The strong magnetic field of neutron stars is intimately coupled to the observed temperature
and spectral properties, as well as to the observed timing properties (distribution of spin …

Scalar-tensor theories with first-derivative self-interactions, known as k-essence, may
provide interesting phenomenology on cosmological scales. On smaller scales, however …

Neutron star mergers are very violent events involving extreme physical processes:
dynamic, strong-field gravity; large magnetic field; very hot, dense matter; and the copious …

Alfvén waves are a particular class of magnetohydrodynamic waves relevant in many
astrophysical and laboratory plasmas. In partially ionized plasmas the dynamics of Alfvén …

The tremendous challenge of comparing our theoretical models with the gravitational-wave
observations in the new era of multimessenger astronomy requires accurate and fast …

In this paper we present a numerical study of the time evolution of solar prominences
embedded in sheared magnetic arcades. The prominence is represented by a density …

In the interior of neutron stars, the induction equation regulates the long-term evolution of the
magnetic fields by means of resistivity, Hall dynamics and ambipolar diffusion. Despite the …

The presence of neutral species in a plasma has been shown to greatly affect the properties
of magnetohydrodynamic waves. For instance, the interaction between ions and neutrals …

Simflowny is a software platform which aims to formalize the main elements of a simulation
flow. It allows users to manage (i) formal representations of physical models based on Initial …

The multi-fluid modeling of high-frequency waves in partially ionized plasmas has shown
that the behavior of magnetohydrodynamic waves in the linear regime is heavily influenced …