In this article, I introduce ideas and techniques to extract information about the equation of
state of matter at very high densities from gravitational waves emitted before, during and …

Neutron stars and quark stars are ideal laboratories to study fundamental physics at supra
nuclear densities and strong gravitational fields. Astrophysical observables, however …

One century after its formulation, Einstein's general relativity (GR) has made remarkable
predictions and turned out to be compatible with all experimental tests. Most of these tests …

Neutron stars are compact and dense celestial objects that offer the unique opportunity to
explore matter and its interactions under conditions that cannot be reproduced elsewhere in …

Among the various oscillation modes of neutron stars, f-and g-modes are the most likely to
be ultimately observed in binary neutron star mergers due to their relatively large coupling …

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 …

The effect of dark matter (DM) on f-mode oscillations in DM admixed neutron stars (NSs) is
investigated in a comprehensive analysis with particular attention to the role of the nuclear …

We present a systematic study of f-mode oscillations in neutron stars containing hyperons,
extending recent results obtained within the Cowling approximation to linearized general …

Gravitational waves (GWs) from inspiraling neutron stars afford us a unique opportunity to
infer the as-of-yet unknown equation of state of cold hadronic matter at supranuclear …

Tidal effects have an important impact on the late inspiral of compact binary systems
containing neutron stars. Most current models of tidal deformations of neutron stars assume …