Add to ORKGThe EOS of strongly interacting matter at densities ten to fifteen orders of magnitude larger than the typical density of terrestrial macroscopic objects determines a number of neutron star properties, including the pattern of gravitational waves emitted following the excitation of nonradial oscillation modes. This paper reviews some of the approaches employed to model neutron star matter, as well as the prospects for obtaining new insights from the experimental study of gravitational waves emitted by neutron stars
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...
This paper reviews the properties of neutron stars based on the recent multi-messenger observations ...
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...
The EOS of strongly interacting matter at densities ten to fifteen orders of magnitude larger than t...
Neutron stars (NS) are among the most extreme objects in the universe. They are the results of the g...
In this paper, we give a brief overview of how the detection of gravitational waves emitted by neutr...
Neutron-star mergers are closely related to nuclear physics. The nuclear equation of state determine...
A non radially oscillating star emits gravitational waves at frequencies and with damping times that...
International audienceGravitational waves from neutron-star mergers are expected to provide stringen...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...
This paper reviews the properties of neutron stars based on the recent multi-messenger observations ...
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...
The EOS of strongly interacting matter at densities ten to fifteen orders of magnitude larger than t...
Neutron stars (NS) are among the most extreme objects in the universe. They are the results of the g...
In this paper, we give a brief overview of how the detection of gravitational waves emitted by neutr...
Neutron-star mergers are closely related to nuclear physics. The nuclear equation of state determine...
A non radially oscillating star emits gravitational waves at frequencies and with damping times that...
International audienceGravitational waves from neutron-star mergers are expected to provide stringen...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
International audienceIn this paper we give a brief overview of how the detection of gravitational w...
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...
This paper reviews the properties of neutron stars based on the recent multi-messenger observations ...
Recently exploratory studies were performed on the possibility of constraining the neutron star equa...