In this chapter, we will be concerned with hadronic interactions in the nuclear medium, particularly under conditions of extreme densities such as those encountered in some compact astrophysical objects. This issue goes to the very core of nuclear physics. In fact, our present knowledge of the nuclear force in free space is, in itself, the result of decades of struggl
I developed my PhD thesis in the aerea of astronuclear theory, an inter- disciplinary field where ma...
We calculate total masses and radii of neutron stars (NS) for pure neutron matter and nuclear matter...
We present results for neutron star models constructed with a new equation of state for nuclear mat...
The equation of state for nuclear matter at finite temperature and the properties of neutron stars a...
International audienceIn this contribution we will review our present understanding of the matter eq...
The goal of microscopic nuclear physics is to describe nuclear structure and nuclear reactions in te...
Neutron stars are remarkable natural laboratories that allow us to investigate the fundamental const...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
We discuss the physics of matter that is relevant to the structure of compact stars. This includes n...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
The density dependencies of various effective interaction strengths in the relativistic mean field a...
Neutron stars are astrophysical objects of extremes, reaching the highest densities we can observe i...
Neutron stars are astrophysical objects of extremes, reaching the highest densities we can observe i...
I developed my PhD thesis in the aerea of astronuclear theory, an inter- disciplinary field where ma...
We calculate total masses and radii of neutron stars (NS) for pure neutron matter and nuclear matter...
We present results for neutron star models constructed with a new equation of state for nuclear mat...
The equation of state for nuclear matter at finite temperature and the properties of neutron stars a...
International audienceIn this contribution we will review our present understanding of the matter eq...
The goal of microscopic nuclear physics is to describe nuclear structure and nuclear reactions in te...
Neutron stars are remarkable natural laboratories that allow us to investigate the fundamental const...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
We discuss the physics of matter that is relevant to the structure of compact stars. This includes n...
We present part of our (direct or indirect) knowledge on the equation of state of nuclear matter in ...
The density dependencies of various effective interaction strengths in the relativistic mean field a...
Neutron stars are astrophysical objects of extremes, reaching the highest densities we can observe i...
Neutron stars are astrophysical objects of extremes, reaching the highest densities we can observe i...
I developed my PhD thesis in the aerea of astronuclear theory, an inter- disciplinary field where ma...
We calculate total masses and radii of neutron stars (NS) for pure neutron matter and nuclear matter...
We present results for neutron star models constructed with a new equation of state for nuclear mat...