Two types of gamma-ray bursts (GRBs) are observed: short-duration hard spectrum GRBs
and long-duration soft spectrum GRBs. For many years long GRBs were the focus of intense …

Remnants of neutron-star mergers are essentially massive, hot, differentially rotating neutron
stars, which are initially strongly oscillating. As such they represent a unique probe for high …

We investigate the possibility that the low mass companion of the black hole in the source of
GW190814 was a strange quark star. This possibility is viable within the so-called two …

We discuss the formation of Δ isobars in neutron star matter. We show that their threshold
density strictly correlates with the density derivative of the symmetry energy of nuclear …

Formed in the aftermath of gravitational core-collapse supernova explosions, neutron stars
are unique cosmic laboratories for probing the properties of matter under extreme conditions …

The existence of neutron stars with masses of∼ 2 M⊙ requires a stiff equation of state at
high densities. On the other hand, the necessary appearance also at high densities of new …

We investigate the properties of anisotropic, spherically symmetric compact stars, especially
neutron stars (NSs) and strange quark stars (SQSs), made of strongly magnetized matter …

We study radial oscillations of hybrid nonrotating neutron stars composed by a quark matter
core and hadronic external layers. At first, we physically deduce the junction conditions that …

We investigate the hadron-quark phase transition in cold neutron stars in light of (i) the
observed limits on the maximum-mass of heavy pulsars,(ii) constraints on the tidal properties …

The detection of gravitational waves (GWs) from a binary neutron star (BNS) has opened a
new window on gravitational wave astronomy. With current sensitivities, detectable signals …