∼ 6% of all known pulsars have been observed to exhibit sudden spin-up events, known as
glitches. For more than fifty years, these phenomena have played an important role in …

In this work, we propose a metamodeling technique to nuclear matter on the basis of a
relativistic density functional with density-dependent couplings. Identical density …

We report here on the first results of a systematic monitoring of southern glitching pulsars at
the Argentine Institute of Radioastronomy that started in the year 2019. We detected a major …

Understanding the average motion of a multitude of superfluid vortices in the interior of a
neutron star is a key ingredient for most theories of pulsar glitches. In this paper, we propose …

The presence of superfluid phases in the interior of a neutron star affects its dynamics, as it
allows for neutrons to flow relative to the non-superfluid (normal) components of the star with …

Measuring a pulsar's rotational evolution is crucial to understanding the nature of the pulsar.
Here, we provide updated timing models for the rotational evolution of six pulsars, five of …

We investigate the effect of a pinned superfluid component on the gravitational wave
emissions of a rotating neutron star. The pinning of superfluid vortices to the flux-tubes in the …

Radio pulsar glitches probe far-from-equilibrium processes involving stress accumulation
and relaxation in neutron star interiors. Previous studies of glitch rates have focused on …

Context. The observation of the first pulse-to-pulse glitch in the Vela pulsar opens a new
window among theoretical speculations on the internal dynamics of neutron stars as it …

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 …