs). These GWs …

Recently, it has been reported that a candidate for a quark star may have been observed. In
this article, we consider quark stars with radiation radii in the reported range. We calculate …

The observation of gravitational waves from compact stars (neutron and quark stars) is a
promising method of determining their internal composition. This research presents the …

We study the relativistic quadrupole oscillations (l= 2) of strange-quark stars by calculating
their quasi-normal modes, and we thus explore the possibility of using these oscillation …

It has recently been claimed, with a 4.2 σ significance level, that gravitational wave echoes
at a frequency of about 72 Hz have been produced in the GW170817 event. The merging of …

We propose here a robust scheme to infer the physical parameters of compact stars from
their f-mode gravitational wave signals. We first show that the frequency and the damping …

One of the key aspects in the comprehension of neutron star (NS) interiors is the
identification of observables that may impose constraints on the equation of state (EoS). At …